## Subset of objects corresponding to 13511.html ## ## RELICS: Reionization Lensing Cluster Survey ## Cycle 23 Hubble Treasury program (GO 14096; PI Coe) ## http://relics.stsci.edu ## ## cl0152-13 HST source catalog ## Photometric + Bayesian Photometric Redshift (BPZ) catalog (produced 2017-04-12 by Dan Coe) ## based on drizzled 0.06"/pix images (produced 2017-04-12 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) = 0.01260 ## 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 = 25.6646) # 14 f435w_magerr F435W isophotal magnitude uncertainty (Edges vulnerable to cosmic rays) # 15 f435w_flux F435W isophotal flux (multiplied by 1.049 to correct for extinction (-0.052 mag)) # 16 f435w_fluxerr F435W isophotal flux uncertainty (1.049 factor applied here as well) # 17 f435w_fluxnJy F435W isophotal flux in nJy (multiplied by 1.049 to correct for extinction (-0.052 mag)) # 18 f435w_fluxnJyerr F435W isophotal flux in nJy uncertainty (1.049 factor applied here as well) # 19 f435w_sig F435W detection significance # 20 f625w_mag F625W isophotal magnitude (ZP = 25.9215) # 21 f625w_magerr F625W isophotal magnitude uncertainty (Edges vulnerable to cosmic rays) # 22 f625w_flux F625W isophotal flux (multiplied by 1.031 to correct for extinction (-0.034 mag)) # 23 f625w_fluxerr F625W isophotal flux uncertainty (1.031 factor applied here as well) # 24 f625w_fluxnJy F625W isophotal flux in nJy (multiplied by 1.031 to correct for extinction (-0.034 mag)) # 25 f625w_fluxnJyerr F625W isophotal flux in nJy uncertainty (1.031 factor applied here as well) # 26 f625w_sig F625W detection significance # 27 f775w_mag F775W isophotal magnitude (ZP = 25.6759) # 28 f775w_magerr F775W isophotal magnitude uncertainty (Edges vulnerable to cosmic rays) # 29 f775w_flux F775W isophotal flux (multiplied by 1.024 to correct for extinction (-0.025 mag)) # 30 f775w_fluxerr F775W isophotal flux uncertainty (1.024 factor applied here as well) # 31 f775w_fluxnJy F775W isophotal flux in nJy (multiplied by 1.024 to correct for extinction (-0.025 mag)) # 32 f775w_fluxnJyerr F775W isophotal flux in nJy uncertainty (1.024 factor applied here as well) # 33 f775w_sig F775W detection significance # 34 f850lp_mag F850LP isophotal magnitude (ZP = 24.8792) # 35 f850lp_magerr F850LP isophotal magnitude uncertainty (Edges vulnerable to cosmic rays) # 36 f850lp_flux F850LP isophotal flux (multiplied by 1.017 to correct for extinction (-0.019 mag)) # 37 f850lp_fluxerr F850LP isophotal flux uncertainty (1.017 factor applied here as well) # 38 f850lp_fluxnJy F850LP isophotal flux in nJy (multiplied by 1.017 to correct for extinction (-0.019 mag)) # 39 f850lp_fluxnJyerr F850LP isophotal flux in nJy uncertainty (1.017 factor applied here as well) # 40 f850lp_sig F850LP 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 1.012 to correct for extinction (-0.013 mag)) # 44 f105w_fluxerr F105W isophotal flux uncertainty (1.012 factor applied here as well) # 45 f105w_fluxnJy F105W isophotal flux in nJy (multiplied by 1.012 to correct for extinction (-0.013 mag)) # 46 f105w_fluxnJyerr F105W isophotal flux in nJy uncertainty (1.012 factor applied here as well) # 47 f105w_sig F105W detection significance # 48 f125w_mag F125W isophotal magnitude (ZP = 26.2303) # 49 f125w_magerr F125W isophotal magnitude uncertainty # 50 f125w_flux F125W isophotal flux (multiplied by 1.009 to correct for extinction (-0.010 mag)) # 51 f125w_fluxerr F125W isophotal flux uncertainty (1.009 factor applied here as well) # 52 f125w_fluxnJy F125W isophotal flux in nJy (multiplied by 1.009 to correct for extinction (-0.010 mag)) # 53 f125w_fluxnJyerr F125W isophotal flux in nJy uncertainty (1.009 factor applied here as well) # 54 f125w_sig F125W detection significance # 55 f140w_mag F140W isophotal magnitude (ZP = 26.4524) # 56 f140w_magerr F140W isophotal magnitude uncertainty # 57 f140w_flux F140W isophotal flux (multiplied by 1.007 to correct for extinction (-0.008 mag)) # 58 f140w_fluxerr F140W isophotal flux uncertainty (1.007 factor applied here as well) # 59 f140w_fluxnJy F140W isophotal flux in nJy (multiplied by 1.007 to correct for extinction (-0.008 mag)) # 60 f140w_fluxnJyerr F140W isophotal flux in nJy uncertainty (1.007 factor applied here as well) # 61 f140w_sig F140W detection significance # 62 f160w_mag F160W isophotal magnitude (ZP = 25.9463) # 63 f160w_magerr F160W isophotal magnitude uncertainty # 64 f160w_flux F160W isophotal flux (multiplied by 1.005 to correct for extinction (-0.006 mag)) # 65 f160w_fluxerr F160W isophotal flux uncertainty (1.005 factor applied here as well) # 66 f160w_fluxnJy F160W isophotal flux in nJy (multiplied by 1.005 to correct for extinction (-0.006 mag)) # 67 f160w_fluxnJyerr F160W isophotal flux in nJy uncertainty (1.005 factor applied here as well) # 68 f160w_sig F160W detection significance # 69 bright_mag Brightest magnitude in any filter # 70 bright_magerr Brightest magnitude uncertainty # 71 zb # 72 zbmin # 73 zbmax # 74 tb # 75 odds # 76 zml # 77 tml # 78 chisq # 79 M0 Magnitude used for BPZ prior: F814W or closest observed filter # 80 chisq2 # 81 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 f625w_mag f625w_magerr f625w_flux f625w_fluxerr f625w_fluxnJy f625w_fluxnJyerr f625w_sig f775w_mag f775w_magerr f775w_flux f775w_fluxerr f775w_fluxnJy f775w_fluxnJyerr f775w_sig f850lp_mag f850lp_magerr f850lp_flux f850lp_fluxerr f850lp_fluxnJy f850lp_fluxnJyerr f850lp_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 13511 28.2001 -13.9493 3438.283 5055.498 1.103 600 0 0.195 32.4 6 6 24.7466 0.0912 2.329 0.2041 458.5 40.1807 11.41 23.6089 0.0199 8.4143 0.1556 1307.472 24.1784 54.08 23.3506 0.0154 8.5139 0.1216 1658.62 23.6939 70 23.206 0.0284 4.6693 0.1239 1894.896 50.2908 37.68 -99 0 -9.623e+32 inf -1.086e+35 inf 0 23.1333 0.0227 17.33 0.3658 2026 42.7638 47.38 -99 0 -9.577e+32 inf -9.126e+34 inf 0 23.0346 0.0262 14.61 0.3564 2219 54.1278 41 23.0614 27.0664 0.292 0.25 0.493 8.3 0.577 0.29 8.2 1.687 23.133 0.5041 6