1. General object description: Col.# 1:Nr Unit: Format:I8 I*4 object number Col.# 2:ID Unit: Format:A10 C*1 Col.# 3:CLASS Unit: Format:A12 C*8 morphology class = s/g/u Col.# 4:X Unit:arcsec Format:F10.2 R*4 x-position on deep R-frame Col.# 5:Y Unit:arcsec Format:F10.2 R*4 y-position on deep R-frame Col.# 6:CLASS_VAL Unit: Format:I9 I*4 stellarity index 0..1000 Col.# 7:MORPH1 Unit: Format:F7.2 R*4 major axis Col.# 8:MORPH2 Unit: Format:F7.2 R*4 minor axis Col.# 9:MORPH3 Unit: Format:F7.1 R*4 axis angle Col.# 10:FLAG_all Unit: Format:I8 I*4 warning flags, 0..7=mostly ok Col.# 29:mag_best Unit: Format:F7.3 R*4 R-band SExtractor-MAG_BEST Col.# 227:mag_best_err Unit: Format:F7.3 R*4 error of MAG_BEST in mag Col.# 30:add_m_best Unit: Format:E12.6 R*4 Aperture correction (mag) Col.# 31:varflag Unit: Format:I11 I*4 variability flag 0 / >=1 Col.# 32:r_a Unit: Format:R12.7 R*8 right ascension (J2000) Col.# 33:dec Unit: Format:S12.6 R*8 declination (J2000) Col.# 229:mu_max Unit: Format:E12.6 R*4 R-band cen. surf. brightness 2. Classification columns (see MCCLASS/CLASSIFY) Col.# 11:MC_class Unit: Format:A16 C*16 object class by multi-colour Col.# 12:MC_z Unit: Format:F7.3 R*4 mean redshift (galaxy/QSO only) Col.# 13:MC_sz Unit: Format:F7.3 R*4 redshift error (1-sigma) Col.# 14:MC_z_bin Unit: Format:I8 I*4 redshift bimodality flag Col.# 15:MC_gSED Unit: Format:F8.1 R*4 mean SED type (galaxy only) Col.# 16:MC_sgSED Unit: Format:F8.1 R*4 SED type error (1-sigma) Col.# 515:MC_gSED2 Unit: Format:F8.1 R*4 mean SED2 type (galaxy only) Col.# 516:MC_sgSED2 Unit: Format:F8.1 R*4 SED2 type error (1-sigma) Col.# 17:MC_z_ml Unit: Format:F8.3 R*4 probability peak in redshift Col.# 18:MC_gSED_ml Unit: Format:I10 I*4 probability peak in SED Col.# 518:MC_gSED2_ml Unit: Format:I10 I*4 probability peak in SED2 Col.# 12:MC_z2 Unit: Format:F7.3 R*4 2nd guess redshift if ambiguous Col.# 13:MC_sz2 Unit: Format:F7.3 R*4 2nd guess redshift error Col.# 477:chi2red Unit: Format:F7.3 R*4 chi-squared/Nf of best-fit Col.# 19:MC_dist Unit:sigma Format:F8.2 R*4 strangeness in colour space, normalised to sigma(obj-templ) Col.# 20:prob_star Unit:% Format:F9.1 R*4 probability to be a FGKM star Col.# 21:prob_gal Unit:% Format:F9.1 R*4 probability to be a galaxy Col.# 22:prob_qso Unit:% Format:F9.1 R*4 probability to be a quasar Col.# 28:prob_wd Unit:% Format:F9.1 R*4 probability to be a blue star Col.# 23:MC_nextlib Unit: Format:I11 I*4 library ID of best-fitting Col.# 24:MC_next_0 Unit: Format:I10 I*4 template and its 4-D index Col.# 25:MC_next_1 Unit: Format:I10 I*4 position Col.# 26:MC_next_2 Unit: Format:I10 I*4 Col.# 27:MC_next_3 Unit: Format:I10 I*4 3. Galaxy restframe luminosities Col.# 34:dl_37 Unit:Mpc Format:F8.1 R*8 luminosity distance 0.3/0.7 Col.# 35:dl_01 Unit:Mpc Format:F8.1 R*4 luminosity distance 0.2/0.0 Col.# 36:dl_05 Unit:Mpc Format:F8.1 R*4 luminosity distance 1.0/0.0 all for H_0=100 km/sec/Mpc Col.# 337:muc_37 Unit:mag Format:F7.2 R*8 M_280/40 (Vega-mag) Col.# 338:muj_37 Unit:mag Format:F7.2 R*8 M_Johnson-U Col.# 339:mbj_37 Unit:mag Format:F7.2 R*8 M_Johnson-B Col.# 340:mvj_37 Unit:mag Format:F7.2 R*8 M_Johnson-V Col.# 341:mus_37 Unit:mag Format:F7.2 R*8 M_SDSS-u Col.# 342:mgs_37 Unit:mag Format:F7.2 R*8 M_SDSS-g Col.# 343:mrs_37 Unit:mag Format:F7.2 R*8 M_SDSS-r Col.# 338:mub_37 Unit:mag Format:F7.2 R*8 M_Bessell-U Col.# 339:mbb_37 Unit:mag Format:F7.2 R*8 M_Bessell-B Col.# 340:mvb_37 Unit:mag Format:F7.2 R*8 M_Bessell-V Col.# 537:smuc_37 Unit:mag Format:F7.2 R*8 error of M_280/40 (Vega-mag) Col.# 538:smuj_37 Unit:mag Format:F7.2 R*8 error of M_Johnson-U Col.# 539:smbj_37 Unit:mag Format:F7.2 R*8 error of M_Johnson-B Col.# 540:smvj_37 Unit:mag Format:F7.2 R*8 error of M_Johnson-V Col.# 541:smus_37 Unit:mag Format:F7.2 R*8 error of M_SDSS-u Col.# 542:smgs_37 Unit:mag Format:F7.2 R*8 error of M_SDSS-g Col.# 543:smrs_37 Unit:mag Format:F7.2 R*8 error of M_SDSS-r Col.# 538:smub_37 Unit:mag Format:F7.2 R*8 error of M_Bessell-U Col.# 539:smbb_37 Unit:mag Format:F7.2 R*8 error of M_Bessell-B Col.# 540:smvb_37 Unit:mag Format:F7.2 R*8 error of M_Bessell-V Col.# 601:rf_umv Unit:mag Format:F7.2 R*8 restframe colour U-V Johnson Col.# 601:smrf_umv Unit:mag Format:F7.2 R*8 error of restframe colour U-V ... some more of those colour indices, their errors are different from the squared sum of the restframe luminosities as the total mag does not matter. 3b. Quasar restframe luminosities Col.# 337:m145_37 Unit:mag Format:F7.2 R*8 M_145/4 (Vega-mag) Col.# 337:sm145_37 Unit:mag Format:F7.2 R*8 error of M_145/4 (mag) 4. More classification columns, also needed for plotting filter spectra Col.# 42:gz_ml Unit:Unitless Format:F5.3 R*4 see classification for details Col.# 43:qz_ml Unit: Format:E12.6 R*4 Col.# 44:sdmg Unit:sigma Format:F6.1 R*4 Col.# 45:gdmg Unit:sigma Format:F6.1 R*4 Col.# 46:qdmg Unit:sigma Format:F6.1 R*4 Col.# 47:wdmg Unit:sigma Format:F6.1 R*4 Col.# 48:gdmg1 Unit:Unitless Format:I5 I*4 Col.# 49:qdmg1 Unit:Unitless Format:I5 I*4 Col.# 50:qdmg2 Unit:Unitless Format:I5 I*4 Col.# 51:sdmg3 Unit:Unitless Format:I5 I*4 Col.# 52:wdmg3 Unit:Unitless Format:I5 I*4 Col.# 53:gdmnr Unit:Unitless Format:I5 I*4 Col.# 54:qdmnr Unit:Unitless Format:I5 I*4 5. Photometric measurements - for every observed filter there is a block of columns like the example given below - identifiers (420E e.g.) are composed of a filter name (420, R__, B__, 646, etc.) and a letter denominating the observing run (A = Feb 1999 ... G = Feb 2001) - observing run "S" denotes combined sum measurement of all runs for a given filter - a given filter observed in different runs can show variation due to long-term variability Col.# 55:_Fk420E Unit:phot/m^2/s/nm Format:E12.4 R*4 measured aperture flux Col.# 56:sFk420E Unit:phot/m^2/s/nm Format:E12.4 R*4 measured flux error Col.# 57:_M_420E Unit:mag Format:F10.3 R*4 measured aperture magnitude Col.# 58:sM_420E Unit:mag Format:F10.3 R*4 measured magnitude error Col.# 59:_Fk464E Unit:phot/m^2/s/nm Format:E12.4 R*4 Col.# 60:sFk464E Unit:phot/m^2/s/nm Format:E12.4 R*4 Col.# 61:_M_464E Unit:mag Format:F10.3 R*4 Col.# 62:sM_464E Unit:mag Format:F10.3 R*4 Col.# 63:_Fk485D Unit:phot/m^2/s/nm Format:E12.4 R*4 Col.# 64:sFk485D Unit:phot/m^2/s/nm Format:E12.4 R*4 Col.# 65:_M_485D Unit:mag Format:F10.3 R*4 Col.# 66:sM_485D Unit:mag Format:F10.3 R*4 ...followed by several more 4-column blocks for all other filters. Extension: ---------- The full catalogue versions known as "FLUX" tables contain many more columns of rather technical meaning and they are usually not relevant for team members. However, if you do require to use them, consult the classification page or the responsible people creating the columns. In the following list column numbers are not to be relied upon as they are taken from various tables. 6. Classification columns for emission-line galaxies (by Hans and Klaus) Col.# 35:flag_A Unit: Format:I6 I*4 Col.# 36:maxFsg_A Unit: Format:F8.2 R*4 Col.# 37:ELflag_A Unit: Format:I8 I*4 Col.# 38:maxsgn_A Unit: Format:F8.2 R*4 Col.# 39:ELclss_A Unit: Format:A12 C*12 Col.# 40:EL_z_A Unit: Format:F8.3 R*4 Col.# 41:Sline_A Unit:W/m^2 Format:E12.4 R*4 Col.# 42:flag_B Unit: Format:I6 I*4 Col.# 43:maxFsg_B Unit: Format:F8.2 R*4 Col.# 44:ELflag_B Unit: Format:I8 I*4 Col.# 45:maxsgn_B Unit: Format:F8.2 R*4 Col.# 46:ELclss_B Unit: Format:A12 C*12 Col.# 47:EL_z_B Unit: Format:F8.3 R*4 Col.# 48:Sline_B Unit:W/m^2 Format:E12.4 R*4 Col.# 49:flag_C Unit: Format:I6 I*4 Col.# 50:maxFsg_C Unit: Format:F8.2 R*4 Col.# 51:ELflag_C Unit: Format:I8 I*4 Col.# 52:maxsgn_C Unit: Format:F8.2 R*4 Col.# 53:ELclss_C Unit: Format:A12 C*12 Col.# 54:EL_z_C Unit: Format:F8.3 R*4 Col.# 55:Sline_C Unit:W/m^2 Format:E12.4 R*4 Col.# 56:rflx_NR Unit: Format:I8 I*4 Col.# 57:rflx_ID Unit: Format:A8 C*8 Col.# 58:rflx_DX Unit:arcsec Format:F8.2 R*4 Col.# 59:rflx_DY Unit:arcsec Format:F8.2 R*4 Col.# 60:rflx_LIM Unit:ph/m^2/s/nm Format:E10.4 R*4 Col.# 61:rflx_FLX Unit:ph/m^2/s/nm Format:E10.4 R*4 Col.# 62:SCRATCH1 Unit: Format:G12.4 R*4 Col.# 63:SCRATCH2 Unit: Format:G12.4 R*4 7. More photometric measurements - for every observed filter there is a block of columns like the example given below - identifiers (420E e.g.) are composed of a filter name (420, R__, B__, 646, etc.) and a letter denominating the observing run (A = Feb 1999 ... G = Feb 2001) - observing run "S" denotes combined sum measurement of all runs for a given filter - a given filter observed in different runs can show variation due to long-term variability Col.# 64:_F_420E Unit:phot/m^2/s/nm Format:E12.4 R*4 measured aperture flux Col.# 65:sF_420E Unit:phot/m^2/s/nm Format:E12.4 R*4 pure photon noise Col.# 66:sFc420E Unit:phot/m^2/s/nm Format:E12.4 R*4 most likely error Col.# 67:_Fm420E Unit:phot/m^2/s/nm Format:E12.4 R*4 Col.# 68:sFm420E Unit:phot/m^2/s/nm Format:E12.4 R*4 Col.# 69:_Fk420E Unit:phot/m^2/s/nm Format:E12.4 R*4 Col.# 70:vld420E Unit:fraction Format:F10.3 R*4 Col.# 71:chi2420E Unit: Format:E12.4 R*4 Col.# 72:det_420E Unit: Format:A8 C*8 Col.# 73:cosI420E Unit: Format:E12.4 R*4 Col.# 74:cosN420E Unit: Format:I4 I*4 Col.# 75:trns420E Unit: Format:E12.4 R*4 Col.# 76:_M_420E Unit:mag Format:F10.3 R*4 aperture magnitude (Vega) Col.# 77:sM_420E Unit:mag Format:F10.3 R*4 error of magnitude Col.# 78:sc1420E Unit: Format:E12.4 R*4 Col.# 79:sc2420E Unit: Format:E12.4 R*4 8. Colour indices and their errors (s_*) - constructed from the photometric measurements above (see MCCLASS/COLORS) - corrected for long-term variability and galactic extinction Col.# 495:wufmwb Unit:CDmag Format:F6.2 R*4 Col.# 496:wugmwb Unit:CDmag Format:F6.2 R*4 Col.# 497:s_wufmwb Unit:mag Format:F6.2 R*4 Col.# 498:s_wugmwb Unit:mag Format:F6.2 R*4 Col.# 499:wumwb Unit:CDmag Format:F6.2 R*4 Col.# 500:s_wumwb Unit:mag Format:F6.2 R*4 Col.# 501:wbmwv Unit:CDmag Format:F6.2 R*4 Col.# 502:wvmwr Unit:CDmag Format:F6.2 R*4 Col.# 503:wrmwi Unit:CDmag Format:F6.2 R*4 Col.# 504:w418mb Unit:CDmag Format:F6.2 R*4 Col.# 505:bmw464 Unit:CDmag Format:F6.2 R*4 Col.# 506:bmw486 Unit:CDmag Format:F6.2 R*4 Col.# 507:w520mr Unit:CDmag Format:F6.2 R*4 Col.# 508:w573dmr Unit:CDmag Format:F6.2 R*4 Col.# 509:w573emr Unit:CDmag Format:F6.2 R*4 Col.# 510:s_w573dmr Unit:mag Format:F6.2 R*4 Col.# 511:s_w573emr Unit:mag Format:F6.2 R*4 Col.# 512:w573mr Unit:CDmag Format:F6.2 R*4 Col.# 513:s_w573mr Unit:mag Format:F6.2 R*4 Col.# 514:w605mr Unit:CDmag Format:F6.2 R*4 Col.# 515:w643mr Unit:CDmag Format:F6.2 R*4 Col.# 516:rmw697 Unit:CDmag Format:F6.2 R*4 Col.# 517:rmw752 Unit:CDmag Format:F6.2 R*4 Col.# 518:rmw816 Unit:CDmag Format:F6.2 R*4 Col.# 519:imw856 Unit:CDmag Format:F6.2 R*4 Col.# 520:imw915 Unit:CDmag Format:F6.2 R*4 Col.# 521:s_wbmwv Unit:mag Format:F6.2 R*4 Col.# 522:s_wvmwr Unit:mag Format:F6.2 R*4 Col.# 523:s_wrmwi Unit:mag Format:F6.2 R*4 Col.# 524:s_w418mb Unit:mag Format:F6.2 R*4 Col.# 525:s_bmw464 Unit:mag Format:F6.2 R*4 Col.# 526:s_bmw486 Unit:mag Format:F6.2 R*4 Col.# 527:s_w520mr Unit:mag Format:F6.2 R*4 Col.# 528:s_w605mr Unit:mag Format:F6.2 R*4 Col.# 529:s_w643mr Unit:mag Format:F6.2 R*4 Col.# 530:s_rmw697 Unit:mag Format:F6.2 R*4 Col.# 531:s_rmw752 Unit:mag Format:F6.2 R*4 Col.# 532:s_rmw816 Unit:mag Format:F6.2 R*4 Col.# 533:s_imw856 Unit:mag Format:F6.2 R*4 Col.# 534:s_imw915 Unit:mag Format:F6.2 R*4 Col.# 582:w486mv Unit:CDmag Format:F6.2 R*4 Col.# 583:w520mv Unit:CDmag Format:F6.2 R*4 Col.# 584:s_w486mv Unit:mag Format:F6.2 R*4 Col.# 585:s_w520mv Unit:mag Format:F6.2 R*4
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Last update Feb 5, 2004, CW