## Subset of objects corresponding to 1804.html ## ## RELICS: Reionization Lensing Cluster Survey ## Cycle 23 Hubble Treasury program (GO 14096; PI Coe) ## http://relics.stsci.edu ## ## plckg287+32 HST source catalog ## Photometric + Bayesian Photometric Redshift (BPZ) catalog (produced 2017-07-06 by Dan Coe) ## based on drizzled 0.06"/pix images (produced 2017-06-29 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) = 0.08130 ## 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 f435w_mag F435W isophotal magnitude (ZP = 25.6644) # 14 f435w_magerr F435W isophotal magnitude uncertainty (Edges vulnerable to cosmic rays) # 15 f435w_flux F435W isophotal flux (multiplied by 1.361 to correct for extinction (-0.335 mag)) # 16 f435w_fluxerr F435W isophotal flux uncertainty (1.361 factor applied here as well) # 17 f435w_fluxnJy F435W isophotal flux in nJy (multiplied by 1.361 to correct for extinction (-0.335 mag)) # 18 f435w_fluxnJyerr F435W isophotal flux in nJy uncertainty (1.361 factor applied here as well) # 19 f435w_sig F435W detection significance # 20 f475w_mag F475W isophotal magnitude (ZP = 26.0558) # 21 f475w_magerr F475W isophotal magnitude uncertainty (Edges vulnerable to cosmic rays) # 22 f475w_flux F475W isophotal flux (multiplied by 1.322 to correct for extinction (-0.303 mag)) # 23 f475w_fluxerr F475W isophotal flux uncertainty (1.322 factor applied here as well) # 24 f475w_fluxnJy F475W isophotal flux in nJy (multiplied by 1.322 to correct for extinction (-0.303 mag)) # 25 f475w_fluxnJyerr F475W isophotal flux in nJy uncertainty (1.322 factor applied here as well) # 26 f475w_sig F475W detection significance # 27 f606w_mag F606W isophotal magnitude (ZP = 26.4978) # 28 f606w_magerr F606W isophotal magnitude uncertainty (Edges vulnerable to cosmic rays) # 29 f606w_flux F606W isophotal flux (multiplied by 1.245 to correct for extinction (-0.238 mag)) # 30 f606w_fluxerr F606W isophotal flux uncertainty (1.245 factor applied here as well) # 31 f606w_fluxnJy F606W isophotal flux in nJy (multiplied by 1.245 to correct for extinction (-0.238 mag)) # 32 f606w_fluxnJyerr F606W isophotal flux in nJy uncertainty (1.245 factor applied here as well) # 33 f606w_sig F606W detection significance # 34 f814w_mag F814W isophotal magnitude (ZP = 25.9443) # 35 f814w_magerr F814W isophotal magnitude uncertainty (Edges vulnerable to cosmic rays) # 36 f814w_flux F814W isophotal flux (multiplied by 1.146 to correct for extinction (-0.148 mag)) # 37 f814w_fluxerr F814W isophotal flux uncertainty (1.146 factor applied here as well) # 38 f814w_fluxnJy F814W isophotal flux in nJy (multiplied by 1.146 to correct for extinction (-0.148 mag)) # 39 f814w_fluxnJyerr F814W isophotal flux in nJy uncertainty (1.146 factor applied here as well) # 40 f814w_sig F814W detection significance # 41 f105w_mag F105W isophotal magnitude (ZP = 26.2689) # 42 f105w_magerr F105W isophotal magnitude uncertainty # 43 f105w_flux F105W isophotal flux (multiplied by 1.079 to correct for extinction (-0.083 mag)) # 44 f105w_fluxerr F105W isophotal flux uncertainty (1.079 factor applied here as well) # 45 f105w_fluxnJy F105W isophotal flux in nJy (multiplied by 1.079 to correct for extinction (-0.083 mag)) # 46 f105w_fluxnJyerr F105W isophotal flux in nJy uncertainty (1.079 factor applied here as well) # 47 f105w_sig F105W detection significance # 48 f110w_mag F110W isophotal magnitude (ZP = 26.8222) # 49 f110w_magerr F110W isophotal magnitude uncertainty # 50 f110w_flux F110W isophotal flux (multiplied by 1.068 to correct for extinction (-0.071 mag)) # 51 f110w_fluxerr F110W isophotal flux uncertainty (1.068 factor applied here as well) # 52 f110w_fluxnJy F110W isophotal flux in nJy (multiplied by 1.068 to correct for extinction (-0.071 mag)) # 53 f110w_fluxnJyerr F110W isophotal flux in nJy uncertainty (1.068 factor applied here as well) # 54 f110w_sig F110W detection significance # 55 f125w_mag F125W isophotal magnitude (ZP = 26.2303) # 56 f125w_magerr F125W isophotal magnitude uncertainty # 57 f125w_flux F125W isophotal flux (multiplied by 1.058 to correct for extinction (-0.062 mag)) # 58 f125w_fluxerr F125W isophotal flux uncertainty (1.058 factor applied here as well) # 59 f125w_fluxnJy F125W isophotal flux in nJy (multiplied by 1.058 to correct for extinction (-0.062 mag)) # 60 f125w_fluxnJyerr F125W isophotal flux in nJy uncertainty (1.058 factor applied here as well) # 61 f125w_sig F125W detection significance # 62 f140w_mag F140W isophotal magnitude (ZP = 26.4524) # 63 f140w_magerr F140W isophotal magnitude uncertainty # 64 f140w_flux F140W isophotal flux (multiplied by 1.047 to correct for extinction (-0.050 mag)) # 65 f140w_fluxerr F140W isophotal flux uncertainty (1.047 factor applied here as well) # 66 f140w_fluxnJy F140W isophotal flux in nJy (multiplied by 1.047 to correct for extinction (-0.050 mag)) # 67 f140w_fluxnJyerr F140W isophotal flux in nJy uncertainty (1.047 factor applied here as well) # 68 f140w_sig F140W detection significance # 69 f160w_mag F160W isophotal magnitude (ZP = 25.9463) # 70 f160w_magerr F160W isophotal magnitude uncertainty # 71 f160w_flux F160W isophotal flux (multiplied by 1.036 to correct for extinction (-0.038 mag)) # 72 f160w_fluxerr F160W isophotal flux uncertainty (1.036 factor applied here as well) # 73 f160w_fluxnJy F160W isophotal flux in nJy (multiplied by 1.036 to correct for extinction (-0.038 mag)) # 74 f160w_fluxnJyerr F160W isophotal flux in nJy uncertainty (1.036 factor applied here as well) # 75 f160w_sig F160W detection significance # 76 bright_mag Brightest magnitude in any filter # 77 bright_magerr Brightest magnitude uncertainty # 78 zb # 79 zbmin # 80 zbmax # 81 tb # 82 odds # 83 zml # 84 tml # 85 chisq # 86 M0 Magnitude used for BPZ prior: F814W or closest observed filter # 87 chisq2 # 88 nfdet ## ## id RA Dec x y fwhm area stel ell theta nf5sig nfobs f435w_mag f435w_magerr f435w_flux f435w_fluxerr f435w_fluxnJy f435w_fluxnJyerr f435w_sig f475w_mag f475w_magerr f475w_flux f475w_fluxerr f475w_fluxnJy f475w_fluxnJyerr f475w_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 f110w_mag f110w_magerr f110w_flux f110w_fluxerr f110w_fluxnJy f110w_fluxnJyerr f110w_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 1804 177.6943 -28.0831 3548.004 2607.332 0.415 9 0.07 0.663 -25.3 1 9 28.9628 0.7487 0.0479 0.0476 9.438 9.3704 1.01 99 29.1493 -0.0416 0.0579 -5.715 7.9487 -0.72 99 29.4017 -0.0275 0.0689 -2.512 6.2999 -0.4 28.8616 0.5241 0.0681 0.0422 10.36 6.428 1.61 28.914 0.8068 0.0875 0.0965 9.871 10.8833 0.91 27.6692 0.1106 0.4583 0.0491 31.07 3.3315 9.33 99 28.172 -0.0818 0.1672 -9.56 19.5515 -0.49 28.4351 0.7761 0.161 0.1681 15.34 16.0166 0.96 28.4792 0.5797 0.097 0.0685 14.73 10.3965 1.42 27.7924 30.0934 0.961 0.5 6.723 8 0.0797 6.031 11 0.974 28.862 1.812 6