## Subset of objects corresponding to 5259.html
##
## RELICS: Reionization Lensing Cluster Survey 
## Cycle 23 Hubble Treasury program (GO 14096; PI Coe)
## http://relics.stsci.edu
##
## rxs0603+42-S HST source catalog
## Photometric + Bayesian Photometric Redshift (BPZ) catalog (produced 2017-06-30 by Dan Coe)
## based on drizzled 0.06"/pix images (produced 2017-06-23 by Roberto Avila and Sara Ogaz)
## HST observation plan (Phase 2) by Larry Bradley
## HST program coordinated by Bill Januszewski
##
## 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 2.8.6) in a weighted sum of ACS+WFC3/IR images
## Pruned to discard 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) = 0.19680
## 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 and template are given by zb and tb,
## and the 95% confidence range is given by zbmin - zbmax.
## The templates used here are 5 ellipticals (1-5), 2 spirals (6-7), and 4 starburst galaxies (8-11).
## Higher values of tb generally correspond to bluer templates.
## Here we use the origninal Bayesian prior P(z,t | mag) derived from the HDFN (Benitez 2000).
## This prior is less conservative with regard to high redshifts
## than some updated priors used in later works (Benitez+09, Coe+13).
## 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.
## The "maximum likelihood" (flat prior) redshift zml and type tml are also reported.
#  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 theta             Position angle (CCW/x) [deg]
# 11 nf5sig            Number of filters with a 5-sigma detection
# 12 nfobs             Number of filters observed (not in chip gap, etc.)
# 13 f390w_mag         F390W isophotal magnitude (ZP = 25.2796)
# 14 f390w_magerr      F390W isophotal magnitude uncertainty (* Vulnerable to cosmic rays)
# 15 f390w_flux        F390W isophotal flux  (multiplied by 2.266 to correct for extinction (-0.888 mag))
# 16 f390w_fluxerr     F390W isophotal flux uncertainty    (2.266 factor applied here as well)
# 17 f390w_fluxnJy     F390W isophotal flux in nJy  (multiplied by 2.266 to correct for extinction (-0.888 mag))
# 18 f390w_fluxnJyerr  F390W isophotal flux in nJy uncertainty    (2.266 factor applied here as well)
# 19 f390w_sig         F390W detection significance
# 20 f606w_mag         F606W isophotal magnitude (ZP = 26.0044)
# 21 f606w_magerr      F606W isophotal magnitude uncertainty (* Vulnerable to cosmic rays)
# 22 f606w_flux        F606W isophotal flux  (multiplied by 1.700 to correct for extinction (-0.576 mag))
# 23 f606w_fluxerr     F606W isophotal flux uncertainty    (1.700 factor applied here as well)
# 24 f606w_fluxnJy     F606W isophotal flux in nJy  (multiplied by 1.700 to correct for extinction (-0.576 mag))
# 25 f606w_fluxnJyerr  F606W isophotal flux in nJy uncertainty    (1.700 factor applied here as well)
# 26 f606w_sig         F606W detection significance
# 27 f814w_mag         F814W isophotal magnitude (ZP = 25.9462)
# 28 f814w_magerr      F814W isophotal magnitude uncertainty (Edges vulnerable to cosmic rays)
# 29 f814w_flux        F814W isophotal flux  (multiplied by 1.391 to correct for extinction (-0.359 mag))
# 30 f814w_fluxerr     F814W isophotal flux uncertainty    (1.391 factor applied here as well)
# 31 f814w_fluxnJy     F814W isophotal flux in nJy  (multiplied by 1.391 to correct for extinction (-0.359 mag))
# 32 f814w_fluxnJyerr  F814W isophotal flux in nJy uncertainty    (1.391 factor applied here as well)
# 33 f814w_sig         F814W detection significance
# 34 f105w_mag         F105W isophotal magnitude (ZP = 26.2689)
# 35 f105w_magerr      F105W isophotal magnitude uncertainty
# 36 f105w_flux        F105W isophotal flux  (multiplied by 1.202 to correct for extinction (-0.200 mag))
# 37 f105w_fluxerr     F105W isophotal flux uncertainty    (1.202 factor applied here as well)
# 38 f105w_fluxnJy     F105W isophotal flux in nJy  (multiplied by 1.202 to correct for extinction (-0.200 mag))
# 39 f105w_fluxnJyerr  F105W isophotal flux in nJy uncertainty    (1.202 factor applied here as well)
# 40 f105w_sig         F105W detection significance
# 41 f125w_mag         F125W isophotal magnitude (ZP = 26.2303)
# 42 f125w_magerr      F125W isophotal magnitude uncertainty
# 43 f125w_flux        F125W isophotal flux  (multiplied by 1.147 to correct for extinction (-0.149 mag))
# 44 f125w_fluxerr     F125W isophotal flux uncertainty    (1.147 factor applied here as well)
# 45 f125w_fluxnJy     F125W isophotal flux in nJy  (multiplied by 1.147 to correct for extinction (-0.149 mag))
# 46 f125w_fluxnJyerr  F125W isophotal flux in nJy uncertainty    (1.147 factor applied here as well)
# 47 f125w_sig         F125W detection significance
# 48 f140w_mag         F140W isophotal magnitude (ZP = 26.4524)
# 49 f140w_magerr      F140W isophotal magnitude uncertainty
# 50 f140w_flux        F140W isophotal flux  (multiplied by 1.117 to correct for extinction (-0.120 mag))
# 51 f140w_fluxerr     F140W isophotal flux uncertainty    (1.117 factor applied here as well)
# 52 f140w_fluxnJy     F140W isophotal flux in nJy  (multiplied by 1.117 to correct for extinction (-0.120 mag))
# 53 f140w_fluxnJyerr  F140W isophotal flux in nJy uncertainty    (1.117 factor applied here as well)
# 54 f140w_sig         F140W detection significance
# 55 f160w_mag         F160W isophotal magnitude (ZP = 25.9463)
# 56 f160w_magerr      F160W isophotal magnitude uncertainty
# 57 f160w_flux        F160W isophotal flux  (multiplied by 1.089 to correct for extinction (-0.092 mag))
# 58 f160w_fluxerr     F160W isophotal flux uncertainty    (1.089 factor applied here as well)
# 59 f160w_fluxnJy     F160W isophotal flux in nJy  (multiplied by 1.089 to correct for extinction (-0.092 mag))
# 60 f160w_fluxnJyerr  F160W isophotal flux in nJy uncertainty    (1.089 factor applied here as well)
# 61 f160w_sig         F160W detection significance
# 62 bright_mag        Brightest magnitude in any filter
# 63 bright_magerr     Brightest magnitude uncertainty
# 64 zb              
# 65 zbmin           
# 66 zbmax           
# 67 tb              
# 68 odds            
# 69 zml             
# 70 tml             
# 71 chisq           
# 72 M0                Magnitude used for BPZ prior: F814W or closest observed filter
# 73 chisq2          
# 74 nfdet           
##
##  id      RA      Dec       x         y       fwhm    area  stel   ell   theta  nf5sig  nfobs  f390w_mag  f390w_magerr  f390w_flux  f390w_fluxerr  f390w_fluxnJy  f390w_fluxnJyerr  f390w_sig  f606w_mag  f606w_magerr  f606w_flux  f606w_fluxerr  f606w_fluxnJy  f606w_fluxnJyerr  f606w_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  bright_mag  bright_magerr     zb    zbmin   zbmax    tb    odds    zml    tml    chisq     M0      chisq2   nfdet  
  5259  90.8348  42.1664  3625.155  2547.304     0     1  0.41  0.761  -62.6       2      7    25.9803        0.1594      0.5245         0.0829          147.2           23.2776       6.32    25.0548        0.0493       2.398         0.1114          345.2            16.036      21.53    29.8087        1.2727      0.0285         0.0636           4.33            9.6535       0.45         99       28.1629     -0.0051         0.1747        -0.5793           19.7167      -0.03         99       27.5353     -0.5161         0.3006         -60.34           35.1455      -1.72         99       27.7355      -0.084         0.3067         -8.004           29.2282      -0.27         99       28.2835      -0.046         0.1162         -6.988           17.6447       -0.4     25.1064        28.3873  0.019   0.01  0.043  11  0.9998  0.016   11  38.741  29.809    47.7      3