## Subset of objects corresponding to 7.html
##
## RELICS: Reionization Lensing Cluster Survey - Cycle 23 Hubble Treasury program (GO 14096; PI Coe)
## Photometric + Bayesian Photometric Redshift (BPZ) catalog (produced 2016-01-29 by Dan Coe)
## from 0.06"/pix images of plckg138-10-par (produced 2016-01-29)
## 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) = 0.19020
## 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 1.505 to correct for extinction (-0.444 mag))
# 17 f350lp_fluxerr     F350LP isophotal flux uncertainty    (1.505 factor applied here as well)
# 18 f350lp_fluxnJy     F350LP isophotal flux in nJy  (multiplied by 1.505 to correct for extinction (-0.444 mag))
# 19 f350lp_fluxnJyerr  F350LP isophotal flux in nJy uncertainty    (1.505 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 1.195 to correct for extinction (-0.193 mag))
# 24 f105w_fluxerr      F105W isophotal flux uncertainty    (1.195 factor applied here as well)
# 25 f105w_fluxnJy      F105W isophotal flux in nJy  (multiplied by 1.195 to correct for extinction (-0.193 mag))
# 26 f105w_fluxnJyerr   F105W isophotal flux in nJy uncertainty    (1.195 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 1.142 to correct for extinction (-0.144 mag))
# 31 f125w_fluxerr      F125W isophotal flux uncertainty    (1.142 factor applied here as well)
# 32 f125w_fluxnJy      F125W isophotal flux in nJy  (multiplied by 1.142 to correct for extinction (-0.144 mag))
# 33 f125w_fluxnJyerr   F125W isophotal flux in nJy uncertainty    (1.142 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 1.113 to correct for extinction (-0.116 mag))
# 38 f140w_fluxerr      F140W isophotal flux uncertainty    (1.113 factor applied here as well)
# 39 f140w_fluxnJy      F140W isophotal flux in nJy  (multiplied by 1.113 to correct for extinction (-0.116 mag))
# 40 f140w_fluxnJyerr   F140W isophotal flux in nJy uncertainty    (1.113 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 1.086 to correct for extinction (-0.089 mag))
# 45 f160w_fluxerr      F160W isophotal flux uncertainty    (1.086 factor applied here as well)
# 46 f160w_fluxnJy      F160W isophotal flux in nJy  (multiplied by 1.086 to correct for extinction (-0.089 mag))
# 47 f160w_fluxnJyerr   F160W isophotal flux in nJy uncertainty    (1.086 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  
   7  36.8616  48.9458  2317.213  3903.427  0.357     7     0  0.19         2       0         0      3     29.1689         0.3342       0.1294          0.0466          7.8065             2.8135        2.77        -99             0      0.0867            inf         9.7828               inf          0    28.0984        0.4451       0.179         0.0907        20.9232           10.6041       1.97    28.2868        0.4594      0.1846         0.0972        17.5901            9.2656        1.9        -99             0      0.0039            inf          0.598               inf          0     28.8659        28.8363  0.689  0.183  4.822  8.7  0.0533  4.719   11  0.004  28.098  0.0677      3