Reduction Log for Sept. 06, 2003 -----> IRAS 18250-0351 <----- 1) Subtract dark imarith IRAS18250.011.fits - dark10.fits IRAS18250.011d.fits imarith IRAS18250.012.fits - dark10.fits IRAS18250.012d.fits imarith IRAS18250.013.fits - dark10.fits IRAS18250.013d.fits imarith IRAS18250.014.fits - dark10.fits IRAS18250.014d.fits imarith IRAS18250.015.fits - dark10.fits IRAS18250.015d.fits imarith IRAS18250.016.fits - dark10.fits IRAS18250.016d.fits imarith IRAS18250.017.fits - dark10.fits IRAS18250.017d.fits imarith IRAS18250.018.fits - dark10.fits IRAS18250.018d.fits imarith IRAS18250.019.fits - dark10.fits IRAS18250.019d.fits 2) Scale images to same (mean = 5655.44 sky) value imstat IRAS18250.*d.fits >> awklist.txt imarith IRAS18250.011d.fits * 0.990965 IRAS18250.011a.fits imarith IRAS18250.012d.fits * 1.01552 IRAS18250.012a.fits imarith IRAS18250.013d.fits * 1.00756 IRAS18250.013a.fits imarith IRAS18250.014d.fits * 1.00416 IRAS18250.014a.fits imarith IRAS18250.015d.fits * 0.999901 IRAS18250.015a.fits imarith IRAS18250.016d.fits * 1.0022 IRAS18250.016a.fits imarith IRAS18250.017d.fits * 0.993577 IRAS18250.017a.fits imarith IRAS18250.018d.fits * 1.00096 IRAS18250.018a.fits imarith IRAS18250.019d.fits * 0.985784 IRAS18250.019a.fits imstat IRAS18250*a.fits 3) Make skyflat (avg combine, min=0 max=2 reject) epar imcomb imcomb IRAS18250.*a.fits IRAS18250.sky.fits 4) Normalize by midpt imstat IRAS18250.sky.fits imarith IRAS18250.sky.fits / 5608. IRAS18250.skyN.fits 5) Divide by skyflat imarith IRAS18250.011d.fits / IRAS18250.skyN.fits IRAS18250.011df.fits imarith IRAS18250.012d.fits / IRAS18250.skyN.fits IRAS18250.012df.fits imarith IRAS18250.013d.fits / IRAS18250.skyN.fits IRAS18250.013df.fits imarith IRAS18250.014d.fits / IRAS18250.skyN.fits IRAS18250.014df.fits imarith IRAS18250.015d.fits / IRAS18250.skyN.fits IRAS18250.015df.fits imarith IRAS18250.016d.fits / IRAS18250.skyN.fits IRAS18250.016df.fits imarith IRAS18250.017d.fits / IRAS18250.skyN.fits IRAS18250.017df.fits imarith IRAS18250.018d.fits / IRAS18250.skyN.fits IRAS18250.018df.fits imarith IRAS18250.019d.fits / IRAS18250.skyN.fits IRAS18250.019df.fits 6) Subtract by constant (midpt) imstat IRAS18250.*df.fits imarith IRAS18250.011df.fits - 5677. IRAS18250.011dfs.fits imarith IRAS18250.012df.fits - 5534. IRAS18250.012dfs.fits imarith IRAS18250.013df.fits - 5581. IRAS18250.013dfs.fits imarith IRAS18250.014df.fits - 5598. IRAS18250.014dfs.fits imarith IRAS18250.015df.fits - 5630. IRAS18250.015dfs.fits imarith IRAS18250.016df.fits - 5609. IRAS18250.016dfs.fits imarith IRAS18250.017df.fits - 5663. IRAS18250.017dfs.fits imarith IRAS18250.018df.fits - 5618. IRAS18250.018dfs.fits imarith IRAS18250.019df.fits - 5705. IRAS18250.019dfs.fits 7) get coords and shifts shifts: 553.80 604.05 661.85 502.54 553.38 501.16 449.06 503.16 659.36 604.04 449.86 604.23 661.13 708.44 556.24 709.00 455.23 709.26 0. 0. -108.05 101.51 0.42 102.89 104.74 100.89 -105.56 0.01 103.94 -0.18 -107.33 -104.39 -2.44 -104.95 98.57 -105.21 coords: 280.03 395.19 414.56 187.14 481.03 235.10 585.49 397.45 701.99 568.98 553.80 604.05 741.03 215.25 -----> IRAS 18318-0434 <----- 1) Subtract dark imarith IRAS18318.021.fits - dark60.fits IRAS18318.021d.fits imarith IRAS18318.022.fits - dark60.fits IRAS18318.022d.fits imarith IRAS18318.023.fits - dark60.fits IRAS18318.023d.fits imarith IRAS18318.024.fits - dark60.fits IRAS18318.024d.fits imarith IRAS18318.025.fits - dark60.fits IRAS18318.025d.fits imarith IRAS18318.026.fits - dark60.fits IRAS18318.026d.fits imarith IRAS18318.027.fits - dark60.fits IRAS18318.027d.fits imarith IRAS18318.028.fits - dark60.fits IRAS18318.028d.fits imarith IRAS18318.029.fits - dark60.fits IRAS18318.029d.fits 2) Scale images to same (mean = 13362.8 sky) value imstat IRAS18318.*d.fits >> awklist.txt imarith IRAS18318.021d.fits * 1.03021 IRAS18318.021a.fits imarith IRAS18318.022d.fits * 1.02201 IRAS18318.022a.fits imarith IRAS18318.023d.fits * 1.00844 IRAS18318.023a.fits imarith IRAS18318.024d.fits * 1.00096 IRAS18318.024a.fits imarith IRAS18318.025d.fits * 0.998938 IRAS18318.025a.fits imarith IRAS18318.026d.fits * 0.991894 IRAS18318.026a.fits imarith IRAS18318.027d.fits * 0.982776 IRAS18318.027a.fits imarith IRAS18318.028d.fits * 0.986476 IRAS18318.028a.fits imarith IRAS18318.029d.fits * 0.980684 IRAS18318.029a.fits imstat IRAS18318*a.fits 3) Make skyflat (avg combine, min=0 max=2 reject) epar imcomb imcomb IRAS18318.*a.fits IRAS18318.sky.fits 4) Normalize by midpt imstat IRAS18318.sky.fits imarith IRAS18318.sky.fits / 13267. IRAS18318.skyN.fits 5) Divide by skyflat imarith IRAS18318.021d.fits / IRAS18318.skyN.fits IRAS18318.021df.fits imarith IRAS18318.022d.fits / IRAS18318.skyN.fits IRAS18318.022df.fits imarith IRAS18318.023d.fits / IRAS18318.skyN.fits IRAS18318.023df.fits imarith IRAS18318.024d.fits / IRAS18318.skyN.fits IRAS18318.024df.fits imarith IRAS18318.025d.fits / IRAS18318.skyN.fits IRAS18318.025df.fits imarith IRAS18318.026d.fits / IRAS18318.skyN.fits IRAS18318.026df.fits imarith IRAS18318.027d.fits / IRAS18318.skyN.fits IRAS18318.027df.fits imarith IRAS18318.028d.fits / IRAS18318.skyN.fits IRAS18318.028df.fits imarith IRAS18318.029d.fits / IRAS18318.skyN.fits IRAS18318.029df.fits 6) Subtract by constant (midpt) imstat IRAS18318.*df.fits imarith IRAS18318.021df.fits - 12891. IRAS18318.021dfs.fits imarith IRAS18318.022df.fits - 12980. IRAS18318.022dfs.fits imarith IRAS18318.023df.fits - 13164. IRAS18318.023dfs.fits imarith IRAS18318.024df.fits - 13269. IRAS18318.024dfs.fits imarith IRAS18318.025df.fits - 13290. IRAS18318.025dfs.fits imarith IRAS18318.026df.fits - 13402. IRAS18318.026dfs.fits imarith IRAS18318.027df.fits - 13519. IRAS18318.027dfs.fits imarith IRAS18318.028df.fits - 13484. IRAS18318.028dfs.fits imarith IRAS18318.029df.fits - 13545. IRAS18318.029dfs.fits 7) get coords and shifts shifts: 531.63 576.88 636.96 471.85 533.67 471.47 428.45 472.89 641.14 574.74 431.72 577.09 644.02 680.25 538.67 682.29 434.48 684.45 0. 0. -105.33 105.03 -2.04 105.41 103.18 103.99 -109.51 2.14 99.91 -0.21 -112.39 -103.37 -7.04 -105.41 97.15 -107.57 coords: 256.87 552.19 348.93 430.71 405.06 268.97 770.77 163.40 531.59 576.89 533.95 645.18 ----> IRAS 18339-0224 <----- 1) Subtract dark imarith IRAS18339.034.fits - dark60.fits IRAS18339.034d.fits imarith IRAS18339.035.fits - dark60.fits IRAS18339.035d.fits imarith IRAS18339.036.fits - dark60.fits IRAS18339.036d.fits imarith IRAS18339.037.fits - dark60.fits IRAS18339.037d.fits imarith IRAS18339.038.fits - dark60.fits IRAS18339.038d.fits imarith IRAS18339.039.fits - dark60.fits IRAS18339.039d.fits imarith IRAS18339.040.fits - dark60.fits IRAS18339.040d.fits imarith IRAS18339.041.fits - dark60.fits IRAS18339.041d.fits imarith IRAS18339.042.fits - dark60.fits IRAS18339.042d.fits 2) Scale images to same (mean = 13632.9 sky) value imstat IRAS18339.*d.fits >> awklist.txt imarith IRAS18339.034d.fits * 1.02311 IRAS18339.034a.fits imarith IRAS18339.035d.fits * 1.01503 IRAS18339.035a.fits imarith IRAS18339.036d.fits * 1.01164 IRAS18339.036a.fits imarith IRAS18339.037d.fits * 1.0022 IRAS18339.037a.fits imarith IRAS18339.038d.fits * 1.00323 IRAS18339.038a.fits imarith IRAS18339.039d.fits * 1.00065 IRAS18339.039a.fits imarith IRAS18339.040d.fits * 0.985463 IRAS18339.040a.fits imarith IRAS18339.041d.fits * 0.989612 IRAS18339.041a.fits imarith IRAS18339.042d.fits * 0.971143 IRAS18339.042a.fits imstat IRAS18339*a.fits 3) Make skyflat (avg combine, min=0 max=2 reject) epar imcomb imcomb IRAS18339.*a.fits IRAS18339.sky.fits 4) Normalize by midpt imstat IRAS18339.sky.fits imarith IRAS18339.sky.fits / 13579. IRAS18339.skyN.fits 5) Divide by skyflat imarith IRAS18339.034d.fits / IRAS18339.skyN.fits IRAS18339.034df.fits imarith IRAS18339.035d.fits / IRAS18339.skyN.fits IRAS18339.035df.fits imarith IRAS18339.036d.fits / IRAS18339.skyN.fits IRAS18339.036df.fits imarith IRAS18339.037d.fits / IRAS18339.skyN.fits IRAS18339.037df.fits imarith IRAS18339.038d.fits / IRAS18339.skyN.fits IRAS18339.038df.fits imarith IRAS18339.039d.fits / IRAS18339.skyN.fits IRAS18339.039df.fits imarith IRAS18339.040d.fits / IRAS18339.skyN.fits IRAS18339.040df.fits imarith IRAS18339.041d.fits / IRAS18339.skyN.fits IRAS18339.041df.fits imarith IRAS18339.042d.fits / IRAS18339.skyN.fits IRAS18339.042df.fits 6) Subtract by constant (midpt) imstat IRAS18339.*df.fits imarith IRAS18339.034df.fits - 13301. IRAS18339.034dfs.fits imarith IRAS18339.035df.fits - 13389. IRAS18339.035dfs.fits imarith IRAS18339.036df.fits - 13443. IRAS18339.036dfs.fits imarith IRAS18339.037df.fits - 13563. IRAS18339.037dfs.fits imarith IRAS18339.038df.fits - 13562. IRAS18339.038dfs.fits imarith IRAS18339.039df.fits - 13603. IRAS18339.039dfs.fits imarith IRAS18339.040df.fits - 13792. IRAS18339.040dfs.fits imarith IRAS18339.041df.fits - 13742. IRAS18339.041dfs.fits imarith IRAS18339.042df.fits - 14005. IRAS18339.042dfs.fits 7) get coords and shifts shifts: 515.93 516.29 623.09 411.14 517.50 411.47 412.79 411.91 624.45 509.09 414.56 512.22 625.85 613.05 520.34 615.13 413.96 617.94 0. 0. -107.16 105.15 -1.57 104.82 103.14 104.38 -108.52 7.2 101.37 4.07 -109.92 -96.76 -4.41 -98.84 101.97 -101.65 coords: 264.44 485.42 350.14 587.46 540.11 702.40 624.41 718.70 721.00 776.10 366.12 308.50 721.83 187.60 -----> IRAS 18558+0041 <------ 1) Subtract dark imarith IRAS18558.044.fits - dark60.fits IRAS18558.044d.fits imarith IRAS18558.045.fits - dark60.fits IRAS18558.045d.fits imarith IRAS18558.046.fits - dark60.fits IRAS18558.046d.fits imarith IRAS18558.047.fits - dark60.fits IRAS18558.047d.fits imarith IRAS18558.048.fits - dark60.fits IRAS18558.048d.fits imarith IRAS18558.049.fits - dark60.fits IRAS18558.049d.fits imarith IRAS18558.050.fits - dark60.fits IRAS18558.050d.fits imarith IRAS18558.051.fits - dark60.fits IRAS18558.051d.fits imarith IRAS18558.052.fits - dark60.fits IRAS18558.052d.fits 2) Scale images to same (mean = 13429.3 sky) value imstat IRAS18558.*d.fits >> awklist.txt imarith IRAS18558.044d.fits * 1.00752 IRAS18558.044a.fits imarith IRAS18558.045d.fits * 0.968576 IRAS18558.045a.fits imarith IRAS18558.046d.fits * 1.00768 IRAS18558.046a.fits imarith IRAS18558.047d.fits * 1.00519 IRAS18558.047a.fits imarith IRAS18558.048d.fits * 1.00768 IRAS18558.048a.fits imarith IRAS18558.049d.fits * 1.00421 IRAS18558.049a.fits imarith IRAS18558.050d.fits * 1.00541 IRAS18558.050a.fits imarith IRAS18558.051d.fits * 1.00204 IRAS18558.051a.fits imarith IRAS18558.052d.fits * 0.992998 IRAS18558.052a.fits imstat IRAS18558*a.fits 3) Make skyflat (avg combine, min=0 max=2 reject) epar imcomb imcomb IRAS18558.*a.fits IRAS18558.sky.fits 4) Normalize by midpt imstat IRAS18558.sky.fits imarith IRAS18558.sky.fits / 13377. IRAS18558.skyN.fits 5) Divide by skyflat imarith IRAS18558.044d.fits / IRAS18558.skyN.fits IRAS18558.044df.fits imarith IRAS18558.045d.fits / IRAS18558.skyN.fits IRAS18558.045df.fits imarith IRAS18558.046d.fits / IRAS18558.skyN.fits IRAS18558.046df.fits imarith IRAS18558.047d.fits / IRAS18558.skyN.fits IRAS18558.047df.fits imarith IRAS18558.048d.fits / IRAS18558.skyN.fits IRAS18558.048df.fits imarith IRAS18558.049d.fits / IRAS18558.skyN.fits IRAS18558.049df.fits imarith IRAS18558.050d.fits / IRAS18558.skyN.fits IRAS18558.050df.fits imarith IRAS18558.051d.fits / IRAS18558.skyN.fits IRAS18558.051df.fits imarith IRAS18558.052d.fits / IRAS18558.skyN.fits IRAS18558.052df.fits 6) Subtract by constant (midpt) imstat IRAS18558.*df.fits imarith IRAS18558.044df.fits - 13300. IRAS18558.044dfs.fits imarith IRAS18558.045df.fits - 13844. IRAS18558.045dfs.fits imarith IRAS18558.046df.fits - 13292. IRAS18558.046dfs.fits imarith IRAS18558.047df.fits - 13341. IRAS18558.047dfs.fits imarith IRAS18558.048df.fits - 13288. IRAS18558.048dfs.fits imarith IRAS18558.049df.fits - 13348. IRAS18558.049dfs.fits imarith IRAS18558.050df.fits - 13313. IRAS18558.050dfs.fits imarith IRAS18558.051df.fits - 13362. IRAS18558.051dfs.fits imarith IRAS18558.052df.fits - 13497. IRAS18558.052dfs.fits 7) get coords and shifts shifts: 500.77 553.84 603.72 449.97 500.25 448.96 396.16 450.31 608.20 548.86 397.39 551.29 609.90 652.54 507.40 654.63 402.81 656.95 0. 0. -102.95 103.87 0.52 104.88 104.61 103.53 -107.43 4.98 103.38 2.55 -109.13 -98.7 -6.63 -100.79 97.96 -103.11 coords: 400.80 531.72 439.74 419.68 572.80 397.84 774.30 589.57 642.20 682.00 515.31 697.96 611.75 588.17 ----> IRAS 22376+7455 <----- 1) Subtract dark imarith IRAS22376.054.fits - dark60.fits IRAS22376.054d.fits imarith IRAS22376.055.fits - dark60.fits IRAS22376.055d.fits imarith IRAS22376.056.fits - dark60.fits IRAS22376.056d.fits imarith IRAS22376.057.fits - dark60.fits IRAS22376.057d.fits imarith IRAS22376.058.fits - dark60.fits IRAS22376.058d.fits imarith IRAS22376.059.fits - dark60.fits IRAS22376.059d.fits imarith IRAS22376.060.fits - dark60.fits IRAS22376.060d.fits imarith IRAS22376.061.fits - dark60.fits IRAS22376.061d.fits imarith IRAS22376.062.fits - dark60.fits IRAS22376.062d.fits 2) Scale images to same (mean = 13253.3 sky) value imstat IRAS22376.*d.fits >> awklist.txt imarith IRAS22376.054d.fits * 0.997614 IRAS22376.054a.fits imarith IRAS22376.055d.fits * 1.00678 IRAS22376.055a.fits imarith IRAS22376.056d.fits * 1.00801 IRAS22376.056a.fits imarith IRAS22376.057d.fits * 1.00343 IRAS22376.057a.fits imarith IRAS22376.058d.fits * 0.998215 IRAS22376.058a.fits imarith IRAS22376.059d.fits * 1.00017 IRAS22376.059a.fits imarith IRAS22376.060d.fits * 0.996189 IRAS22376.060a.fits imarith IRAS22376.061d.fits * 0.998967 IRAS22376.061a.fits imarith IRAS22376.062d.fits * 0.990827 IRAS22376.062a.fits imstat IRAS22376*a.fits 3) Make skyflat (avg combine, min=0 max=2 reject) epar imcomb imcomb IRAS22376.*a.fits IRAS22376.sky.fits 4) Normalize by midpt imstat IRAS22376.sky.fits imarith IRAS22376.sky.fits / 13262. IRAS22376.skyN.fits 5) Divide by skyflat imarith IRAS22376.054d.fits / IRAS22376.skyN.fits IRAS22376.054df.fits imarith IRAS22376.055d.fits / IRAS22376.skyN.fits IRAS22376.055df.fits imarith IRAS22376.056d.fits / IRAS22376.skyN.fits IRAS22376.056df.fits imarith IRAS22376.057d.fits / IRAS22376.skyN.fits IRAS22376.057df.fits imarith IRAS22376.058d.fits / IRAS22376.skyN.fits IRAS22376.058df.fits imarith IRAS22376.059d.fits / IRAS22376.skyN.fits IRAS22376.059df.fits imarith IRAS22376.060d.fits / IRAS22376.skyN.fits IRAS22376.060df.fits imarith IRAS22376.061d.fits / IRAS22376.skyN.fits IRAS22376.061df.fits imarith IRAS22376.062d.fits / IRAS22376.skyN.fits IRAS22376.062df.fits 6) Subtract by constant (midpt) imstat IRAS22376.*df.fits imarith IRAS22376.054df.fits - 13322. IRAS22376.054dfs.fits imarith IRAS22376.055df.fits - 13200. IRAS22376.055dfs.fits imarith IRAS22376.056df.fits - 13182. IRAS22376.056dfs.fits imarith IRAS22376.057df.fits - 13246. IRAS22376.057dfs.fits imarith IRAS22376.058df.fits - 13305. IRAS22376.058dfs.fits imarith IRAS22376.059df.fits - 13288. IRAS22376.059dfs.fits imarith IRAS22376.060df.fits - 13331. IRAS22376.060dfs.fits imarith IRAS22376.061df.fits - 13301. IRAS22376.061dfs.fits imarith IRAS22376.062df.fits - 13414. IRAS22376.062dfs.fits 7) get coords and shifts shifts: 474.91 428.96 580.85 326.39 476.14 325.95 371.62 324.54 583.02 423.10 373.82 424.16 585.88 527.92 481.84 528.13 378.79 528.20 0. 0. -105.94 102.57 -1.23 103.01 103.29 104.42 -108.11 5.86 101.09 4.8 -110.97 -98.96 -6.93 -99.17 96.12 -99.24 coords: 474.91 428.96 236.90 311.67 540.83 581.80 572.95 560.99 655.16 445.34 520.00 174.22 838.20 633.64 ------> IRAS 23238+7401 <----- 1) Subtract dark imarith IRAS23238.064.fits - dark60.fits IRAS23238.064d.fits imarith IRAS23238.065.fits - dark60.fits IRAS23238.065d.fits imarith IRAS23238.066.fits - dark60.fits IRAS23238.066d.fits imarith IRAS23238.067.fits - dark60.fits IRAS23238.067d.fits imarith IRAS23238.068.fits - dark60.fits IRAS23238.068d.fits imarith IRAS23238.069.fits - dark60.fits IRAS23238.069d.fits imarith IRAS23238.070.fits - dark60.fits IRAS23238.070d.fits imarith IRAS23238.071.fits - dark60.fits IRAS23238.071d.fits imarith IRAS23238.072.fits - dark60.fits IRAS23238.072d.fits 2) Scale images to same (mean = 13498.8 sky) value imstat IRAS23238.*d.fits >> awklist.txt imarith IRAS23238.064d.fits * 1.01449 IRAS23238.064a.fits imarith IRAS23238.065d.fits * 0.99446 IRAS23238.065a.fits imarith IRAS23238.066d.fits * 1.00258 IRAS23238.066a.fits imarith IRAS23238.067d.fits * 1.00073 IRAS23238.067a.fits imarith IRAS23238.068d.fits * 1.00527 IRAS23238.068a.fits imarith IRAS23238.069d.fits * 1.00692 IRAS23238.069a.fits imarith IRAS23238.070d.fits * 0.998063 IRAS23238.070a.fits imarith IRAS23238.071d.fits * 0.996442 IRAS23238.071a.fits imarith IRAS23238.072d.fits * 0.981731 IRAS23238.072a.fits imstat IRAS23238*a.fits 3) Make skyflat (avg combine, min=0 max=2 reject) epar imcomb imcomb IRAS23238.*a.fits IRAS23238.sky.fits 4) Normalize by midpt imstat IRAS23238.sky.fits imarith IRAS23238.sky.fits / 13498. IRAS23238.skyN.fits 5) Divide by skyflat imarith IRAS23238.064d.fits / IRAS23238.skyN.fits IRAS23238.064df.fits imarith IRAS23238.065d.fits / IRAS23238.skyN.fits IRAS23238.065df.fits imarith IRAS23238.066d.fits / IRAS23238.skyN.fits IRAS23238.066df.fits imarith IRAS23238.067d.fits / IRAS23238.skyN.fits IRAS23238.067df.fits imarith IRAS23238.068d.fits / IRAS23238.skyN.fits IRAS23238.068df.fits imarith IRAS23238.069d.fits / IRAS23238.skyN.fits IRAS23238.069df.fits imarith IRAS23238.070d.fits / IRAS23238.skyN.fits IRAS23238.070df.fits imarith IRAS23238.071d.fits / IRAS23238.skyN.fits IRAS23238.071df.fits imarith IRAS23238.072d.fits / IRAS23238.skyN.fits IRAS23238.072df.fits 6) Subtract by constant (midpt) imstat IRAS23238.*df.fits imarith IRAS23238.064df.fits - 13333. IRAS23238.064dfs.fits imarith IRAS23238.065df.fits - 13594. IRAS23238.065dfs.fits imarith IRAS23238.066df.fits - 13492. IRAS23238.066dfs.fits imarith IRAS23238.067df.fits - 13513. IRAS23238.067dfs.fits imarith IRAS23238.068df.fits - 13454. IRAS23238.068dfs.fits imarith IRAS23238.069df.fits - 13424. IRAS23238.069dfs.fits imarith IRAS23238.070df.fits - 13545. IRAS23238.070dfs.fits imarith IRAS23238.071df.fits - 13569. IRAS23238.071dfs.fits imarith IRAS23238.072df.fits - 13774. IRAS23238.072dfs.fits 7) get coords and shifts shifts: 548.48 536.04 651.18 433.48 545.68 433.69 439.51 432.01 649.51 534.01 438.19 535.11 648.26 639.26 542.20 640.74 434.84 641.70 0. 0. -102.7 102.56 2.8 102.35 108.97 104.03 -101.03 2.03 110.29 0.93 -99.78 -103.22 6.28 -104.7 113.64 -105.66 coords: 478.45 699.04 571.48 668.10 288.07 231.45 458.37 339.69 616.36 398.28 837.22 435.41 210.84 807.10 244.32 817.14 ----> IRAS 02232+6138 <----- 1) Subtract dark imarith IRAS02232.081.fits - dark60.fits IRAS02232.081d.fits imarith IRAS02232.082.fits - dark60.fits IRAS02232.082d.fits imarith IRAS02232.083.fits - dark60.fits IRAS02232.083d.fits imarith IRAS02232.084.fits - dark60.fits IRAS02232.084d.fits imarith IRAS02232.085.fits - dark60.fits IRAS02232.085d.fits imarith IRAS02232.086.fits - dark60.fits IRAS02232.086d.fits imarith IRAS02232.087.fits - dark60.fits IRAS02232.087d.fits imarith IRAS02232.088.fits - dark60.fits IRAS02232.088d.fits imarith IRAS02232.089.fits - dark60.fits IRAS02232.089d.fits 2) Scale images to same (mean = 13027.8 sky) value imstat IRAS02232.*d.fits >> awklist.txt imarith IRAS02232.081d.fits * 1.02581 IRAS02232.081a.fits imarith IRAS02232.082d.fits * 1.01558 IRAS02232.082a.fits imarith IRAS02232.083d.fits * 0.995552 IRAS02232.083a.fits imarith IRAS02232.084d.fits * 1.00068 IRAS02232.084a.fits imarith IRAS02232.085d.fits * 1.00021 IRAS02232.085a.fits imarith IRAS02232.086d.fits * 0.997764 IRAS02232.086a.fits imarith IRAS02232.087d.fits * 0.980418 IRAS02232.087a.fits imarith IRAS02232.088d.fits * 0.991914 IRAS02232.088a.fits imarith IRAS02232.089d.fits * 0.993503 IRAS02232.089a.fits imstat IRAS02232*a.fits 3) Make skyflat (avg combine, min=0 max=2 reject) epar imcomb imcomb IRAS02232.*a.fits IRAS02232.sky.fits 4) Normalize by midpt imstat IRAS02232.sky.fits imarith IRAS02232.sky.fits / 13008. IRAS02232.skyN.fits 5) Divide by skyflat imarith IRAS02232.081d.fits / IRAS02232.skyN.fits IRAS02232.081df.fits imarith IRAS02232.082d.fits / IRAS02232.skyN.fits IRAS02232.082df.fits imarith IRAS02232.083d.fits / IRAS02232.skyN.fits IRAS02232.083df.fits imarith IRAS02232.084d.fits / IRAS02232.skyN.fits IRAS02232.084df.fits imarith IRAS02232.085d.fits / IRAS02232.skyN.fits IRAS02232.085df.fits imarith IRAS02232.086d.fits / IRAS02232.skyN.fits IRAS02232.086df.fits imarith IRAS02232.087d.fits / IRAS02232.skyN.fits IRAS02232.087df.fits imarith IRAS02232.088d.fits / IRAS02232.skyN.fits IRAS02232.088df.fits imarith IRAS02232.089d.fits / IRAS02232.skyN.fits IRAS02232.089df.fits 6) Subtract by constant (midpt) imstat IRAS02232.*df.fits imarith IRAS02232.081df.fits - 12703. IRAS02232.081dfs.fits imarith IRAS02232.082df.fits - 12826. IRAS02232.082dfs.fits imarith IRAS02232.083df.fits - 13086. IRAS02232.083dfs.fits imarith IRAS02232.084df.fits - 13022. IRAS02232.084dfs.fits imarith IRAS02232.085df.fits - 13028. IRAS02232.085dfs.fits imarith IRAS02232.086df.fits - 13061. IRAS02232.086dfs.fits imarith IRAS02232.087df.fits - 13293. IRAS02232.087dfs.fits imarith IRAS02232.088df.fits - 13141. IRAS02232.088dfs.fits imarith IRAS02232.089df.fits - 13118. IRAS02232.089dfs.fits 7) get coords and shifts shifts: 551.78 447.09 657.36 350.82 553.32 348.77 448.04 348.90 658.86 448.74 449.63 449.59 661.23 552.58 556.01 552.85 450.96 553.66 0. 0. -105.58 96.27 -1.54 98.32 103.74 98.19 -107.08 -1.65 102.15 -2.5 -109.45 -105.49 -4.23 -105.76 100.82 -106.57 coords: 347.66 295.83 363.70 746.14 678.70 742.90 673.28 680.96 698.12 266.32 602.35 148.68 -----> IRAS 02086+7600 <----- 1) Subtract dark imarith IRAS02086.091.fits - dark60.fits IRAS02086.091d.fits imarith IRAS02086.092.fits - dark60.fits IRAS02086.092d.fits imarith IRAS02086.093.fits - dark60.fits IRAS02086.093d.fits imarith IRAS02086.094.fits - dark60.fits IRAS02086.094d.fits imarith IRAS02086.095.fits - dark60.fits IRAS02086.095d.fits imarith IRAS02086.096.fits - dark60.fits IRAS02086.096d.fits imarith IRAS02086.097.fits - dark60.fits IRAS02086.097d.fits imarith IRAS02086.098.fits - dark60.fits IRAS02086.098d.fits imarith IRAS02086.099.fits - dark60.fits IRAS02086.099d.fits 2) Scale images to same (mean = 13623 sky) value imstat IRAS02086.*d.fits >> awklist.txt imarith IRAS02086.091d.fits * 0.995251 IRAS02086.091a.fits imarith IRAS02086.092d.fits * 1.00391 IRAS02086.092a.fits imarith IRAS02086.093d.fits * 1.00851 IRAS02086.093a.fits imarith IRAS02086.094d.fits * 0.99026 IRAS02086.094a.fits imarith IRAS02086.095d.fits * 1.00235 IRAS02086.095a.fits imarith IRAS02086.096d.fits * 1.00302 IRAS02086.096a.fits imarith IRAS02086.097d.fits * 1.00911 IRAS02086.097a.fits imarith IRAS02086.098d.fits * 1.00739 IRAS02086.098a.fits imarith IRAS02086.099d.fits * 0.980919 IRAS02086.099a.fits imstat IRAS02086*a.fits 3) Make skyflat (avg combine, min=0 max=2 reject) epar imcomb imcomb IRAS02086.*a.fits IRAS02086.sky.fits 4) Normalize by midpt imstat IRAS02086.sky.fits imarith IRAS02086.sky.fits / 13634. IRAS02086.skyN.fits 5) Divide by skyflat imarith IRAS02086.091d.fits / IRAS02086.skyN.fits IRAS02086.091df.fits imarith IRAS02086.092d.fits / IRAS02086.skyN.fits IRAS02086.092df.fits imarith IRAS02086.093d.fits / IRAS02086.skyN.fits IRAS02086.093df.fits imarith IRAS02086.094d.fits / IRAS02086.skyN.fits IRAS02086.094df.fits imarith IRAS02086.095d.fits / IRAS02086.skyN.fits IRAS02086.095df.fits imarith IRAS02086.096d.fits / IRAS02086.skyN.fits IRAS02086.096df.fits imarith IRAS02086.097d.fits / IRAS02086.skyN.fits IRAS02086.097df.fits imarith IRAS02086.098d.fits / IRAS02086.skyN.fits IRAS02086.098df.fits imarith IRAS02086.099d.fits / IRAS02086.skyN.fits IRAS02086.099df.fits 6) Subtract by constant (midpt) imstat IRAS02086.*df.fits imarith IRAS02086.091df.fits - 13723. IRAS02086.091dfs.fits imarith IRAS02086.092df.fits - 13608. IRAS02086.092dfs.fits imarith IRAS02086.093df.fits - 13548. IRAS02086.093dfs.fits imarith IRAS02086.094df.fits - 13790. IRAS02086.094dfs.fits imarith IRAS02086.095df.fits - 13628. IRAS02086.095dfs.fits imarith IRAS02086.096df.fits - 13618. IRAS02086.096dfs.fits imarith IRAS02086.097df.fits - 13530. IRAS02086.097dfs.fits imarith IRAS02086.098df.fits - 13556. IRAS02086.098dfs.fits imarith IRAS02086.099df.fits - 13921. IRAS02086.099dfs.fits 7) get coords and shifts shifts: 511.93 513.15 617.27 409.32 512.41 407.24 408.11 407.38 618.39 506.64 409.46 507.05 619.92 610.19 515.69 610.91 409.97 612.08 0. 0. -105.34 103.83 -0.48 105.91 103.82 105.77 -106.46 6.51 102.47 6.1 -107.99 -97.04 -3.76 -97.76 101.96 -98.93 coords: 146.96 687.88 456.06 814.50 689.78 743.07 555.99 155.95 142.95 262.90 781.33 166.75 828.09 145.95 ----> IRAS F04113+2758 <----- 1) Subtract dark imarith IRASF04113.135.fits - dark10.fits IRASF04113.135d.fits imarith IRASF04113.136.fits - dark10.fits IRASF04113.136d.fits imarith IRASF04113.137.fits - dark10.fits IRASF04113.137d.fits imarith IRASF04113.138.fits - dark10.fits IRASF04113.138d.fits imarith IRASF04113.139.fits - dark10.fits IRASF04113.139d.fits imarith IRASF04113.140.fits - dark10.fits IRASF04113.140d.fits imarith IRASF04113.141.fits - dark10.fits IRASF04113.141d.fits imarith IRASF04113.142.fits - dark10.fits IRASF04113.142d.fits imarith IRASF04113.143.fits - dark10.fits IRASF04113.143d.fits 2) Scale images to same (mean = 5524.89 sky) value imstat IRASF04113.*d.fits >> awklist.txt imarith IRASF04113.135d.fits * 1.01077 IRASF04113.135a.fits imarith IRASF04113.136d.fits * 1.02218 IRASF04113.136a.fits imarith IRASF04113.137d.fits * 1.02029 IRASF04113.137a.fits imarith IRASF04113.138d.fits * 1.00985 IRASF04113.138a.fits imarith IRASF04113.139d.fits * 1.01003 IRASF04113.139a.fits imarith IRASF04113.140d.fits * 0.984127 IRASF04113.140a.fits imarith IRASF04113.141d.fits * 1.00288 IRASF04113.141a.fits imarith IRASF04113.142d.fits * 0.97372 IRASF04113.142a.fits imarith IRASF04113.143d.fits * 0.969279 IRASF04113.143a.fits imstat IRASF04113*a.fits 3) Make skyflat (avg combine, min=0 max=2 reject) epar imcomb imcomb IRASF04113.*a.fits IRASF04113.sky.fits 4) Normalize by midpt imstat IRASF04113.sky.fits imarith IRASF04113.sky.fits / 5513. IRASF04113.skyN.fits 5) Divide by skyflat imarith IRASF04113.135d.fits / IRASF04113.skyN.fits IRASF04113.135df.fits imarith IRASF04113.136d.fits / IRASF04113.skyN.fits IRASF04113.136df.fits imarith IRASF04113.137d.fits / IRASF04113.skyN.fits IRASF04113.137df.fits imarith IRASF04113.138d.fits / IRASF04113.skyN.fits IRASF04113.138df.fits imarith IRASF04113.139d.fits / IRASF04113.skyN.fits IRASF04113.139df.fits imarith IRASF04113.140d.fits / IRASF04113.skyN.fits IRASF04113.140df.fits imarith IRASF04113.141d.fits / IRASF04113.skyN.fits IRASF04113.141df.fits imarith IRASF04113.142d.fits / IRASF04113.skyN.fits IRASF04113.142df.fits imarith IRASF04113.143d.fits / IRASF04113.skyN.fits IRASF04113.143df.fits 6) Subtract by constant (midpt) imstat IRASF04113.*df.fits imarith IRASF04113.135df.fits - 5472. IRASF04113.135dfs.fits imarith IRASF04113.136df.fits - 5411. IRASF04113.136dfs.fits imarith IRASF04113.137df.fits - 5422. IRASF04113.137dfs.fits imarith IRASF04113.138df.fits - 5474. IRASF04113.138dfs.fits imarith IRASF04113.139df.fits - 5477. IRASF04113.139dfs.fits imarith IRASF04113.140df.fits - 5617. IRASF04113.140dfs.fits imarith IRASF04113.141df.fits - 5516. IRASF04113.141dfs.fits imarith IRASF04113.142df.fits - 5680. IRASF04113.142dfs.fits imarith IRASF04113.143df.fits - 5703. IRASF04113.143dfs.fits 7) get coords and shifts shifts: 640.80 601.98 747.52 501.25 639.56 500.06 535.32 499.71 745.40 599.22 535.03 600.25 743.15 704.13 639.59 703.72 534.56 704.78 0. 0. -106.72 100.73 1.24 101.92 105.48 102.27 -104.6 2.76 105.77 1.73 -102.35 -102.15 1.21 -101.74 106.24 -102.8 coords: 206.91 933.19 640.80 601.98 -----> IRAS F04239+2559 <------ 1) Subtract dark imarith IRASF04239.146.fits - dark10.fits IRASF04239.146d.fits imarith IRASF04239.147.fits - dark10.fits IRASF04239.147d.fits imarith IRASF04239.148.fits - dark10.fits IRASF04239.148d.fits imarith IRASF04239.149.fits - dark10.fits IRASF04239.149d.fits imarith IRASF04239.150.fits - dark10.fits IRASF04239.150d.fits imarith IRASF04239.151.fits - dark10.fits IRASF04239.151d.fits imarith IRASF04239.152.fits - dark10.fits IRASF04239.152d.fits imarith IRASF04239.153.fits - dark10.fits IRASF04239.153d.fits imarith IRASF04239.154.fits - dark10.fits IRASF04239.154d.fits 2) Scale images to same (mean = 12694.3 sky) value imstat IRASF04239.*d.fits >> awklist.txt imarith IRASF04239.146d.fits * 1.00223 IRASF04239.146a.fits imarith IRASF04239.147d.fits * 1.0111 IRASF04239.147a.fits imarith IRASF04239.148d.fits * 1.01676 IRASF04239.148a.fits imarith IRASF04239.149d.fits * 1.02241 IRASF04239.149a.fits imarith IRASF04239.150d.fits * 1.01538 IRASF04239.150a.fits imarith IRASF04239.151d.fits * 1.00129 IRASF04239.151a.fits imarith IRASF04239.152d.fits * 0.999709 IRASF04239.152a.fits imarith IRASF04239.153d.fits * 0.957988 IRASF04239.153a.fits imarith IRASF04239.154d.fits * 0.976635 IRASF04239.154a.fits imstat IRASF04239*a.fits 3) Make skyflat (avg combine, min=0 max=2 reject) epar imcomb imcomb IRASF04239.*a.fits IRASF04239.sky.fits 4) Normalize by midpt imstat IRASF04239.sky.fits imarith IRASF04239.sky.fits / 12691. IRASF04239.skyN.fits 5) Divide by skyflat imarith IRASF04239.146d.fits / IRASF04239.skyN.fits IRASF04239.146df.fits imarith IRASF04239.147d.fits / IRASF04239.skyN.fits IRASF04239.147df.fits imarith IRASF04239.148d.fits / IRASF04239.skyN.fits IRASF04239.148df.fits imarith IRASF04239.149d.fits / IRASF04239.skyN.fits IRASF04239.149df.fits imarith IRASF04239.150d.fits / IRASF04239.skyN.fits IRASF04239.150df.fits imarith IRASF04239.151d.fits / IRASF04239.skyN.fits IRASF04239.151df.fits imarith IRASF04239.152d.fits / IRASF04239.skyN.fits IRASF04239.152df.fits imarith IRASF04239.153d.fits / IRASF04239.skyN.fits IRASF04239.153df.fits imarith IRASF04239.154d.fits / IRASF04239.skyN.fits IRASF04239.154df.fits 6) Subtract by constant (midpt) imstat IRASF04239.*df.fits imarith IRASF04239.146df.fits - 12681. IRASF04239.146dfs.fits imarith IRASF04239.147df.fits - 12568. IRASF04239.147dfs.fits imarith IRASF04239.148df.fits - 12499. IRASF04239.148dfs.fits imarith IRASF04239.149df.fits - 12430. IRASF04239.149dfs.fits imarith IRASF04239.150df.fits - 12521. IRASF04239.150dfs.fits imarith IRASF04239.151df.fits - 12695. IRASF04239.151dfs.fits imarith IRASF04239.152df.fits - 12717. IRASF04239.152dfs.fits imarith IRASF04239.153df.fits - 13278. IRASF04239.153dfs.fits imarith IRASF04239.154df.fits - 13019. IRASF04239.154dfs.fits 7) get coords and shifts shifts: 470.07 515.99 575.10 416.77 468.94 415.29 365.15 415.21 575.20 517.94 364.20 518.91 575.34 623.57 470.66 624.45 364.13 625.20 0. 0. -105.03 99.22 1.13 100.7 104.92 100.78 -105.13 -1.95 105.87 -2.92 -105.27 -107.58 -0.59 -108.46 105.94 -109.21 coords: 215.19 525.26 470.16 515.99 862.73 385.72 549.34 325.87 ------> IRAS 04302+2247 <------ 1) Subtract dark imarith IRAS04302.156.fits - dark60.fits IRAS04302.156d.fits imarith IRAS04302.157.fits - dark60.fits IRAS04302.157d.fits imarith IRAS04302.158.fits - dark60.fits IRAS04302.158d.fits imarith IRAS04302.159.fits - dark60.fits IRAS04302.159d.fits imarith IRAS04302.160.fits - dark60.fits IRAS04302.160d.fits imarith IRAS04302.161.fits - dark60.fits IRAS04302.161d.fits imarith IRAS04302.162.fits - dark60.fits IRAS04302.162d.fits imarith IRAS04302.163.fits - dark60.fits IRAS04302.163d.fits imarith IRAS04302.164.fits - dark60.fits IRAS04302.164d.fits 2) Scale images to same (mean = 12513.6 sky) value imstat IRAS04302.*d.fits >> awklist.txt imarith IRAS04302.156d.fits * 1.01571 IRAS04302.156a.fits imarith IRAS04302.157d.fits * 0.979998 IRAS04302.157a.fits imarith IRAS04302.158d.fits * 0.961549 IRAS04302.158a.fits imarith IRAS04302.159d.fits * 1.01448 IRAS04302.159a.fits imarith IRAS04302.160d.fits * 1.01811 IRAS04302.160a.fits imarith IRAS04302.161d.fits * 1.00527 IRAS04302.161a.fits imarith IRAS04302.162d.fits * 1.00221 IRAS04302.162a.fits imarith IRAS04302.163d.fits * 0.994564 IRAS04302.163a.fits imarith IRAS04302.164d.fits * 1.01104 IRAS04302.164a.fits imstat IRAS04302*a.fits 3) Make skyflat (avg combine, min=0 max=2 reject) epar imcomb imcomb IRAS04302.*a.fits IRAS04302.sky.fits 4) Normalize by midpt imstat IRAS04302.sky.fits imarith IRAS04302.sky.fits / 12518. IRAS04302.skyN.fits 5) Divide by skyflat imarith IRAS04302.156d.fits / IRAS04302.skyN.fits IRAS04302.156df.fits imarith IRAS04302.157d.fits / IRAS04302.skyN.fits IRAS04302.157df.fits imarith IRAS04302.158d.fits / IRAS04302.skyN.fits IRAS04302.158df.fits imarith IRAS04302.159d.fits / IRAS04302.skyN.fits IRAS04302.159df.fits imarith IRAS04302.160d.fits / IRAS04302.skyN.fits IRAS04302.160df.fits imarith IRAS04302.161d.fits / IRAS04302.skyN.fits IRAS04302.161df.fits imarith IRAS04302.162d.fits / IRAS04302.skyN.fits IRAS04302.162df.fits imarith IRAS04302.163d.fits / IRAS04302.skyN.fits IRAS04302.163df.fits imarith IRAS04302.164d.fits / IRAS04302.skyN.fits IRAS04302.164df.fits 6) Subtract by constant (midpt) imstat IRAS04302.*df.fits imarith IRAS04302.156df.fits - 12348. IRAS04302.156dfs.fits imarith IRAS04302.157df.fits - 12802. IRAS04302.157dfs.fits imarith IRAS04302.158df.fits - 13047. IRAS04302.158dfs.fits imarith IRAS04302.159df.fits - 12364. IRAS04302.159dfs.fits imarith IRAS04302.160df.fits - 12320. IRAS04302.160dfs.fits imarith IRAS04302.161df.fits - 12475. IRAS04302.161dfs.fits imarith IRAS04302.162df.fits - 12512. IRAS04302.162dfs.fits imarith IRAS04302.163df.fits - 12611. IRAS04302.163dfs.fits imarith IRAS04302.164df.fits - 12408. IRAS04302.164dfs.fits 7) get coords and shifts shifts: 227.34 572.15 333.06 470.55 228.82 469.35 123.10 468.78 336.27 570.89 126.64 571.97 340.23 676.84 237.49 677.43 135.00 678.11 0. 0. -105.72 101.6 -1.48 102.8 104.24 103.37 -108.93 1.26 100.7 0.18 -112.89 -104.69 -10.15 -105.28 92.34 -105.96 coords: 223.07 850.22 227.34 572.15 880.62 212.32 -----> IRAS 04368+2557 <----- 1) Subtract dark imarith IRAS04368.166.fits - dark60.fits IRAS04368.166d.fits imarith IRAS04368.167.fits - dark60.fits IRAS04368.167d.fits imarith IRAS04368.168.fits - dark60.fits IRAS04368.168d.fits imarith IRAS04368.169.fits - dark60.fits IRAS04368.169d.fits imarith IRAS04368.170.fits - dark60.fits IRAS04368.170d.fits imarith IRAS04368.171.fits - dark60.fits IRAS04368.171d.fits imarith IRAS04368.172.fits - dark60.fits IRAS04368.172d.fits imarith IRAS04368.173.fits - dark60.fits IRAS04368.173d.fits imarith IRAS04368.174.fits - dark60.fits IRAS04368.174d.fits 2) Scale images to same (mean = 12501.7 sky) value imstat IRAS04368.*d.fits >> awklist.txt imarith IRAS04368.166d.fits * 1.01425 IRAS04368.166a.fits imarith IRAS04368.167d.fits * 0.997901 IRAS04368.167a.fits imarith IRAS04368.168d.fits * 1.0023 IRAS04368.168a.fits imarith IRAS04368.169d.fits * 1.00198 IRAS04368.169a.fits imarith IRAS04368.170d.fits * 1.00674 IRAS04368.170a.fits imarith IRAS04368.171d.fits * 0.997741 IRAS04368.171a.fits imarith IRAS04368.172d.fits * 1.00222 IRAS04368.172a.fits imarith IRAS04368.173d.fits * 0.987886 IRAS04368.173a.fits imarith IRAS04368.174d.fits * 0.989528 IRAS04368.174a.fits imstat IRAS04368*a.fits 3) Make skyflat (avg combine, min=0 max=2 reject) epar imcomb imcomb IRAS04368.*a.fits IRAS04368.sky.fits 4) Normalize by midpt imstat IRAS04368.sky.fits imarith IRAS04368.sky.fits / 12518. IRAS04368.skyN.fits 5) Divide by skyflat imarith IRAS04368.166d.fits / IRAS04368.skyN.fits IRAS04368.166df.fits imarith IRAS04368.167d.fits / IRAS04368.skyN.fits IRAS04368.167df.fits imarith IRAS04368.168d.fits / IRAS04368.skyN.fits IRAS04368.168df.fits imarith IRAS04368.169d.fits / IRAS04368.skyN.fits IRAS04368.169df.fits imarith IRAS04368.170d.fits / IRAS04368.skyN.fits IRAS04368.170df.fits imarith IRAS04368.171d.fits / IRAS04368.skyN.fits IRAS04368.171df.fits imarith IRAS04368.172d.fits / IRAS04368.skyN.fits IRAS04368.172df.fits imarith IRAS04368.173d.fits / IRAS04368.skyN.fits IRAS04368.173df.fits imarith IRAS04368.174d.fits / IRAS04368.skyN.fits IRAS04368.174df.fits 6) Subtract by constant (midpt) imstat IRAS04368.*df.fits imarith IRAS04368.166df.fits - 12365. IRAS04368.166dfs.fits imarith IRAS04368.167df.fits - 12569. IRAS04368.167dfs.fits imarith IRAS04368.168df.fits - 12513. IRAS04368.168dfs.fits imarith IRAS04368.169df.fits - 12520. IRAS04368.169dfs.fits imarith IRAS04368.170df.fits - 12462. IRAS04368.170dfs.fits imarith IRAS04368.171df.fits - 12568. IRAS04368.171dfs.fits imarith IRAS04368.172df.fits - 12519. IRAS04368.172dfs.fits imarith IRAS04368.173df.fits - 12699. IRAS04368.173dfs.fits imarith IRAS04368.174df.fits - 12674. IRAS04368.174dfs.fits 7) get coords and shifts shifts: 740.73 125.40 849.93 20.25 745.64 19.28 642.91 18.38 856.42 119.92 644.07 121.51 855.98 224.20 752.54 224.76 647.27 226.68 0. 0. -109.2 105.15 -4.91 106.12 97.82 107.02 -115.69 5.48 96.66 3.89 -115.25 -98.8 -11.81 -99.36 93.46 -101.28 coords: 369.91 815.12 309.59 199.10 796.92 452.76 740.73 125.40 -----> IRAS 05319-0542 <------ 1) Subtract dark imarith IRAS05319.0542.186.fits - dark60.fits IRAS05319.0542.186d.fits imarith IRAS05319.0542.187.fits - dark60.fits IRAS05319.0542.187d.fits imarith IRAS05319.0542.188.fits - dark60.fits IRAS05319.0542.188d.fits imarith IRAS05319.0542.189.fits - dark60.fits IRAS05319.0542.189d.fits imarith IRAS05319.0542.190.fits - dark60.fits IRAS05319.0542.190d.fits imarith IRAS05319.0542.191.fits - dark60.fits IRAS05319.0542.191d.fits imarith IRAS05319.0542.192.fits - dark60.fits IRAS05319.0542.192d.fits imarith IRAS05319.0542.193.fits - dark60.fits IRAS05319.0542.193d.fits imarith IRAS05319.0542.194.fits - dark60.fits IRAS05319.0542.194d.fits 2) Scale images to same (mean = 13701.8 sky) value imstat IRAS05319.0542.*d.fits >> awklist.txt imarith IRAS05319.0542.186d.fits * 0.99606 IRAS05319.0542.186a.fits imarith IRAS05319.0542.187d.fits * 0.996712 IRAS05319.0542.187a.fits imarith IRAS05319.0542.188d.fits * 0.984891 IRAS05319.0542.188a.fits imarith IRAS05319.0542.189d.fits * 1.00306 IRAS05319.0542.189a.fits imarith IRAS05319.0542.190d.fits * 1.00838 IRAS05319.0542.190a.fits imarith IRAS05319.0542.191d.fits * 1.00299 IRAS05319.0542.191a.fits imarith IRAS05319.0542.192d.fits * 1.00446 IRAS05319.0542.192a.fits imarith IRAS05319.0542.193d.fits * 1.00335 IRAS05319.0542.193a.fits imarith IRAS05319.0542.194d.fits * 1.0005 IRAS05319.0542.194a.fits imstat IRAS05319.0542*a.fits 3) Make skyflat (avg combine, min=0 max=2 reject) epar imcomb imcomb IRAS05319.0542.*a.fits IRAS05319.0542.sky.fits 4) Normalize by midpt imstat IRAS05319.0542.sky.fits imarith IRAS05319.0542.sky.fits / 13714. IRAS05319.0542.skyN.fits 5) Divide by skyflat imarith IRAS05319.0542.186d.fits / IRAS05319.0542.skyN.fits IRAS05319.0542.186df.fits imarith IRAS05319.0542.187d.fits / IRAS05319.0542.skyN.fits IRAS05319.0542.187df.fits imarith IRAS05319.0542.188d.fits / IRAS05319.0542.skyN.fits IRAS05319.0542.188df.fits imarith IRAS05319.0542.189d.fits / IRAS05319.0542.skyN.fits IRAS05319.0542.189df.fits imarith IRAS05319.0542.190d.fits / IRAS05319.0542.skyN.fits IRAS05319.0542.190df.fits imarith IRAS05319.0542.191d.fits / IRAS05319.0542.skyN.fits IRAS05319.0542.191df.fits imarith IRAS05319.0542.192d.fits / IRAS05319.0542.skyN.fits IRAS05319.0542.192df.fits imarith IRAS05319.0542.193d.fits / IRAS05319.0542.skyN.fits IRAS05319.0542.193df.fits imarith IRAS05319.0542.194d.fits / IRAS05319.0542.skyN.fits IRAS05319.0542.194df.fits 6) Subtract by constant (midpt) imstat IRAS05319.0542.*df.fits imarith IRAS05319.0542.186df.fits - 13787. IRAS05319.0542.186dfs.fits imarith IRAS05319.0542.187df.fits - 13782. IRAS05319.0542.187dfs.fits imarith IRAS05319.0542.188df.fits - 13948. IRAS05319.0542.188dfs.fits imarith IRAS05319.0542.189df.fits - 13694. IRAS05319.0542.189dfs.fits imarith IRAS05319.0542.190df.fits - 13623. IRAS05319.0542.190dfs.fits imarith IRAS05319.0542.191df.fits - 13697. IRAS05319.0542.191dfs.fits imarith IRAS05319.0542.192df.fits - 13678. IRAS05319.0542.192dfs.fits imarith IRAS05319.0542.193df.fits - 13688. IRAS05319.0542.193dfs.fits imarith IRAS05319.0542.194df.fits - 13729. IRAS05319.0542.194dfs.fits 7) get coords and shifts shifts: 235.00 332.79 339.22 234.16 234.54 232.57 128.37 233.46 339.66 335.55 129.13 335.89 341.13 441.31 234.42 442.14 129.38 441.85 0. 0. -104.22 98.63 0.46 100.22 106.63 99.33 -104.66 -2.76 105.87 -3.1 -106.13 -108.52 0.58 -109.35 105.62 -109.06 coords: 235.00 332.79 783.21 554.79 850.12 649.73 295.64 399.24 -----> IRAS 05319-0551 <------ 1) Subtract dark imarith IRAS05319.0551.199.fits - dark60.fits IRAS05319.0551.199d.fits imarith IRAS05319.0551.200.fits - dark60.fits IRAS05319.0551.200d.fits imarith IRAS05319.0551.201.fits - dark60.fits IRAS05319.0551.201d.fits imarith IRAS05319.0551.202.fits - dark60.fits IRAS05319.0551.202d.fits imarith IRAS05319.0551.203.fits - dark60.fits IRAS05319.0551.203d.fits imarith IRAS05319.0551.204.fits - dark60.fits IRAS05319.0551.204d.fits imarith IRAS05319.0551.205.fits - dark60.fits IRAS05319.0551.205d.fits imarith IRAS05319.0551.206.fits - dark60.fits IRAS05319.0551.206d.fits imarith IRAS05319.0551.207.fits - dark60.fits IRAS05319.0551.207d.fits 2) Scale images to same (mean = 13552.1 sky) value imstat IRAS05319.0551.*d.fits >> awklist.txt imarith IRAS05319.0551.199d.fits * 1.00969 IRAS05319.0551.199a.fits imarith IRAS05319.0551.200d.fits * 1.0023 IRAS05319.0551.200a.fits imarith IRAS05319.0551.201d.fits * 1.00008 IRAS05319.0551.201a.fits imarith IRAS05319.0551.202d.fits * 1.00364 IRAS05319.0551.202a.fits imarith IRAS05319.0551.203d.fits * 0.996185 IRAS05319.0551.203a.fits imarith IRAS05319.0551.204d.fits * 1.00141 IRAS05319.0551.204a.fits imarith IRAS05319.0551.205d.fits * 1.00038 IRAS05319.0551.205a.fits imarith IRAS05319.0551.206d.fits * 0.99392 IRAS05319.0551.206a.fits imarith IRAS05319.0551.207d.fits * 0.99261 IRAS05319.0551.207a.fits imstat IRAS05319.0551*a.fits 3) Make skyflat (avg combine, min=0 max=2 reject) epar imcomb imcomb IRAS05319.0551.*a.fits IRAS05319.0551.sky.fits 4) Normalize by midpt imstat IRAS05319.0551.sky.fits imarith IRAS05319.0551.sky.fits / 13545. IRAS05319.0551.skyN.fits 5) Divide by skyflat imarith IRAS05319.0551.199d.fits / IRAS05319.0551.skyN.fits IRAS05319.0551.199df.fits imarith IRAS05319.0551.200d.fits / IRAS05319.0551.skyN.fits IRAS05319.0551.200df.fits imarith IRAS05319.0551.201d.fits / IRAS05319.0551.skyN.fits IRAS05319.0551.201df.fits imarith IRAS05319.0551.202d.fits / IRAS05319.0551.skyN.fits IRAS05319.0551.202df.fits imarith IRAS05319.0551.203d.fits / IRAS05319.0551.skyN.fits IRAS05319.0551.203df.fits imarith IRAS05319.0551.204d.fits / IRAS05319.0551.skyN.fits IRAS05319.0551.204df.fits imarith IRAS05319.0551.205d.fits / IRAS05319.0551.skyN.fits IRAS05319.0551.205df.fits imarith IRAS05319.0551.206d.fits / IRAS05319.0551.skyN.fits IRAS05319.0551.206df.fits imarith IRAS05319.0551.207d.fits / IRAS05319.0551.skyN.fits IRAS05319.0551.207df.fits 6) Subtract by constant (midpt) imstat IRAS05319.0551.*df.fits imarith IRAS05319.0551.199df.fits - 13441. IRAS05319.0551.199dfs.fits imarith IRAS05319.0551.200df.fits - 13539. IRAS05319.0551.200dfs.fits imarith IRAS05319.0551.201df.fits - 13568. IRAS05319.0551.201dfs.fits imarith IRAS05319.0551.202df.fits - 13518. IRAS05319.0551.202dfs.fits imarith IRAS05319.0551.203df.fits - 13625. IRAS05319.0551.203dfs.fits imarith IRAS05319.0551.204df.fits - 13550. IRAS05319.0551.204dfs.fits imarith IRAS05319.0551.205df.fits - 13562. IRAS05319.0551.205dfs.fits imarith IRAS05319.0551.206df.fits - 13656. IRAS05319.0551.206dfs.fits imarith IRAS05319.0551.207df.fits - 13672. IRAS05319.0551.207dfs.fits 7) get coords and shifts shifts: 797.77 510.02 900.72 410.21 795.16 408.98 690.58 408.99 901.00 511.50 690.02 512.11 903.13 616.90 799.32 617.86 696.55 618.57 0. 0. -102.95 99.81 2.61 101.04 107.19 101.03 -103.23 -1.48 107.75 -2.09 -105.36 -106.88 -1.55 -107.84 101.22 -108.55 coords: 726.70 813.52 855.71 849.88 797.77 510.02 836.55 403.98 ------> IRAS 05338-0529 <------ 1) Subtract dark imarith IRAS05338.210.fits - dark60.fits IRAS05338.210d.fits imarith IRAS05338.211.fits - dark60.fits IRAS05338.211d.fits imarith IRAS05338.212.fits - dark60.fits IRAS05338.212d.fits imarith IRAS05338.213.fits - dark60.fits IRAS05338.213d.fits imarith IRAS05338.214.fits - dark60.fits IRAS05338.214d.fits imarith IRAS05338.215.fits - dark60.fits IRAS05338.215d.fits imarith IRAS05338.216.fits - dark60.fits IRAS05338.216d.fits imarith IRAS05338.217.fits - dark60.fits IRAS05338.217d.fits imarith IRAS05338.218.fits - dark60.fits IRAS05338.218d.fits 2) Scale images to same (mean = 13779.9 sky) value imstat IRAS05338.*d.fits >> awklist.txt imarith IRAS05338.210d.fits * 1.01286 IRAS05338.210a.fits imarith IRAS05338.211d.fits * 1.00708 IRAS05338.211a.fits imarith IRAS05338.212d.fits * 0.981894 IRAS05338.212a.fits imarith IRAS05338.213d.fits * 0.96735 IRAS05338.213a.fits imarith IRAS05338.214d.fits * 0.979799 IRAS05338.214a.fits imarith IRAS05338.215d.fits * 0.98449 IRAS05338.215a.fits imarith IRAS05338.216d.fits * 1.01509 IRAS05338.216a.fits imarith IRAS05338.217d.fits * 1.04149 IRAS05338.217a.fits imarith IRAS05338.218d.fits * 1.01435 IRAS05338.218a.fits imstat IRAS05338*a.fits 3) Make skyflat (avg combine, min=0 max=2 reject) epar imcomb imcomb IRAS05338.*a.fits IRAS05338.sky.fits 4) Normalize by midpt imstat IRAS05338.sky.fits imarith IRAS05338.sky.fits / 13786. IRAS05338.skyN.fits 5) Divide by skyflat imarith IRAS05338.210d.fits / IRAS05338.skyN.fits IRAS05338.210df.fits imarith IRAS05338.211d.fits / IRAS05338.skyN.fits IRAS05338.211df.fits imarith IRAS05338.212d.fits / IRAS05338.skyN.fits IRAS05338.212df.fits imarith IRAS05338.213d.fits / IRAS05338.skyN.fits IRAS05338.213df.fits imarith IRAS05338.214d.fits / IRAS05338.skyN.fits IRAS05338.214df.fits imarith IRAS05338.215d.fits / IRAS05338.skyN.fits IRAS05338.215df.fits imarith IRAS05338.216d.fits / IRAS05338.skyN.fits IRAS05338.216df.fits imarith IRAS05338.217d.fits / IRAS05338.skyN.fits IRAS05338.217df.fits imarith IRAS05338.218d.fits / IRAS05338.skyN.fits IRAS05338.218df.fits 6) Subtract by constant (midpt) imstat IRAS05338.*df.fits imarith IRAS05338.210df.fits - 13640. IRAS05338.210dfs.fits imarith IRAS05338.211df.fits - 13718. IRAS05338.211dfs.fits imarith IRAS05338.212df.fits - 14067. IRAS05338.212dfs.fits imarith IRAS05338.213df.fits - 14276. IRAS05338.213dfs.fits imarith IRAS05338.214df.fits - 14097. IRAS05338.214dfs.fits imarith IRAS05338.215df.fits - 14027. IRAS05338.215dfs.fits imarith IRAS05338.216df.fits - 13603. IRAS05338.216dfs.fits imarith IRAS05338.217df.fits - 13258. IRAS05338.217dfs.fits imarith IRAS05338.218df.fits - 13613. IRAS05338.218dfs.fits 7) get coords and shifts shifts: 742.05 376.94 848.67 271.27 744.00 270.20 640.93 270.26 854.51 371.28 644.81 372.53 859.17 475.69 755.87 475.53 650.06 476.38 0. 0. -106.62 105.67 -1.95 106.74 101.12 106.68 -112.46 5.66 97.24 4.41 -117.12 -98.75 -13.82 -98.59 91.99 -99.44 coords: 280.87 653.90 163.93 592.66 266.94 537.24 599.89 812.26 786.86 505.65 742.05 376.94 ------> IRAS 05354-0438 <------ 1) Subtract dark imarith IRAS05354.220.fits - dark60.fits IRAS05354.220d.fits imarith IRAS05354.221.fits - dark60.fits IRAS05354.221d.fits imarith IRAS05354.222.fits - dark60.fits IRAS05354.222d.fits imarith IRAS05354.223.fits - dark60.fits IRAS05354.223d.fits imarith IRAS05354.224.fits - dark60.fits IRAS05354.224d.fits imarith IRAS05354.225.fits - dark60.fits IRAS05354.225d.fits imarith IRAS05354.226.fits - dark60.fits IRAS05354.226d.fits imarith IRAS05354.227.fits - dark60.fits IRAS05354.227d.fits imarith IRAS05354.228.fits - dark60.fits IRAS05354.228d.fits 2) Scale images to same (mean = 13723.2 sky) value imstat IRAS05354.*d.fits >> awklist.txt imarith IRAS05354.220d.fits * 1.0151 IRAS05354.220a.fits imarith IRAS05354.221d.fits * 1.01062 IRAS05354.221a.fits imarith IRAS05354.222d.fits * 1.00758 IRAS05354.222a.fits imarith IRAS05354.223d.fits * 1.01865 IRAS05354.223a.fits imarith IRAS05354.224d.fits * 1.00647 IRAS05354.224a.fits imarith IRAS05354.225d.fits * 0.994363 IRAS05354.225a.fits imarith IRAS05354.226d.fits * 0.985084 IRAS05354.226a.fits imarith IRAS05354.227d.fits * 0.979529 IRAS05354.227a.fits imarith IRAS05354.228d.fits * 0.984306 IRAS05354.228a.fits imstat IRAS05354*a.fits 3) Make skyflat (avg combine, min=0 max=2 reject) epar imcomb imcomb IRAS05354.*a.fits IRAS05354.sky.fits 4) Normalize by midpt imstat IRAS05354.sky.fits imarith IRAS05354.sky.fits / 13732. IRAS05354.skyN.fits 5) Divide by skyflat imarith IRAS05354.220d.fits / IRAS05354.skyN.fits IRAS05354.220df.fits imarith IRAS05354.221d.fits / IRAS05354.skyN.fits IRAS05354.221df.fits imarith IRAS05354.222d.fits / IRAS05354.skyN.fits IRAS05354.222df.fits imarith IRAS05354.223d.fits / IRAS05354.skyN.fits IRAS05354.223df.fits imarith IRAS05354.224d.fits / IRAS05354.skyN.fits IRAS05354.224df.fits imarith IRAS05354.225d.fits / IRAS05354.skyN.fits IRAS05354.225df.fits imarith IRAS05354.226d.fits / IRAS05354.skyN.fits IRAS05354.226df.fits imarith IRAS05354.227d.fits / IRAS05354.skyN.fits IRAS05354.227df.fits imarith IRAS05354.228d.fits / IRAS05354.skyN.fits IRAS05354.228df.fits 6) Subtract by constant (midpt) imstat IRAS05354.*df.fits imarith IRAS05354.220df.fits - 13556. IRAS05354.220dfs.fits imarith IRAS05354.221df.fits - 13609. IRAS05354.221dfs.fits imarith IRAS05354.222df.fits - 13655. IRAS05354.222dfs.fits imarith IRAS05354.223df.fits - 13509. IRAS05354.223dfs.fits imarith IRAS05354.224df.fits - 13670. IRAS05354.224dfs.fits imarith IRAS05354.225df.fits - 13834. IRAS05354.225dfs.fits imarith IRAS05354.226df.fits - 13967. IRAS05354.226dfs.fits imarith IRAS05354.227df.fits - 14045. IRAS05354.227dfs.fits imarith IRAS05354.228df.fits - 13976. IRAS05354.228dfs.fits 7) get coords and shifts shifts: 635.72 380.71 739.50 277.71 635.64 276.05 528.98 275.72 739.15 377.05 529.90 378.52 742.12 481.71 637.08 482.33 532.44 482.64 0. 0. -103.78 103 0.08 104.66 106.74 104.99 -103.43 3.66 105.82 2.19 -106.4 -101 -1.36 -101.62 103.28 -101.93 coords: 449.47 659.04 528.46 723.83 635.72 380.71 922.68 478.51 688.84 183.68 ------> IRAS 05356-0530 <------ 1) Subtract dark imarith IRAS05356.236.fits - dark60.fits IRAS05356.236d.fits imarith IRAS05356.237.fits - dark60.fits IRAS05356.237d.fits imarith IRAS05356.238.fits - dark60.fits IRAS05356.238d.fits imarith IRAS05356.239.fits - dark60.fits IRAS05356.239d.fits imarith IRAS05356.240.fits - dark60.fits IRAS05356.240d.fits imarith IRAS05356.241.fits - dark60.fits IRAS05356.241d.fits imarith IRAS05356.242.fits - dark60.fits IRAS05356.242d.fits imarith IRAS05356.243.fits - dark60.fits IRAS05356.243d.fits imarith IRAS05356.244.fits - dark60.fits IRAS05356.244d.fits 2) Scale images to same (mean = 13355.2 sky) value imstat IRAS05356.*d.fits >> awklist.txt imarith IRAS05356.236d.fits * 1.018 IRAS05356.236a.fits imarith IRAS05356.237d.fits * 1.00657 IRAS05356.237a.fits imarith IRAS05356.238d.fits * 1.00197 IRAS05356.238a.fits imarith IRAS05356.239d.fits * 1.00076 IRAS05356.239a.fits imarith IRAS05356.240d.fits * 0.982361 IRAS05356.240a.fits imarith IRAS05356.241d.fits * 0.986279 IRAS05356.241a.fits imarith IRAS05356.242d.fits * 0.986133 IRAS05356.242a.fits imarith IRAS05356.243d.fits * 1.00733 IRAS05356.243a.fits imarith IRAS05356.244d.fits * 1.01183 IRAS05356.244a.fits imstat IRAS05356*a.fits 3) Make skyflat (avg combine, min=0 max=2 reject) epar imcomb imcomb IRAS05356.*a.fits IRAS05356.sky.fits 4) Normalize by midpt imstat IRAS05356.sky.fits imarith IRAS05356.sky.fits / 13355. IRAS05356.skyN.fits 5) Divide by skyflat imarith IRAS05356.236d.fits / IRAS05356.skyN.fits IRAS05356.236df.fits imarith IRAS05356.237d.fits / IRAS05356.skyN.fits IRAS05356.237df.fits imarith IRAS05356.238d.fits / IRAS05356.skyN.fits IRAS05356.238df.fits imarith IRAS05356.239d.fits / IRAS05356.skyN.fits IRAS05356.239df.fits imarith IRAS05356.240d.fits / IRAS05356.skyN.fits IRAS05356.240df.fits imarith IRAS05356.241d.fits / IRAS05356.skyN.fits IRAS05356.241df.fits imarith IRAS05356.242d.fits / IRAS05356.skyN.fits IRAS05356.242df.fits imarith IRAS05356.243d.fits / IRAS05356.skyN.fits IRAS05356.243df.fits imarith IRAS05356.244d.fits / IRAS05356.skyN.fits IRAS05356.244df.fits 6) Subtract by constant (midpt) imstat IRAS05356.*df.fits imarith IRAS05356.236df.fits - 13146. IRAS05356.236dfs.fits imarith IRAS05356.237df.fits - 13294. IRAS05356.237dfs.fits imarith IRAS05356.238df.fits - 13355. IRAS05356.238dfs.fits imarith IRAS05356.239df.fits - 13366. IRAS05356.239dfs.fits imarith IRAS05356.240df.fits - 13619. IRAS05356.240dfs.fits imarith IRAS05356.241df.fits - 13567. IRAS05356.241dfs.fits imarith IRAS05356.242df.fits - 13565. IRAS05356.242dfs.fits imarith IRAS05356.243df.fits - 13279. IRAS05356.243dfs.fits imarith IRAS05356.244df.fits - 13221. IRAS05356.244dfs.fits 7) get coords and shifts shifts: 482.72 605.78 590.17 503.03 486.15 501.46 380.36 501.80 590.43 605.73 379.27 606.21 587.11 711.77 478.99 713.01 371.62 714.31 0. 0. -107.45 102.75 -3.43 104.32 102.36 103.98 -107.71 0.05 103.45 -0.43 -104.39 -105.99 3.73 -107.23 111.1 -108.53 coords: 266.52 673.48 232.58 576.42 482.72 605.78 722.81 666.27 819.26 493.44 734.32 432.14 702.74 412.47 538.53 329.65 ------> IRAS 05356-0541 <------ 1) Subtract dark imarith IRAS05356.0541.246.fits - dark60.fits IRAS05356.0541.246d.fits imarith IRAS05356.0541.247.fits - dark60.fits IRAS05356.0541.247d.fits imarith IRAS05356.0541.248.fits - dark60.fits IRAS05356.0541.248d.fits imarith IRAS05356.0541.249.fits - dark60.fits IRAS05356.0541.249d.fits imarith IRAS05356.0541.250.fits - dark60.fits IRAS05356.0541.250d.fits imarith IRAS05356.0541.251.fits - dark60.fits IRAS05356.0541.251d.fits imarith IRAS05356.0541.252.fits - dark60.fits IRAS05356.0541.252d.fits imarith IRAS05356.0541.253.fits - dark60.fits IRAS05356.0541.253d.fits imarith IRAS05356.0541.254.fits - dark60.fits IRAS05356.0541.254d.fits 2) Scale images to same (mean = 13170.0 sky) value imstat IRAS05356.0541.*d.fits >> awklist.txt imarith IRAS05356.0541.246d.fits * 0.97722 IRAS05356.0541.246a.fits imarith IRAS05356.0541.247d.fits * 0.990226 IRAS05356.0541.247a.fits imarith IRAS05356.0541.248d.fits * 1.01284 IRAS05356.0541.248a.fits imarith IRAS05356.0541.249d.fits * 0.994187 IRAS05356.0541.249a.fits imarith IRAS05356.0541.250d.fits * 0.997652 IRAS05356.0541.250a.fits imarith IRAS05356.0541.251d.fits * 1.00015 IRAS05356.0541.251a.fits imarith IRAS05356.0541.252d.fits * 0.997954 IRAS05356.0541.252a.fits imarith IRAS05356.0541.253d.fits * 1.01464 IRAS05356.0541.253a.fits imarith IRAS05356.0541.254d.fits * 1.01644 IRAS05356.0541.254a.fits imstat IRAS05356.0541*a.fits 3) Make skyflat (avg combine, min=0 max=2 reject) epar imcomb imcomb IRAS05356.0541.*a.fits IRAS05356.0541.sky.fits 4) Normalize by midpt imstat IRAS05356.0541.sky.fits imarith IRAS05356.0541.sky.fits / 13196. IRAS05356.0541.skyN.fits 5) Divide by skyflat imarith IRAS05356.0541.246d.fits / IRAS05356.0541.skyN.fits IRAS05356.0541.246df.fits imarith IRAS05356.0541.247d.fits / IRAS05356.0541.skyN.fits IRAS05356.0541.247df.fits imarith IRAS05356.0541.248d.fits / IRAS05356.0541.skyN.fits IRAS05356.0541.248df.fits imarith IRAS05356.0541.249d.fits / IRAS05356.0541.skyN.fits IRAS05356.0541.249df.fits imarith IRAS05356.0541.250d.fits / IRAS05356.0541.skyN.fits IRAS05356.0541.250df.fits imarith IRAS05356.0541.251d.fits / IRAS05356.0541.skyN.fits IRAS05356.0541.251df.fits imarith IRAS05356.0541.252d.fits / IRAS05356.0541.skyN.fits IRAS05356.0541.252df.fits imarith IRAS05356.0541.253d.fits / IRAS05356.0541.skyN.fits IRAS05356.0541.253df.fits imarith IRAS05356.0541.254d.fits / IRAS05356.0541.skyN.fits IRAS05356.0541.254df.fits 6) Subtract by constant (midpt) imstat IRAS05356.0541.*df.fits imarith IRAS05356.0541.246df.fits - 13523. IRAS05356.0541.246dfs.fits imarith IRAS05356.0541.247df.fits - 13352. IRAS05356.0541.247dfs.fits imarith IRAS05356.0541.248df.fits - 13052. IRAS05356.0541.248dfs.fits imarith IRAS05356.0541.249df.fits - 13298. IRAS05356.0541.249dfs.fits imarith IRAS05356.0541.250df.fits - 13255. IRAS05356.0541.250dfs.fits imarith IRAS05356.0541.251df.fits - 13221. IRAS05356.0541.251dfs.fits imarith IRAS05356.0541.252df.fits - 13244. IRAS05356.0541.252dfs.fits imarith IRAS05356.0541.253df.fits - 13028. IRAS05356.0541.253dfs.fits imarith IRAS05356.0541.254df.fits - 13008. IRAS05356.0541.254dfs.fits 7) get coords and shifts shifts: 440.28 463.75 543.13 361.77 437.95 359.82 332.18 358.65 540.53 459.62 330.90 461.31 542.44 565.04 439.13 566.13 333.09 566.51 0. 0. -102.85 101.98 2.33 103.93 108.1 105.1 -100.25 4.13 109.38 2.44 -102.16 -101.29 1.15 -102.38 107.19 -102.76 coords: 267.97 884.00 440.23 463.77 419.48 447.74 459.39 315.46 444.90 241.95 651.42 165.94 698.95 236.05 -----> IRAS 05378-0750 <------ 1) Subtract dark imarith IRAS05378.257.fits - dark60.fits IRAS05378.257d.fits imarith IRAS05378.258.fits - dark60.fits IRAS05378.258d.fits imarith IRAS05378.259.fits - dark60.fits IRAS05378.259d.fits imarith IRAS05378.260.fits - dark60.fits IRAS05378.260d.fits imarith IRAS05378.261.fits - dark60.fits IRAS05378.261d.fits imarith IRAS05378.262.fits - dark60.fits IRAS05378.262d.fits imarith IRAS05378.263.fits - dark60.fits IRAS05378.263d.fits imarith IRAS05378.264.fits - dark60.fits IRAS05378.264d.fits imarith IRAS05378.265.fits - dark60.fits IRAS05378.265d.fits imstat IRAS05378.*d.fits >> awklist.txt 2) Scale images to same (mean = 13088.0 sky) value imarith IRAS05378.257d.fits * 1.02075 IRAS05378.257a.fits imarith IRAS05378.258d.fits * 1.00115 IRAS05378.258a.fits imarith IRAS05378.259d.fits * 0.987475 IRAS05378.259a.fits imarith IRAS05378.260d.fits * 0.989043 IRAS05378.260a.fits imarith IRAS05378.261d.fits * 1.00284 IRAS05378.261a.fits imarith IRAS05378.262d.fits * 1.00054 IRAS05378.262a.fits imarith IRAS05378.263d.fits * 0.99099 IRAS05378.263a.fits imarith IRAS05378.264d.fits * 0.999542 IRAS05378.264a.fits imarith IRAS05378.265d.fits * 1.00855 IRAS05378.265a.fits imstat IRAS05378*a.fits 3) Make skyflat (avg combine, min=0 max=2 reject) epar imcomb imcomb IRAS05378.*a.fits IRAS05378.sky.fits 4) Normalize by midpt imstat IRAS05378.sky.fits imarith IRAS05378.sky.fits / 13085. IRAS05378.skyN.fits 5) Divide by skyflat imarith IRAS05378.257d.fits / IRAS05378.skyN.fits IRAS05378.257df.fits imarith IRAS05378.258d.fits / IRAS05378.skyN.fits IRAS05378.258df.fits imarith IRAS05378.259d.fits / IRAS05378.skyN.fits IRAS05378.259df.fits imarith IRAS05378.260d.fits / IRAS05378.skyN.fits IRAS05378.260df.fits imarith IRAS05378.261d.fits / IRAS05378.skyN.fits IRAS05378.261df.fits imarith IRAS05378.262d.fits / IRAS05378.skyN.fits IRAS05378.262df.fits imarith IRAS05378.263d.fits / IRAS05378.skyN.fits IRAS05378.263df.fits imarith IRAS05378.264d.fits / IRAS05378.skyN.fits IRAS05378.264df.fits imarith IRAS05378.265d.fits / IRAS05378.skyN.fits IRAS05378.265df.fits 6) Subtract by constant (midpt) imstat IRAS05378.*df.fits imarith IRAS05378.257df.fits - 12845. IRAS05378.257dfs.fits imarith IRAS05378.258df.fits - 13092. IRAS05378.258dfs.fits imarith IRAS05378.259df.fits - 13275. IRAS05378.259dfs.fits imarith IRAS05378.260df.fits - 13255. IRAS05378.260dfs.fits imarith IRAS05378.261df.fits - 13077. IRAS05378.261dfs.fits imarith IRAS05378.262df.fits - 13100. IRAS05378.262dfs.fits imarith IRAS05378.263df.fits - 13233. IRAS05378.263dfs.fits imarith IRAS05378.264df.fits - 13114. IRAS05378.264dfs.fits imarith IRAS05378.265df.fits - 12996. IRAS05378.265dfs.fits 7) get coords and shifts shifts: 625.51 488.87 733.53 388.96 631.93 388.63 528.59 387.52 739.57 489.53 529.32 490.16 739.91 595.81 632.56 596.35 527.39 596.70 0. 0. -108.02 99.91 -6.42 100.24 96.92 101.35 -114.06 -0.66 96.19 -1.29 -114.4 -106.94 -7.05 -107.48 98.12 -107.83 coords: 165.33 609.67 219.39 507.06 495.57 764.88 625.51 488.92 349.93 394.80 ------> IRAS 05379-0758 <------- 1) Subtract dark imarith IRAS05379.268.fits - dark60.fits IRAS05379.268d.fits imarith IRAS05379.269.fits - dark60.fits IRAS05379.269d.fits imarith IRAS05379.270.fits - dark60.fits IRAS05379.270d.fits imarith IRAS05379.271.fits - dark60.fits IRAS05379.271d.fits imarith IRAS05379.272.fits - dark60.fits IRAS05379.272d.fits imarith IRAS05379.273.fits - dark60.fits IRAS05379.273d.fits imarith IRAS05379.274.fits - dark60.fits IRAS05379.274d.fits imarith IRAS05379.275.fits - dark60.fits IRAS05379.275d.fits imarith IRAS05379.276.fits - dark60.fits IRAS05379.276d.fits imstat IRAS05379.*d.fits >> awklist.txt 2) Scale images to same (mean = 5829.78 sky) value imarith IRAS05379.268d.fits * 0.995523 IRAS05379.268a.fits imarith IRAS05379.269d.fits * 0.974228 IRAS05379.269a.fits imarith IRAS05379.270d.fits * 1.00722 IRAS05379.270a.fits imarith IRAS05379.271d.fits * 0.999277 IRAS05379.271a.fits imarith IRAS05379.272d.fits * 0.996033 IRAS05379.272a.fits imarith IRAS05379.273d.fits * 1.00914 IRAS05379.273a.fits imarith IRAS05379.274d.fits * 1.00323 IRAS05379.274a.fits imarith IRAS05379.275d.fits * 1.01054 IRAS05379.275a.fits imarith IRAS05379.276d.fits * 1.00583 IRAS05379.276a.fits imstat IRAS05379*a.fits 3) Make skyflat (avg combine, min=0 max=2 reject) epar imcomb imcomb IRAS05379.*a.fits IRAS05379.sky.fits 4) Normalize by midpt imstat IRAS05379.sky.fits imarith IRAS05379.sky.fits / 5828. IRAS05379.skyN.fits 5) Divide by skyflat imarith IRAS05379.268d.fits / IRAS05379.skyN.fits IRAS05379.268df.fits imarith IRAS05379.269d.fits / IRAS05379.skyN.fits IRAS05379.269df.fits imarith IRAS05379.270d.fits / IRAS05379.skyN.fits IRAS05379.270df.fits imarith IRAS05379.271d.fits / IRAS05379.skyN.fits IRAS05379.271df.fits imarith IRAS05379.272d.fits / IRAS05379.skyN.fits IRAS05379.272df.fits imarith IRAS05379.273d.fits / IRAS05379.skyN.fits IRAS05379.273df.fits imarith IRAS05379.274d.fits / IRAS05379.skyN.fits IRAS05379.274df.fits imarith IRAS05379.275d.fits / IRAS05379.skyN.fits IRAS05379.275df.fits imarith IRAS05379.276d.fits / IRAS05379.skyN.fits IRAS05379.276df.fits 6) Subtract by constant (midpt) imstat IRAS05379.*df.fits imarith IRAS05379.268df.fits - 5872. IRAS05379.268dfs.fits imarith IRAS05379.269df.fits - 6000. IRAS05379.269dfs.fits imarith IRAS05379.270df.fits - 5802. IRAS05379.270dfs.fits imarith IRAS05379.271df.fits - 5847. IRAS05379.271dfs.fits imarith IRAS05379.272df.fits - 5870. IRAS05379.272dfs.fits imarith IRAS05379.273df.fits - 5794. IRAS05379.273dfs.fits imarith IRAS05379.274df.fits - 5828. IRAS05379.274dfs.fits imarith IRAS05379.275df.fits - 5785. IRAS05379.275dfs.fits imarith IRAS05379.276df.fits - 5814. IRAS05379.276dfs.fits 7) get coords and shifts shifts: 525.32 558.38 629.98 454.82 524.51 454.63 416.77 455.06 627.68 553.70 418.02 554.64 627.16 658.22 521.32 658.57 416.20 659.86 0. 0. -104.66 103.56 0.81 103.75 108.55 103.32 -102.36 4.68 107.3 3.74 -101.84 -99.84 4 -100.19 109.12 -101.48 coords: 137.92 766.23 160.92 821.39 478.89 559.57 525.32 558.38 ------> IRAS F05391-0841 <------ 1) Subtract dark imarith IRASF05391.279.fits - dark60.fits IRASF05391.279d.fits imarith IRASF05391.280.fits - dark60.fits IRASF05391.280d.fits imarith IRASF05391.281.fits - dark60.fits IRASF05391.281d.fits imarith IRASF05391.282.fits - dark60.fits IRASF05391.282d.fits imarith IRASF05391.283.fits - dark60.fits IRASF05391.283d.fits imarith IRASF05391.284.fits - dark60.fits IRASF05391.284d.fits imarith IRASF05391.285.fits - dark60.fits IRASF05391.285d.fits imarith IRASF05391.286.fits - dark60.fits IRASF05391.286d.fits imarith IRASF05391.287.fits - dark60.fits IRASF05391.287d.fits imstat IRASF05391.*d.fits >> awklist.txt 2) Scale images to same (mean = 12754.2 sky) value imarith IRASF05391.279d.fits * 1.01457 IRASF05391.279a.fits imarith IRASF05391.280d.fits * 1.0132 IRASF05391.280a.fits imarith IRASF05391.281d.fits * 1.00744 IRASF05391.281a.fits imarith IRASF05391.282d.fits * 0.99448 IRASF05391.282a.fits imarith IRASF05391.283d.fits * 0.986404 IRASF05391.283a.fits imarith IRASF05391.284d.fits * 0.991079 IRASF05391.284a.fits imarith IRASF05391.285d.fits * 0.997981 IRASF05391.285a.fits imarith IRASF05391.286d.fits * 0.999311 IRASF05391.286a.fits imarith IRASF05391.287d.fits * 0.996266 IRASF05391.287a.fits imstat IRASF05391*a.fits 3) Make skyflat (avg combine, min=0 max=2 reject) epar imcomb imcomb IRASF05391.*a.fits IRASF05391.sky.fits 4) Normalize by midpt imstat IRASF05391.sky.fits imarith IRASF05391.sky.fits / 12770. IRASF05391.skyN.fits 5) Divide by skyflat imarith IRASF05391.279d.fits / IRASF05391.skyN.fits IRASF05391.279df.fits imarith IRASF05391.280d.fits / IRASF05391.skyN.fits IRASF05391.280df.fits imarith IRASF05391.281d.fits / IRASF05391.skyN.fits IRASF05391.281df.fits imarith IRASF05391.282d.fits / IRASF05391.skyN.fits IRASF05391.282df.fits imarith IRASF05391.283d.fits / IRASF05391.skyN.fits IRASF05391.283df.fits imarith IRASF05391.284d.fits / IRASF05391.skyN.fits IRASF05391.284df.fits imarith IRASF05391.285d.fits / IRASF05391.skyN.fits IRASF05391.285df.fits imarith IRASF05391.286d.fits / IRASF05391.skyN.fits IRASF05391.286df.fits imarith IRASF05391.287d.fits / IRASF05391.skyN.fits IRASF05391.287df.fits 6) Subtract by constant (midpt) imstat IRASF05391.*df.fits imarith IRASF05391.279df.fits - 12611. IRASF05391.279dfs.fits imarith IRASF05391.280df.fits - 12630. IRASF05391.280dfs.fits imarith IRASF05391.281df.fits - 12698. IRASF05391.281dfs.fits imarith IRASF05391.282df.fits - 12868. IRASF05391.282dfs.fits imarith IRASF05391.283df.fits - 12973. IRASF05391.283dfs.fits imarith IRASF05391.284df.fits - 12911. IRASF05391.284dfs.fits imarith IRASF05391.285df.fits - 12824. IRASF05391.285dfs.fits imarith IRASF05391.286df.fits - 12802. IRASF05391.286dfs.fits imarith IRASF05391.287df.fits - 12841. IRASF05391.287dfs.fits 7) get coords and shifts shifts: 520.62 537.86 624.41 433.35 519.97 432.77 416.92 431.94 624.73 535.25 412.68 536.10 622.53 639.92 514.22 640.45 406.06 641.15 0. 0. -103.79 104.51 0.65 105.09 103.7 105.92 -104.11 2.61 107.94 1.76 -101.91 -102.06 6.4 -102.59 114.56 -103.29 coords: 490.17 465.83 498.12 493.05 520.65 537.89 -----> IRAS 06087-1008 <----- 1) Subtract dark imarith IRAS06087.289.fits - dark60.fits IRAS06087.289d.fits imarith IRAS06087.290.fits - dark60.fits IRAS06087.290d.fits imarith IRAS06087.291.fits - dark60.fits IRAS06087.291d.fits imarith IRAS06087.292.fits - dark60.fits IRAS06087.292d.fits imarith IRAS06087.293.fits - dark60.fits IRAS06087.293d.fits imarith IRAS06087.294.fits - dark60.fits IRAS06087.294d.fits imarith IRAS06087.295.fits - dark60.fits IRAS06087.295d.fits imarith IRAS06087.296.fits - dark60.fits IRAS06087.296d.fits imarith IRAS06087.297.fits - dark60.fits IRAS06087.297d.fits imstat IRAS06087.*d.fits >> awklist.txt 2) Scale images to same (mean = 12976.3 sky) value imarith IRAS06087.289d.fits * 0.993439 IRAS06087.289a.fits imarith IRAS06087.290d.fits * 0.996032 IRAS06087.290a.fits imarith IRAS06087.291d.fits * 0.992755 IRAS06087.291a.fits imarith IRAS06087.292d.fits * 0.995573 IRAS06087.292a.fits imarith IRAS06087.293d.fits * 1.01203 IRAS06087.293a.fits imarith IRAS06087.294d.fits * 1.00366 IRAS06087.294a.fits imarith IRAS06087.295d.fits * 1.00889 IRAS06087.295a.fits imarith IRAS06087.296d.fits * 0.998561 IRAS06087.296a.fits imarith IRAS06087.297d.fits * 0.999407 IRAS06087.297a.fits imstat IRAS06087*a.fits 3) Make skyflat (avg combine, min=0 max=2 reject) epar imcomb imcomb IRAS06087.*a.fits IRAS06087.sky.fits 4) Normalize by midpt imstat IRAS06087.sky.fits imarith IRAS06087.sky.fits / 12993. IRAS06087.skyN.fits 5) Divide by skyflat imarith IRAS06087.289d.fits / IRAS06087.skyN.fits IRAS06087.289df.fits imarith IRAS06087.290d.fits / IRAS06087.skyN.fits IRAS06087.290df.fits imarith IRAS06087.291d.fits / IRAS06087.skyN.fits IRAS06087.291df.fits imarith IRAS06087.292d.fits / IRAS06087.skyN.fits IRAS06087.292df.fits imarith IRAS06087.293d.fits / IRAS06087.skyN.fits IRAS06087.293df.fits imarith IRAS06087.294d.fits / IRAS06087.skyN.fits IRAS06087.294df.fits imarith IRAS06087.295d.fits / IRAS06087.skyN.fits IRAS06087.295df.fits imarith IRAS06087.296d.fits / IRAS06087.skyN.fits IRAS06087.296df.fits imarith IRAS06087.297d.fits / IRAS06087.skyN.fits IRAS06087.297df.fits 6) Subtract by constant (midpt) imstat IRAS06087.*df.fits imarith IRAS06087.289df.fits - 13101. IRAS06087.289dfs.fits imarith IRAS06087.290df.fits - 13071. IRAS06087.290dfs.fits imarith IRAS06087.291df.fits - 13116. IRAS06087.291dfs.fits imarith IRAS06087.292df.fits - 13074. IRAS06087.292dfs.fits imarith IRAS06087.293df.fits - 12862. IRAS06087.293dfs.fits imarith IRAS06087.294df.fits - 12968. IRAS06087.294dfs.fits imarith IRAS06087.295df.fits - 12906. IRAS06087.295dfs.fits imarith IRAS06087.296df.fits - 13039. IRAS06087.296dfs.fits imarith IRAS06087.297df.fits - 13022. IRAS06087.297dfs.fits 7) get coords and shifts shifts: 426.03 549.08 531.63 448.97 425.27 448.04 318.96 447.59 530.92 550.13 319.33 551.09 527.79 656.22 421.18 656.94 315.18 657.58 0. 0. -105.6 100.11 0.76 101.04 107.07 101.49 -104.89 -1.05 106.7 -2.01 -101.76 -107.14 4.85 -107.86 110.85 -108.5 coords: 236.79 432.09 426.03 549.08 601.48 579.02 606.21 303.34 733.09 341.17 763.55 332.12 675.92 698.17 -----> fs101 <----- 1) Subtract dark imarith fs101.075.fits - dark5.fits fs101.075d.fits imarith fs101.076.fits - dark5.fits fs101.076d.fits imarith fs101.077.fits - dark5.fits fs101.077d.fits imarith fs101.078.fits - dark5.fits fs101.078d.fits imarith fs101.079.fits - dark5.fits fs101.079d.fits imstat fs101.*d.fits >> awklist.txt 2) Scale images to same (mean = 4895.2 sky) value imarith fs101.075d.fits * 0.962296 fs101.075a.fits imarith fs101.076d.fits * 1.01182 fs101.076a.fits imarith fs101.077d.fits * 0.996986 fs101.077a.fits imarith fs101.078d.fits * 1.00849 fs101.078a.fits imarith fs101.079d.fits * 1.0226 fs101.079a.fits imstat fs101*a.fits 3) Make skyflat (avg combine, min=0 max=2 reject) epar imcomb imcomb fs101.*a.fits fs101.sky.fits 4) Normalize by midpt imstat fs101.sky.fits imarith fs101.sky.fits / 4881. fs101.skyN.fits 5) Divide by skyflat imarith fs101.075d.fits / fs101.skyN.fits fs101.075df.fits imarith fs101.076d.fits / fs101.skyN.fits fs101.076df.fits imarith fs101.077d.fits / fs101.skyN.fits fs101.077df.fits imarith fs101.078d.fits / fs101.skyN.fits fs101.078df.fits imarith fs101.079d.fits / fs101.skyN.fits fs101.079df.fits 6) Subtract by constant (midpt) imstat fs101.*df.fits imarith fs101.075df.fits - 5098. fs101.075dfs.fits imarith fs101.076df.fits - 4848. fs101.076dfs.fits imarith fs101.077df.fits - 4920. fs101.077dfs.fits imarith fs101.078df.fits - 4864. fs101.078dfs.fits imarith fs101.079df.fits - 4795. fs101.079dfs.fits 7) get coords and shifts shifts: 515.28 519.58 513.89 416.68 512.82 620.88 408.51 523.92 620.86 523.14 0. 0. 1.39 102.9 2.46 -101.3 106.77 -4.34 -105.58 -3.56 coords: 515.28 519.58 402.78 688.01 376.48 330.26 ------> fs119 <------- 1) Subtract dark imarith fs119.178.fits - dark5.fits fs119.178d.fits imarith fs119.179.fits - dark5.fits fs119.179d.fits imarith fs119.180.fits - dark5.fits fs119.180d.fits imarith fs119.181.fits - dark5.fits fs119.181d.fits imarith fs119.182.fits - dark5.fits fs119.182d.fits imstat fs119.*d.fits >> awklist.txt 2) Scale images to same (mean = 5069.4 sky) value imarith fs119.178d.fits * 1.00404 fs119.178a.fits imarith fs119.179d.fits * 0.990504 fs119.179a.fits imarith fs119.180d.fits * 0.976575 fs119.180a.fits imarith fs119.181d.fits * 1.00964 fs119.181a.fits imarith fs119.182d.fits * 1.02041 fs119.182a.fits imstat fs119*a.fits 3) Make skyflat (avg combine, min=0 max=2 reject) epar imcomb imcomb fs119.*a.fits fs119.sky.fits 4) Normalize by midpt imstat fs119.sky.fits imarith fs119.sky.fits / 5049. fs119.skyN.fits 5) Divide by skyflat imarith fs119.178d.fits / fs119.skyN.fits fs119.178df.fits imarith fs119.179d.fits / fs119.skyN.fits fs119.179df.fits imarith fs119.180d.fits / fs119.skyN.fits fs119.180df.fits imarith fs119.181d.fits / fs119.skyN.fits fs119.181df.fits imarith fs119.182d.fits / fs119.skyN.fits fs119.182df.fits 6) Subtract by constant (midpt) imstat fs119.*df.fits imarith fs119.178df.fits - 5053. fs119.178dfs.fits imarith fs119.179df.fits - 5122. fs119.179dfs.fits imarith fs119.180df.fits - 5195. fs119.180dfs.fits imarith fs119.181df.fits - 5024. fs119.181dfs.fits imarith fs119.182df.fits - 4973. fs119.182dfs.fits 7) get coords and shifts shifts: 510.15 512.27 510.04 411.55 512.69 615.50 407.76 516.46 615.97 514.69 0. 0. 0.11 100.72 -2.54 -103.23 102.39 -4.19 -105.82 -2.42 coords: 510.15 512.27 210.24 465.07 751.33 824.97 --> for fin2.fits 1) Subtract dark imarith fs119.299.fits - dark5.fits fs119.299d.fits imarith fs119.300.fits - dark5.fits fs119.300d.fits imarith fs119.301.fits - dark5.fits fs119.301d.fits imarith fs119.302.fits - dark5.fits fs119.302d.fits imarith fs119.303.fits - dark5.fits fs119.303d.fits imstat fs119.*d.fits >> awklist.txt 2) Scale images to same (mean = 5326.4 sky) value imarith fs119.299d.fits * 0.989485 fs119.299a.fits imarith fs119.300d.fits * 1.01339 fs119.300a.fits imarith fs119.301d.fits * 0.981463 fs119.301a.fits imarith fs119.302d.fits * 1.01224 fs119.302a.fits imarith fs119.303d.fits * 1.00422 fs119.303a.fits imstat fs119*a.fits 3) Make skyflat (avg combine, min=0 max=2 reject) epar imcomb imcomb fs119.*a.fits fs119.sky2.fits 4) Normalize by midpt imstat fs119.sky2.fits imarith fs119.sky2.fits / 5314. fs119.sky2N.fits 5) Divide by skyflat imarith fs119.299d.fits / fs119.sky2N.fits fs119.299df.fits imarith fs119.300d.fits / fs119.sky2N.fits fs119.300df.fits imarith fs119.301d.fits / fs119.sky2N.fits fs119.301df.fits imarith fs119.302d.fits / fs119.sky2N.fits fs119.302df.fits imarith fs119.303d.fits / fs119.sky2N.fits fs119.303df.fits 6) Subtract by constant (midpt) imstat fs119.*df.fits imarith fs119.299df.fits - 5397. fs119.299dfs.fits imarith fs119.300df.fits - 5269. fs119.300dfs.fits imarith fs119.301df.fits - 5441. fs119.301dfs.fits imarith fs119.302df.fits - 5273. fs119.302dfs.fits imarith fs119.303df.fits - 5317. fs119.303dfs.fits 7) get coords and shifts shifts: 445.90 588.60 444.90 484.48 445.71 689.93 340.54 589.62 547.42 588.74 0. 0. 1. 104.12 0.19 -101.33 105.36 -1.02 -101.52 -0.14 coords: 445.90 588.60 146.36 541.45 687.55 901.60 767.40 176.58 -----> IRAS 3507+3801 <----- Round 1 1) Subtract dark imarith IRAS03507.102.fits - dark60.fits IRAS03507.102d.fits imarith IRAS03507.103.fits - dark60.fits IRAS03507.103d.fits imarith IRAS03507.104.fits - dark60.fits IRAS03507.104d.fits imarith IRAS03507.105.fits - dark60.fits IRAS03507.105d.fits imarith IRAS03507.106.fits - dark60.fits IRAS03507.106d.fits imarith IRAS03507.107.fits - dark60.fits IRAS03507.107d.fits imarith IRAS03507.108.fits - dark60.fits IRAS03507.108d.fits imarith IRAS03507.109.fits - dark60.fits IRAS03507.109d.fits imarith IRAS03507.110.fits - dark60.fits IRAS03507.110d.fits imstat IRAS03507.*d.fits >> awklist.txt 2) Scale images to same (mean = 13265.3 sky) value imarith IRAS03507.102d.fits * 1.00762 IRAS03507.102a.fits imarith IRAS03507.103d.fits * 0.998367 IRAS03507.103a.fits imarith IRAS03507.104d.fits * 0.997841 IRAS03507.104a.fits imarith IRAS03507.105d.fits * 0.994251 IRAS03507.105a.fits imarith IRAS03507.106d.fits * 0.99942 IRAS03507.106a.fits imarith IRAS03507.107d.fits * 1.00017 IRAS03507.107a.fits imarith IRAS03507.108d.fits * 0.997841 IRAS03507.108a.fits imarith IRAS03507.109d.fits * 1.00017 IRAS03507.109a.fits imarith IRAS03507.110d.fits * 1.00441 IRAS03507.110a.fits imstat IRAS03507*a.fits 3) Make skyflat (avg combine, min=0 max=2 reject) epar imcomb imcomb IRAS03507.*a.fits IRAS03507.sky.fits 4) Normalize by midpt imstat IRAS03507.sky.fits imarith IRAS03507.sky.fits / 13264. IRAS03507.skyN.fits 5) Divide by skyflat imarith IRAS03507.102d.fits / IRAS03507.skyN.fits IRAS03507.102df.fits imarith IRAS03507.103d.fits / IRAS03507.skyN.fits IRAS03507.103df.fits imarith IRAS03507.104d.fits / IRAS03507.skyN.fits IRAS03507.104df.fits imarith IRAS03507.105d.fits / IRAS03507.skyN.fits IRAS03507.105df.fits imarith IRAS03507.106d.fits / IRAS03507.skyN.fits IRAS03507.106df.fits imarith IRAS03507.107d.fits / IRAS03507.skyN.fits IRAS03507.107df.fits imarith IRAS03507.108d.fits / IRAS03507.skyN.fits IRAS03507.108df.fits imarith IRAS03507.109d.fits / IRAS03507.skyN.fits IRAS03507.109df.fits imarith IRAS03507.110d.fits / IRAS03507.skyN.fits IRAS03507.110df.fits 6) Subtract by constant (midpt) imstat IRAS03507.*df.fits imarith IRAS03507.102df.fits - 13188. IRAS03507.102dfs.fits imarith IRAS03507.103df.fits - 13314. IRAS03507.103dfs.fits imarith IRAS03507.104df.fits - 13316. IRAS03507.104dfs.fits imarith IRAS03507.105df.fits - 13364. IRAS03507.105dfs.fits imarith IRAS03507.106df.fits - 13295. IRAS03507.106dfs.fits imarith IRAS03507.107df.fits - 13283. IRAS03507.107dfs.fits imarith IRAS03507.108df.fits - 13322. IRAS03507.108dfs.fits imarith IRAS03507.109df.fits - 13285. IRAS03507.109dfs.fits imarith IRAS03507.110df.fits - 13228. IRAS03507.110dfs.fits Round 2 1) Subtract dark imarith IRAS03507.113.fits - dark60.fits IRAS03507.113d.fits imarith IRAS03507.114.fits - dark60.fits IRAS03507.114d.fits imarith IRAS03507.115.fits - dark60.fits IRAS03507.115d.fits imarith IRAS03507.116.fits - dark60.fits IRAS03507.116d.fits imarith IRAS03507.117.fits - dark60.fits IRAS03507.117d.fits imarith IRAS03507.118.fits - dark60.fits IRAS03507.118d.fits imarith IRAS03507.119.fits - dark60.fits IRAS03507.119d.fits imarith IRAS03507.120.fits - dark60.fits IRAS03507.120d.fits imarith IRAS03507.121.fits - dark60.fits IRAS03507.121d.fits imstat IRAS03507.*d.fits >> awklist.txt 2) Scale images to same (mean = 12994.4 sky) value imarith IRAS03507.113d.fits * 1.00545 IRAS03507.113a.fits imarith IRAS03507.114d.fits * 1.00912 IRAS03507.114a.fits imarith IRAS03507.115d.fits * 1.0063 IRAS03507.115a.fits imarith IRAS03507.116d.fits * 1.00623 IRAS03507.116a.fits imarith IRAS03507.117d.fits * 0.997191 IRAS03507.117a.fits imarith IRAS03507.118d.fits * 0.997498 IRAS03507.118a.fits imarith IRAS03507.119d.fits * 0.998264 IRAS03507.119a.fits imarith IRAS03507.120d.fits * 0.988769 IRAS03507.120a.fits imarith IRAS03507.121d.fits * 0.99156 IRAS03507.121a.fits imstat IRAS03507*a.fits 3) Make skyflat (avg combine, min=0 max=2 reject) epar imcomb imcomb IRAS03507.*a.fits IRAS03507.sky2.fits 4) Normalize by midpt imstat IRAS03507.sky2.fits imarith IRAS03507.sky2.fits / 13010. IRAS03507.sky2N.fits 5) Divide by skyflat imarith IRAS03507.113d.fits / IRAS03507.sky2N.fits IRAS03507.113df.fits imarith IRAS03507.114d.fits / IRAS03507.sky2N.fits IRAS03507.114df.fits imarith IRAS03507.115d.fits / IRAS03507.sky2N.fits IRAS03507.115df.fits imarith IRAS03507.116d.fits / IRAS03507.sky2N.fits IRAS03507.116df.fits imarith IRAS03507.117d.fits / IRAS03507.sky2N.fits IRAS03507.117df.fits imarith IRAS03507.118d.fits / IRAS03507.sky2N.fits IRAS03507.118df.fits imarith IRAS03507.119d.fits / IRAS03507.sky2N.fits IRAS03507.119df.fits imarith IRAS03507.120d.fits / IRAS03507.sky2N.fits IRAS03507.120df.fits imarith IRAS03507.121d.fits / IRAS03507.sky2N.fits IRAS03507.121df.fits 6) Subtract by constant (midpt) imstat IRAS03507.*df.fits imarith IRAS03507.113df.fits - 12966. IRAS03507.113dfs.fits imarith IRAS03507.114df.fits - 12920. IRAS03507.114dfs.fits imarith IRAS03507.115df.fits - 12955. IRAS03507.115dfs.fits imarith IRAS03507.116df.fits - 12954. IRAS03507.116dfs.fits imarith IRAS03507.117df.fits - 13069. IRAS03507.117dfs.fits imarith IRAS03507.118df.fits - 13066. IRAS03507.118dfs.fits imarith IRAS03507.119df.fits - 13059. IRAS03507.119dfs.fits imarith IRAS03507.120df.fits - 13186. IRAS03507.120dfs.fits imarith IRAS03507.121df.fits - 13146. IRAS03507.121dfs.fits Round 3 1) Subtract dark imarith IRAS03507.122.fits - dark60.fits IRAS03507.122d.fits imarith IRAS03507.123.fits - dark60.fits IRAS03507.123d.fits imarith IRAS03507.124.fits - dark60.fits IRAS03507.124d.fits imarith IRAS03507.125.fits - dark60.fits IRAS03507.125d.fits imarith IRAS03507.126.fits - dark60.fits IRAS03507.126d.fits imarith IRAS03507.127.fits - dark60.fits IRAS03507.127d.fits imarith IRAS03507.128.fits - dark60.fits IRAS03507.128d.fits imarith IRAS03507.129.fits - dark60.fits IRAS03507.129d.fits imarith IRAS03507.130.fits - dark60.fits IRAS03507.130d.fits imstat IRAS03507.*d.fits >> awklist.txt 2) Scale images to same (mean = 12754.9 sky) value imarith IRAS03507.122d.fits * 0.985086 IRAS03507.122a.fits imarith IRAS03507.123d.fits * 0.994224 IRAS03507.123a.fits imarith IRAS03507.124d.fits * 1.00424 IRAS03507.124a.fits imarith IRAS03507.125d.fits * 0.99314 IRAS03507.125a.fits imarith IRAS03507.126d.fits * 0.989365 IRAS03507.126a.fits imarith IRAS03507.127d.fits * 0.994767 IRAS03507.127a.fits imarith IRAS03507.128d.fits * 0.998974 IRAS03507.128a.fits imarith IRAS03507.129d.fits * 1.01511 IRAS03507.129a.fits imarith IRAS03507.130d.fits * 1.02647 IRAS03507.130a.fits imstat IRAS03507*a.fits 3) Make skyflat (avg combine, min=0 max=2 reject) epar imcomb imcomb IRAS03507.*a.fits IRAS03507.sky3.fits 4) Normalize by midpt imstat IRAS03507.sky3.fits imarith IRAS03507.sky3.fits / 12758. IRAS03507.sky3N.fits 5) Divide by skyflat imarith IRAS03507.122d.fits / IRAS03507.sky3N.fits IRAS03507.122df.fits imarith IRAS03507.123d.fits / IRAS03507.sky3N.fits IRAS03507.123df.fits imarith IRAS03507.124d.fits / IRAS03507.sky3N.fits IRAS03507.124df.fits imarith IRAS03507.125d.fits / IRAS03507.sky3N.fits IRAS03507.125df.fits imarith IRAS03507.126d.fits / IRAS03507.sky3N.fits IRAS03507.126df.fits imarith IRAS03507.127d.fits / IRAS03507.sky3N.fits IRAS03507.127df.fits imarith IRAS03507.128d.fits / IRAS03507.sky3N.fits IRAS03507.128df.fits imarith IRAS03507.129d.fits / IRAS03507.sky3N.fits IRAS03507.129df.fits imarith IRAS03507.130d.fits / IRAS03507.sky3N.fits IRAS03507.130df.fits 6) Subtract by constant (midpt) imstat IRAS03507.*df.fits imarith IRAS03507.122df.fits - 12973. IRAS03507.122dfs.fits imarith IRAS03507.123df.fits - 12859. IRAS03507.123dfs.fits imarith IRAS03507.124df.fits - 12727. IRAS03507.124dfs.fits imarith IRAS03507.125df.fits - 12871. IRAS03507.125dfs.fits imarith IRAS03507.126df.fits - 12923. IRAS03507.126dfs.fits imarith IRAS03507.127df.fits - 12848. IRAS03507.127dfs.fits imarith IRAS03507.128df.fits - 12798. IRAS03507.128dfs.fits imarith IRAS03507.129df.fits - 12593. IRAS03507.129dfs.fits imarith IRAS03507.130df.fits - 12454. IRAS03507.130dfs.fits