## Subset of objects corresponding to 9.html ## ## RELICS: Reionization Lensing Cluster Survey ## Cycle 23 Hubble Treasury program (GO 14096; PI Coe) ## http://relics.stsci.edu ## ## ms1008-12 HST source catalog ## Photometric + Bayesian Photometric Redshift (BPZ) catalog (produced 2017-05-09 by Dan Coe) ## based on drizzled 0.06"/pix images (produced 2017-05-09 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) = 0.06010 ## 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 = 25.6649) # 14 f435w_magerr F435W isophotal magnitude uncertainty (Edges vulnerable to cosmic rays) # 15 f435w_flux F435W isophotal flux (multiplied by 1.256 to correct for extinction (-0.247 mag)) # 16 f435w_fluxerr F435W isophotal flux uncertainty (1.256 factor applied here as well) # 17 f435w_fluxnJy F435W isophotal flux in nJy (multiplied by 1.256 to correct for extinction (-0.247 mag)) # 18 f435w_fluxnJyerr F435W isophotal flux in nJy uncertainty (1.256 factor applied here as well) # 19 f435w_sig F435W detection significance # 20 f606w_mag F606W isophotal magnitude (ZP = 26.5118) # 21 f606w_magerr F606W isophotal magnitude uncertainty (Edges vulnerable to cosmic rays) # 22 f606w_flux F606W isophotal flux (multiplied by 1.176 to correct for extinction (-0.176 mag)) # 23 f606w_fluxerr F606W isophotal flux uncertainty (1.176 factor applied here as well) # 24 f606w_fluxnJy F606W isophotal flux in nJy (multiplied by 1.176 to correct for extinction (-0.176 mag)) # 25 f606w_fluxnJyerr F606W isophotal flux in nJy uncertainty (1.176 factor applied here as well) # 26 f606w_sig F606W detection significance # 27 f775w_mag F775W isophotal magnitude (ZP = 25.6802) # 28 f775w_magerr F775W isophotal magnitude uncertainty (* Vulnerable to cosmic rays) # 29 f775w_flux F775W isophotal flux (multiplied by 1.118 to correct for extinction (-0.121 mag)) # 30 f775w_fluxerr F775W isophotal flux uncertainty (1.118 factor applied here as well) # 31 f775w_fluxnJy F775W isophotal flux in nJy (multiplied by 1.118 to correct for extinction (-0.121 mag)) # 32 f775w_fluxnJyerr F775W isophotal flux in nJy uncertainty (1.118 factor applied here as well) # 33 f775w_sig F775W detection significance # 34 f850lp_mag F850LP isophotal magnitude (ZP = 24.8709) # 35 f850lp_magerr F850LP isophotal magnitude uncertainty (* Vulnerable to cosmic rays) # 36 f850lp_flux F850LP isophotal flux (multiplied by 1.085 to correct for extinction (-0.089 mag)) # 37 f850lp_fluxerr F850LP isophotal flux uncertainty (1.085 factor applied here as well) # 38 f850lp_fluxnJy F850LP isophotal flux in nJy (multiplied by 1.085 to correct for extinction (-0.089 mag)) # 39 f850lp_fluxnJyerr F850LP isophotal flux in nJy uncertainty (1.085 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 1.058 to correct for extinction (-0.061 mag)) # 44 f105w_fluxerr F105W isophotal flux uncertainty (1.058 factor applied here as well) # 45 f105w_fluxnJy F105W isophotal flux in nJy (multiplied by 1.058 to correct for extinction (-0.061 mag)) # 46 f105w_fluxnJyerr F105W isophotal flux in nJy uncertainty (1.058 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 1.043 to correct for extinction (-0.045 mag)) # 51 f125w_fluxerr F125W isophotal flux uncertainty (1.043 factor applied here as well) # 52 f125w_fluxnJy F125W isophotal flux in nJy (multiplied by 1.043 to correct for extinction (-0.045 mag)) # 53 f125w_fluxnJyerr F125W isophotal flux in nJy uncertainty (1.043 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 1.034 to correct for extinction (-0.037 mag)) # 58 f140w_fluxerr F140W isophotal flux uncertainty (1.034 factor applied here as well) # 59 f140w_fluxnJy F140W isophotal flux in nJy (multiplied by 1.034 to correct for extinction (-0.037 mag)) # 60 f140w_fluxnJyerr F140W isophotal flux in nJy uncertainty (1.034 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 1.026 to correct for extinction (-0.028 mag)) # 65 f160w_fluxerr F160W isophotal flux uncertainty (1.026 factor applied here as well) # 66 f160w_fluxnJy F160W isophotal flux in nJy (multiplied by 1.026 to correct for extinction (-0.028 mag)) # 67 f160w_fluxnJyerr F160W isophotal flux in nJy uncertainty (1.026 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 f606w_mag f606w_magerr f606w_flux f606w_fluxerr f606w_fluxnJy f606w_fluxnJyerr f606w_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 9 152.6394 -12.6374 4950.263 6540.189 0.853 105 0.01 0.369 19.9 7 8 27.2879 0.3932 0.2243 0.0979 44.1394 19.2611 2.29 25.5513 0.0645 2.422 0.1482 218.5 13.3734 16.34 25.3233 0.0723 1.389 0.0957 269.6 18.5726 14.51 25.0831 0.0942 0.8225 0.0745 336.3 30.4783 11.03 25.2374 0.1218 2.586 0.3069 291.8 34.6343 8.42 25.0377 0.1577 2.999 0.4688 350.7 54.8102 6.4 24.9356 0.1278 4.043 0.5049 385.3 48.1099 8.01 24.6695 0.069 3.241 0.2125 492.3 32.2773 15.25 24.7431 27.6278 3.358 2.938 3.655 8.7 0.7974 3.357 8.7 0.59 25.551 0.3349 8