## Subset of objects corresponding to 59.html
##
## RELICS: Reionization Lensing Cluster Survey - Cycle 23 Hubble Treasury program (GO 14096; PI Coe)
## Photometric + Bayesian Photometric Redshift (BPZ) catalog (produced 2015-12-16 by Dan Coe)
## from 0.06"/pix images of rxc2211-03-par (produced 2015-12-16)
## 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) = 0.07780
## 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 = 26.9487)
# 15 f350lp_magerr      F350LP isophotal magnitude uncertainty (Edges vulnerable to cosmic rays)
# 16 f350lp_flux        F350LP isophotal flux  (multiplied by 1.182 to correct for extinction (-0.182 mag))
# 17 f350lp_fluxerr     F350LP isophotal flux uncertainty    (1.182 factor applied here as well)
# 18 f350lp_fluxnJy     F350LP isophotal flux in nJy  (multiplied by 1.182 to correct for extinction (-0.182 mag))
# 19 f350lp_fluxnJyerr  F350LP isophotal flux in nJy uncertainty    (1.182 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 1.075 to correct for extinction (-0.079 mag))
# 24 f105w_fluxerr      F105W isophotal flux uncertainty    (1.075 factor applied here as well)
# 25 f105w_fluxnJy      F105W isophotal flux in nJy  (multiplied by 1.075 to correct for extinction (-0.079 mag))
# 26 f105w_fluxnJyerr   F105W isophotal flux in nJy uncertainty    (1.075 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 1.056 to correct for extinction (-0.059 mag))
# 31 f125w_fluxerr      F125W isophotal flux uncertainty    (1.056 factor applied here as well)
# 32 f125w_fluxnJy      F125W isophotal flux in nJy  (multiplied by 1.056 to correct for extinction (-0.059 mag))
# 33 f125w_fluxnJyerr   F125W isophotal flux in nJy uncertainty    (1.056 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 1.045 to correct for extinction (-0.047 mag))
# 38 f140w_fluxerr      F140W isophotal flux uncertainty    (1.045 factor applied here as well)
# 39 f140w_fluxnJy      F140W isophotal flux in nJy  (multiplied by 1.045 to correct for extinction (-0.047 mag))
# 40 f140w_fluxnJyerr   F140W isophotal flux in nJy uncertainty    (1.045 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 1.034 to correct for extinction (-0.037 mag))
# 45 f160w_fluxerr      F160W isophotal flux uncertainty    (1.034 factor applied here as well)
# 46 f160w_fluxnJy      F160W isophotal flux in nJy  (multiplied by 1.034 to correct for extinction (-0.037 mag))
# 47 f160w_fluxnJyerr   F160W isophotal flux in nJy uncertainty    (1.034 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  
  59  333.0054  -3.8842  2742.813  3628.374  0.545    25     0  0.523         0       2         1      5       27.82         0.1661       0.4482          0.0741         27.0404             4.4688        6.05    27.3072        0.2761      0.3843         0.1113        43.3641            12.558       3.45    27.4341        0.3131        0.33         0.1103        38.5809            12.897       2.99    26.9024        0.1967      0.6607         0.1312        62.9543           12.5065       5.03    27.0116         0.279      0.3749         0.1099         56.935           16.6843       3.41     27.1429        28.6572  1.151   0.16  3.993  9.8  0.0732  1.158  9.8  0.177  27.307  0.3452      5