## Subset of objects corresponding to 41.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  
  41  137.795  17.7989  2928.088  3494.417  0.25    10     0  0.383         0       2         2      9    28.2732        0.2599      0.0959         0.0259        17.8126            4.8166        3.7    28.1846        0.1826      0.1275         0.0234        19.3275            3.5394       5.46    28.1846        0.1826      0.1275         0.0234        19.3275            3.5394       5.46    28.1183        0.4212      0.1821         0.0863        20.5435            9.7359       2.11    28.1629        0.6554      0.1686         0.1398        19.7175            16.341       1.21    27.7325        0.4362      0.3076         0.1521        29.3094           14.4917       2.02    28.8653        0.6816       0.068         0.0594        10.3248             9.018       1.14    28.8653        0.6816       0.068         0.0594        10.3248             9.018       1.14    28.8653        0.6816       0.068         0.0594        10.3248             9.018       1.14     28.4042        30.0277  0.399  0.136  3.887  10  0.0913  0.348   10  0.093  28.185  0.1832      9
