## Subset of objects corresponding to 766.html
##
## RELICS: Reionization Lensing Cluster Survey - Cycle 23 Hubble Treasury program (GO 14096; PI Coe)
## Photometric + Bayesian Photometric Redshift (BPZ) catalog (produced 2016-04-20 by Dan Coe)
## from 0.06"/pix images of rxc0911+17 (produced 2016-04-19)
## by Roberto Avila and Sara Ogaz (STScI)
##
## Note: photo-z estimates are intended for galaxies only
## Stars may be identified as having higher values of SExtracor stellarity
##
## Objects detected by SExtractor (version 2.19.5) in a weighted sum of ACS+IR images
## Pruned by selecting flag5sig = 0 (gets rid of cosmic rays and < 5-sigma detections)
## Position, aperture, and shape measurements determined in the detection image
##
## Photometry measured in isophotal apertures by SExtractor in dual-image mode
## For each filter, we provide:
##  - AB magnitude & uncertainty
##  - flux & uncertainty (electrons / second = native units)
##  - flux & uncertainty (nJy = nanoJanskys)
##  - detection significance
##  - zeropoints to convert native fluxes (e-/s) to AB magnitudes
##
## AB mag = zeropoint - 2.5 * log10(flux) = 31.4 - 2.5 * log10(fluxnJy)
## Magnitude uncertainties correspond to the flux 1-sigma upper limits:
##   magerr = 2.5 * log10(1 + fluxerr / flux)
##
## Both fluxes and magnitudes have been corrected for
## galactic extinction: E(B-V) = 0.03590
## based on Schlafly & Finkbeiner 2011 (ApJ 737, 103)
## extracted using http://irsa.ipac.caltech.edu/applications/DUST/docs/dustProgramInterface.html
##
## mag, magerr =  99, 1-sigma limit: non-detection (flux < 0)
## mag, magerr = -99, 0: unobserved (outside FOV, in chip gap, etc.)
##
## For each object, we also provide the brightest magnitude in any filter
## based on the highest observed flux - fluxerr (lower limit)
##
## Bayesian Photometric Redshifts are derived using BPZ (Benitez et al. 2000, 2004; Coe et al. 2006)
## These results are intended for galaxies only.
## (Stars may be pruned as having higher values of SExtractor stellarity.)
## For each object, the most likely redshift is given by zb,
## and the 95% confidence range is given by zbmin - zbmax.
## Objects with high ODDS values have sharply peaked unimodal redshift likelihood distributions.
## Objects with chisq2 < 1 generally have photometry well fit by the model SEDs.
#  1 id                Object ID Number
#  2 RA                Right Ascension in decimal degrees
#  3 Dec               Declination in decimal degrees
#  4 x                 x pixel coordinate
#  5 y                 y pixel coordinate
#  6 fwhm              Full width at half maximum (arcsec)
#  7 area              Isophotal aperture area (pixels)
#  8 stel              SExtractor "stellarity" (1 = star; 0 = galaxy)
#  9 ell               Ellipticity = 1 - B/A
# 10 flag5sig          0 = probably real; 1 = probable CR; 2 = no 5-sigma detection
# 11 nf5sig            Number of filters with a 5-sigma detection
# 12 nfcr5sig          Number of CR-vulnerable filters with a 5-sigma detection
# 13 nfobs             Number of filters observed (not in chip gap, etc.)
# 14 f555w_mag         F555W isophotal magnitude (ZP = 25.7275)
# 15 f555w_magerr      F555W isophotal magnitude uncertainty (Edges vulnerable to cosmic rays)
# 16 f555w_flux        F555W isophotal flux  (multiplied by 1.113 to correct for extinction (-0.116 mag))
# 17 f555w_fluxerr     F555W isophotal flux uncertainty    (1.113 factor applied here as well)
# 18 f555w_fluxnJy     F555W isophotal flux in nJy  (multiplied by 1.113 to correct for extinction (-0.116 mag))
# 19 f555w_fluxnJyerr  F555W isophotal flux in nJy uncertainty    (1.113 factor applied here as well)
# 20 f555w_sig         F555W detection significance
# 21 f814w_mag         F814W isophotal magnitude (ZP = 25.9487)
# 22 f814w_magerr      F814W isophotal magnitude uncertainty (Edges vulnerable to cosmic rays)
# 23 f814w_flux        F814W isophotal flux  (multiplied by 1.062 to correct for extinction (-0.065 mag))
# 24 f814w_fluxerr     F814W isophotal flux uncertainty    (1.062 factor applied here as well)
# 25 f814w_fluxnJy     F814W isophotal flux in nJy  (multiplied by 1.062 to correct for extinction (-0.065 mag))
# 26 f814w_fluxnJyerr  F814W isophotal flux in nJy uncertainty    (1.062 factor applied here as well)
# 27 f814w_sig         F814W detection significance
# 28 f814w_mag         F814W isophotal magnitude (ZP = 25.9487)
# 29 f814w_magerr      F814W isophotal magnitude uncertainty (Edges vulnerable to cosmic rays)
# 30 f814w_flux        F814W isophotal flux  (multiplied by 1.062 to correct for extinction (-0.065 mag))
# 31 f814w_fluxerr     F814W isophotal flux uncertainty    (1.062 factor applied here as well)
# 32 f814w_fluxnJy     F814W isophotal flux in nJy  (multiplied by 1.062 to correct for extinction (-0.065 mag))
# 33 f814w_fluxnJyerr  F814W isophotal flux in nJy uncertainty    (1.062 factor applied here as well)
# 34 f814w_sig         F814W detection significance
# 35 f105w_mag         F105W isophotal magnitude (ZP = 26.2689)
# 36 f105w_magerr      F105W isophotal magnitude uncertainty
# 37 f105w_flux        F105W isophotal flux  (multiplied by 1.034 to correct for extinction (-0.036 mag))
# 38 f105w_fluxerr     F105W isophotal flux uncertainty    (1.034 factor applied here as well)
# 39 f105w_fluxnJy     F105W isophotal flux in nJy  (multiplied by 1.034 to correct for extinction (-0.036 mag))
# 40 f105w_fluxnJyerr  F105W isophotal flux in nJy uncertainty    (1.034 factor applied here as well)
# 41 f105w_sig         F105W detection significance
# 42 f125w_mag         F125W isophotal magnitude (ZP = 26.2303)
# 43 f125w_magerr      F125W isophotal magnitude uncertainty
# 44 f125w_flux        F125W isophotal flux  (multiplied by 1.025 to correct for extinction (-0.027 mag))
# 45 f125w_fluxerr     F125W isophotal flux uncertainty    (1.025 factor applied here as well)
# 46 f125w_fluxnJy     F125W isophotal flux in nJy  (multiplied by 1.025 to correct for extinction (-0.027 mag))
# 47 f125w_fluxnJyerr  F125W isophotal flux in nJy uncertainty    (1.025 factor applied here as well)
# 48 f125w_sig         F125W detection significance
# 49 f140w_mag         F140W isophotal magnitude (ZP = 26.4524)
# 50 f140w_magerr      F140W isophotal magnitude uncertainty
# 51 f140w_flux        F140W isophotal flux  (multiplied by 1.020 to correct for extinction (-0.022 mag))
# 52 f140w_fluxerr     F140W isophotal flux uncertainty    (1.020 factor applied here as well)
# 53 f140w_fluxnJy     F140W isophotal flux in nJy  (multiplied by 1.020 to correct for extinction (-0.022 mag))
# 54 f140w_fluxnJyerr  F140W isophotal flux in nJy uncertainty    (1.020 factor applied here as well)
# 55 f140w_sig         F140W detection significance
# 56 f160w_mag         F160W isophotal magnitude (ZP = 25.9463)
# 57 f160w_magerr      F160W isophotal magnitude uncertainty
# 58 f160w_flux        F160W isophotal flux  (multiplied by 1.016 to correct for extinction (-0.017 mag))
# 59 f160w_fluxerr     F160W isophotal flux uncertainty    (1.016 factor applied here as well)
# 60 f160w_fluxnJy     F160W isophotal flux in nJy  (multiplied by 1.016 to correct for extinction (-0.017 mag))
# 61 f160w_fluxnJyerr  F160W isophotal flux in nJy uncertainty    (1.016 factor applied here as well)
# 62 f160w_sig         F160W detection significance
# 63 f160w_mag         F160W isophotal magnitude (ZP = 25.9463)
# 64 f160w_magerr      F160W isophotal magnitude uncertainty
# 65 f160w_flux        F160W isophotal flux  (multiplied by 1.016 to correct for extinction (-0.017 mag))
# 66 f160w_fluxerr     F160W isophotal flux uncertainty    (1.016 factor applied here as well)
# 67 f160w_fluxnJy     F160W isophotal flux in nJy  (multiplied by 1.016 to correct for extinction (-0.017 mag))
# 68 f160w_fluxnJyerr  F160W isophotal flux in nJy uncertainty    (1.016 factor applied here as well)
# 69 f160w_sig         F160W detection significance
# 70 f160w_mag         F160W isophotal magnitude (ZP = 25.9463)
# 71 f160w_magerr      F160W isophotal magnitude uncertainty
# 72 f160w_flux        F160W isophotal flux  (multiplied by 1.016 to correct for extinction (-0.017 mag))
# 73 f160w_fluxerr     F160W isophotal flux uncertainty    (1.016 factor applied here as well)
# 74 f160w_fluxnJy     F160W isophotal flux in nJy  (multiplied by 1.016 to correct for extinction (-0.017 mag))
# 75 f160w_fluxnJyerr  F160W isophotal flux in nJy uncertainty    (1.016 factor applied here as well)
# 76 f160w_sig         F160W detection significance
# 77 bright_mag        Brightest magnitude in any filter
# 78 bright_magerr     Brightest magnitude uncertainty
# 79 zb              
# 80 zbmin           
# 81 zbmax           
# 82 tb              
# 83 odds            
# 84 zml             
# 85 tml             
# 86 chisq           
# 87 M0                Magnitude used for BPZ prior: F814W or closest observed filter
# 88 chisq2          
# 89 nfdet           
##
##  id      RA       Dec       x         y       fwhm   area  stel   ell   flag5sig  nf5sig  nfcr5sig  nfobs  f555w_mag  f555w_magerr  f555w_flux  f555w_fluxerr  f555w_fluxnJy  f555w_fluxnJyerr  f555w_sig  f814w_mag  f814w_magerr  f814w_flux  f814w_fluxerr  f814w_fluxnJy  f814w_fluxnJyerr  f814w_sig  f814w_mag  f814w_magerr  f814w_flux  f814w_fluxerr  f814w_fluxnJy  f814w_fluxnJyerr  f814w_sig  f105w_mag  f105w_magerr  f105w_flux  f105w_fluxerr  f105w_fluxnJy  f105w_fluxnJyerr  f105w_sig  f125w_mag  f125w_magerr  f125w_flux  f125w_fluxerr  f125w_fluxnJy  f125w_fluxnJyerr  f125w_sig  f140w_mag  f140w_magerr  f140w_flux  f140w_fluxerr  f140w_fluxnJy  f140w_fluxnJyerr  f140w_sig  f160w_mag  f160w_magerr  f160w_flux  f160w_fluxerr  f160w_fluxnJy  f160w_fluxnJyerr  f160w_sig  f160w_mag  f160w_magerr  f160w_flux  f160w_fluxerr  f160w_fluxnJy  f160w_fluxnJyerr  f160w_sig  f160w_mag  f160w_magerr  f160w_flux  f160w_fluxerr  f160w_fluxnJy  f160w_fluxnJyerr  f160w_sig  bright_mag  bright_magerr    zb    zbmin  zbmax   tb    odds    zml   tml   chisq     M0      chisq2   nfdet  
  766  137.8107  17.7794  2032.886  2326.178  0.211    10  0.14  0.192         0       2         2      9    28.0342        0.2028      0.1195         0.0245        22.1978            4.5576       4.87    27.9292         0.142      0.1614         0.0226        24.4519            3.4176       7.15    27.9292         0.142      0.1614         0.0226        24.4519            3.4176       7.15     28.219        0.4351      0.1659         0.0818        18.7244            9.2293       2.03         99       28.3808     -0.0263          0.138        -3.0805           16.1323      -0.19    29.5672        1.3503      0.0568         0.1401         5.4092            13.352       0.41         99       28.9817     -0.0066         0.0611        -1.0094            9.2754      -0.11         99       28.9817     -0.0066         0.0611        -1.0094            9.2754      -0.11         99       28.9817     -0.0066         0.0611        -1.0094            9.2754      -0.11     28.0927        30.0657  0.136  0.055  3.649  10  0.3704  0.085   10  0.425  27.929  0.6625      5
