measured ----------- SDSS_RA F SDSS_DEC F SDSS_Z F PLATEID F FIBERID F MJD F E_BV F ;galex supplied value FUV_MAG F ;AB magnitudes, exinction corrected by david schiminovich's algorithm. Set to 0. for undetected and unobserved sources FUV_MAGERR F ;AB magnitude errors, from david schiminovich's algorithm. FUV_WEIGHT F NUV_MAG F NUV_MAGERR F NUV_WEIGHT F U_MAG F ;AB petrosian magnitudes (fnal), galactic extinction corrected (petromag_u-extinction_u) U_MAGERR F G_MAG F G_MAGERR F R_MAG F R_MAGERR F I_MAG F I_MAGERR F Z_MAG F Z_MAGERR F J_MAG F J_MAGERR F H_MAG F H_MAGERR F K_MAG F K_MAGERR F S3pt6_MAG F ;AB magnitudes, =2.5*log(f(microJy))+Const. Set to 0 for unobserved or 'negative' flux sources S3pt6_MAGERR F ;=2.5*log(1+flux_err/flux) errors are wrong for 24 micron S4pt5_MAG F S4pt5_MAGERR F S5pt6_MAG F S5pt6_MAGERR F S7pt8_MAG F S7pt8_MAGERR F S24_MAG F S24_MAGERR F S70_MAG F S70_MAGERR F UV_COVERAGE F ;distance from center of 'nearest' galex image, arcseconds (=0 if not in galex) UV_FLAGS F ;empty for now UV_MATCH_FLAG F ;number of uv matches within 3" of the SDSS object. DIST_UV F ;distance of closest match from the SDSS object, arcsec IR_COVERAGE F ;sum over i of (2*i_band) where i_band=1,2... for 3.6 micron, 4.5 micron, 5.8 micron etc. IR_FLAGS F ;photometry flags, empty for now SDSS_FLAGS A ;the flag field in PhotoObjAll; 64-bit integer (converted to string here) INDEX I ;index in the original region catalog set PETRORAD_R F (Standard stuff from SDSS catalogs) PETRORADERR_R F PETROR50_R F PETROR50ERR_R F PETROR90_R F PETROR90ERR_R F ISOA_R F ISOB_R F ISOPHI_R F OII_3726_FLUX F From gal_line file (SDSS/MPA raw) - Units are 10^-17 erg/cm^2/s. fluxes are correct (not low by 1+z) OII_3726_FLUX_ERR F OII_3729_FLUX F OII_3729_FLUX_ERR F H_BETA_FLUX F H_BETA_FLUX_ERR F OIII_5007_FLUX F OIII_5007_FLUX_ERR F H_ALPHA_FLUX F H_ALPHA_FLUX_ERR F NII_6584_FLUX F NII_6584_FLUX_ERR F SII_6717_FLUX F SII_6717_FLUX_ERR F SII_6731_FLUX F SII_6731_FLUX_ERR F derived ------------- D4N F from index file (i.e the NOT the MPA mass catalog, not NeIII corrected) HDA F from gk, corrected for emission lines A_Z_50 F d50 from gk - estimate of z band attenuation, median of PD (in mags) TAU F log(h_alpha_flux/h_beta_flux/2.88), i.e balmer decrement TAU_V F the visual band effective opacity from the best fitting charlot model LOG_M_DC F log of dust corrected stellar mass (M_sun) from gk, median of PD (rml50) Z_ABS_DC F dust corrected z' absolute magnitude from gk (rz) LOG_OH F metallicity, median from tremonti. LOGMU F SPEC_CLASS F VDISP F LUM_O3 F ;agn parameters LUM_O3_EXTCOR F LOG_O3HB F LOG_N2HA F MU F CONC F D4000N_COR F HDA_COR F SFR_MEDIAN F from Brinchmann SFR_MODE F SFR_AVG F SFR_P16 F SFR_P84 F FSFR_MEDIAN F ;within the fiber SSFR_MEDIAN F ;specific SFR FSSFR_MEDIAN F ;specific SFR within the fiber BETA F k-corrected, may be off a bit - deprecated ALPHA_IR F alpha of the dale+helou IR model SED LOG_LFIR F log of FIR (8-1000 micron) luminosity, L_sun LOG_LTIR F log of FIR (3-1100 micron) luminosity, L_sun LOG_LFUV F log of FUV luminosity, L_sun IRX F LOG_LTIR-LOG_LFUV