## Subset of objects corresponding to 886.html
##
## RELICS: Reionization Lensing Cluster Survey - Cycle 23 Hubble Treasury program (GO 14096; PI Coe)
## Photometric + Bayesian Photometric Redshift (BPZ) catalog (produced 2016-06-02 by Dan Coe)
## from 0.06"/pix images of abell1763-par (produced 2016-06-02)
## 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 IR images
## Not pruned: a few < 5-sigma detections may remain (flagsig > 0)
## 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) = 0.00690
## 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 f350lp_mag         F350LP isophotal magnitude (ZP = 26.8757)
# 15 f350lp_magerr      F350LP isophotal magnitude uncertainty (Edges vulnerable to cosmic rays)
# 16 f350lp_flux        F350LP isophotal flux  (multiplied by 1.015 to correct for extinction (-0.016 mag))
# 17 f350lp_fluxerr     F350LP isophotal flux uncertainty    (1.015 factor applied here as well)
# 18 f350lp_fluxnJy     F350LP isophotal flux in nJy  (multiplied by 1.015 to correct for extinction (-0.016 mag))
# 19 f350lp_fluxnJyerr  F350LP isophotal flux in nJy uncertainty    (1.015 factor applied here as well)
# 20 f350lp_sig         F350LP detection significance
# 21 f105w_mag          F105W isophotal magnitude (ZP = 26.2689)
# 22 f105w_magerr       F105W isophotal magnitude uncertainty
# 23 f105w_flux         F105W isophotal flux  (multiplied by 1.006 to correct for extinction (-0.007 mag))
# 24 f105w_fluxerr      F105W isophotal flux uncertainty    (1.006 factor applied here as well)
# 25 f105w_fluxnJy      F105W isophotal flux in nJy  (multiplied by 1.006 to correct for extinction (-0.007 mag))
# 26 f105w_fluxnJyerr   F105W isophotal flux in nJy uncertainty    (1.006 factor applied here as well)
# 27 f105w_sig          F105W detection significance
# 28 f125w_mag          F125W isophotal magnitude (ZP = 26.2303)
# 29 f125w_magerr       F125W isophotal magnitude uncertainty
# 30 f125w_flux         F125W isophotal flux  (multiplied by 1.005 to correct for extinction (-0.005 mag))
# 31 f125w_fluxerr      F125W isophotal flux uncertainty    (1.005 factor applied here as well)
# 32 f125w_fluxnJy      F125W isophotal flux in nJy  (multiplied by 1.005 to correct for extinction (-0.005 mag))
# 33 f125w_fluxnJyerr   F125W isophotal flux in nJy uncertainty    (1.005 factor applied here as well)
# 34 f125w_sig          F125W detection significance
# 35 f140w_mag          F140W isophotal magnitude (ZP = 26.4524)
# 36 f140w_magerr       F140W isophotal magnitude uncertainty
# 37 f140w_flux         F140W isophotal flux  (multiplied by 1.004 to correct for extinction (-0.004 mag))
# 38 f140w_fluxerr      F140W isophotal flux uncertainty    (1.004 factor applied here as well)
# 39 f140w_fluxnJy      F140W isophotal flux in nJy  (multiplied by 1.004 to correct for extinction (-0.004 mag))
# 40 f140w_fluxnJyerr   F140W isophotal flux in nJy uncertainty    (1.004 factor applied here as well)
# 41 f140w_sig          F140W detection significance
# 42 f160w_mag          F160W isophotal magnitude (ZP = 25.9463)
# 43 f160w_magerr       F160W isophotal magnitude uncertainty
# 44 f160w_flux         F160W isophotal flux  (multiplied by 1.003 to correct for extinction (-0.003 mag))
# 45 f160w_fluxerr      F160W isophotal flux uncertainty    (1.003 factor applied here as well)
# 46 f160w_fluxnJy      F160W isophotal flux in nJy  (multiplied by 1.003 to correct for extinction (-0.003 mag))
# 47 f160w_fluxnJyerr   F160W isophotal flux in nJy uncertainty    (1.003 factor applied here as well)
# 48 f160w_sig          F160W detection significance
# 49 bright_mag         Brightest magnitude in any filter
# 50 bright_magerr      Brightest magnitude uncertainty
# 51 zb               
# 52 zbmin            
# 53 zbmax            
# 54 tb               
# 55 odds             
# 56 zml              
# 57 tml              
# 58 chisq            
# 59 M0                 Magnitude used for BPZ prior: F814W or closest observed filter
# 60 chisq2           
# 61 nfdet            
##
##  id      RA       Dec       x         y       fwhm  area  stel   ell   flag5sig  nf5sig  nfcr5sig  nfobs  f350lp_mag  f350lp_magerr  f350lp_flux  f350lp_fluxerr  f350lp_fluxnJy  f350lp_fluxnJyerr  f350lp_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  bright_mag  bright_magerr     zb    zbmin   zbmax    tb    odds    zml    tml   chisq      M0      chisq2   nfdet  
  886  203.8167  40.9014  2326.586  2631.543  0.113    10     1  0.225         0       1         0      5     32.5372         2.2963       0.0054          0.0396          0.3509             2.5576        0.14     30.554        1.8203      0.0193          0.084         2.1796            9.4756       0.23    24.4315        0.0572      5.2421         0.2838       612.8992           33.1835      18.47         99       28.8935     -0.0544         0.1056        -5.1818           10.0596      -0.52         99       28.6853     -0.1162         0.0802       -17.6404           12.1867      -1.45      24.492        27.5977  0.983  0.362  8.223   3  0.0589  7.954   11  64.256  30.554   131.4      3