SIMPLE = T / Fits standard BITPIX = -32 / Bits per pixel NAXIS = 3 / Number of axes NAXIS1 = 853 / Axis length NAXIS2 = 1 / Axis length NAXIS3 = 4 / Axis length EXTEND = F / File may contain extensions ORIGIN = 'NOAO-IRAF FITS Image Kernel July 2003' / FITS file originator DATE = '2013-08-07T21:44:42' / Date FITS file was generated IRAF-TLM= '2013-08-07T21:44:42' / Time of last modification OBJECT = 'SN 2013ej' / Name of the object observed EXPTIME = 5274 / DETECTOR= 'SITe-2' / detector name XBIN = 2 / YBIN = 4 / PIXSIZE = 15.0 / pixel size, microns CTYPE1 = 'LINEAR ' / axis1 in pixels CTYPE2 = 'LINEAR ' / axis2 in pixels CCDTEMP = -111.2 / detector temperature [C] DATE-OBS= '2013-08-07T09:41:09'/ UT-DATE = '2013-08-07' / UT = ' 9:41:09.00' / MJD-OBS = 56511.40358 / modified Julian Date of observation OBSTYPE = 'object ' / OBSERVATION TYPE TELESCOP= '1.8-m' / This telescope OBSERVAT= 'DAO' / Location WIND_SPD= 0.0 / Wind speed, m/s MAX_WND = 0.2 / Max wind speed last min,m/s WIND_DIR= 302.0 / Wind direction, degrees WIND_CHL= 19.7 / Wind chill, deg C OUT_TEMP= 19.5 / Outside Temperature, deg C REL_HUMI= 53.5 / Outside relative humidity, percent DEWPOINT= 10.0 / Outside dew point, deg C M1_TEMP = 16.81 / M1 (primary) mirror temp [C] M1_RH = 65.15 / RH near M1 M1_RHTEM= 15.66 / RH temp [C] near M1 RA = ' 1:37:35.40' / AT START OF EXPOSURE DEC = '15:47:19.00' / AT START OF EXPOSURE HA = '-03:05:44.4' / AT START OF EXPOSURE ST = '22:31:51.00' / AT START OF EXPOSURE EQUINOX = 2013.6 / AT START OF EXPOSURE DOMEAZ = 104.40 / AT START OF EXPOSURE AIRMASS = 1.55 / AT START OF EXPOSURE ZD = 49.822 / ZD at start of exposure INSTRUME= 'Cassegrain Spectrograph' / Instrument used OBSMODE = 'single-slit spectroscopy' / Observing mode CAMERA = '21 inch' / Spectrograph Camera ID GRATING = '150Y' / Spectrograph grating ID WAVELENG= 5400 / central wavelength [Angstroms] GRAT_ANG= 90.32 / grating angle [degrees] GRAT_ORD= 1 / grating order LAMPTYPE= 'fe-ar' / calibration lamp OBSERVER= 'Balam' / Observer DAOPRGID= 'DAO182_2013C5' / DAO observing program identification PINAME = 'Balam' / Principal investigator name DISPERSI= 120.0 / Angstroms/mm SLIT = 'slit' / slit designation SLIT_WID= 2 / slit width or aperture dia on sky [arcsec] REFPIXEL= 435 / Approx pix where wavelength is WAVELENG DELTA_WL= 3.6000 / Approx spacing of pixels [Angstroms] EXPNUM = 'dao_c182_2013_008056' RELEASE = '2014-08-07T11:09:06'/ WCSDIM = 3 CD1_1 = 3.85671639442444 CD2_2 = 1. LTM1_1 = 1. LTM2_2 = 1. WAT0_001= 'system=equispec' WAT1_001= 'wtype=linear label=Wavelength units=angstroms' WAT2_001= 'wtype=linear' TRIM = 'Aug 7 15:42 Trim data section is [5:870,1:50]' ZEROCOR = 'Aug 7 15:42 Zero level correction image is Z130710.fits' FLATCOR = 'Aug 7 15:42 Flat field image is nF130710.fits with scale=1.' CCDSEC = '[1:866,1:50]' CCDMEANT= 1060357347 CCDPROC = 'Aug 7 15:42 CCD processing done' APNUM1 = '1 1 25.75 31.69' CTYPE3 = 'LINEAR ' CRVAL1 = 3668.56119847298 CRPIX1 = -2. CD3_3 = 1. LTM3_3 = 1. WAT3_001= 'wtype=linear' DC-FLAG = 0 DCLOG1 = 'REFSPEC1 = temp_arc1.ms.fits' DCLOG2 = 'REFSPEC2 = temp_arc2.ms.fits' JD = 2456511.9340972 HJD = 2456511.93577505 LJD = 2456511. BANDID1 = 'spectrum - background fit, weights variance, clean yes' BANDID2 = 'raw - background fit, weights none, clean no' BANDID3 = 'background - background fit' BANDID4 = 'sigma - background fit, weights variance, clean yes' LTV1 = -3. EX-FLAG = 0 CA-FLAG = 0 BUNIT = 'erg/cm2/s/A' END )))u))V**>G*lZ*pp)34* ))Ѡ){);)\)z))匾)0)))0)ރ)I)K^)w)E))));[)ԅ)F)1)yR))X)vm)Ё ))g)ӺO)ש)z)$O)z)^))Q)))G5)* Z*tT*_^** f* * ^*61**Z0***hE* [U**WN* * *(C**9*L6*eB**܊*+**֓*Y* r*(* EG*ķ*A*<*Ng*)**** N* * * * |* r* *f**\U*D**G*_ *A*g**6*@*X5**O:*g*ѡ** *Q*|*X**:** *{j**N*^*****,***R*;**)*Q*R****l*:*@*g*0x* *U*@* **t*K**8* *f9**y*#*1***k)*{*$u*>*L** *V*$** ********o**)*s*˖***#***+**¾* c*S**P**,*