## Subset of objects corresponding to 1171.html
##
## RELICS: Reionization Lensing Cluster Survey
## Cycle 23 Hubble Treasury program (GO 14096; PI Coe)
## http://relics.stsci.edu
##
## plckg308-20-par HST source catalog
## Photometric + Bayesian Photometric Redshift (BPZ) catalog (produced 2016-11-16 by Dan Coe)
## based on drizzled 0.06"/pix images (produced 2016-11-16 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 WFC3/IR images
## Not pruned: a few < 5-sigma detections may remain
## 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) = 0.23730
## 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 f350lp_mag F350LP isophotal magnitude (ZP = 26.8757)
# 14 f350lp_magerr F350LP isophotal magnitude uncertainty (Edges vulnerable to cosmic rays)
# 15 f350lp_flux F350LP isophotal flux (multiplied by 1.666 to correct for extinction (-0.554 mag))
# 16 f350lp_fluxerr F350LP isophotal flux uncertainty (1.666 factor applied here as well)
# 17 f350lp_fluxnJy F350LP isophotal flux in nJy (multiplied by 1.666 to correct for extinction (-0.554 mag))
# 18 f350lp_fluxnJyerr F350LP isophotal flux in nJy uncertainty (1.666 factor applied here as well)
# 19 f350lp_sig F350LP detection significance
# 20 f105w_mag F105W isophotal magnitude (ZP = 26.2689)
# 21 f105w_magerr F105W isophotal magnitude uncertainty
# 22 f105w_flux F105W isophotal flux (multiplied by 1.248 to correct for extinction (-0.241 mag))
# 23 f105w_fluxerr F105W isophotal flux uncertainty (1.248 factor applied here as well)
# 24 f105w_fluxnJy F105W isophotal flux in nJy (multiplied by 1.248 to correct for extinction (-0.241 mag))
# 25 f105w_fluxnJyerr F105W isophotal flux in nJy uncertainty (1.248 factor applied here as well)
# 26 f105w_sig F105W detection significance
# 27 f125w_mag F125W isophotal magnitude (ZP = 26.2303)
# 28 f125w_magerr F125W isophotal magnitude uncertainty
# 29 f125w_flux F125W isophotal flux (multiplied by 1.180 to correct for extinction (-0.180 mag))
# 30 f125w_fluxerr F125W isophotal flux uncertainty (1.180 factor applied here as well)
# 31 f125w_fluxnJy F125W isophotal flux in nJy (multiplied by 1.180 to correct for extinction (-0.180 mag))
# 32 f125w_fluxnJyerr F125W isophotal flux in nJy uncertainty (1.180 factor applied here as well)
# 33 f125w_sig F125W detection significance
# 34 f140w_mag F140W isophotal magnitude (ZP = 26.4524)
# 35 f140w_magerr F140W isophotal magnitude uncertainty
# 36 f140w_flux F140W isophotal flux (multiplied by 1.142 to correct for extinction (-0.145 mag))
# 37 f140w_fluxerr F140W isophotal flux uncertainty (1.142 factor applied here as well)
# 38 f140w_fluxnJy F140W isophotal flux in nJy (multiplied by 1.142 to correct for extinction (-0.145 mag))
# 39 f140w_fluxnJyerr F140W isophotal flux in nJy uncertainty (1.142 factor applied here as well)
# 40 f140w_sig F140W detection significance
# 41 f160w_mag F160W isophotal magnitude (ZP = 25.9463)
# 42 f160w_magerr F160W isophotal magnitude uncertainty
# 43 f160w_flux F160W isophotal flux (multiplied by 1.108 to correct for extinction (-0.112 mag))
# 44 f160w_fluxerr F160W isophotal flux uncertainty (1.108 factor applied here as well)
# 45 f160w_fluxnJy F160W isophotal flux in nJy (multiplied by 1.108 to correct for extinction (-0.112 mag))
# 46 f160w_fluxnJyerr F160W isophotal flux in nJy uncertainty (1.108 factor applied here as well)
# 47 f160w_sig F160W detection significance
# 48 bright_mag Brightest magnitude in any filter
# 49 bright_magerr Brightest magnitude uncertainty
# 50 zb
# 51 zbmin
# 52 zbmax
# 53 tb
# 54 odds
# 55 zml
# 56 tml
# 57 chisq
# 58 M0 Magnitude used for BPZ prior: F814W or closest observed filter
# 59 chisq2
# 60 nfdet
##
## id RA Dec x y fwhm area stel ell theta nf5sig 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
1171 230.2223 -81.564 2619.435 3049.167 0.065 3 0.66 0.07 5.7 1 5 25.5318 0.0334 3.448 0.1077 222.5 6.9521 32 30.57 1.7018 0.019 0.0722 2.148 8.1491 0.26 30.8477 1.8351 0.0142 0.0629 1.663 7.352 0.23 29.3797 0.7391 0.0675 0.0658 6.428 6.2704 1.03 99 29.117 -0.0256 0.0539 -3.884 8.1884 -0.47 25.5663 29.2947 0.013 0.01 0.034 10 0.9993 0.01 10 92.823 30.57 141.9002 4