Keck spectra Apr/May 1996 Data reduction (LBL, May 1996) data in ka = /home/astro26/deepsearch/keckspectra/apr96/ data in km = /home/astro26/deepsearch/keckspectra/may96/ made lists: apr_all.list ccdproc Trim: [21:2069,40:448] AS BEFORE overscan: [2080:2145,45:445] apr96 data: overscan level 990-1010 ? may96 data: overscan level 780-800 BIASES ------ look at 014-019 >> bias1 : combine & see if there's structure. and 092-095 >> bias2 : also look for changes over course of night. no repeatable pattern so ignore bias frames. FLATS ----- Apr96 ----- Use rotator position of all frames to decide which flat goes with which observation. hedit lris*.imh ROTPOSN . update- cl> hedit lris*.imh ROTPOSN . update- lris0001.imh,ROTPOSN = -90.00000081 lris0002.imh,ROTPOSN = -90.00000081 lris0003.imh,ROTPOSN = -90.00000081 lris0004.imh,ROTPOSN = -90.00000081 lris0005.imh,ROTPOSN = -90.00000081 lris0006.imh,ROTPOSN = -90.00000081 lris0007.imh,ROTPOSN = -90.00009236 lris0008.imh,ROTPOSN = -90.00000081 lris0009.imh,ROTPOSN = -90.00000081 lris0010.imh,ROTPOSN = -90.00000081 lris0011.imh,ROTPOSN = -90.00000081 lris0012.imh,ROTPOSN = -90.00000081 lris0013.imh,ROTPOSN = -90.00000081 lris0014.imh,ROTPOSN = -90.00000081 lris0015.imh,ROTPOSN = -90.00000081 lris0016.imh,ROTPOSN = -30.02966336 lris0017.imh,ROTPOSN = 51.93200730 lris0018.imh,ROTPOSN = 89.99945149 lris0019.imh,ROTPOSN = 90.00000081 lris0020.imh,ROTPOSN = 90.00000081 lris0021.imh,ROTPOSN = 90.00000081 lris0022.imh,ROTPOSN = 90.00000081 lris0023.imh,ROTPOSN = 90.00000081 lris0024.imh,ROTPOSN = 0.00000000 lris0025.imh,ROTPOSN = 50.00757076 lris0026.imh,ROTPOSN = 50.00614926 lris0027.imh,ROTPOSN = 50.00203966 lris0028.imh,ROTPOSN = 50.00741976 lris0029.imh,ROTPOSN = 50.00174130 lris0030.imh,ROTPOSN = 50.00069565 lris0031.imh,ROTPOSN = 48.90782542 lris0032.imh,ROTPOSN = 49.99779919 lris0033.imh,ROTPOSN = 49.99469332 lris0034.imh,ROTPOSN = 49.99919960 lris0035.imh,ROTPOSN = 50.42364550 lris0036.imh,ROTPOSN = 50.62595189 lris0037.imh,ROTPOSN = 50.82311844 lris0038.imh,ROTPOSN = 51.01851709 lris0039.imh,ROTPOSN = 51.21199150 lris0040.imh,ROTPOSN = -30.00331848 lris0041.imh,ROTPOSN = -29.99990696 lris0042.imh,ROTPOSN = -30.00006650 lris0043.imh,ROTPOSN = -29.99931676 lris0044.imh,ROTPOSN = -30.00085408 lris0045.imh,ROTPOSN = -30.00012352 lris0046.imh,ROTPOSN = -30.00189935 lris0047.imh,ROTPOSN = -30.00165458 lris0048.imh,ROTPOSN = -30.00267719 lris0049.imh,ROTPOSN = -30.00356462 lris0050.imh,ROTPOSN = -30.00223565 lris0051.imh,ROTPOSN = -30.00271207 lris0052.imh,ROTPOSN = -31.00207729 lris0053.imh,ROTPOSN = -31.00259768 lris0054.imh,ROTPOSN = -26.50254314 lris0055.imh,ROTPOSN = -26.50357388 lris0056.imh,ROTPOSN = -26.19688277 lris0057.imh,ROTPOSN = -26.05778650 lris0058.imh,ROTPOSN = -25.94363451 lris0059.imh,ROTPOSN = 44.99907683 lris0060.imh,ROTPOSN = 44.99815090 lris0061.imh,ROTPOSN = 44.99738203 lris0062.imh,ROTPOSN = 44.99775549 lris0063.imh,ROTPOSN = 44.99855070 lris0064.imh,ROTPOSN = 44.99949971 lris0065.imh,ROTPOSN = 44.99856232 lris0066.imh,ROTPOSN = -36.00038019 lris0067.imh,ROTPOSN = -36.00185971 lris0068.imh,ROTPOSN = -36.00066341 lris0069.imh,ROTPOSN = -36.00061128 lris0070.imh,ROTPOSN = -35.99980197 lris0071.imh,ROTPOSN = -36.00047757 lris0072.imh,ROTPOSN = -25.99953643 lris0073.imh,ROTPOSN = -25.99887019 lris0074.imh,ROTPOSN = 10.00081154 lris0075.imh,ROTPOSN = 10.00061371 lris0076.imh,ROTPOSN = 10.00047671 lris0077.imh,ROTPOSN = 9.99947308 lris0078.imh,ROTPOSN = 9.99998140 lris0079.imh,ROTPOSN = 10.00091621 lris0080.imh,ROTPOSN = 9.99958230 lris0081.imh,ROTPOSN = 10.00206333 lris0082.imh,ROTPOSN = 10.00111371 lris0083.imh,ROTPOSN = 10.00044976 lris0084.imh,ROTPOSN = 9.99952885 lris0085.imh,ROTPOSN = 10.00176501 lris0086.imh,ROTPOSN = 9.99988313 lris0087.imh,ROTPOSN = 9.99960651 lris0088.imh,ROTPOSN = 10.00013998 lris0089.imh,ROTPOSN = 10.00002013 lris0090.imh,ROTPOSN = 9.99999812 lris0091.imh,ROTPOSN = 10.00117928 lris0092.imh,ROTPOSN = 90.00064168 lris0093.imh,ROTPOSN = 90.00000081 lris0094.imh,ROTPOSN = 90.00000081 lris0095.imh,ROTPOSN = 90.00000081 flats type use for ----------------------------------- 002-008 dome 001,009-013 020-023 internal 024 twilight 035-039 dome 025-034 044-047 dome 040-043, 048-053 056-058 dome 054-055 059-061 dome 062-065 068-070 dome 066-067, 071-073 077-080 dome 074-076, 082 083 twilight 084 twilight 085-091 twilight ========================================== ccdhedit *.imh dispaxis 1 ccdhedit *.imh disptype lambda ccdhedit *.imh dispunit angstroms ========================================== COMBINING FLATS: -julia --------------- imcombine lris0002,lris0003,lris0004,lris0005,lris0006,lris0007,lris0008 flat2to8 imcombine lris0035,lris0036,lris0037,lris0038,lris0039 flat35to39 imcombine lris0056,lris0057,lris0058 flat56to58 imcombine lris0059,lris0060,lris0061 flat59to61 imcombine lris0068,lris0069,lris0070 flat68to70 imcombine lris0077,lris0078,lris0079,lris0080 flat77to80 RESPONSE: -julia -------- response flat2to8 flat2to8 rflat2to8 response flat35to39 flat35to39 rflat35to39 response flat44to47 flat44to47 rflat44to47 response flat56to58 flat56to58 rflat56to58 response flat59to61 flat59to61 rflat59to61 response flat68to70 flat68to70 rflat68to70 response flat77to80 flat77to80 rflat77to80 =========================================== FLATFIELDING OBJECTS: -julia -------------------- ccdproc @obs1.list flat=rflat2to8 ccdtype=object flatcor+ ccdproc @obs2.list flat=rflat35to39 ccdtype=object flatcor+ ccdproc @obs3.list flat=rflat44to47 ccdtype=object flatcor+ ccdproc @obs4.list flat=rflat56to58 ccdtype=object flatcor+ ccdproc @obs5.list flat=rflat59to61 ccdtype=object flatcor+ ccdproc @obs6.list flat=rflat68to70 ccdtype=object flatcor+ ccdproc @obs7.list flat=rflat77to80 ccdtype=object flatcor+ where: obs1.list = 001,009-013 obs2.list = 025-034 obs3.list = 040-043, 048-053 obs4.list = 054-055 obs5.list = 062-065 obs6.list = 066-067, 071-073 obs7.list = 074-076, 082 CHECKING CR CLEANING - Isobel -------------------- data in /home/astro26/deepsearch/julia/apr96/ Targets: 029 lris0029 SN1996W 030 lris0030 -other object plus sky line getting zapped 033 l033s4cr SN1996M 034 l034s4cr 040 lris0040 bad sky lines (963) 041 l041s8cr 042 lris0042 049 lris0049 sky line even at 15 sig SN962 050 l050s4cr 051 l051s4cr 052 l052s5cr SN964 053 lris0053 054 lris0054 SN969 055 lris0055 063 lris0063 sky problems SN9611 064 l064s6cr 065 lris0065 066 lris0066 9624 067 l067s5cr 072 lris0072 SN1996 O 073 l073s5cr EXTRACTIONS - Isobel ----------- imh's extractions in /home/astro26/deepsearch/keck/apr96/is/ In apall set gain=1.9, readnoise =6.0 (from LRIS manual/IMH's notes at telescope). We were using 'low' gain setting. --------------------------------------- SN1996W, runs #029,#030 extracted 1 object (did 3 in May data) W calib 025 F calib 027 combined with sarith >> sn1996w listpix sn1996w[*,1,1] > sn1996w.asc --------------------------------------- SN1996M, runs #033, #034 033 l033s4cr 034 l034s4cr extracted one object W calib 032 F calib 027 combined with sarith >> sn1996m listpix sn1996m[*,1,1] > sn1996m.asc --------------------------------------- SN963 runs #040, 41, 42 040 lris0040 041 l041s8cr - not at all flat 042 lris0042 - " v hard to trace. used 041 as ref extracted one object W calib 048 F calib 027 combined with scombine (medianed with scaling) >> sn963c cant see any lines. 5577 a slight problem listpix sn963c[*,1,1] > sn963c.asc --------------------------------------- SN962 runs 049, 050, 051 049 lris0049 cr - problem with this frame ? 050 l050s4cr 051 l051s4cr extracted one object - possible line in 051, but may be 5577 ? W calib: 048 F claib: 027 combined with scombine (medianed with scaling) >> sn962c listpix sn962c[*,1,1] > sn962c.asc looks like there's a bump at ~7200 A --------------------------------------- SN964 052 l052s5cr 053 lris0053 4 objects ap#1 row 120 ap#2 row 200 target: brighter obj used as ref ap#3 row 213 bright obj ap#4 row 269 lots of horrid CRs W calib 048 F calib 027 combined with scombine >> sn964c listpix sn964c[*,1,1] > sn964c_ap1.asc listpix sn964c[*,2,1] > sn964c_ap2.asc listpix sn964c[*,3,1] > sn964c_ap3.asc listpix sn964c[*,4,1] > sn964c_ap4.asc wfits sn964c[*,1,1] sn964c_ap1.fits wfits sn964c[*,2,1] sn964c_ap2.fits wfits sn964c[*,3,1] sn964c_ap3.fits wfits sn964c[*,4,1] sn964c_ap4.fits --------------------------------------- SN969 054 lris0054 SN969 055 lris0055 3 objects ap#1 row #150 ap#2 row #200 target : wiggles/lines ? ap#3 row #245 z=0.384 -ish. OIII, Hb, OII (but OII/OIII give slightly different z's) lots of horrid CRs esp in ap#1 of #055 W calib 048 F calib 027 combined with sarith > sn969c listpix sn969c[*,1,1] > sn969c_ap1.asc listpix sn969c[*,2,1] > sn969c_ap2.asc listpix sn969c[*,3,1] > sn969c_ap3.asc wfits sn969c[*,1,1] sn969c_ap1.fits wfits sn969c[*,2,1] sn969c_ap2.fits wfits sn969c[*,3,1] sn969c_ap3.fits --------------------------------------- SN9611 063 lris0063 sky problems SN9611 064 l064s6cr - extracted later - Oct 3 96 065 lris0065 extracted 2 objects ap#1 row 205 : target -type II features ap#2 row 313 : W calib 062 F calib 027 combined with scombine > sn9611c listpix sn9611c[*,1,1] > sn9611c_ap1.asc > sn9611c_ap1.apr96.asc listpix sn9611c[*,2,1] > sn9611c_ap2.asc > sn9611c_ap2.apr96.asc wfits sn9611c[*,1,1] sn9611c_ap1.apr96.fits wfits sn9611c[*,2,1] sn9611c_ap2.apr96.fits --------------------------------------- SN9624 066 lris0066 067 l067s5cr - extracted later - 3 oct 96 4 objects ap#1 row 118 - narrow emission line - possibly OII at z=1.03 ! ap#2 row 157 -H&K, hg, hb, etc z=0.432 ap#3 row 204 target ap#4 row 272 bright W calib: 071 F calib 027 combined with sarith > sn9624c listpix sn9624c[*,1,1] > sn9624_ap1.asc listpix sn9624c[*,2,1] > sn9624_ap2.asc listpix sn9624c[*,3,1] > sn9624_ap3.asc listpix sn9624c[*,4,1] > sn9624_ap4.asc wfits sn9624c[*,1,1] sn9624_ap1.fits wfits sn9624c[*,2,1] sn9624_ap2.fits wfits sn9624c[*,3,1] sn9624_ap3.fits wfits sn9624c[*,4,1] sn9624_ap4.fits --------------------------------------- SN1996 O 072 lris0072 073 l073s5cr W calib 071 F calib 027 extracted one object (some galaxy contamination ? - but did set background regions on the galaxy either side of object) combined with sarith > sn1996o listpix sn1996o[*,1,1] > sn1996o.asc ===================================================================== - arcs and standards: - julia OBJECTS -> CORRESPONDING ARC ----------------------------------------- 29,30 25 33,34 31,32 40-42,49-53 48 54,55 48 ? 63-65 62 66,67,72,73 71 STANDARDS -> CORRESPONDING ARC ----------------------------------------- 26,27,28 25 74,75,76 82 apall lris0025 out=alris0025arc refer=lris0026 trace=no backg=none apall lris0031 out=alris0031arc refer=033s4cr trace=no backg=none apall lris0032 out=alris0032arc refer=033s4cr trace=no backg=none apall lris0048 out=alris0048arc refer=052s5cr trace=no backg=none apall lris0062 out=alris0062arc refer=lris0066 trace=no backg=none apall lris0071 out=alris0071arc refer=lris0072 trace=no backg=none apall lris0082 out=alris0082arc refer=lris0074 trace=no backg=none copying Isobel's extractions - have to try to fool IRAF with names cop ../../../keck/apr96/is/database/apkajl033s4cr ap033s4cr cop ../../../keck/apr96/is/database/apkajl052s5cr ap052s5cr cop ../../../keck/apr96/is/database/apkajlris0066 ap066 cop ../../../keck/apr96/is/database/apkajlris0072 ap072 NOTE: Julia edited database file that was copied from Isobel's database corresponding to objects 52 and 66 with names respectively apl052s5cr & aplris0066 in Julia's database. 52 ws editied to only contain information on ap2; 66 was edited to contain only info on ap3. These 2 apertures corresponding to the aperture for the host. Also, the paerture and imagename had to be changed from kaj$l052s5cr to l052s5cr and kaj$lris0066 to lris0066 respectively. -j. ===================================================================== standards located in /home/astro26/deepsearch/julia/apr96 note : background = "fit" apall lris0074 out=alris0074 apall lris0075 out=alris0075 apall lris0076 out=alris0076 * note: 76 may be saturated -j. ===================================================================== Arcs seem to be flipped (ie. higher->lower wavelengths from left to right) -j. Julia flipped back for purposes of identification by doing SFLIP IMH: this is not a good idea unless you flip EVERYTHING. This produced final spectra with the wavelength scale backwards ! See below Julia: redid arcs without flipping IDENT: ----- images = "alris0082arc" Images containing features to be identified (section = "middle line") Section to apply to two dimensional images (database = "database") Database in which to record feature data (coordlist = "/home/astro10/julia/iraf/IRAFlinelist") User coordinate list (nsum = "10") Number of lines/columns/bands to sum in 2D imag (match = 10.) Coordinate list matching limit in user units (maxfeatures = 50) Maximum number of features for automatic identi (zwidth = 100.) Zoom graph width in user units (ftype = "emission") Feature type (fwidth = 4.) Feature width in pixels (cradius = 5.) Centering radius in pixels (threshold = 10.) Feature threshold for centering (minsep = 2.) Minimum pixel separation (function = "spline3") Coordinate function (order = 1) Order of coordinate function (sample = "*") Coordinate sample regions (niterate = 0) Rejection iterations (low_reject = 3.) Lower rejection sigma (high_reject = 3.) Upper rejection sigma (grow = 0.) Rejection growing radius (autowrite = no) Automatically write to database (graphics = "stdgraph") Graphics output device (cursor = "") Graphics cursor input (mode = "ql") ident alris0025arc (Isobel identified) julia renamed alris0025arc apr96k025arc REIDENT: -------- reference = "alris0025arc" Reference image images = "alris0082arc" Images to be reidentified answer = "yes" Fit dispersion function interactively? (interactive = "no") Interactive fitting? (section = "middle line") Section to apply to two dimensional images (newaps = yes) Reidentify apertures in images not in reference (override = no) Override previous solutions? (refit = yes) Refit coordinate function?\n (trace = no) Trace reference image? (step = "10") Step in lines/columns/bands for tracing an imag (nsum = "10") Number of lines/columns/bands to sum (shift = "0.") Shift to add to reference features (nlost = 0) Maximum number of features which may be lost\n (cradius = 5.) Centering radius (threshold = 10.) Feature threshold for centering (addfeatures = no) Add features from a line list? (coordlist = " /home/astro10/imh/iraf/keck_nov95/cuarne") User coordinate li (match = 10.) Coordinate list matching limit in user units (maxfeatures = 50) Maximum number of features for automatic identi (minsep = 2.) Minimum pixel separation\n (database = "database") Database (logfiles = "logfile") List of log files (plotfile = "") Plot file for residuals (verbose = no) Verbose output? (graphics = "stdgraph") Graphics output device (cursor = "") Graphics cursor input (mode = "ql") reident apr96k025arc apr96k031arc reident apr96k025arc apr96k032arc reident apr96k025arc apr96k048arc reident apr96k025arc apr96k062arc reident apr96k025arc apr96k071arc reident apr96k025arc apr96k082arc ident apr96k032arc ident apr96k048arc ident apr96k062arc ident apr96k071arc ident apr96k071arc ident apr96k082arc ident apr96k082arc ____________________________________________________________________ imh identified alris0025arc (not flipped) directly 4th order legendre >> rms=0.25. NB blue end not tied down too well- Hg lines not very strong. ===================================================================== ASSIGNING ARCLAMPS and WAVELENGTH CALIBRATING: - julia DISPCOR: -------- input = "kais$049x" List of input spectra output = "dlris049" List of output spectra (linearize = yes) Linearize (interpolate) spectra? (database = "database") Dispersion solution database (table = "") Wavelength table for apertures (w1 = INDEF) Starting wavelength (w2 = INDEF) Ending wavelength (dw = INDEF) Wavelength interval per pixel (nw = INDEF) Number of output pixels (log = no) Logarithmic wavelength scale? (flux = yes) Conserve flux? (samedisp = yes) Same dispersion in all apertures? (global = no) Apply global defaults? ignoreaps = yes) Ignore apertures? (confirm = no) Confirm dispersion coordinates? (listonly = no) List the dispersion coordinates only? (verbose = yes) Print linear dispersion assignments? (logfile = "") Log file (mode = "ql") OBJECTS -> CORRESPONDING ARC ----------------------------------------- 29,30 25 33,34 31,32 40-42,49-53 48 54,55 48 ? 63-65 62 66,67,72,73 71 STANDARDS -> CORRESPONDING ARC ----------------------------------------- 26,27,28 25 74,75,76 82 Standards: ccdhedit alris0026 REFSPEC1 apr96k025arc ccdhedit alris0027 REFSPEC1 apr96k025arc ccdhedit alris0028 REFSPEC1 apr96k025arc ccdhedit alris0074 REFSPEC1 apr96k082arc ccdhedit alris0075 REFSPEC1 apr96k082arc ccdhedit alris0076 REFSPEC1 apr96k082arc dispcor alris0026 dapr96k026 > dispcor.log dispcor alris0027 dapr96k027 >> dispcor.log dispcor alris0028 dapr96k028 >> dispcor.log dispcor alris0074 dapr96k074 >> dispcor.log dispcor alris0075 dapr96k075 >> dispcor.log dispcor alris0076 dapr96k076 >> dispcor.log imh: cant find these. copied alris0027 to kais$a027x and re-did NOTE: kais$ = /home/astro26/deepsearch/keck/apr96/is/ (This is set up in Julia's login.cl directory to easily access Isobel's directory in which she extracted the SNe spectra; The following steps are performed in the directory /home/astro26/deepsearch/julia/apr96/) Supernovae: ccdhedit kais$029x REFSPEC1 alris0025arc ccdhedit kais$030x REFSPEC1 alris0025arc ccdhedit kais$033x REFSPEC1 alris0032arc ccdhedit kais$034x REFSPEC1 alris0032arc ccdhedit kais$040x REFSPEC1 alris0048arc ccdhedit kais$041x REFSPEC1 alris0048arc ccdhedit kais$042x REFSPEC1 alris0048arc ccdhedit kais$049x REFSPEC1 alris0048arc ccdhedit kais$050x REFSPEC1 alris0048arc ccdhedit kais$051x REFSPEC1 alris0048arc ccdhedit kais$052x REFSPEC1 alris0048arc ccdhedit kais$053x REFSPEC1 alris0048arc ccdhedit kais$054x REFSPEC1 alris0048arc ??? arc 48? ccdhedit kais$055x REFSPEC1 alris0048arc ??? ccdhedit kais$063x REFSPEC1 alris0062arc ccdhedit kais$064x REFSPEC1 alris0062arc 064x does not exist in kais$ ccdhedit kais$065x REFSPEC1 alris0062arc ccdhedit kais$066x REFSPEC1 alris0071arc ccdhedit kais$067x REFSPEC1 alris0071arc 067x does not exist in kais$ ccdhedit kais$072x REFSPEC1 alris0071arc ccdhedit kais$073x REFSPEC1 alris0071arc dispcor kais$029x dapr96k029 >> dispcor.log dispcor kais$030x dapr96k030 >> dispcor.log dispcor kais$033x dapr96k033 >> dispcor.log dispcor kais$034x dapr96k034 >> dispcor.log dispcor kais$040x dapr96k040 >> dispcor.log dispcor kais$041x dapr96k041 >> dispcor.log dispcor kais$042x dapr96k042 >> dispcor.log dispcor kais$050x dapr96k050 >> dispcor.log dispcor kais$051x dapr96k051 >> dispcor.log dispcor kais$052x dapr96k052 >> dispcor.log dispcor kais$053x dapr96k053 >> dispcor.log dispcor kais$054x dapr96k054 >> dispcor.log dispcor kais$055x dapr96k055 >> dispcor.log dispcor kais$063x dapr96k063 >> dispcor.log dispcor kais$065x dapr96k065 >> dispcor.log dispcor kais$066x dapr96k066 >> dispcor.log dispcor kais$072x dapr96k072 >> dispcor.log dispcor kais$073x dapr96k073 >> dispcor.log - imh : I cant find these. Also did they get fluxed ? In fact it looks as though different arcs got put in headers: hedit *x.imh REFSPEC1 . update- 029x.imh,REFSPEC1 = apr96k025arc 030x.imh,REFSPEC1 = apr96k025arc 033x.imh,REFSPEC1 = apr96k032arc 034x.imh,REFSPEC1 = apr96k032arc 040x.imh,REFSPEC1 = apr96k048arc 041x.imh,REFSPEC1 = apr96k048arc 042x.imh,REFSPEC1 = apr96k048arc 049x.imh,REFSPEC1 = apr96k048arc 050x.imh,REFSPEC1 = apr96k048arc 051x.imh,REFSPEC1 = apr96k048arc 052x.imh,REFSPEC1 = apr96k048arc 053x.imh,REFSPEC1 = apr96k048arc 054x.imh,REFSPEC1 = apr96k048arc 055x.imh,REFSPEC1 = apr96k048arc 063x.imh,REFSPEC1 = apr96k062arc 065x.imh,REFSPEC1 = apr96k062arc 066x.imh,REFSPEC1 = apr96k071arc 067x.imh REFSPEC1 = apr96k071arc 072x.imh,REFSPEC1 = apr96k071arc 073x.imh,REFSPEC1 = apr96k071arc Imh did dispcor in /home/astro26/deepsearch/julia/apr96/ (where the arcs are) dispcor kais$029x kais$029w dispcor kais$030x kais$030w dispcor kais$033x kais$033w dispcor kais$034x kais$034w dispcor kais$040x kais$040w dispcor kais$041x kais$041w dispcor kais$042x kais$042w dispcor kais$050x kais$050w dispcor kais$051x kais$051w dispcor kais$052x kais$052w dispcor kais$053x kais$053w dispcor kais$054x kais$054w dispcor kais$055x kais$055w dispcor kais$063x kais$063w dispcor kais$065x kais$065w dispcor kais$066x kais$066w dispcor kais$067x kais$067w dispcor kais$072x kais$072w dispcor kais$073x kais$073w ===================================================================== SENSITIVITY FUNCTIONS & CALIBRATION FOR STANDARD STARS: -julia HD84937 stand dapr96k027 stdapr96k027 star=hd84937 sensfunc stdapr96k027 sfapr96k027; rms=0.0808, spline3 order=19 CALIBRATIONS: CALIB: ------ input = "dlris0076" Input spectra to calibrate output = "clris0076" Output calibrated spectra (extinct = yes) Apply extinction correction? (flux = yes) Apply flux calibration? (extinction = "onedstds$kpnoextinct.dat") Extinction file (observatory = "obspars") Observatory of observation (ignoreaps = yes) Ignore aperture numbers in flux calibration? (sensitivity = "sens") Image root name for sensitivity spectra (fnu = no) Create spectra having units of FNU? (mode = "ql") Note: Standard stars calibrated with respect to themselves: calib dapr96k027 capr96k027 sens=sfapr96k027 ------------------------------------------------------------------- CALIBRATIONS (Objects): - julia calib dlris029 clris029 sens=apr96k027sens calib dlris030 clris030 sens=apr96k027sens calib dlris033 clris033 sens=apr96k027sens calib dlris034 clris034 sens=apr96k027sens calib dlris040 clris040 sens=apr96k027sens calib dlris041 clris041 sens=apr96k027sens calib dlris042 clris042 sens=apr96k027sens calib dlris049 clris049 sens=apr96k027sens calib dlris050 clris050 sens=apr96k027sens calib dlris051 clris051 sens=apr96k027sens calib dlris052 clris052 sens=apr96k027sens calib dlris053 clris053 sens=apr96k027sens calib dlris054 clris054 sens=apr96k027sens calib dlris055 clris055 sens=apr96k027sens calib dlris063 clris063 sens=apr96k027sens calib dlris065 clris065 sens=apr96k027sens calib dlris066 clris066 sens=apr96k027sens calib dlris072 clris072 sens=apr96k027sens calib dlris073 clris073 sens=apr96k027sens calibrations: isobel calibrate kais$029w kais$029c sens=a027sens calibrate kais$030w kais$030c sens=a027sens calibrate kais$033w kais$033c sens=a027sens calibrate kais$034w kais$034c sens=a027sens calibrate kais$040w kais$040c sens=a027sens calibrate kais$041w kais$041c sens=a027sens calibrate kais$042w kais$042c sens=a027sens calibrate kais$049w kais$049c sens=a027sens calibrate kais$050w kais$050c sens=a027sens calibrate kais$051w kais$051c sens=a027sens calibrate kais$052w kais$052c sens=a027sens calibrate kais$053w kais$053c sens=a027sens calibrate kais$054w kais$054c sens=a027sens calibrate kais$055w kais$055c sens=a027sens calibrate kais$063w kais$063c sens=a027sens calibrate kais$064w kais$064c sens=a027sens calibrate kais$065w kais$065c sens=a027sens calibrate kais$066w kais$066c sens=a027sens calibrate kais$067w kais$067c sens=a027sens calibrate kais$072w kais$072c sens=a027sens calibrate kais$073w kais$073c sens=a027sens Things still need to be done: extract, dispersion correct & fluxcalibrate: 64, 67 dispersion correct and flux-calibrate: 049x (IRAF error)