........ MAKEE: Keck Echelle Reduction Program ....... This is a HIRES2 raw FITS file. Use CCD mosaic location (CCDLOC) number is 2 (green) Read raw object file HI.20060118.24256.fits, write HI.20060118.24256_2.fits . Read raw star file HI.20060118.24256.fits, write HI.20060118.24256_2.fits . Read raw flat file HI.20060118.12269.fits, write HI.20060118.12269_2.fits . Read raw arc1 file HI.20060118.14792.fits, write HI.20060118.14792_2.fits . ... MAKEE: Keck HIRES2 (Mosaic 2004) Reduction .......... Mon Feb 11 17:27:11 2008 MAKEE VERSION= 5.2.2 : February 2008 NOTE: CDDGAIN is set to low NOTE: Try to read e-/DN file: /users/tab/makee///eperdnHIRES2_logain.dat NOTE: Using default e-/DN value: 2.2000 NOTE: Using instrument default readout noise value. WARNING: Cannot find mask file: WARNING: Not using bad column masking. WARNING: No default bias file exists for HIRES2. OBJECT: -0.0395 -0.0740 B5 1 713 1 4096 HI.20060118.24256_2.fits STAR: -0.0395 -0.0740 B5 1 713 1 4096 HI.20060118.24256_2.fits FLAT: -0.0395 -0.0760 C1 1 713 1 4096 HI.20060118.12269_2.fits ARC: -0.0395 -0.0760 B5 1 713 1 4096 HI.20060118.14792_2.fits Setting EPERDN = 2.2000 Setting RONOISE = 2.9000 Column binning= 3 Row binning= 1 NOTE: Flip binning for ASPP_ cards. Lamp= none Lamp Filter= ng3 Shutter= open B5 Frame#= 2336 : ECHANGL= -0.0395 XDANGL= -0.0740 () 2324.4+5751 Expos= 500s Object=object Object to extract: object 2322+5734 06/01/18 06:44:17 2336 500s none ng3 kv370 -0.0395 -0.0740 B5 10.21 open open re 3x1 HI.20060118.24256_2.fits Mode= 1 Extract all orders. Masking file: Bias file: WARNING: makee: Using zero bias image. ............ Reading flat : HI.20060118.12269_2.fits Setting EPERDN = 2.2000 Setting RONOISE = 2.9000 Column binning= 3 Row binning= 1 NOTE: Flip binning for ASPP_ cards. Lamp= quartz1 Lamp Filter= ng3 Shutter= open C1 Frame#= 2303 : ECHANGL= -0.0395 XDANGL= -0.0760 (HI.20060118.12269_2.fits) 1520.0+4500 Expos= 2s Object=flatlamp What is this EPOCH? : 0 Calling biw() subroutine. NOTE: biw: X binning: 3 Y binning: 1 Subtracting baseline from image ( 701 --> 713 ) NOTE: No maskfile, no bad column interpolation. NOTE: HIRES2 CCD is number 2 Clip image (sc,ec,sr,er): 7 686 1 4056 Rotating ESI or HIRES2 image by 90 degrees... Flipping ESI or HIRES2 image in columns... Flipping HIRES2 image in rows... NOTE: New binning in header: 1, 3 Prepix: 0 Postpix: 80 Original Window: cols= 1 687 rows= 1 4096 New Clipped Window: cols= 0 4055 rows= 0 679 ............ Estimate slit length from flat field... Estimate for slit length (px) = 20.900 NOTE: Estimate HIRES2 arcsec/pixel at 0.120 . NOTE: decker=C1 , swas= 7.00, ybin= 3, swpx= 19.54 Slit length lookup (px) = 19.542 NOTE: Estimate HIRES2 arcsec/pixel at 0.120 . NOTE: decker=B5 , swas= 3.50, ybin= 3, swpx= 9.77 Object header slit lookup (px) = 9.771 WARNING: Object header slit length appears different. WARNING: Use two different slit lengths (in pixels): Global_sw_flat= 20.900 Global_sw = 9.771 Global_sw_adj = 4.886 Saving flat image... junk-flat_1202779631002336001.fits ............ Reading star : HI.20060118.24256_2.fits Setting EPERDN = 2.2000 Setting RONOISE = 2.9000 Column binning= 3 Row binning= 1 NOTE: Flip binning for ASPP_ cards. Lamp= none Lamp Filter= ng3 Shutter= open B5 Frame#= 2336 : ECHANGL= -0.0395 XDANGL= -0.0740 (HI.20060118.24256_2.fits) 2324.4+5751 Expos= 500s Object=object NOTE: Not interpolating or masking bad columns on trace star image. Calling biw() subroutine. NOTE: biw: X binning: 3 Y binning: 1 Subtracting baseline from image ( 701 --> 713 ) NOTE: No maskfile, no bad column interpolation. NOTE: HIRES2 CCD is number 2 Clip image (sc,ec,sr,er): 7 686 1 4056 Rotating ESI or HIRES2 image by 90 degrees... Flipping ESI or HIRES2 image in columns... Flipping HIRES2 image in rows... NOTE: New binning in header: 1, 3 Prepix: 0 Postpix: 80 Original Window: cols= 1 687 rows= 1 4096 New Clipped Window: cols= 0 4055 rows= 0 679 Finding and fitting order traces... Trace:1: Right side (col= 3040) Writing PostScript plot file: right_trace-2336_2.ps Writing trace data file: right_trace-2336_2.dat EETO: EON= 1 High= 0.368 WRMS= 0.103 NRej= 10 CRow= 12.1 npt=3052 EETO: EON= 2 High= 0.369 WRMS= 0.099 NRej= 11 CRow= 43.0 npt=3995 EETO: EON= 3 High= 0.365 WRMS= 0.095 NRej= 3 CRow= 74.7 npt=3995 EETO: EON= 4 High= 0.373 WRMS= 0.096 NRej= 2 CRow= 107.4 npt=3995 EETO: EON= 5 High= 0.312 WRMS= 0.088 NRej= 5 CRow= 141.0 npt=3995 EETO: EON= 6 High= 0.303 WRMS= 0.082 NRej= 2 CRow= 175.5 npt=3995 EETO: EON= 7 High= 0.272 WRMS= 0.078 NRej= 0 CRow= 211.0 npt=3995 EETO: EON= 8 High= 0.264 WRMS= 0.079 NRej= 15 CRow= 247.6 npt=3995 EETO: EON= 9 High= 0.286 WRMS= 0.075 NRej= 4 CRow= 285.2 npt=3995 EETO: EON= 10 High= 0.270 WRMS= 0.073 NRej= 4 CRow= 324.1 npt=3995 EETO: EON= 11 High= 0.278 WRMS= 0.071 NRej= 7 CRow= 364.1 npt=3995 EETO: EON= 12 High= 0.265 WRMS= 0.071 NRej= 11 CRow= 405.5 npt=3995 EETO: EON= 13 High= 0.281 WRMS= 0.071 NRej= 14 CRow= 448.2 npt=3995 EETO: EON= 14 High= 0.264 WRMS= 0.067 NRej= 6 CRow= 492.3 npt=3995 EETO: EON= 15 High= 0.238 WRMS= 0.065 NRej= 3 CRow= 537.9 npt=3995 EETO: EON= 16 High= 0.239 WRMS= 0.069 NRej= 5 CRow= 585.1 npt=3995 EETO: EON= 17 High= 0.230 WRMS= 0.063 NRej= 2 CRow= 634.1 npt=3995 Trace: Left side (col= 1014) Writing PostScript plot file: left_trace-2336_2.ps Writing trace data file: left_trace-2336_2.dat EETO: EON= 1 High= 0.378 WRMS= 0.104 NRej= 10 CRow= 12.0 npt=3045 EETO: EON= 2 High= 0.395 WRMS= 0.101 NRej= 9 CRow= 43.0 npt=3995 EETO: EON= 3 High= 0.359 WRMS= 0.095 NRej= 4 CRow= 74.7 npt=3995 EETO: EON= 4 High= 0.373 WRMS= 0.097 NRej= 2 CRow= 107.4 npt=3995 EETO: EON= 5 High= 0.310 WRMS= 0.088 NRej= 5 CRow= 141.0 npt=3995 EETO: EON= 6 High= 0.304 WRMS= 0.082 NRej= 4 CRow= 175.5 npt=3995 EETO: EON= 7 High= 0.273 WRMS= 0.078 NRej= 0 CRow= 211.0 npt=3995 EETO: EON= 8 High= 0.248 WRMS= 0.078 NRej= 15 CRow= 247.6 npt=3995 EETO: EON= 9 High= 0.301 WRMS= 0.075 NRej= 3 CRow= 285.2 npt=3995 EETO: EON= 10 High= 0.270 WRMS= 0.073 NRej= 2 CRow= 324.1 npt=3995 EETO: EON= 11 High= 0.278 WRMS= 0.070 NRej= 7 CRow= 364.1 npt=3995 EETO: EON= 12 High= 0.266 WRMS= 0.071 NRej= 11 CRow= 405.5 npt=3995 EETO: EON= 13 High= 0.281 WRMS= 0.071 NRej= 14 CRow= 448.2 npt=3995 EETO: EON= 14 High= 0.264 WRMS= 0.067 NRej= 7 CRow= 492.3 npt=3995 EETO: EON= 15 High= 0.238 WRMS= 0.065 NRej= 3 CRow= 537.9 npt=3995 EETO: EON= 16 High= 0.243 WRMS= 0.069 NRej= 4 CRow= 585.1 npt=3995 EETO: EON= 17 High= 0.230 WRMS= 0.063 NRej= 2 CRow= 634.1 npt=3995 NOTE: EE_TraceOrders: Partial echelle order found. No. of col.= 1397 EE_TraceOrders: Decrease polynomial order to <=3. EETO: EON= 18 High= 0.228 WRMS= 0.062 NRej= 3 CRow= 684.7 npt=1397 Both traces look OK. Save plot for right trace. Save table for right trace. Number of echelle orders = 18 Recovering flat image... junk-flat_1202779631002336001.fits Estimating background limits... NOTE: Apply object vs. flat slit adjustment of 4.886 NOTE: Background between widely separated orders: 3.2860E+02 (Global_sw_flat= 2.090E+01). NOTE: EEFB: EON= 1 Slit Edge Lower= 10.2 Upper= -8.7 Width= 18.9 NOTE: EEFB: EON= 2 Slit Edge Lower= 10.2 Upper= -8.8 Width= 19.0 NOTE: EEFB: EON= 3 Slit Edge Lower= 10.0 Upper= -8.9 Width= 18.9 NOTE: EEFB: EON= 4 Slit Edge Lower= 9.9 Upper= -9.1 Width= 19.0 NOTE: EEFB: EON= 5 Slit Edge Lower= 9.7 Upper= -9.2 Width= 18.9 NOTE: EEFB: EON= 6 Slit Edge Lower= 9.5 Upper= -9.4 Width= 18.9 NOTE: EEFB: EON= 7 Slit Edge Lower= 9.4 Upper= -9.5 Width= 18.9 NOTE: EEFB: EON= 8 Slit Edge Lower= 9.2 Upper= -9.6 Width= 18.8 NOTE: EEFB: EON= 9 Slit Edge Lower= 9.1 Upper= -9.8 Width= 18.9 NOTE: EEFB: EON= 10 Slit Edge Lower= 8.9 Upper= -9.9 Width= 18.8 NOTE: EEFB: EON= 11 Slit Edge Lower= 8.8 Upper= -10.1 Width= 18.9 NOTE: EEFB: EON= 12 Slit Edge Lower= 8.7 Upper= -10.2 Width= 18.9 NOTE: EEFB: EON= 13 Slit Edge Lower= 8.5 Upper= -10.3 Width= 18.8 NOTE: EEFB: EON= 14 Slit Edge Lower= 8.4 Upper= -10.5 Width= 18.9 NOTE: EEFB: EON= 15 Slit Edge Lower= 8.3 Upper= -10.6 Width= 18.9 NOTE: EEFB: EON= 16 Slit Edge Lower= 8.1 Upper= -10.7 Width= 18.8 NOTE: EEFB: EON= 17 Slit Edge Lower= 8.0 Upper= -10.9 Width= 18.9 NOTE: EEFB: EON= 18 Slit Edge Lower= 7.8 Upper= -11.0 Width= 18.8 EEFB: Fitting background lower offsets. EEFB: Fitting background upper offsets. NOTE: Applying object vs. flat slit adjustment of 4.886 NOTE: Deleting order number 18 (too small) [usable columns= -2] Flat field scale factor= 1.404906E+04 Saving flat image... junk-flat_1202779631002336001.fits ............ Reading object : HI.20060118.24256_2.fits Setting EPERDN = 2.2000 Setting RONOISE = 2.9000 Column binning= 3 Row binning= 1 NOTE: Flip binning for ASPP_ cards. Lamp= none Lamp Filter= ng3 Shutter= open B5 Frame#= 2336 : ECHANGL= -0.0395 XDANGL= -0.0740 (HI.20060118.24256_2.fits) 2324.4+5751 Expos= 500s Object=object Calling biw() subroutine. NOTE: biw: X binning: 3 Y binning: 1 Subtracting baseline from image ( 701 --> 713 ) NOTE: No maskfile, no bad column interpolation. NOTE: HIRES2 CCD is number 2 Clip image (sc,ec,sr,er): 7 686 1 4056 Rotating ESI or HIRES2 image by 90 degrees... Flipping ESI or HIRES2 image in columns... Flipping HIRES2 image in rows... NOTE: New binning in header: 1, 3 Prepix: 0 Postpix: 80 Original Window: cols= 1 687 rows= 1 4096 New Clipped Window: cols= 0 4055 rows= 0 679 Setting EPERDN = 2.2000 Setting RONOISE = 2.9000 Column binning= 1 Row binning= 3 Lamp= none Lamp Filter= ng3 Shutter= open B5 Frame#= 2336 : ECHANGL= -0.0395 XDANGL= -0.0740 (HI.20060118.24256_2.fits) 2324.4+5751 Expos= 500s Object=object Observation number= 2336 UT date = 18Jan06 NOTE: Object x,y binning is 1 x 3 . Recovering flat image... junk-flat_1202779631002336001.fits Dividing object by flat field... Determine object profile and boundaries... Writing FITS profile file: profiles-2336_2.fits Writing PostScript plot file: profiles-2336_2.ps pse_mode= 1 slit width, neo, eperdn, ronoise, pse_mode = 9.77 17 2.200 2.900 1 ****************************** Extracting echelle order number 1 of 17 Cosmic Ray Fraction: expected= 0.00156 actual= 0.04654 This is a factor of 29.9 larger than expected. Repeating and increasing PSEMRA to 1.500000E+00 Cosmic Ray Fraction: expected= 0.00156 actual= 0.00347 Sky Pixels Masked (primary,adjacent,additional): 10 10 4371 PSE_SkyFit: NOTE: Found column (1167) with too few pixels ( 1) [use sky from previous column]. PSE_SkyFit: NOTE: Found column (3673) with too few pixels ( 1) [use sky from previous column]. 2105 columns affected by nearby night sky lines during SkyFit. Sky areas ratio: 0.366. Sky polynomial order: 0. Rejecting 51 out of 516 points in profile fit# 26 NOTE: PSE_ObjMask: Maximum rejections in profile fit# 26 Rejecting 56 out of 565 points in profile fit# 27 NOTE: PSE_ObjMask: Maximum rejections in profile fit# 27 Rejecting 32 out of 320 points in profile fit# 28 NOTE: PSE_ObjMask: Maximum rejections in profile fit# 28 Rejecting 40 out of 536 points in profile fit# 29 Rejecting 51 out of 516 points in profile fit# 31 NOTE: PSE_ObjMask: Maximum rejections in profile fit# 31 Object Pixels Masked (high,low): 10 0 PSE_ObjSum: Had to deal with 1892 masked pixels. ****************************** Extracting echelle order number 2 of 17 Cosmic Ray Fraction: expected= 0.00156 actual= 0.06797 This is a factor of 43.7 larger than expected. Repeating and increasing PSEMRA to 1.500000E+00 Cosmic Ray Fraction: expected= 0.00156 actual= 0.00680 Sky Pixels Masked (primary,adjacent,additional): 14 13 5452 PSE_SkyFit: NOTE: Found column ( 47) with too few pixels ( 1) [use sky from previous column]. PSE_SkyFit: NOTE: Found column (3971) with too few pixels ( 1) [use sky from previous column]. 2987 columns affected by nearby night sky lines during SkyFit. Sky areas ratio: 0.406. Sky polynomial order: 0. Rejecting 77 out of 773 points in profile fit# 26 NOTE: PSE_ObjMask: Maximum rejections in profile fit# 26 Rejecting 41 out of 418 points in profile fit# 27 NOTE: PSE_ObjMask: Maximum rejections in profile fit# 27 Rejecting 53 out of 531 points in profile fit# 28 NOTE: PSE_ObjMask: Maximum rejections in profile fit# 28 Rejecting 77 out of 773 points in profile fit# 31 NOTE: PSE_ObjMask: Maximum rejections in profile fit# 31 Object Pixels Masked (high,low): 23 0 PSE_ObjSum: Had to deal with 2430 masked pixels. ****************************** Extracting echelle order number 3 of 17 Cosmic Ray Fraction: expected= 0.00156 actual= 0.05567 This is a factor of 35.8 larger than expected. Repeating and increasing PSEMRA to 1.500000E+00 Cosmic Ray Fraction: expected= 0.00156 actual= 0.00565 Sky Pixels Masked (primary,adjacent,additional): 12 11 4449 PSE_SkyFit: NOTE: Found column ( 186) with too few pixels ( 1) [use sky from previous column]. PSE_SkyFit: NOTE: Found column (3855) with too few pixels ( 1) [use sky from previous column]. PSE_SkyFit: NOTE: Found column (3857) with too few pixels ( 1) [use sky from previous column]. 3105 columns affected by nearby night sky lines during SkyFit. Sky areas ratio: 0.457. Sky polynomial order: 0. Rejecting 67 out of 672 points in profile fit# 26 NOTE: PSE_ObjMask: Maximum rejections in profile fit# 26 Rejecting 39 out of 394 points in profile fit# 27 NOTE: PSE_ObjMask: Maximum rejections in profile fit# 27 Rejecting 55 out of 672 points in profile fit# 31 Object Pixels Masked (high,low): 10 0 PSE_ObjSum: Had to deal with 1747 masked pixels. ****************************** Extracting echelle order number 4 of 17 Cosmic Ray Fraction: expected= 0.00156 actual= 0.09978 This is a factor of 64.1 larger than expected. Repeating and increasing PSEMRA to 1.500000E+00 Cosmic Ray Fraction: expected= 0.00156 actual= 0.01559 This is a factor of 10.0 larger than expected. Repeating and increasing PSEMRA to 2.250000E+00 Cosmic Ray Fraction: expected= 0.00156 actual= 0.00025 NOTE: Skip additional sky masking if PSEMRA > 2.0. Sky Pixels Masked (primary,adjacent,additional): 2 2 -1 3207 columns affected by nearby night sky lines during SkyFit. Sky areas ratio: 0.523. Sky polynomial order: 1. Object Pixels Masked (high,low): 12 0 PSE_ObjSum: Had to deal with 12 masked pixels. ****************************** Extracting echelle order number 5 of 17 Cosmic Ray Fraction: expected= 0.00156 actual= 0.12744 This is a factor of 81.9 larger than expected. Repeating and increasing PSEMRA to 1.500000E+00 Cosmic Ray Fraction: expected= 0.00156 actual= 0.02519 This is a factor of 16.2 larger than expected. Repeating and increasing PSEMRA to 2.250000E+00 Cosmic Ray Fraction: expected= 0.00156 actual= 0.00070 NOTE: Skip additional sky masking if PSEMRA > 2.0. Sky Pixels Masked (primary,adjacent,additional): 5 2 -1 PSE_SkyFit: NOTE: Found column (1402) with too few pixels ( 1) [use sky from previous column]. PSE_SkyFit: NOTE: Found column (2287) with too few pixels ( 1) [use sky from previous column]. 3124 columns affected by nearby night sky lines during SkyFit. Sky areas ratio: 0.611. Sky polynomial order: 1. Object Pixels Masked (high,low): 10 0 PSE_ObjSum: Had to deal with 13 masked pixels. ****************************** Extracting echelle order number 6 of 17 Cosmic Ray Fraction: expected= 0.00156 actual= 0.18319 This is a factor of 117.8 larger than expected. Repeating and increasing PSEMRA to 1.500000E+00 Cosmic Ray Fraction: expected= 0.00156 actual= 0.04061 This is a factor of 26.1 larger than expected. Repeating and increasing PSEMRA to 2.250000E+00 Cosmic Ray Fraction: expected= 0.00156 actual= 0.00175 NOTE: Skip additional sky masking if PSEMRA > 2.0. Sky Pixels Masked (primary,adjacent,additional): 4 7 -1 PSE_SkyFit: NOTE: Found column (2513) with too few pixels ( 1) [use sky from previous column]. PSE_SkyFit: NOTE: Found column (2514) with too few pixels ( 1) [use sky from previous column]. 3195 columns affected by nearby night sky lines during SkyFit. Sky areas ratio: 0.741. Sky polynomial order: 1. Object Pixels Masked (high,low): 9 0 PSE_ObjSum: Had to deal with 16 masked pixels. ****************************** Extracting echelle order number 7 of 17 Cosmic Ray Fraction: expected= 0.00156 actual= 0.28596 This is a factor of 183.8 larger than expected. Repeating and increasing PSEMRA to 1.500000E+00 Cosmic Ray Fraction: expected= 0.00156 actual= 0.12499 This is a factor of 80.3 larger than expected. Repeating and increasing PSEMRA to 2.250000E+00 Cosmic Ray Fraction: expected= 0.00156 actual= 0.02239 This is a factor of 14.4 larger than expected. Repeating and increasing PSEMRA to 3.375000E+00 Cosmic Ray Fraction: expected= 0.00156 actual= 0.00084 NOTE: Skip additional sky masking if PSEMRA > 2.0. Sky Pixels Masked (primary,adjacent,additional): 6 5 -1 PSE_SkyFit: NOTE: Found column (3274) with too few pixels ( 1) [use sky from previous column]. 3179 columns affected by nearby night sky lines during SkyFit. Sky areas ratio: 1.171. Sky polynomial order: 1. Object Pixels Masked (high,low): 0 0 ****************************** Extracting echelle order number 8 of 17 Cosmic Ray Fraction: expected= 0.00156 actual= 0.33253 This is a factor of 213.8 larger than expected. Repeating and increasing PSEMRA to 1.500000E+00 Cosmic Ray Fraction: expected= 0.00156 actual= 0.16323 This is a factor of 104.9 larger than expected. Repeating and increasing PSEMRA to 2.250000E+00 Cosmic Ray Fraction: expected= 0.00156 actual= 0.03724 This is a factor of 23.9 larger than expected. Repeating and increasing PSEMRA to 3.375000E+00 Cosmic Ray Fraction: expected= 0.00156 actual= 0.00036 NOTE: Skip additional sky masking if PSEMRA > 2.0. Sky Pixels Masked (primary,adjacent,additional): 5 0 -1 PSE_SkyFit: NOTE: Found column ( 960) with too few pixels ( 1) [use sky from previous column]. PSE_SkyFit: NOTE: Found column ( 961) with too few pixels ( 1) [use sky from previous column]. 3327 columns affected by nearby night sky lines during SkyFit. Sky areas ratio: 1.527. Sky polynomial order: 1. Object Pixels Masked (high,low): 8 0 PSE_ObjSum: Had to deal with 12 masked pixels. ****************************** Extracting echelle order number 9 of 17 Cosmic Ray Fraction: expected= 0.00156 actual= 0.32393 This is a factor of 208.2 larger than expected. Repeating and increasing PSEMRA to 1.500000E+00 Cosmic Ray Fraction: expected= 0.00156 actual= 0.19862 This is a factor of 127.7 larger than expected. Repeating and increasing PSEMRA to 2.250000E+00 Cosmic Ray Fraction: expected= 0.00156 actual= 0.05285 This is a factor of 34.0 larger than expected. Repeating and increasing PSEMRA to 3.375000E+00 Cosmic Ray Fraction: expected= 0.00156 actual= 0.00290 NOTE: Skip additional sky masking if PSEMRA > 2.0. Sky Pixels Masked (primary,adjacent,additional): 34 4 -1 PSE_SkyFit: NOTE: Found column (2414) with too few pixels ( 1) [use sky from previous column]. 3313 columns affected by nearby night sky lines during SkyFit. Sky areas ratio: 1.788. Sky polynomial order: 1. Object Pixels Masked (high,low): 4 0 PSE_ObjSum: Had to deal with 36 masked pixels. ****************************** Extracting echelle order number 10 of 17 Cosmic Ray Fraction: expected= 0.00156 actual= 0.31417 This is a factor of 202.0 larger than expected. Repeating and increasing PSEMRA to 1.500000E+00 Cosmic Ray Fraction: expected= 0.00156 actual= 0.20724 This is a factor of 133.2 larger than expected. Repeating and increasing PSEMRA to 2.250000E+00 Cosmic Ray Fraction: expected= 0.00156 actual= 0.06631 This is a factor of 42.6 larger than expected. Repeating and increasing PSEMRA to 3.375000E+00 Cosmic Ray Fraction: expected= 0.00156 actual= 0.00367 NOTE: Skip additional sky masking if PSEMRA > 2.0. Sky Pixels Masked (primary,adjacent,additional): 69 1 -1 2937 columns affected by nearby night sky lines during SkyFit. Sky areas ratio: 2.047. Sky polynomial order: 0. Object Pixels Masked (high,low): 12 0 PSE_ObjSum: Had to deal with 82 masked pixels. ****************************** Extracting echelle order number 11 of 17 Cosmic Ray Fraction: expected= 0.00156 actual= 0.36583 This is a factor of 235.2 larger than expected. Repeating and increasing PSEMRA to 1.500000E+00 Cosmic Ray Fraction: expected= 0.00156 actual= 0.22583 This is a factor of 145.2 larger than expected. Repeating and increasing PSEMRA to 2.250000E+00 Cosmic Ray Fraction: expected= 0.00156 actual= 0.06910 This is a factor of 44.4 larger than expected. Repeating and increasing PSEMRA to 3.375000E+00 Cosmic Ray Fraction: expected= 0.00156 actual= 0.00164 NOTE: Skip additional sky masking if PSEMRA > 2.0. Sky Pixels Masked (primary,adjacent,additional): 147 7 -1 2888 columns affected by nearby night sky lines during SkyFit. Sky areas ratio: 2.304. Sky polynomial order: 0. Object Pixels Masked (high,low): 26 0 PSE_ObjSum: Had to deal with 168 masked pixels. ****************************** Extracting echelle order number 12 of 17 Cosmic Ray Fraction: expected= 0.00156 actual= 0.32825 This is a factor of 211.0 larger than expected. Repeating and increasing PSEMRA to 1.500000E+00 Cosmic Ray Fraction: expected= 0.00156 actual= 0.18226 This is a factor of 117.2 larger than expected. Repeating and increasing PSEMRA to 2.250000E+00 Cosmic Ray Fraction: expected= 0.00156 actual= 0.03875 This is a factor of 24.9 larger than expected. Repeating and increasing PSEMRA to 3.375000E+00 Cosmic Ray Fraction: expected= 0.00156 actual= 0.00030 NOTE: Skip additional sky masking if PSEMRA > 2.0. Sky Pixels Masked (primary,adjacent,additional): 3 4 -1 2606 columns affected by nearby night sky lines during SkyFit. Sky areas ratio: 2.559. Sky polynomial order: 0. Object Pixels Masked (high,low): 23 0 PSE_ObjSum: Had to deal with 23 masked pixels. ****************************** Extracting echelle order number 13 of 17 Cosmic Ray Fraction: expected= 0.00156 actual= 0.29672 This is a factor of 190.7 larger than expected. Repeating and increasing PSEMRA to 1.500000E+00 Cosmic Ray Fraction: expected= 0.00156 actual= 0.13724 This is a factor of 88.2 larger than expected. Repeating and increasing PSEMRA to 2.250000E+00 Cosmic Ray Fraction: expected= 0.00156 actual= 0.01775 This is a factor of 11.4 larger than expected. Repeating and increasing PSEMRA to 3.375000E+00 Cosmic Ray Fraction: expected= 0.00156 actual= 0.00109 NOTE: Skip additional sky masking if PSEMRA > 2.0. Sky Pixels Masked (primary,adjacent,additional): 22 20 -1 PSE_SkyFit: NOTE: Found column (1518) with too few pixels ( 1) [use sky from previous column]. PSE_SkyFit: NOTE: Found column (1521) with too few pixels ( 1) [use sky from previous column]. PSE_SkyFit: NOTE: Found column (1522) with too few pixels ( 1) [use sky from previous column]. 2552 columns affected by nearby night sky lines during SkyFit. Sky areas ratio: 2.810. Sky polynomial order: 0. Object Pixels Masked (high,low): 43 20 PSE_ObjSum: Had to deal with 92 masked pixels. ****************************** Extracting echelle order number 14 of 17 Cosmic Ray Fraction: expected= 0.00156 actual= 0.33907 This is a factor of 218.0 larger than expected. Repeating and increasing PSEMRA to 1.500000E+00 Cosmic Ray Fraction: expected= 0.00156 actual= 0.17247 This is a factor of 110.9 larger than expected. Repeating and increasing PSEMRA to 2.250000E+00 Cosmic Ray Fraction: expected= 0.00156 actual= 0.03504 This is a factor of 22.5 larger than expected. Repeating and increasing PSEMRA to 3.375000E+00 Cosmic Ray Fraction: expected= 0.00156 actual= 0.00035 NOTE: Skip additional sky masking if PSEMRA > 2.0. Sky Pixels Masked (primary,adjacent,additional): 11 0 -1 2177 columns affected by nearby night sky lines during SkyFit. Sky areas ratio: 3.057. Sky polynomial order: 0. Object Pixels Masked (high,low): 27 0 PSE_ObjSum: Had to deal with 33 masked pixels. ****************************** Extracting echelle order number 15 of 17 Cosmic Ray Fraction: expected= 0.00156 actual= 0.32364 This is a factor of 208.1 larger than expected. Repeating and increasing PSEMRA to 1.500000E+00 Cosmic Ray Fraction: expected= 0.00156 actual= 0.15834 This is a factor of 101.8 larger than expected. Repeating and increasing PSEMRA to 2.250000E+00 Cosmic Ray Fraction: expected= 0.00156 actual= 0.04630 This is a factor of 29.8 larger than expected. Repeating and increasing PSEMRA to 3.375000E+00 Cosmic Ray Fraction: expected= 0.00156 actual= 0.00297 NOTE: Skip additional sky masking if PSEMRA > 2.0. Sky Pixels Masked (primary,adjacent,additional): 154 32 -1 PSE_SkyFit: NOTE: Found column ( 67) with too few pixels ( 1) [use sky from previous column]. PSE_SkyFit: NOTE: Found column (1670) with too few pixels ( 1) [use sky from previous column]. PSE_SkyFit: NOTE: Found column (1671) with too few pixels ( 1) [use sky from previous column]. PSE_SkyFit: NOTE: Found column (3339) with too few pixels ( 1) [use sky from previous column]. 2242 columns affected by nearby night sky lines during SkyFit. Sky areas ratio: 3.299. Sky polynomial order: 0. Object Pixels Masked (high,low): 6 0 PSE_ObjSum: Had to deal with 100 masked pixels. ****************************** Extracting echelle order number 16 of 17 Cosmic Ray Fraction: expected= 0.00156 actual= 0.34159 This is a factor of 219.6 larger than expected. Repeating and increasing PSEMRA to 1.500000E+00 Cosmic Ray Fraction: expected= 0.00156 actual= 0.18057 This is a factor of 116.1 larger than expected. Repeating and increasing PSEMRA to 2.250000E+00 Cosmic Ray Fraction: expected= 0.00156 actual= 0.05923 This is a factor of 38.1 larger than expected. Repeating and increasing PSEMRA to 3.375000E+00 Cosmic Ray Fraction: expected= 0.00156 actual= 0.00288 NOTE: Skip additional sky masking if PSEMRA > 2.0. Sky Pixels Masked (primary,adjacent,additional): 120 0 -1 PSE_SkyFit: NOTE: Found column (2325) with too few pixels ( 1) [use sky from previous column]. 2910 columns affected by nearby night sky lines during SkyFit. Sky areas ratio: 3.536. Sky polynomial order: 0. Rejecting 48 out of 807 points in profile fit# 1 Object Pixels Masked (high,low): 30 0 PSE_ObjSum: Had to deal with 94 masked pixels. ****************************** Extracting echelle order number 17 of 17 Cosmic Ray Fraction: expected= 0.00156 actual= 0.40682 This is a factor of 261.5 larger than expected. Repeating and increasing PSEMRA to 1.500000E+00 Cosmic Ray Fraction: expected= 0.00156 actual= 0.26912 This is a factor of 173.0 larger than expected. Repeating and increasing PSEMRA to 2.250000E+00 Cosmic Ray Fraction: expected= 0.00156 actual= 0.12055 This is a factor of 77.5 larger than expected. Repeating and increasing PSEMRA to 3.375000E+00 Cosmic Ray Fraction: expected= 0.00156 actual= 0.01785 This is a factor of 11.5 larger than expected. Repeating and increasing PSEMRA to 5.062500E+00 Cosmic Ray Fraction: expected= 0.00156 actual= 0.00076 NOTE: Skip additional sky masking if PSEMRA > 2.0. Sky Pixels Masked (primary,adjacent,additional): 14 10 -1 PSE_SkyFit: NOTE: Found column ( 890) with too few pixels ( 1) [use sky from previous column]. PSE_SkyFit: NOTE: Found column ( 892) with too few pixels ( 1) [use sky from previous column]. 2695 columns affected by nearby night sky lines during SkyFit. Sky areas ratio: 3.766. Sky polynomial order: 0. Object Pixels Masked (high,low): 2 0 PSE_ObjSum: Had to deal with 19 masked pixels. Writing : Flux-2336_2.fits Writing : Var-2336_2.fits Writing : Sky-2336_2.fits Writing : Sum-2336_2.fits Mon Feb 11 17:27:38 2008 ..... Extracting Flat Field Spectrum ........... ............ Reading object : HI.20060118.12269_2.fits Setting EPERDN = 2.2000 Setting RONOISE = 2.9000 Column binning= 3 Row binning= 1 NOTE: Flip binning for ASPP_ cards. Lamp= quartz1 Lamp Filter= ng3 Shutter= open C1 Frame#= 2303 : ECHANGL= -0.0395 XDANGL= -0.0760 (HI.20060118.12269_2.fits) 1520.0+4500 Expos= 2s Object=flatlamp What is this EPOCH? : 0 Calling biw() subroutine. NOTE: biw: X binning: 3 Y binning: 1 Subtracting baseline from image ( 701 --> 713 ) NOTE: No maskfile, no bad column interpolation. NOTE: HIRES2 CCD is number 2 Clip image (sc,ec,sr,er): 7 686 1 4056 Rotating ESI or HIRES2 image by 90 degrees... Flipping ESI or HIRES2 image in columns... Flipping HIRES2 image in rows... NOTE: New binning in header: 1, 3 Prepix: 0 Postpix: 80 Original Window: cols= 1 687 rows= 1 4096 New Clipped Window: cols= 0 4055 rows= 0 679 Setting EPERDN = 2.2000 Setting RONOISE = 2.9000 Column binning= 1 Row binning= 3 Lamp= quartz1 Lamp Filter= ng3 Shutter= open C1 Frame#= 2303 : ECHANGL= -0.0395 XDANGL= -0.0760 (HI.20060118.12269_2.fits) 1520.0+4500 Expos= 2s Object=flatlamp What is this EPOCH? : 0 Observation number= 2303 UT date = 18Jan06 NOTE: Object x,y binning is 1 x 3 . Recovering flat image... junk-flat_1202779631002336001.fits Dividing object by flat field... pse_mode= 4 slit width, neo, eperdn, ronoise, pse_mode = 9.77 17 2.200 2.900 4 Extracting whole slit spectrum... ****************************** Extracting echelle order number 1 of 17 ****************************** Extracting echelle order number 2 of 17 ****************************** Extracting echelle order number 3 of 17 ****************************** Extracting echelle order number 4 of 17 ****************************** Extracting echelle order number 5 of 17 ****************************** Extracting echelle order number 6 of 17 ****************************** Extracting echelle order number 7 of 17 ****************************** Extracting echelle order number 8 of 17 ****************************** Extracting echelle order number 9 of 17 ****************************** Extracting echelle order number 10 of 17 ****************************** Extracting echelle order number 11 of 17 ****************************** Extracting echelle order number 12 of 17 ****************************** Extracting echelle order number 13 of 17 ****************************** Extracting echelle order number 14 of 17 ****************************** Extracting echelle order number 15 of 17 ****************************** Extracting echelle order number 16 of 17 ****************************** Extracting echelle order number 17 of 17 Writing : Flat-2336_2.fits Mon Feb 11 17:27:38 2008 ..... Extracting Arc Lamp Spectrum ........... ............ Reading object : HI.20060118.14792_2.fits Setting EPERDN = 2.2000 Setting RONOISE = 2.9000 Column binning= 3 Row binning= 1 NOTE: Flip binning for ASPP_ cards. Lamp= ThAr2 Lamp Filter= bg14 Shutter= open B5 Frame#= 2304 : ECHANGL= -0.0395 XDANGL= -0.0760 (HI.20060118.14792_2.fits) 1520.0+4500 Expos= 1s Object=arclamp What is this EPOCH? : 0 Calling biw() subroutine. NOTE: biw: X binning: 3 Y binning: 1 Subtracting baseline from image ( 701 --> 713 ) NOTE: No maskfile, no bad column interpolation. NOTE: HIRES2 CCD is number 2 Clip image (sc,ec,sr,er): 7 686 1 4056 Rotating ESI or HIRES2 image by 90 degrees... Flipping ESI or HIRES2 image in columns... Flipping HIRES2 image in rows... NOTE: New binning in header: 1, 3 Prepix: 0 Postpix: 80 Original Window: cols= 1 687 rows= 1 4096 New Clipped Window: cols= 0 4055 rows= 0 679 Setting EPERDN = 2.2000 Setting RONOISE = 2.9000 Column binning= 1 Row binning= 3 Lamp= ThAr2 Lamp Filter= bg14 Shutter= open B5 Frame#= 2304 : ECHANGL= -0.0395 XDANGL= -0.0760 (HI.20060118.14792_2.fits) 1520.0+4500 Expos= 1s Object=arclamp What is this EPOCH? : 0 Observation number= 2304 UT date = 18Jan06 NOTE: Object x,y binning is 1 x 3 . Recovering flat image... junk-flat_1202779631002336001.fits Dividing object by flat field... pse_mode= 4 slit width, neo, eperdn, ronoise, pse_mode = 9.77 17 2.200 2.900 4 Extracting whole slit spectrum... ****************************** Extracting echelle order number 1 of 17 ****************************** Extracting echelle order number 2 of 17 ****************************** Extracting echelle order number 3 of 17 ****************************** Extracting echelle order number 4 of 17 ****************************** Extracting echelle order number 5 of 17 ****************************** Extracting echelle order number 6 of 17 ****************************** Extracting echelle order number 7 of 17 ****************************** Extracting echelle order number 8 of 17 ****************************** Extracting echelle order number 9 of 17 ****************************** Extracting echelle order number 10 of 17 ****************************** Extracting echelle order number 11 of 17 ****************************** Extracting echelle order number 12 of 17 ****************************** Extracting echelle order number 13 of 17 ****************************** Extracting echelle order number 14 of 17 ****************************** Extracting echelle order number 15 of 17 ****************************** Extracting echelle order number 16 of 17 ****************************** Extracting echelle order number 17 of 17 Writing : Arc-2336_2.fits Mon Feb 11 17:27:39 2008 Calibrate Arc lamp #1............... autoid Arc-2336_2.fits -clobber File Echelle XD dCol dRow Filt Expos dR # of orders Arc-2336_2 -0.0395 -0.0760 - - bg14 1 - 17 WARNING: Lamp name is not "ThAr1" : ThAr2 Best match (from /users/tab/makee///ArcLineDataBase/adrd_2.list ): adrd_2-01 0.0029 -0.1150 60.5 -0.9 ng3 1 0.2756 17 Obs# Echelle X.D. Lamp Filter Filename 2483 0.0029 -0.1150 ThAr2 ng3 ArcLineDataBase/adrd_2-01.fits 2304 -0.0395 -0.0760 ThAr2 bg14 Arc-2336_2.fits autoid_FindOffsets: Row offset range is -4 to 2 . Saturation level, # of saturated pixels= 64063.58 2 Assume saturation is 64600. Saturation level, # of saturated pixels= 62372.41 84 Row offset: -4 -3 -2 -1 0 1 2 Col offset: 0.9 46.6 25.7 54.0 2.8 75.8 29.4 RMS: 55.7 54.0 81.1 65.9 0.1 73.1 39.6 .....Best row offset= 0 Writing PostScript plot file: Arc-2336_2-cf.ps Writing new ID file: Arc-2336_2.ids 606 line IDs written to file. An average of 35.6 line IDs per order. A total of 606 lines read in. Writing PostScript plot file: Arc-2336_2-fr.ps Final fit: Row= 1 Ord= 6 WRMS= 0.0459 High= 0.1345 NPt= 22 NRej= 0 Final fit: Row= 2 Ord= 6 WRMS= 0.0752 High= -0.1846 NPt= 33 NRej= 0 Final fit: Row= 3 Ord= 6 WRMS= 0.0807 High= -0.1915 NPt= 34 NRej= 0 Final fit: Row= 4 Ord= 6 WRMS= 0.0993 High= -0.3638 NPt= 41 NRej= 0 Final fit: Row= 5 Ord= 6 WRMS= 0.1045 High= 0.3123 NPt= 27 NRej= 0 Final fit: Row= 6 Ord= 6 WRMS= 0.0893 High= 0.3331 NPt= 45 NRej= 1 Final fit: Row= 7 Ord= 6 WRMS= 0.0559 High= 0.1279 NPt= 39 NRej= 0 Final fit: Row= 8 Ord= 6 WRMS= 0.0894 High= 0.2067 NPt= 42 NRej= 0 Final fit: Row= 9 Ord= 6 WRMS= 0.0745 High= 0.1887 NPt= 43 NRej= 0 Final fit: Row= 10 Ord= 6 WRMS= 0.0710 High= -0.2908 NPt= 30 NRej= 0 Final fit: Row= 11 Ord= 6 WRMS= 0.0918 High= 0.2541 NPt= 31 NRej= 0 Final fit: Row= 12 Ord= 6 WRMS= 0.0791 High= -0.3201 NPt= 37 NRej= 0 Final fit: Row= 13 Ord= 6 WRMS= 0.0772 High= 0.2150 NPt= 26 NRej= 0 Final fit: Row= 14 Ord= 6 WRMS= 0.0818 High= 0.3578 NPt= 36 NRej= 0 Final fit: Row= 15 Ord= 6 WRMS= 0.1148 High= -0.2885 NPt= 33 NRej= 0 Final fit: Row= 16 Ord= 6 WRMS= 0.0463 High= 0.1085 NPt= 34 NRej= 0 Final fit: Row= 17 Ord= 6 WRMS= 0.1072 High= 0.3817 NPt= 34 NRej= 0 Lo,Mdn,Hi: R= 0.05 0.08 0.11 H= 0.11 0.25 0.38 Pt= 22 34 45 Rj= 0 0 1 Writing line id file "Arc-2336_2.ids" for all rows. A total of 588 lines written out. Over-Writing: Arc-2336_2.fits ................................................. arc2obj Arc-2336_2.fits Flux-2336_2.fits -sky -var ps=Flux-2336_2-skyshift.ps -sum Reading: Arc-2336_2.fits Arc file= Arc-2336_2.fits ECHA,XDA= -0.0395 -0.0760 NOTE: Skylines from: /users/tab/makee//SkyLineDataBase/sky.results Reading: Flux-2336_2.fits Second file= Flux-2336_2.fits ECHA,XDA= -0.0395 -0.0740 Reading: Var-2336_2.fits Reading: Sum-2336_2.fits Reading: Sky-2336_2.fits *****Night sky line shift results: # row wavelength peak pix.shft weight 1 9 5589.128 27.6 0.42 0.28 2 12 5865.454 26.6 -5.69 0.27 3 12 5867.540 35.5 -2.13 0.35 4 12 5888.183 61.6 -0.22 0.62 5 12 5889.953 482.4 1.71 1.00 6 13 5889.953 482.4 1.34 1.00 7 13 5895.923 301.1 3.95 1.00 8 13 5906.699 34.7 -0.47 0.35 9 13 5915.301 60.8 -5.06 0.61 10 13 5924.723 34.5 -5.28 0.34 11 13 5932.862 47.2 2.69 0.47 12 13 5945.932 27.4 4.46 0.27 13 13 5953.420 39.7 6.14 0.40 14 13 5970.278 32.6 2.40 0.33 15 16 6234.293 26.8 0.12 0.27 16 16 6257.961 69.7 3.78 0.70 17 16 6287.434 62.0 5.20 0.62 18 16 6297.903 31.0 3.61 0.31 19 16 6300.304 673.7 -1.23 1.00 Skyline shift= 1.0947 +/- 3.4494 Npt= 19 NRej= 0 Writing to device: Flux-2336_2-skyshift.ps/PS arc2obj: NOTE: bad skyline fit--RMS>0.4--no shift applied. arc2obj: NOTE: No skyline shift applied. Sky Shift used= 0.0000 measured= 1.0947 RMS= 3.4494 #Pt= 19 Heliocentric velocity correction (km/s) = -17.9831 Air to vacuum correction applied... Heliocentric velocity correction applied... Over-writing file: Flux-2336_2.fits Over-writing file: Sum-2336_2.fits Over-writing file: Sky-2336_2.fits Writing file: Err-2336_2.fits arc2obj: All done. ..................................................... arc2arc Flux-2336_2.fits Sum-2336_2.fits pxsh=0 First file= Flux-2336_2.fits ECHA,XDA= -0.0395 -0.0740 Second file= Sum-2336_2.fits ECHA,XDA= -0.0395 -0.0740 Shift in pixels= 0.000000 Zero shift, no refitting necessary. arc2arc: All done. NOTE: Writing KOA tables. Reading final Flux- file Flux-2336_2.fits Reading final Arc- file Arc-2336_2.fits opim mul Flux-2336_2.fits Flat-2336_2.fits DN-2336_2.fits -clobber Writing file : DN-2336_2.fits opim div DN-2336_2.fits const=+1.4049062E+04 -clobber Writing file : DN-2336_2.fits spim0 DN-2336_2.fits min=0. bin=2 ps=DN-2336_2.ps coflag=3 Output is in : DN-2336_2.ps opim div Flux-2336_2.fits Err-2336_2.fits s2n-2336_2.fits -clobber Writing file : s2n-2336_2.fits opim min s2n-2336_2.fits const=0. -clobber Writing file : s2n-2336_2.fits spim0 s2n-2336_2.fits min=0. bin=2 ps=s2n-2336_2.ps coflag=2 Output is in : s2n-2336_2.ps spim0 Flux-2336_2.fits minp=-0.08 bin=2 ps=Flux-2336_2.ps coflag=1 Output is in : Flux-2336_2.ps NOTE: spectrum plot binning factor is 2 pixels. rhh Flux-2336_2.fits -wave 18Jan06 2336 Flux-2336_2 -0.0395 -0.0740 RED none ng3 500s 4908.5 6423.6 2322+5734 object (Flux) Mon Feb 11 17:27:47 2008 makee: All done.