This file contains the best spectroscopic classifications and redshifts from the Princeton-1D code, specBS. More detailed results from the fits of each object to the full list of templates used can be found in the spZline files. Ths first HDU is the FITS binary table described below. The 2nd HDU is the best-fit eigen-spectrum for each object. These can be regenerated from the tabular information, but for convenience they've been explicitly computed here.
| Column | Description |
|---|---|
| PLATE | Plate number |
| TILE | Tile number |
| MJD | Modified Julian date of observation |
| FIBERID | Fiber ID (1 to 640) |
| OBJID | 4-element PHOTO ID of targetted object: run, re-run, column, ID |
| OBJTYPE | Why this object was targetted. Note that if this field says QSO, it could be the case that this object would have been targetted as a GALAXY or any number of other categories as well. The PRIMTARGET and SECTARGET flags in the plug-map structure (in the spPlate file) gives this full target information. |
| PLUG_RA | Object RA (drilled fiber position) [J2000 degrees]. |
| PLUG_DEC | Object DEC (drilled fiber position) [J2000 degrees]. |
| CLASS | SpecBS classification: GALAXY, QSO, STAR. |
| SUBCLASS |
SpecBS sub-classification. Galaxies and QSO's can be given sub-classifications based upon their emission lines. This text includes the word "AGN" if: log10(OIII/Hbeta) > 0.7 - 1.2 * (log10(NII/Halpha) - 0.4) This text includes the word "STARFORMING" if: log10(OIII/Hbeta) < 0.7 - 1.2 * (log10(NII/Halpha) - 0.4) If the H_alpha E.W. > 500 Ang, then upgrade "STARFORMING" to "STARBURST." In all cases for AGN, STARFORMING, and STARBURST, the 4 emission lines used for that sub-classification must have well-measured errors (e.g., LINEAREA_ERR > 0). If any galaxies or quasars have lines detected at the 10-sigma level with sigmas > 200 km/sec at the 5-sigma level, call them "BROADLINE". For stars, the following subclassifications are in use: O, OB, B6, B9, A0, A0p, F2, F5, F9, G0, G2, G5, K1, K3, K5, K7, M0V, M2V,M1, M2, M3, M4, M5, M6, M7, M8, L0, L1, L2, L3, L4, L5, L5.5, L9, T2, Carbon, Carbon_lines, CarbonWD, CV. |
| Z | Heliocentric Redshift; if the ZWARNING flag is nonzero, then assume that this redshift is incorrect. |
| Z_ERR | Redshift error based upon fit to χ2 minimum; negative for invalid fit. |
| RCHI2 | Reduced χ2 for best fit template. |
| DOF | Degrees of freedom for best fit |
| RCHI2DIFF | Difference in reduced χ2 of best solution to 2nd best solution |
| TFILE | Template file in $IDLSPEC2D_DIR/templates |
| TCOLUMN | Columns to use in template file (0-indexed); unused values set to -1 |
| NPOLY | Number of polynomial terms used in conjunction with TFILE |
| THETA | Eigenvalue coefficients for each column in template file + each polynomial term |
| THETA_COVAR | Covariance matrix for THETA, where the square root of the diagonal elements gives the formal 1-sigma statistical errors |
| VDISP | Velocity dispersion, only computed for galaxies (km/sec) and explicitly masking emission line regions |
| VDISP_ERR | Error in VDISP (km/sec); negative for invalid fit |
| VDISPZ | Redshift for best-fit velocity dispersion |
| VDISP_ERR | Error in VDISPZ |
| VDISPCHI2 | χ2 for best-fit velocity dispersion |
| VDISPNPIX | Number of pixels overlapping the templates used in the velocity dispersion fit |
| VDISPDOF | Degrees of freedom for best-fit velocity dispersion, equal to VDISPNPIX minus the number of templates minus the number of polynomial terms minus 1 (the last 1 is for the velocity dispersion) |
| WAVEMIN | Minimum observed (vacuum) wavelength for this object (Angstroms) |
| WAVEMAX | Maximum observed (vacuum) wavelength for this object (Angstroms) |
| WCOVERAGE | Amount of wavelength coverage in log-10(Angstroms) |
| ZWARNING | A flag set for bad redshift fits in place of calling
CLASS=UNKNOWN. The following bits may be set:
0 = Sky fiber
1 = Too little wavelength coverage (WCOVERAGE < 0.18)
2 = Chi^2 is too close to chi^2 for the next best fit (within 0.01
in the reduced chi^2)
3 = Synthetic spectrum is negative (only set for stars and QSO's)
4 = Fraction of points above 5 sigma is too large (> 5%)
5 = Chi^2 minimum was at the edge of the redshift-fitting range,
resulting in Z_ERR being set to -1
6 = Negative emission in a QSO line, triggered only in QSO spectra
iff C_IV, C_III, Mg_II, H_beta, or H_alpha has
LINEAREA + 3 * LINEAREA_ERR < 0
|
| SN_MEDIAN | Median S/N for all good pixels |
| CHI68P | 68-th percentile value of abs(χ) of the best-fit synthetic spectrum to the actual spectrum, which would be 1.0 for a good fit if the errors are properly normalized. |
| FRACNSIGMA | Fraction of pixels deviant by more than N sigma, where N=[1,2,...10] (ignoring all points blueward of rest-frame 1216 Ang) |
| FRACNSIGHI | Fraction of pixels high by more than N sigma, where N=[1,2,...10] (ignoring all points blueward of rest-frame 1216 Ang) |
| FRACNSIGLO | Fraction of pixels low by more than N sigma, where N=[1,2,...10] (ignoring all points blueward of rest-frame 1216 Ang) (incorrectly computed for versions of the code before v4_9_10) |
| SPECTROFLUX | 5-element array of integrated flux in each of the 5 SDSS imaging
filters (ugriz); the units are nanomaggies, which is 1 at 22.5
magnitude; convert to magnitudes with22.5 - 2.5 * LOG_10(SPECTROFLUX);the u-band and z-band counts are meaningless and should not be used |
| SPECTROFLUX_IVAR | The approximate error (inverse variance) in SPECTROFLUX as measured by the sky fibers; we assign identical errors in linear flux units to all fibers on a plate. |
| SPECTROSYNFLUX | Same as SPECTROFLUX, but measured using the best-fit synthetic eigen-spectrum rather than the actual data points |
| SPECTROSYNFLUX_IVAR | The approximate error (inverse variance) in SPECTROSYNFLUX as measured by the sky fibers; we assign identical errors in linear flux units to all fibers on a plate. |
| SPECTROSKYFLUX | 5-element array of the sky flux in each of the 5 SDSS imaging filters |
| ANYANDMASK | Mask bits which are set if any pixels for an object's ANDMASK have that bit set (these fields incorrect in current reductions) |
| ANYORMASK | Mask bits which are set if any pixels for an object's ORMASK have that bit set (these fields incorrect in current reductions) |
| SPEC1_G | (S/N)2 at g=20.20 for spectrograph #1 (same value for 320 fibers) |
| SPEC1_R | (S/N)2 at r=20.25 for spectrograph #1 (same value for 320 fibers) |
| SPEC1_I | (S/N)2 at i=19.90 for spectrograph #1 (same value for 320 fibers) |
| SPEC2_G | (S/N)2 at g=20.20 for spectrograph #2 (same value for 320 fibers) |
| SPEC2_R | (S/N)2 at r=20.25 for spectrograph #2 (same value for 320 fibers) |
| SPEC2_I | (S/N)2 at i=19.90 for spectrograph #2 (same value for 320 fibers) |
| ELODIE_FILENAME | File name for best-fit Elodie star |
| ELODIE_OBJECT | Star name (mostly Henry Draper names) |
| ELODIE_SPTYPE | Spectral type |
| ELODIE_BV | (B-V) color |
| ELODIE_TEFF | Effective temperature |
| ELODIE_LOGG | Log10(gravity) |
| ELODIE_FEH | [Fe/H] |
| ELODIE_Z | Redshift |
| ELODIE_Z_ERR | Redshift error; negative for invalid fit |
| ELODIE_Z_MODELERR | The standard deviation in redshift amongst the 12 best-fit stars |
| ELODIE_RCHI2 | Reduced χ2 |
| ELODIE_DOF | Degrees of freedom for fit |
| VELOCITY_TAI | Timestamp for each exposure [sec] |
| VELOCITY | Velocity for each exposure [km/s], where the first exposure should be zero within roundoff |
| VELOCITY_ERR | Error in VELOCITY [km/s] |
| VELOCITY_COVAR | Covariance matrix for VELOCITY, where the square root of the diagonal elements gives the formal 1-sigma statistical errors |
SIMPLE = T / FIT STANDARD BITPIX = 16 / FITS BITS/PIXEL NAXIS = 0 / NUMBER OF AXES EXTEND = T / TAI = 4482194319.54 / 1st row - Number of seconds since Nov 17 1858 RA = 28.656976 / 1st row - Right ascension of telescope boresigh DEC = 13.804520 / 1st row - Declination of telescope boresight (d EQUINOX = 2000.00 / RADECSYS= 'FK5 ' / AZ = 306.432220000 / 1st row - Azimuth (encoder) of tele (0=N?) (de ALT = 61.3134576667 / 1st row - Altitude (encoder) of tele (de AIRMASS = 1.10307 / FOCUS = -999999999999.999999 / 1st row - Focus piston (microns?) DATE-OBS= '2000-11-29' / 1st row - TAI date TAIHMS = '05:40:17.51' / 1st row - TAI time (HH:MM:SS.SS) (TAI-UT = appr TIMESYS = 'tai ' / TAI, not UTC TAI-BEG = 4482192260.00 / Exposure Start Time TAI-END = 4482195390.00 / Exposure End Time MJD = 51877 / MJD of observation MJDLIST = '51877 ' / VERSION = 'v3_19_1 ' / version of IOP CAMVER = 'SPEC2 v4_5' / Camera code version OBSERVER= 'harvanek' OBSCOMM = 'science ' TELESCOP= 'SDSS 2.5-M' / Sloan Digital Sky Survey NEXP = 12 / Number of exposures in this file BESTEXP = 7251 / EXPID01 = 'b1-00007250-00007254-00007255' / ID string for exposure 1 EXPID02 = 'b1-00007251-00007254-00007255' / ID string for exposure 2 EXPID03 = 'b1-00007252-00007254-00007255' / ID string for exposure 3 EXPID04 = 'b2-00007250-00007254-00007255' / ID string for exposure 4 EXPID05 = 'b2-00007251-00007254-00007255' / ID string for exposure 5 EXPID06 = 'b2-00007252-00007254-00007255' / ID string for exposure 6 EXPID07 = 'r1-00007250-00007254-00007255' / ID string for exposure 7 EXPID08 = 'r1-00007251-00007254-00007255' / ID string for exposure 8 EXPID09 = 'r1-00007252-00007254-00007255' / ID string for exposure 9 EXPID10 = 'r2-00007250-00007254-00007255' / ID string for exposure 10 EXPID11 = 'r2-00007251-00007254-00007255' / ID string for exposure 11 EXPID12 = 'r2-00007252-00007254-00007255' / ID string for exposure 12 NEXP_B1 = 3 / b1 camera number of exposures NEXP_B2 = 3 / b2 camera number of exposures NEXP_R1 = 3 / r1 camera number of exposures NEXP_R2 = 3 / r2 camera number of exposures EXPT_B1 = 2700.00 / b1 camera exposure time (seconds) EXPT_B2 = 2700.00 / b2 camera exposure time (seconds) EXPT_R1 = 2700.00 / r1 camera exposure time (seconds) EXPT_R2 = 2700.00 / r2 camera exposure time (seconds) EXPTIME = 2700.00 / Minimum of exposure times for all cameras SPCOADD = 'Fri May 11 07:26:36 2007' / SPCOADD finished FLAVOR = 'science ' / Flavor of this sequence (e.g., dome flat, etc.) QUALITY = 'excellent' / night/image quality RADEG = 2.86571000000000E+01 / Right Ascension. (degrees) DECDEG = 1.38045200000000E+01 / Declination. (degrees) PLATEID = 430 / Plate Id TILEID = 208 / Tile Id CARTID = 5 /Cartridge used in this plugging MAPID = 5187701 / Map Id NAME = '0430-51877-01' / Name of target; PlateId-MJD-Mapper ReRun NGUIDE = 21.0000 / Number of guider frames during exposure SEEING20= 2.08333 / 20% seeing during exposure (arcsec) SEEING50= 2.20333 / 50% seeing during exposure (arcsec) SEEING80= 2.36333 / 80% seeing during exposure (arcsec) RMSOFF20= 0.128227666667 / 20% RMS offset of guide fibers (arcsec) RMSOFF50= 0.251879666667 / 50% RMS offset of guide fibers (arcsec) RMSOFF80= 0.442921666667 / 80% RMS offset of guide fibers (arcsec) COLBIN = 1 / Binning factor perpendicular to the columns ROWBIN = 1 / Binning factor perpendicular to the rows PROGRAM = 'binning 1 1 ' / Identifying name for CCD program SECFOCUS= -1.3000000000000E+02 / Secondary Mirror Position as reported by TCC GUIDEIMG= '/data/spectro/guider/gimg0756.fits' / Last archived guider image WTIME = 975476788.000 / weatherData(timeStamp) AIRTEMP = 5.30000000000 / weatherData(airtemp) DEWPOINT= -8.20000000000 / weatherData(dewpoint) DEWDEP = 13.5000000000 / weatherData(dewpointDep) DUSTA = 5254.00000000 / weatherData(dusta) DUSTB = 135.666666667 / weatherData(dustb) DUSTC = 6086.33333333 / weatherData(dustc) DUSTD = 155.000000000 / weatherData(dustd) GUSTD = 7.95000000000000E+01 / weatherData(gustd) GUSTS = 11.7000000000 / weatherData(gusts) HUMIDITY= 37.0666666667 / weatherData(humidity) HUMIDOUT= 36.3333333333 / weatherData(humidout) PRESSURE= 21.5700000000 / weatherData(pressure) WINDD = 87.0666666667 / weatherData(windd) WINDS = 8.83333333333 / weatherData(winds) TEMP01 = -94.1400000000 / CCD 01 Temperature TEMP02 = -92.9700000000 / CCD 02 Temperature TEMP03 = -92.5800000000 / CCD 03 Temperature TEMP04 = -93.4900000000 / CCD 04 Temperature AUTHOR = 'Scott Burles & David Schlegel' / VERSIDL = '6.3 ' / Version of IDL VERSUTIL= 'v5_2_0 ' / Version of idlutils VERSREAD= 'v5_3_3 ' / Version of idlspec2d for pre-processing raw dat VERS2D = 'v5_3_3 ' / Version of idlspec2d for 2D reduction VERSCOMB= 'v5_3_2 ' / Version of idlspec2d for combining multiple spe VERS1D = 'v5_3_2 ' /Version of idlspec2d for 1D reduction VERSLOG = 'fermi-CVS 05/11/07' / Version of SPECLOG product VERSFLAT= 'v1_7 ' / Version of SPECFLAT product OPBC = 'opBC-51813.par' / OPCONFIG= 'opConfig-50000.par' / OPECALIB= 'opECalib-51577.par' / XSIGMA = 0.938221750000 / XSIGMIN = 0.904645000000 / XSIGMAX = 0.997335000000 / WSIGMA = 0.890092998379 / WSIGMIN = 0.845413000000 / WSIGMAX = 1.00929999352 / PLUGFILE= 'plPlugMapM-0430-51877-01.par' / LAMPLIST= 'lamphgcdne.dat' / SKYLIST = 'skylines.dat' / HELIO_RV= 18.0336065943 / Heliocentric correction (added to velocities) VACUUM = T / Wavelengths are in vacuum SFLATTEN= T / Superflat has been applied PSFSKY = 3 / Order of PSF skysubtraction SKYCHI2 = 1.08416902433 / Mean chi^2 of sky-subtraction SCHI2MIN= 1.05534681302 / SCHI2MAX= 1.17834241969 / PREJECT = 0.200000 / Profile area rejection threshold SPEC1_G = 17.7522 /(S/N)^2 for spec 1 at mag 20.20 SPEC1_R = 18.6219 /(S/N)^2 for spec 1 at mag 20.25 SPEC1_I = 17.6288 /(S/N)^2 for spec 1 at mag 19.90 SPEC2_G = 16.2644 /(S/N)^2 for spec 2 at mag 20.20 SPEC2_R = 15.6690 /(S/N)^2 for spec 2 at mag 20.25 SPEC2_I = 13.8085 /(S/N)^2 for spec 2 at mag 19.90 NSTD = 16 / Number of (good) std stars GOFFSTD = -0.0162220 / Spectrophoto offset for std stars in G-band GRMSSTD = 0.0757010 / Spectrophoto RMS for std stars in G-band ROFFSTD = -0.0105619 / Spectrophoto offset for std stars in R-band RRMSSTD = 0.0487866 / Spectrophoto RMS for std stars in R-band IOFFSTD = -0.0130701 / Spectrophoto offset for std stars in I-band IRMSSTD = 0.0493715 / Spectrophoto RMS for std stars in I-band GROFFSTD= -0.0187340 / Spectrophoto offset for std stars in (GR) GRRMSSTD= 0.0497939 / Spectrophoto RMS for std stars in (GR) RIOFFSTD= 0.0102034 / Spectrophoto offset for std stars in (RI) RIRMSSTD= 0.0328852 / Spectrophoto RMS for std stars in (RI) NGAL = 417 / Number of (good) main galaxies GOFFGAL = 0.00672913 / Spectrophoto offset for main galaxies in G-band GRMSGAL = 0.0455279 / Spectrophoto RMS for main galaxies in G-band ROFFGAL = 0.00734711 / Spectrophoto offset for main galaxies in R-band RRMSGAL = 0.0433952 / Spectrophoto RMS for main galaxies in R-band IOFFGAL = 0.00634956 / Spectrophoto offset for main galaxies in I-band IRMSGAL = 0.0454840 / Spectrophoto RMS for main galaxies in I-band GROFFGAL= 0.00297165 / Spectrophoto offset for main galaxies in (GR) GRRMSGAL= 0.0415170 / Spectrophoto RMS for main galaxies in (GR) RIOFFGAL= -0.00133705 / Spectrophoto offset for main galaxies in (RI) RIRMSGAL= 0.0243410 / Spectrophoto RMS for main galaxies in (RI) LOWREJ = 5 / Extraction: low rejection HIGHREJ = 8 / Extraction: high rejection SCATPOLY= 0 / Extraction: Order of scattered light polynomial PROFTYPE= 3 / Extraction profile: 1=Gaussian NFITPOLY= 1 / Extraction: Number of parameters in each profil XCHI2 = 1.20192 / Extraction: Mean chi^2 XCHI2MIN= 1.12970 / XCHI2MAX= 1.28281 / NWORDER = 2 / Linear-log10 coefficients WFITTYPE= 'LOG-LINEAR' / Linear-log10 dispersion COEFF0 = 3.58000000000 / Central wavelength (log10) of first pixel COEFF1 = 0.000100000000000 / Log10 dispersion per pixel UNAME = 'fnpc217.fnal.gov' / FBADPIX = 0.0114787 / Fraction of bad pixels FBADPIX1= 0.00687047 / Fraction of bad pixels on spectro-1 FBADPIX2= 0.0160869 / Fraction of bad pixels on spectro-2 WAT0_001= 'system=linear' / WAT1_001= 'wtype=linear label=Wavelength units=Angstroms' / CRVAL1 = 3.58000000000 / Central wavelength (log10) of first pixel CD1_1 = 0.000100000000000 / Log10 dispersion per pixel CRPIX1 = 1 / Starting pixel (1-indexed) CTYPE1 = 'LINEAR ' / DC-FLAG = 1 / Log-linear flag BUNIT = '1E-17 erg/cm^2/s/Ang' /
XTENSION= 'BINTABLE' /Binary table written by MWRFITS v1.4a BITPIX = 8 /Required value NAXIS = 2 /Required value NAXIS1 = 998 /Number of bytes per row NAXIS2 = 640 /Number of rows PCOUNT = 0 /Normally 0 (no varying arrays) GCOUNT = 1 /Required value TFIELDS = 61 /Number of columns in table COMMENT COMMENT *** End of mandatory fields *** COMMENT * COMMENT *** Column names *** COMMENT TTYPE1 = 'PLATE ' / TTYPE2 = 'TILE ' / TTYPE3 = 'MJD ' / TTYPE4 = 'FIBERID ' / TTYPE5 = 'OBJID ' / TTYPE6 = 'OBJTYPE ' / TTYPE7 = 'PLUG_RA ' / TTYPE8 = 'PLUG_DEC ' / TTYPE9 = 'CLASS ' / TTYPE10 = 'SUBCLASS ' / TTYPE11 = 'Z ' / TTYPE12 = 'Z_ERR ' / TTYPE13 = 'RCHI2 ' / TTYPE14 = 'DOF ' / TTYPE15 = 'RCHI2DIFF ' / TTYPE16 = 'TFILE ' / TTYPE17 = 'TCOLUMN ' / TTYPE18 = 'NPOLY ' / TTYPE19 = 'THETA ' / TTYPE20 = 'THETA_COVAR ' / TTYPE21 = 'VDISP ' / TTYPE22 = 'VDISP_ERR ' / TTYPE23 = 'VDISPZ ' / TTYPE24 = 'VDISPZ_ERR ' / TTYPE25 = 'VDISPCHI2 ' / TTYPE26 = 'VDISPNPIX ' / TTYPE27 = 'VDISPDOF ' / TTYPE28 = 'WAVEMIN ' / TTYPE29 = 'WAVEMAX ' / TTYPE30 = 'WCOVERAGE ' / TTYPE31 = 'ZWARNING ' / TTYPE32 = 'SN_MEDIAN ' / TTYPE33 = 'CHI68P ' / TTYPE34 = 'FRACNSIGMA ' / TTYPE35 = 'FRACNSIGHI ' / TTYPE36 = 'FRACNSIGLO ' / TTYPE37 = 'SPECTROFLUX ' / TTYPE38 = 'SPECTROFLUX_IVAR ' / TTYPE39 = 'SPECTROSYNFLUX ' / TTYPE40 = 'SPECTROSYNFLUX_IVAR ' / TTYPE41 = 'SPECTROSKYFLUX ' / TTYPE42 = 'ANYANDMASK ' / TTYPE43 = 'ANYORMASK ' / TTYPE44 = 'SPEC1_G ' / TTYPE45 = 'SPEC1_R ' / TTYPE46 = 'SPEC1_I ' / TTYPE47 = 'SPEC2_G ' / TTYPE48 = 'SPEC2_R ' / TTYPE49 = 'SPEC2_I ' / TTYPE50 = 'ELODIE_FILENAME ' / TTYPE51 = 'ELODIE_OBJECT ' / TTYPE52 = 'ELODIE_SPTYPE ' / TTYPE53 = 'ELODIE_BV ' / TTYPE54 = 'ELODIE_TEFF ' / TTYPE55 = 'ELODIE_LOGG ' / TTYPE56 = 'ELODIE_FEH ' / TTYPE57 = 'ELODIE_Z ' / TTYPE58 = 'ELODIE_Z_ERR ' / TTYPE59 = 'ELODIE_Z_MODELERR ' / TTYPE60 = 'ELODIE_RCHI2 ' / TTYPE61 = 'ELODIE_DOF ' / COMMENT COMMENT *** Column formats *** COMMENT TFORM1 = 'J ' / TFORM2 = 'J ' / TFORM3 = 'J ' / TFORM4 = 'J ' / TFORM5 = '5J ' / TFORM6 = '18A ' / TFORM7 = 'D ' / TFORM8 = 'D ' / TFORM9 = '6A ' / TFORM10 = '19A ' / TFORM11 = 'E ' / TFORM12 = 'E ' / TFORM13 = 'E ' / TFORM14 = 'J ' / TFORM15 = 'E ' / TFORM16 = '24A ' / TFORM17 = '10J ' / TFORM18 = 'J ' / TFORM19 = '10E ' / TFORM20 = '100E ' / TFORM21 = 'E ' / TFORM22 = 'E ' / TFORM23 = 'E ' / TFORM24 = 'E ' / TFORM25 = 'E ' / TFORM26 = 'E ' / TFORM27 = 'J ' / TFORM28 = 'E ' / TFORM29 = 'E ' / TFORM30 = 'E ' / TFORM31 = 'J ' / TFORM32 = 'E ' / TFORM33 = 'E ' / TFORM34 = '10E ' / TFORM35 = '10E ' / TFORM36 = '10E ' / TFORM37 = '5E ' / TFORM38 = '5E ' / TFORM39 = '5E ' / TFORM40 = '5E ' / TFORM41 = '5E ' / TFORM42 = 'J ' / TFORM43 = 'J ' / TFORM44 = 'E ' / TFORM45 = 'E ' / TFORM46 = 'E ' / TFORM47 = 'E ' / TFORM48 = 'E ' / TFORM49 = 'E ' / TFORM50 = '16A ' / TFORM51 = '9A ' / TFORM52 = '10A ' / TFORM53 = 'E ' / TFORM54 = 'E ' / TFORM55 = 'E ' / TFORM56 = 'E ' / TFORM57 = 'E ' / TFORM58 = 'E ' / TFORM59 = 'E ' / TFORM60 = 'E ' / TFORM61 = 'J ' / COMMENT COMMENT *** Column dimensions (2 D or greater) *** COMMENT TDIM20 = '( 10, 10)' /
Best-fit SDSS template spectrum, in units of 1E-17 erg/cm^2/s/Ang.
XTENSION= 'IMAGE ' /Image Extension created by MWRFITS v1.4a BITPIX = -32 / NAXIS = 2 / NAXIS1 = 3863 / NAXIS2 = 640 / PCOUNT = 0 / GCOUNT = 1 /
Best-fit velocity dispersion template spectrum for galaxies, in units of 1E-17 erg/cm^2/s/Ang. For testing purposes only; not for doing science.
XTENSION= 'IMAGE ' /Image Extension created by MWRFITS v1.4a BITPIX = -32 / NAXIS = 2 / NAXIS1 = 3863 / NAXIS2 = 640 / PCOUNT = 0 / GCOUNT = 1 /