J/ApJ/830/51 FourStar galaxy evolution survey (ZFOURGE) (Straatman+, 2016) ================================================================================ The FourStar galaxy evolution survey (ZFOURGE): ultraviolet to far-infrared catalogs, medium-bandwidth photometric redshifts with improved accuracy, stellar masses, and confirmation of quiescent galaxies to z ~ 3.5. Straatman C.M.S., Spitler L.R., Quadri R.F., Labbe I., Glazebrook K., Persson S.E., Papovich C., Tran K.-V., Brammer G.B., Cowley M., Tomczak A., Nanayakkara T., Alcorn L., Allen R., Broussard A., van Dokkum P., Forrest B., van Houdt J., Kacprzak G.G., Kawinwanichakij L., Kelson D.D., Lee J., McCarthy P.J., Mehrtens N., Monson A., Murphy D., Rees G., Tilvi V., Whitaker K.E. =2016ApJ...830...51S (SIMBAD/NED BibCode) ================================================================================ ADC_Keywords: Photometry, infrared ; Galaxies, IR ; Redshifts ; Surveys ; Photometry, HST Keywords: cosmology: observations; galaxies: evolution; galaxies: high-redshift; infrared: galaxies Abstract: The FourStar galaxy evolution survey (ZFOURGE) is a 45 night legacy program with the FourStar near-infrared camera on Magellan and one of the most sensitive surveys to date. ZFOURGE covers a total of 400arcmin^2^ in cosmic fields CDFS, COSMOS and UDS, overlapping the CANDELS fields. Description: We present the FourStar galaxy evolution survey (ZFOURGE) photometric catalogs comprising >70000 galaxies, selected from ultradeep Ks-band detection images (25.5-26.5 AB mag, 5{sigma}, total). We use 5 near-IR medium-bandwidth filters (J1, J2, J3, Hs, Hl) as well as broad-band Ks at 1.05-2.16 micron to 25-26 AB at a seeing of ~0.5 arcsec. Each field has ancillary imaging in 26-40 filters at 0.3-8 micron. We derive photometric redshifts, rest-frame U-V and V-J colors, and stellar population properties from SED fitting. The photometric redshifts have uncertainty {sigma}_z_=0.010, 0.009, and 0.011 in CDFS, COSMOS and UDS, respectively, if compared with spectroscopic redshifts. A pair test indicates {sigma}_z,pairs_=0.01-0.02 at 1 175 All filter curves can be found in calibrations/FILTER_RES_DR34.latest. *The uv13 filter is only 110{AA} wide to avoid contamination from Lya. Note on *rad.dat: A total of 370 radio sources (218 in CDFS, 122 in COSMOS, 30 in UDS) were cross-matched with the primary ZFOURGE catalogues. Radio sources were matched to ZFOURGE to within 1" and positionally corrected by calculating the median positional uncertainty in each field. In arcsecs, the corrections are CDFS: RA=-0.19;DEC=-0.23, COSMOS: RA=+0.08;DEC=+0.07, UDS: RA=+0.03;DEC=+0.37. The following resources were used to crossmatch: the LA 1.4GHz Survey of the Extended Chandra Deep Field South: 2nd DR (Miller+ 2013, J/ApJS/205/13), the VLA-COSMOS Survey IV: Deep Data and Joint Catalogue (Schinnerer+ 2010, J/ApJS/188/384) and the Subaru/XMM-Newton Deep Field I: 100uJy Catalogue (Simpson+ 2006, J/MNRAS/372/741). Note on *x.dat: A total of 736 X-ray sources (596 in CDFS, 109 in COSMOS, 31 in UDS) were cross-matched with the primary ZFOURGE catalogues. X-ray sources were matched to ZFOURGE to within 1" and positionally corrected by calculating the median positional uncertainty in each field. In arcsecs, the corrections are CDFS: RA=-0.15;DEC=-0.26, COSMOS: RA=+0.13;DEC=+0.14, UDS: RA=+0.02;DEC=-0.16. The following AGN classification criteria are adopted in Cowley+ (2016MNRAS.457..629C): (L_x_>=10**41) & (HR>-0.2) (L_x_>=10**42) & (HR<=-0.2) -------------------------------------------------------------------------------- See also: II/253 : Chandra Deep Field South: multi-colour data (Wolf+, 2008) II/261 : GOODS initial results (Giavalisco+, 2004) J/ApJ/817/118 : SFR-M_*_ relation from ZFOURGE (Tomczak+, 2016) J/ApJS/214/24 : 3D-HST+CANDELS catalog (Skelton+, 2014) J/A+A/570/A11 : The Hawk-I UDS and GOODS Survey (HUGS) (Fontana+, 2014) J/ApJ/777/18 : Stellar mass functions of galaxies to z=4 (Muzzin+, 2013) J/ApJS/206/8 : COSMOS/UltraVISTA Ks-selected catalogs v4.1 (Muzzin+, 2013) J/ApJ/769/80 : Spitzer/IRAC observations of five deep fields (Ashby+, 2013) J/MNRAS/428/1128 : UDS/COSMOS HiZELS galaxies (Sobral+, 2013) J/ApJS/203/24 : Structural param. of galaxies in CANDELS (van der Wel+, 2012) J/A+A/544/A156 : UltraVISTA Catalogue Release DR1 (McCracken+, 2012) J/ApJ/753/121 : zCOSMOS 20k sample group catalog to z<~1.2 (Knobel+, 2012) J/A+A/533/A119 : GOODS-Herschel North and South catalogs (Elbaz+, 2011) J/ApJ/735/86 : NEWFIRM MBS: photometric catalogs (Whitaker+, 2011) J/ApJS/189/270 : MUSYC optical imaging in ECDF-S (Cardamone+, 2010) J/A+A/511/A50 : JHks of GOODS-South field (Retzlaff+, 2010) J/ApJ/682/985 : FIREWORKS photometry of GOODS CDF-S (Wuyts+, 2008) J/ApJ/675/234 : Stellar mass functions for gal. 01.1" images) and CFHT/WIRCAM/K-band imaging (Hsieh+ 2012ApJS..203...23H). KsHI comes from a combined VLT/HAWKI and Magellan/FOURSTAR image. Note (2): Same meaning as column "Use" (see Note (G3)) but without the snr>=5 criterion. -------------------------------------------------------------------------------- Byte-by-byte Description of file: cdfszout.dat cos_zout.dat uds_zout.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 I5 --- Seq [1/30911] Running sequence number 7- 16 F10.6 --- zspec [0/6.2]?=-99 Spectroscopic redshift 18- 24 F7.3 --- za [0.005/10]?=-99 Photometric redshift derived without a K luminosity prior 26- 32 F7.3 --- zml [0.005/10]?=-99 Weighted redshift derived without a K luminosity prior 34- 45 E12.7 --- Chia [/3683]?=-99 Minimum {chi}^2^ derived without a K luminosity prior 47- 53 F7.3 --- zp [0.005/10]?=-99 Best-fit redshift after applying the prior 55- 66 E12.7 --- Chip [/1e+08]?=-99 Minimum {chi}^2^ after applying the prior 68- 74 F7.3 --- zm2 [0.005/10]?=-99 Weighted redshift after applying the prior 76- 82 F7.3 --- odds [0/1]?=-99 Parameter indicating presence of second {chi}^2^ minimum (1 if no minimum) 84- 90 F7.3 --- l68 [0.005/9.9]?=-99 1 sigma lower confidence interval 92- 98 F7.3 --- u68 [0.01/10]?=-99 1 sigma upper confidence interval 100-106 F7.3 --- l95 [0.005/9.8]?=-99 2 sigma lower confidence interval 108-114 F7.3 --- u95 [0.01/10]?=-99 2 sigma upper confidence interval 116-122 F7.3 --- l99 [0.005/9.8]?=-99 3 sigma lower confidence interval 124-130 F7.3 --- u99 [0.01/10]?=-99 3 sigma upper confidence interval 132-134 I3 --- nfilt [3/39]?=-99 Number of filters used in the fit 136-147 E12.6 --- Qual ? z quality parameter 149-156 F8.4 --- zpk [/9.9]? Default derived photometric redshift 158-164 F7.3 --- pkProb [0/1]?=-99 Peak probability 166-173 F8.4 --- zmc [0.005/10]?=-99 Randomly drawn redshift value from redshift probability distribution -------------------------------------------------------------------------------- Byte-by-byte Description of file: *zsp.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 I5 --- Seq [1/30911] Running sequence number 7- 14 F8.4 --- zsp [0/6.2]?=-99 Redshift spectroscopic (G5) -------------------------------------------------------------------------------- Byte-by-byte Description of file: cdfsfout.dat cos_fout.dat uds_fout.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 I5 --- Seq [1/30911] Running sequence number 7- 13 F7.4 --- z [0.01/9.9]? z_peak (or z_spec if available) 15- 19 F5.2 [yr-1] ltau [7/11]? Log of timescale {tau} 21- 27 F7.4 [-] Metal [0.02]? Metallicity (fixed to 0.020) 29- 33 F5.2 [yr] lage [7.5/10.1]? Log of age 35- 39 F5.2 mag Av [0/4]? Dust reddening 41- 46 F6.2 [Msun] lmass [2.5/14.4]? Log of mass 48- 53 F6.2 [Msun/yr] lsfr [-37.1/4.6]? Log of star formation rate 55- 60 F6.2 [yr-1] lssfr [-42.3/-7.4]? Log of specific star formation rate 62- 66 F5.2 --- la2t [-3.5/3.1]? log(age/tau) 68- 75 E8.3 --- chi2 [0.01/386]? minimum {chi}^2^ -------------------------------------------------------------------------------- Byte-by-byte Description of file: *sfr.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 I5 --- Seq [1/30911] Running sequence number 7- 13 F7.4 --- zPk [0.01/9.9]?=-1 Redshift peak 15- 25 E11.5 mJy F24 [-0.4/9.1]?=-99 Spitzer/MIPS 24um total flux 27- 37 E11.5 mJy e_F24 [/2]?=-99 F24 uncertainty 39- 50 E12.6 Lsun LIR ?=-99 Total integrated IR luminosity 52- 62 E11.6 Lsun L2800 [0.001/]?=-99 2800{AA} UV luminosity (1) 64- 73 E10.4 Msun/yr SFR [-4287/50740]?=-99 UV-IR star formation rate 75- 84 E10.4 Msun/yr e_SFR ?=-99 Lower uncertainty on SFR 86- 95 E10.4 Msun/yr E_SFR ?=-99 Upper uncertainty on SFR -------------------------------------------------------------------------------- Note (1): Rest-frame flux at 2800{AA} was computed using EAZY and a tophat filter of 200{AA} width (filter 274 in calibrations/FILTER_RES_DR34.latest). -------------------------------------------------------------------------------- Byte-by-byte Description of file: *3dhst.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 I5 --- Seq [1/30911] Running sequence number 7- 11 I5 --- Name [1/50506]?=-99 3D-HST ID of nearest neighbour (1) 13- 15 I3 --- Use [0/1]?=-99 3D-HST use flag (0=DON'T USE) 17- 19 I3 --- N [1/4]?=-99 Number of 3D-HST sources within 0.7" of ZFOURGE source -------------------------------------------------------------------------------- Note (1): 3D-HST sources were matched to ZFOURGE to within r<0.7". Only the ID of the nearest neighbour is displayed. 3D-HST data is available at http://3dhst.research.yale.edu/; see also Skelton+, 2014, J/ApJS/214/24 -------------------------------------------------------------------------------- Byte-by-byte Description of file: *agn.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 I5 --- Seq [1/30911] Running sequence number 7 I1 --- irAGN [0/1] Infrared AGN? (1=positive detection, 0=no detection) (1) 9- 10 I2 --- radAGN [0/1]?=-1 Radio AGN? (1=positive detection, 0=no detection) (2) 12- 13 I2 --- xAGN [0/1]?=-1 X-ray AGN? (1=positive detection, O=no detection) (3) -------------------------------------------------------------------------------- Note (1): Infrared AGN are selected using the colour-colour classifications of Messias et al. (2012): z<1.8: Ks-[4.5]>0, [4.5]-[8.0]>0 z>1.8: [8.0]-[24]>2.9x([4.5]-[8.0])+2.8, [8.0]-[24]>0.5 Note (2): Radio AGN are selected using the Rees et al. (2015) Radio AGN activity index: SFR_Radio_/SFR_IR+UV_>3.0 The minimum root-mean-square (RMS) sensitivity for the 1.4GHz data in CDFS, COSMOS and UDS fields are 6, 10 and 100uJy/beam, respectively. Note (3): X-ray AGN are selected using the Szokoly et al. (2004) classification: L_x_>=1e41erg/s & HR>-0.2 L_x_>=1e42erg/s & HR<=-0.2 The on-axis limiting X-ray flux in the soft and hard bands for the CDFS, COSMOS and UDS fields are 9.1e-18 and 5.5e-17erg/cm^2^/s, 1.9e-16 and 7.3e-16erg/cm^2^/s, and 6.0e-16 and 3.0e-15erg/cm^2^/s, respectively. -------------------------------------------------------------------------------- Byte-by-byte Description of file: *rest.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 I5 --- Seq [1/30911] Running sequence number 7- 18 E12.6 uJy Fu [-36/82505] Computed flux in the rest frame filter SDSS u (I73) (1) 20- 30 E11.6 uJy e_Fu [0/1046]? Fu uncertainty (1) 32- 43 E12.6 uJy Fg [-36/162538] Computed flux in the rest frame filter SDSS g (I74) (1) 45- 55 E11.6 uJy e_Fg [0/1799] Fg uncertainty (1) 57- 68 E12.6 uJy Fr [-36/16490] Computed flux in the rest frame filter SDSS r (I75) (1) 70- 80 E11.6 uJy e_Fr [0/2773]? Fr uncertainty (1) 82- 93 E12.6 uJy Fi [-36/19332] Computed flux in the rest frame filter SDSS i (I76) (1) 95-105 E11.6 uJy e_Fi [0/]? Fi uncertainty (1) 107-118 E12.6 uJy Fz [-36/26394] Computed flux in the rest frame filter SDSS z (I77) (1) 120-130 E11.6 uJy e_Fz [0/492]? Fz uncertainty (1) 132-143 E12.6 uJy FU [-36/83749] Computed flux in the rest frame filter Johnson U filter (I153) (1) 145-155 E11.6 uJy e_FU [0/1110]? FU uncertainty (1) 157-168 E12.6 uJy FB [-36/81872] Computed flux in the rest frame filter Johnson B filter (I154) (1) 170-180 E11.6 uJy e_FB [0/]? FB uncertainty (1) 182-193 E12.6 uJy FV [-36/136753] Computed flux in the rest frame filter Johnson V filter (I155) (1) 195-205 E11.6 uJy e_FV [0/512]? FV uncertainty (1) 207-218 E12.6 uJy FJ [-36/38317] Computed flux in the rest frame filter 2MASS J filter (I161) (1) 220-230 E11.6 uJy e_FJ [0/477]? FJ uncertainty (1) 232-243 E12.6 uJy FH [-36/26626] Computed flux in the rest frame filter 2MASS H filter (I162) (1) 245-255 E11.6 uJy e_FH [0/170]? FH uncertainty (1) 257-268 E12.6 uJy FK [-36/21396] Computed flux in the rest frame filter 2MASS Ks filter (I163) (1) 270-280 E11.6 uJy e_FK [0/]? FK uncertainty (1) 282-293 E12.6 uJy Fuv13 [-36/59450] Computed flux in the rest frame filter centered at 1300{AA} (I293) (1) 295-305 E11.6 uJy e_Fuv13 [0/]? Fuv13 uncertainty (1) 307-318 E12.6 uJy Fuv15 [-36/61064] Computed flux in the rest frame filter centered at 1500{AA} (I294) (1) 320-330 E11.6 uJy e_Fuv15 [0/624]? Fuv15 uncertainty (1) 332-343 E12.6 uJy Fuv19 [-36/55309] Computed flux in the rest frame filter centered at 1900{AA} (I295) (1) 345-355 E11.6 uJy e_Fuv19 [0/550]? Fuv19 uncertainty (1) 357-368 E12.6 uJy Fuv22 [-36/49546] Computed flux in the rest frame filter centered at 2200{AA} (I296) (1) 370-380 E11.6 uJy e_Fuv22 [0/522]? Fuv22 uncertainty (1) 382-393 E12.6 uJy Fuv28 [-36/44349] Computed flux in the rest frame filter centered at 2800{AA} (I297) (1) 395-405 E11.6 uJy e_Fuv28 [0/]? Fuv28 uncertainty (1) -------------------------------------------------------------------------------- Note (1): These catalogs are in units of uJy. To convert back to catalog fluxes (AB flux densities with zeropoint 25), divide by 10**((23.9-25)/2.5). To convert to solar luminosities: 1. Convert to ergs/cm^2^/s/{AA} -- flux density [uJy] *10**-29 *3*10**18 /lambda_c**2, where lambda_c is the central wavelength of the filter bandpass. 2. Convert from flux density to flux -- multiply by lambda_c -------------------------------------------------------------------------------- Byte-by-byte Description of file: *rad.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 I5 --- Seq [1/30911] Running sequence number 7- 13 F7.1 uJy/beam F1.4GHz [0/53640]?=-99 Peak or integrated flux density at 1.4GHz (f_14) (1) 15- 19 F5.1 uJy/beam e_F1.4GHz [6/147]?=-99 F1.4GHz uncertainty 21- 27 E7.3 W/Hz L1.4GHz ?=-99 Rest-frame 1.4GHz luminosity (2) -------------------------------------------------------------------------------- Note (1): For M13, F1.4GHz includes a combination of peak and integrated fluxes, with the final value chosen based on the author's recommendation. For the other fields, the integrated flux is used. Note (2): The rest-frame radio luminosity is calculated using: L1.4GHz=(4*pi*ld**2)*F1.4GHz*(1+z_peak)**({alpha}-2) where ld is the luminosity distance (cm) and {alpha} is the radio spectral index (fixed to {alpha}=-0.3). -------------------------------------------------------------------------------- Byte-by-byte Description of file: *vdw.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 I5 --- Seq [1/30911] Running sequence number 7- 11 F5.2 --- wmin [0/33.4] wmin>0 for HST coverage 13- 19 F7.2 arcsec Sep [0/0.7]?=-999 Separation of the ZFOURGE object and the vdW14 (1) 21 A1 --- f_Sep Number of matches flag (0=single match) (2) 23- 27 I5 --- [SWM2014] [/50506]?=-999 Number in vdW14 (3) 29- 39 F11.6 deg RAdeg ?=-999 vdW14 right ascension (J2000) 41- 51 F11.6 deg DEdeg ?=-999 vdW14 declination (J2000) 53- 59 F7.2 arcsec Reff [0.02/24]?=-999 vdW14 effective radius 61- 69 F9.2 arcsec e_Reff [0/348635]?=-999 Reff uncertainty 71- 77 F7.2 --- n [0.2/8]?=-999 vdW14 sersic index 79- 86 F8.2 --- e_n [0/50193]?=-999 n uncertainty 88- 94 F7.2 --- q [0/1]?=-999 vdW14 axis ratio 96-103 F8.2 --- e_q [0/25330]?=-999 q uncertainty 105-111 F7.2 mag mag [9/30]?=-999 vdW14 HST/WFC3 F160W AB magnitude 113-120 F8.2 mag e_mag [0/59353]?=-999 mag uncertainty 122-128 F7.2 deg PA [-90/90]?=-999 vdW14 position angle 130-139 F10.2 deg e_PA ?=-999 PA uncertainty 141-150 F10.2 --- S/N ?=-999 vdW14 object S/N 152-155 I4 --- Fit [/3]?=-999 vdW14 goodness of fit flag -------------------------------------------------------------------------------- Note (1): Sources from X_F160W_galfit_v4.0.cat (vdW14) were matched to ZFOURGE to within r<0.7". If an object has multiple or no matches, the 'Sep' column has a value of -999. Note (2): Flags the number of van der Wel+ 2014ApJ...788...28V catalog matches to a single ZFOURGE object as follows: 0 = single matches, 1 = multiple matches, 2 = no matches Note (3): Objects are <[SWM2014] GOODS-S NNNNN> or <[SWM2014] COSMOS NNNNN> or <[SWM2014] UDS NNNNN> in Simbad. -------------------------------------------------------------------------------- Byte-by-byte Description of file: cdfsx.dat cosmosx.dat udsx.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 I5 --- Seq [1/30911] Running sequence number 7- 14 E8.2 10-3W/m2 Fx ?=-99 Full band X-ray flux in erg/cm^2^/s (1) 16- 23 E8.3 10-7W Lx ?=-99 Rest-frame X-ray luminosity in erg/s (2) 25- 30 F6.2 --- HR [-0.9/0.9]?=-99 Hardness ratio (3) -------------------------------------------------------------------------------- Note (1): In the absence of a full-band flux value, Fx is calculated considering a counts-to-flux conversion factor with photon index {Gamma}=1.4 For sources from X11, the intrinsic flux is derived from counts in the 0.5-8keV full band, while from E09 and U08 it is derived from the sum of the counts in the relevant bands over 0.5-10keV. Flux values were adjusted for sources from E09 and U08 to align with the full bandpass values of X11 by assuming a power-law model with photon index {Gamma}=1.4 (i.e. E09 and U08 fluxes are multiplied by a factor of 0.95). Note (2): The rest-frame X-ray luminosity is calculated using: Lx=(4*pi*ld**2)*f_x*(1+z_peak)**({Gamma}-2) where ld is the luminosity distance (cm) and {Gamma} is the photon index (fixed to {Gamma}=1.4). Note (3): The hardness ratio (HR) is calculated using: HR = (H-S)/(H+S) where H and S are the count rates in the hard (2-8 or 2-10keV) and soft (0.5-2keV) bands, respectively. -------------------------------------------------------------------------------- Byte-by-byte Description of file: cdfs_her.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 I5 --- Seq [1/30911] Running sequence number 7- 13 F7.4 --- z [0.01/9.7]?=-1 Photometric redshift (or spectroscopic if available) 15- 25 E11.5 mJy F24 [-0.3/8.1]?=-99 Spitzer/MIPS 24um total flux 27- 37 E11.5 mJy e_F24 [0/0.3]?=-99 F24 uncertainty 39- 49 E11.5 mJy F100 [-8.1/196.1]?=-99 Herschel/PACS 100um flux 51- 61 E11.5 mJy e_F100 [0/1.2]?=-99 F100 uncertainty 63- 73 E11.5 mJy F160 [-7.2/224.8]?=-99 Herschel/PACS 160um flux 75- 85 E11.5 mJy e_F160 [0/3.6]?=-99 F160 uncertainty 87- 98 E12.6 Lsun LIR ?=-99 Total integrated IR luminosity 100-110 E11.6 Lsun LUV ?=-99 Total UV luminosity 112-122 E11.5 --- SFR Star formation rate (equation 6) (1) -------------------------------------------------------------------------------- Note (1): We use the conversion from Bell+ (2005ApJ...625...23B) to calculate SFRs from our data, scaled to a Chabrier (2003PASP..115..763C) IMF Equation (6): SFR[M_{sun}_/yr]=1.09x10^-10^(L_IR_+2.2L_UV_). -------------------------------------------------------------------------------- Byte-by-byte Description of file: zf_cosmos.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 I5 --- Seq [1/20786] Running sequence number (id) 7- 14 F8.3 pix xpos Pixel X coordinates (scale:0.15"/pixel) (x) 16- 23 F8.3 pix ypos Pixel Y coordinates (scale:0.15"/pixel) (y) 25- 35 F11.7 deg RAdeg Right ascension (J2000) 37- 45 F9.7 deg DEdeg Declination (J2000) 47- 48 I2 --- SE [0/19] Source Extractor flag (SEflags) (G4) 50- 56 F7.1 pix2 IsoArea [1/26678] Isophotal area above Source Extractor analysis threshold (iso_area) 58- 71 F14.8 0.3631uJy FKsap [0.07/12352]?=-99 (convolved) Ks-band aperture flux within a 1.2" diameter circular aperture (fap_Ksall) 73- 84 F12.8 0.3631uJy e_FKsap [0.07/0.3]?=-99 FKsap uncertainty (eap_Ksall) 86- 94 F9.7 --- apcorr [0.9/1.7] Aperture correction applied to FKsauto to obtain FKsall (FKsall=FKsauto*apcorr) (apcorr) 96- 106 F11.7 --- KsR [0.5/309] Ratio between FKsap and FKsall (KsR=FKsall/FKsap) (Ks_ratio) 108- 120 F13.7 0.3631uJy FKsapD [0.1/10933]?=-99 Aperture flux measured within 0.9" diameter (seeing dependent) circular aperture (fapcirc09_Ksall) 122- 133 F12.8 0.3631uJy e_FKsapD [0.06/0.3]?=-99 FKsapD uncertainty (eapcirc09_Ksall) 135- 142 F8.6 --- apcorrD [1.6/1.7] Aperture correction applied to FKsapD to obtain FKsD (FKsD=FKsapD*apcorrD) (apcorr09) 144- 156 F13.7 0.3631uJy FKsD [0.2/18001]?=-99 Total (aperture corrected) Ks-band flux within a 0.9" diameter (seeing dependent) circular aperture (fcirc09_Ksall) 158- 168 F11.7 0.3631uJy e_FKsD [0.1/0.4]?=-99 FKsD uncertainty (ecirc09_Ksall) 170- 182 F13.7 0.3631uJy FKsauto [0.06/47726] Ks-band flux within a Kron-like elliptical aperture (fauto_Ksall) 184- 190 F7.3 pix R50 [0.7/139] Radius enclosing 50% of the Ks-band flux (flux50_radius) 192- 198 F7.3 pix amaj [0.5/231] Major axis of a Kron-like elliptical aperture (a_vector) 200- 205 F6.3 pix bmin [0.2/19.5] Minor axis of a Kron-like elliptical aperture (b_vector) 207- 212 F6.3 --- Rad [0/76.5] Radius of a circularized Kron-like elliptical aperture (kron_radius) 214- 226 F13.7 0.3631uJy FKsall [0.2/48199]?=-99 Total (aperture corrected) Ks-band flux within a Kron-like elliptical aperture (f_Ksall) 228- 238 F11.7 0.3631uJy e_FKsall [0.1/9.1]?=-99 FKsall uncertainty (e_Ksall) 240- 243 F4.2 --- w_FKsall [0/1.4] Weight corresponding to FKsall, median normalized (w_Ksall) 245- 267 E23.20 0.3631uJy FB [-106.3/1687] Aperture flux in Subaru/Suprime-Cam B-band, corrected to total (f_B) (1) 269- 288 F20.18 0.3631uJy e_FB [0.006/3.5] FB uncertainty (e_B) 290- 292 F3.1 --- w_FB [1] Weight corresponding to FB, median normalized (w_B) 294- 316 E23.20 0.3631uJy Fg [-8/3738] Aperture flux in CFHT g-band, corrected to total (f_G) (1) 318- 337 F20.18 0.3631uJy e_Fg [0.008/4.7] Fg uncertainty (e_G) 339- 341 F3.1 --- w_Fg [1] Weight corresponding to Fg, median normalized (w_G) 343- 364 E22.19 0.3631uJy Fi [-13.4/7044] Aperture flux in CFHT i-band, corrected to total (f_I) (1) 366- 385 F20.18 0.3631uJy e_Fi [0.009/5.5] Fi uncertainty (e_I) 387- 389 F3.1 --- w_Fi [1] Weight corresponding to Fi, median normalized (w_I) 391- 413 E23.20 0.3631uJy IA427 [-134.1/7821] Aperture flux in Subaru/Suprime-Cam IA427 band, corrected to total (f_IA427) (1) 415- 435 F21.18 0.3631uJy e_IA427 [0.02/13] IA427 uncertainty (e_IA427) 437- 439 F3.1 --- w_IA427 [1] Weight corresponding to FI, median normalized (w_IA427) 441- 462 E22.20 0.3631uJy IA484 [-134/4489] Aperture flux in Subaru/Suprime-Cam IA484 band, corrected to total (f_IA484) (1) 464- 484 F21.18 0.3631uJy e_IA484 [0.02/12] IA484 uncertainty (e_IA484) 486- 488 F3.1 --- w_IA484 [1] Weight corresponding to IA484, median normalized (w_IA484) 490- 512 E23.20 0.3631uJy IA505 [-521/5478] Aperture flux in Subaru/Suprime-Cam IA505 band, corrected to total (f_IA505) (1) 514- 534 F21.18 0.3631uJy e_IA505 [0.02/14] IA505 uncertainty (e_IA505) 536- 538 F3.1 --- w_IA505 [1] Weight corresponding to IA505, median normalized (w_IA505) 540- 562 E23.20 0.3631uJy IA527 [-269/5411] Aperture flux in Subaru/Suprime-Cam IA527 band, corrected to total (f_IA527) (1) 564- 584 F21.18 0.3631uJy e_IA527 [0.01/11] IA527 uncertainty (e_IA527) 586- 588 F3.1 --- w_IA527 [1] Weight corresponding to IA527, median normalized (w_IA527) 590- 612 E23.20 0.3631uJy IA624 [-508/4105] Aperture flux in Subaru/Suprime-Cam IA624 band, corrected to total (f_IA624) (1) 614- 634 F21.18 0.3631uJy e_IA624 [0.01/12] IA624 uncertainty (e_IA624) 636- 638 F3.1 --- w_IA624 [1] Weight corresponding to IA624, median normalized (w_IA624) 640- 661 E22.20 0.3631uJy IA709 [-657/3754] Aperture flux in Subaru/Suprime-Cam IA709 band, corrected to total (f_IA709) (1) 663- 683 F21.18 0.3631uJy e_IA709 [0.02/14] IA709 uncertainty (e_IA709) 685- 687 F3.1 --- w_IA709 [1] Weight corresponding to IA709, median normalized (w_IA709) 689- 713 F25.20 0.3631uJy IA738 [-714/5741] Aperture flux in Subaru/Suprime-Cam IA738 band, corrected to total (f_IA738) (1) 715- 735 F21.18 0.3631uJy e_IA738 [0.02/17] IA738 uncertainty (e_IA738) 737- 739 F3.1 --- w_IA738 [1] Weight corresponding to IA738, median normalized (w_IA738) 741- 765 F25.20 0.3631uJy Fr [-11/5958] Aperture flux in CFHT r-band, corrected to total (f_R) (1) 767- 786 F20.18 0.3631uJy e_Fr [0.008/5] Fr uncertainty (e_R) 788- 790 F3.1 --- w_Fr [1] Weight corresponding to Fr, median normalized (w_R) 792- 814 E23.20 0.3631uJy Fu [-16/3387] Aperture flux in CFHT u-band, corrected to total (f_U) (1) 816- 835 F20.18 0.3631uJy e_Fu [0.01/7] Fu uncertainty (e_U) 837- 839 F3.1 --- w_Fu [1] Weight corresponding to Fu, median normalized (w_U) 841- 866 F26.20 0.3631uJy FV [-179/3909] Aperture flux in Subaru/Suprime-Cam V-band, corrected to total (f_V) (1) 868- 887 F20.18 0.3631uJy e_FV [0.01/6] FV uncertainty (e_V) 889- 891 F3.1 --- w_FV [1] Weight corresponding to FV, median normalized (w_V) 893- 917 F25.20 0.3631uJy FRp [-181/3572] Aperture flux in Subaru/Suprime-Cam r+ -band, corrected to total (f_Rp) (1) 919- 938 F20.18 0.3631uJy e_FRp [0.009/5.4] Rp uncertainty (e_Rp) 940- 942 F3.1 --- w_FRp [1] Weight corresponding to FRp, median normalized (w_Rp) 944- 965 E22.20 0.3631uJy Fz [-4.1/12315] Aperture flux in CFHT z-band, corrected to total (f_Z) (1) 967- 987 F21.18 0.3631uJy e_Fz [0.02/16] Fz uncertainty (e_Z) 989- 991 F3.1 --- w_Fz [1] Weight corresponding to Fz, median normalized (w_Z) 993-1016 F24.19 0.3631uJy FZp [-393/2186] Aperture flux in Subaru/Suprime-Cam z+ -band, corrected to total (f_Zp) (1) 1018-1038 F21.18 0.3631uJy e_FZp [0.03/21] FZp uncertainty (e_Zp) 1040-1042 F3.1 --- w_FZp [1] Weight corresponding to FZp, median normalized (w_Zp) 1044-1069 F26.20 0.3631uJy FHl [-8/48610]?=-99 Aperture flux in FourStar Hl-band, corrected to total (f_Hl) (1) 1071-1091 F21.17 0.3631uJy e_FHl [0.1/15.4]?=-99 FHl uncertainty (e_Hl) 1093-1096 F4.2 --- w_FHl [0/1.3] Weight corresponding to FHl, median normalized (w_Hl) 1098-1123 F26.20 0.3631uJy FHs [-33/41119]?=-99 Aperture flux in FourStar Hs-band, corrected to total (f_Hs) (1) 1125-1145 F21.17 0.3631uJy e_FHs [0.1/26]?=-99 FHs uncertainty (e_Hs) 1147-1150 F4.2 --- w_FHs [0/1.3] Weight corresponding to FHs, median normalized (w_Hs) 1152-1176 F25.19 0.3631uJy FJ1 [-33/25077]?=-99 Aperture flux in FourStar J1-band, corrected to total (f_J1) (1) 1178-1199 F22.18 0.3631uJy e_FJ1 [0.04/22]?=-99 FJ1 uncertainty (e_J1) 1201-1204 F4.2 --- w_FJ1 [0/1.4] Weight corresponding to FJ1, median normalized (w_J1) 1206-1227 E22.20 0.3631uJy FJ2 [-13/23328]?=-99 Aperture flux in FourStar J2-band, corrected to total (f_J2) (1) 1229-1250 F22.18 0.3631uJy e_FJ2 [0.04/23]?=-99 FJ2 uncertainty (e_J2) 1252-1255 F4.2 --- w_FJ2 [0/1.4] Weight corresponding to FJ2, median normalized (w_J2) 1257-1282 F26.20 0.3631uJy FJ3 [-7/24545]?=-99 Aperture flux in FourStar J3-band, corrected to total (f_J3) (1) 1284-1304 F21.17 0.3631uJy e_FJ3 [0.06/9.1]?=-99 FJ3 uncertainty (e_J3) 1306-1309 F4.2 --- w_FJ3 [0/1.4] Weight corresponding to FJ3, median normalized (w_J3) 1311-1335 F25.19 0.3631uJy FKs [-22/31171]?=-99 Aperture flux in FourStar Ks-band, corrected to total (f_Ks) (1) 1337-1357 F21.17 0.3631uJy e_FKs [0.09/49]?=-99 FKs uncertainty (e_Ks) 1359-1362 F4.2 --- w_FKs [0/1.4] Weight corresponding to FKs, median normalized (w_Ks) 1364-1379 F16.10 0.3631uJy NB118 [-13/48391]?=-99 Aperture flux in FourStar NB118, corrected to total (f_NB118) (1) 1381-1391 F11.7 0.3631uJy e_NB118 [0.1/8]?=-99 NB118 uncertainty (e_NB118) 1393-1396 F4.2 --- w_NB118 [0/1.3] Weight corresponding to NB118, median normalized (w_NB118) 1398-1410 E13.10 0.3631uJy NB209 [-33/42375]?=-99 Aperture flux in FourStar NB209, corrected to total (f_NB209) (1) 1412-1422 F11.7 0.3631uJy e_NB209 [0.2/20.6]?=-99 NB209 uncertainty (e_NB209) 1424-1427 F4.2 --- w_NB209 [0/1.2] Weight corresponding to NB209, median normalized (w_NB209) 1429-1440 E12.9 0.3631uJy F125W [-8/157256]?=-99 Aperture flux in HST/WFC3 F125W-band, corrected to total (f_F125W) (1) 1442-1452 F11.7 0.3631uJy e_F125W [0.02/3]?=-99 F125W uncertainty (e_F125W) 1454-1457 F4.2 --- w_F125W [0/6.6] Weight corresponding to F125W, median normalized (w_F125W) 1459-1470 E12.9 0.3631uJy F140W [-6/100892]?=-99 Aperture flux in HST/WFC3 F140W-band, corrected to total (f_F140W) (1) 1472-1482 F11.7 0.3631uJy e_F140W [0.07/4.5]?=-99 F140W uncertainty (e_F140W) 1484-1487 F4.2 --- w_F140W [0/3] Weight corresponding to F140W, median normalized (w_F140W) 1489-1504 F16.9 0.3631uJy F160W [-10/173059]?=-99 Aperture flux in HST/WFC3 F160W-band, corrected to total (f_F160W) (1) 1506-1516 F11.7 0.3631uJy e_F160W [0.02/2.6]?=-99 F160W uncertainty (e_F160W) 1518-1521 F4.2 --- w_F160W [0/3.7] Weight corresponding to F160W, median normalized (w_F160W) 1523-1547 F25.20 0.3631uJy F606W [-6/2170]?=-99 Aperture flux in HST/ACS F606W, corrected to total (f_F606W) (1) 1549-1570 F22.18 0.3631uJy e_F606W [0.02/9]?=-99 F606W uncertainty (e_F606W) 1572-1575 F4.2 --- w_F606W [0/2.6] Weight corresponding to F606W, median normalized (w_F606W) 1577-1601 F25.20 0.3631uJy F814W [-7/7950]?=-99 Aperture flux in HST/ACS F814W, corrected to total (f_F814W) (1) 1603-1624 F22.18 0.3631uJy e_F814W [0.02/4.7]?=-99 F814W uncertainty (e_F814W) 1626-1629 F4.2 --- w_F814W [0/2.6] Weight corresponding to F814W, median normalized (w_F814W) 1631-1656 F26.20 0.3631uJy FJvista [-38.3/57162] Aperture flux UVISTA J-band, corrected to total (f_UVISTA_J) (1) 1658-1677 F20.17 0.3631uJy e_FJvista [0.04/29] FJvista uncertainty (e_UVISTA_J) 1679-1682 F4.2 --- w_FJvista [0.4/1.3] Weight corresponding to FJvista, median normalized (w_UVISTA_J) 1684-1708 F25.19 0.3631uJy FHvista [-28/64424] Aperture flux UVISTA H-band, corrected to total (f_UVISTA_H) (1) 1710-1729 F20.17 0.3631uJy e_FHvista [0.07/41] FJvista uncertainty (e_UVISTA_H) 1731-1734 F4.2 --- w_FHvista [0.2/1.3] Weight corresponding to FHvista, median normalized (w_UVISTA_H) 1736-1760 F25.19 0.3631uJy FKsvista [-8/50829]?=-99 Aperture flux UVISTA Ks-band, corrected to total (f_UVISTA_Ks) (1) 1762-1782 F21.17 0.3631uJy e_FKsvista [0.07/47]?=-99 FKsvista error (e_UVISTA_Ks) 1784-1787 F4.2 --- w_FKsvista [0.05/1.3] Weight corresponding to FKsvista, median normalized (w_UVISTA_Ks) 1789-1814 F26.20 0.3631uJy FYvista [-23/62157]?=-99 Aperture flux UVISTA Y-band, corrected to total (f_UVISTA_Y) (1) 1816-1837 F22.18 0.3631uJy e_FYvista [0.03/23]?=-99 FYvista error (e_UVISTA_Y) 1839-1842 F4.2 --- w_FYvista [0.3/1.3] Weight corresponding to FYvista, median normalized (w_UVISTA_Y) 1844-1866 E23.20 0.3631uJy F3.6 [-1141/19908] Spitzer/IRAC 3.6um-band, corrected to total (f_IRAC_36) (1) 1868-1888 F21.17 0.3631uJy e_F3.6 [-3/25]?=-99 F3.6 uncertainty (e_IRAC_36) 1890-1895 F6.2 --- w_F3.6 [0.02/1.4]?=-99 Weight corresponding to 3.6um, median normalized (w_IRAC_36) 1897-1918 E22.20 0.3631uJy F4.5 [-527/27177] Spitzer/IRAC 4.5um-band, corrected to total (f_IRAC_45) (1) 1920-1940 F21.17 0.3631uJy e_F4.5 [-3/20]?=-99 F4.5 uncertainty (e_IRAC_45) 1942-1947 F6.2 --- w_F4.5 [0.07/1.3]?=-99 Weight corresponding to 4.5um, median normalized (w_IRAC_45) 1949-1974 F26.20 0.3631uJy F5.8 [-197/45331] Spitzer/IRAC 5.8um-band, corrected to total (f_IRAC_58) (1) 1976-1995 F20.16 0.3631uJy e_F5.8 [-53/269]?=-99 F5.8 uncertainty (e_IRAC_58) 1997-2002 F6.2 --- w_F5.8 [0.6/1.5]?=-99 Weight corresponding to 5.8um, median normalized (w_IRAC_58) 2004-2028 F25.19 0.3631uJy F8.0 [-278/21088] Spitzer/IRAC 8.0um-band, corrected to total (f_IRAC_80) (1) 2030-2049 F20.16 0.3631uJy e_F8.0 [-65/317]?=-99 F8.0 uncertainty (e_IRAC_80) 2051-2056 F6.2 --- w_F8.0 [0.7/1.5]?=-99 Weight corresponding to 8.0um, median normalized (w_IRAC_80) 2058-2060 F3.1 --- wminOpt [0/1] Minimum weight of groundbased optical filters (wmin_optical) 2062-2065 F4.2 --- wminHST1 [0/1] Minimum weight of HST optical filters (wmin_hst_optical) 2067-2070 F4.2 --- wminfs [0/2.6] Minimum weight of FourStar filters (wmin_fs) 2072-2075 F4.2 --- wminjhk [0/1.4] Minimum weight of broadband JHK filters (wmin_jhk) 2077-2080 F4.2 --- wminHST2 [0/1.3] Minimum weight of HST NIR filters (wmin_hst) 2082-2085 F4.2 --- wminIRAC [0/1.4] Minimum weight of Spitzer/IRAC filters (wmin_irac) 2087-2090 F4.2 --- wminall [0/1.4] Minimum weight of all filters (wmin_all) 2092 I1 --- Star [0/1] 1=star (star) (G1) 2094 I1 --- Nghb [0/1] 1=near a bright star (nearstar) (G2) 2096 I1 --- Use [0/1] 1=source selected (use) (G3) 2098-2110 F13.6 --- SNR [0/149626] signal-to-noise (=FKsapD/e_FKsapD) (snr) 2112-2119 F8.4 --- zspec [0/6.1]?=-99 Spectroscopic redshift (z_spec) (G5) -------------------------------------------------------------------------------- Note (1): (convolved) aperture flux in filter [] within a 1.2" diameter circular aperture, corrected to total (Fap[]=F[]/KsR) CDFS passband parameters as in table 3: -------------------------------------------------------------- Filter lam_C_ FWHM Zeropoint Offset Galactic (um) (arcsec) (AB mag) extinction (G6) (AB mag) (AB mag) -------------------------------------------------------------- B 0.4448 0.61 31.129 -0.195 -0.076 G 0.4870 0.90 26.290 -0.015 -0.069 I 0.7676 0.77 25.759 0.091 -0.034 IA427 0.4260 0.79 31.119 -0.202 -0.079 IA484 0.4847 0.75 31.214 -0.116 -0.069 IA505 0.5061 0.82 31.252 -0.083 -0.065 IA527 0.5259 0.74 31.281 -0.058 -0.061 IA624 0.6231 0.72 31.348 -0.002 -0.050 IA709 0.7074 0.81 31.343 -0.015 -0.042 IA738 0.7359 0.80 31.347 -0.014 -0.039 R 0.6245 0.79 25.903 0.023 -0.047 U 0.3828 0.82 24.913 -0.235 -0.086 V 0.5470 0.80 31.418 0.077 -0.059 Rp 0.6276 0.83 31.453 0.100 -0.047 Z 0.8872 0.74 24.859 0.121 -0.030 Zp 0.9028 0.90 31.557 0.187 -0.030 Hl 1.7020 0.60 26.624 0.033 -0.010 Hs 1.5544 0.54 26.673 0.062 -0.012 J1 1.0540 0.57 26.358 0.026 -0.020 J2 1.1448 0.55 26.590 0.038 -0.018 J3 1.2802 0.53 26.573 0.011 -0.016 Ks 2.1538 0.47 26.918 -0.011 -0.006 NB118 1.1909 0.58 24.637 0.000 -0.018 NB209 2.0990 0.52 24.849 0.000 -0.006 F125W 1.2471 0.26 26.236 -0.000 -0.011 F140W 1.3924 0.26 26.455 -0.000 -0.010 F160W 1.5396 0.26 25.948 -0.000 -0.008 F606W 0.5921 0.20 26.437 -0.016 -0.038 F814W 0.8057 0.21 25.951 0.032 -0.024 UVISTA_J 1.2527 0.82 30.052 0.062 -0.011 UVISTA_H 1.6433 0.81 29.995 0.003 -0.008 UVISTA_Ks 2.1503 0.79 30.028 0.035 -0.006 UVISTA_Y 1.0217 0.85 30.045 0.061 -0.016 IRAC_36 3.5569 1.70 21.530 -0.051 0.000 IRAC_45 4.5020 1.70 21.537 -0.044 0.000 IRAC_58 5.7450 1.90 21.577 -0.004 0.000 IRAC_80 7.9158 2.00 21.520 -0.061 0.000 -------------------------------------------------------------- In COSMOS we added CFHT/u, g, r, i, z-imaging (Erben+ 2009A&A...493.1197E; Hildebrandt+ 2009A&A...498..725H), Subaru/Suprime-Cam/B, V, r+, z+-imaging and 7 Subaru/Suprime-Cam optical medium-bandwidth filters (Taniguchi+ 2007ApJS..172....9T) with seeing <1.1" (from a set of 12, including seeing >1.1" images), HST/WFC3/F125W, F140W,F160W and HST/ACSF606W, F814W-imaging (Grogin+ 2011ApJS..197...35G; Koekemoer+ 2011ApJS..197...36K; Brammer+ 2012ApJS..200...13B) and UltraVISTA/Y, J, H, Ks-imaging (McCracken+ 2012, J/A+A/544/A156). -------------------------------------------------------------------------------- Byte-by-byte Description of file: zf_uds.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 I5 --- Seq [1/22093] Running sequence number (id) 7- 14 F8.3 pix xpos X pixel coordinate (scale: 0.15"/pixel) (x) 16- 23 F8.3 pix ypos Y pixel coordinate (scale: 0.15"/pixel) (y) 25- 34 F10.7 deg RAdeg [34.1/34.5] Right ascension (J2000) (ra) 36- 45 F10.7 deg DEdeg [-5.4/-5] Declination (J2000) (dec) 47- 48 I2 --- SE [0/19] Source Extractor flags (SEflags) (G4) 50- 56 F7.1 pix2 isoArea [0/11593] Isophotal area above Source Extractor analysis threshold (iso_area) 58- 71 F14.8 0.3631uJy FKsap [0.08/27497] (convolved) Ks-band aperture flux within a 1.2" diameter circular aperture (fap_Ksall) 73- 82 F10.8 0.3631uJy e_FKsap [0.04/0.2] FKsap uncertainty (eap_Ksall) 84- 92 F9.7 --- apcorr [0.9/1.8] Aperture correction applied to FKsauto to obtain FKsall (FKsall=FKsauto*apcorr) (apcorr) 94- 103 F10.7 0.3631uJy KsR [0.6/36.4] Ratio between FKsap and FKsall (KsR=FKsall/FKsap) (Ks_ratio) 105- 118 F14.8 0.3631uJy FKsapD [0.09/20499] Aperture flux measured within 0.9" diameter (seeing dependent) circular aperture (fapcirc09_Ksall) 120- 129 F10.8 0.3631uJy e_FKsapD [0.04/0.2] FKsapD uncertainty (eapcirc09_Ksall) 131- 138 F8.6 --- apcorrD [1.7/1.8] Aperture correction applied to FKsapD to obtain FKsD (FKsD=FKsapD*apcorrD) (apcorr09) 140- 152 F13.7 0.3631uJy FKsD [0.1/36322] Total (aperture corrected) Ks-band flux within 0.9" diameter (seeing dependent) circular aperture (fcirc09_Ksall) 154- 163 F10.8 0.3631uJy e_FKsD [0.08/0.2] FKsD uncertainty (ecirc09_Ksall) 165- 179 F15.8 0.3631uJy FKsauto [0.08/66825] Ks-band flux within a Kron-like elliptical aperture (fauto_Ksall) 181- 186 F6.3 pix R50 [0.7/32.5] Radius enclosing 50% of the Ks-band flux (flux50_radius) 188- 193 F6.3 pix amaj [0.5/32.4] Major axis of a Kron-like elliptical aperture (a_vector) 195- 200 F6.3 pix bmin [0.2/13.8] Minor axis of a Kron-like elliptical aperture (b_vector) 202- 207 F6.3 --- Rad [0/63.3] Radius of a circularized Kron-like elliptical aperture (kron_radius) 209- 221 F13.7 0.3631uJy FKsall [0.1/68011]?=-99 Total (aperture corrected) Ks-band flux within a Kron-like elliptical aperture (f_Ksall) 223- 234 F12.8 0.3631uJy e_FKsall [0.08/2.6]?=-99 FKsall uncertainty (e_Ksall) 236- 239 F4.2 --- w_FKsall [0/1.8] Weight corresponding to FKsall, median normalized (w_Ksall) 241- 263 E23.20 0.3631uJy Fu [-0.5/1577]?=-99 Aperture flux in CFHT/MegaCam U-band, corrected to total (f_u) (1) 265- 286 F22.18 0.3631uJy e_Fu [0.02/1.3]?=-99 Fu uncertainty (e_u) 288- 290 F3.1 --- w_Fu [0/1] Weight corresponding to Fu, median normalized (w_u) 292- 314 E23.20 0.3631uJy FB [-0.1/968]?=-99 Aperture flux in Subaru/Suprime-Cam B-band, corrected to total (f_B) (1) 316- 338 F23.19 0.3631uJy e_FB [0.004/0.2]?=-99 FB uncertainty (e_B) 340- 342 F3.1 --- w_FB [0/1] Weight corresponding to Fu, median normalized (w_B) 344- 366 E23.20 0.3631uJy FV [-0.2/1126]?=-99 Aperture flux in Subaru/Suprime-Cam V-band, corrected to total (f_V) (1) 368- 390 F23.19 0.3631uJy e_FV [0.004/0.3]?=-99 FV uncertainty (e_V) 392- 394 F3.1 --- w_FV [0/1] Weight corresponding to FV, median normalized (w_V) 396- 418 E23.20 0.3631uJy FR [-0.2/1210]?=-99 Aperture flux in Subaru/Suprime-Cam R-band, corrected to total (f_R) (1) 420- 441 F22.18 0.3631uJy e_FR [0.006/0.4]?=-99 FR uncertainty (e_R) 443- 445 F3.1 --- w_FR [0/1] Weight corresponding to FR, median normalized (w_R) 447- 468 E22.20 0.3631uJy Fi [-0.09/1217]?=-99 Aperture flux in Subaru/Suprime-Cam i-band, corrected to total (f_i) (1) 470- 492 F23.19 0.3631uJy e_Fi [0.006/0.4]?=-99 Fi uncertainty (e_i) 494- 496 F3.1 --- w_Fi [0/1] Weight corresponding to Fi, median normalized (w_i) 498- 522 F25.20 0.3631uJy Fz [-0.5/2716]?=-99 Aperture flux in Subaru/Suprime-Cam z-band, corrected to total (f_z) (1) 524- 545 F22.18 0.3631uJy e_Fz [0.01/1]?=-99 Fz uncertainty (e_z) 547- 549 F3.1 --- w_Fz [0/1] Weight corresponding to Fz, median normalized (w_z) 551- 573 E23.20 0.3631uJy FJ1 [-7/22115]?=-99 Aperture flux in FourStar J1-band, corrected to total (f_J1) (1) 575- 596 F22.18 0.3631uJy e_FJ1 [0.04/23.5]?=-99 FJ1 uncertainty (e_J1) 598- 601 F4.2 --- w_FJ1 [0/1.3] Weight corresponding to FJ1, median normalized (w_J1) 603- 624 E22.20 0.3631uJy FJ2 [-4/15074]?=-99 Aperture flux in FourStar J2-band, corrected to total (f_J2) (1) 626- 647 F22.18 0.3631uJy e_FJ2 [0.04/2.8]?=-99 FJ2 uncertainty (e_J2) 649- 652 F4.2 --- w_FJ2 [0/1.3] Weight corresponding to FJ2, median normalized (w_J2) 654- 679 F26.20 0.3631uJy FJ3 [-19/30881]?=-99 Aperture flux in FourStar J3-band, corrected to total (f_J3) (1) 681- 702 F22.18 0.3631uJy e_FJ3 [0.05/26.4]?=-99 FJ3 uncertainty (e_J3) 704- 707 F4.2 --- w_FJ3 [0/1.3] Weight corresponding to FJ3, median normalized (w_J3) 709- 720 E12.9 0.3631uJy FHs [-6/31381]?=-99 Aperture flux in FourStar Hs-band, corrected to total (f_Hs) (1) 722- 732 F11.7 0.3631uJy e_FHs [0.08/29]?=-99 FHs uncertainty (e_Hs) 734- 737 F4.2 --- w_FHs [0/1.2] Weight corresponding to FHs, median normalized (w_Hs) 739- 763 F25.19 0.3631uJy FHl [-5/28665]?=-99 Aperture flux in FourStar Hl-band, corrected to total (f_Hl) (1) 765- 785 F21.17 0.3631uJy e_FHl [0.09/42]?=-99 FHl uncertainty (e_Hl) 787- 790 F4.2 --- w_FHl [0/1.2] Weight corresponding to FHl, median normalized (w_Hl) 792- 814 E23.20 0.3631uJy FKs [-16/26455]?=-99 Aperture flux in FourStar Ks-band, corrected to total (f_Ks) (1) 816- 836 F21.17 0.3631uJy e_FKs [0.1/38]?=-99 FKs uncertainty (e_Ks) 838- 841 F4.2 --- w_FKs [0/1.4] Weight corresponding to FKs, median normalized (w_Ks) 843- 869 F27.20 0.3631uJy FJ [-0.6/135112]?=-99 Aperture flux in UKIRT/WFCAM J-band, corrected to total (f_J) (1) 871- 892 F22.18 0.3631uJy e_FJ [0.05/2.7]?=-99 FJ uncertainty (e_J) 894- 896 F3.1 --- w_FJ [0/1] Weight corresponding to FJ, median normalized (w_J) 898- 923 F26.20 0.3631uJy FH [-1.6/84305]?=-99 Aperture flux in UKIRT/WFCAM H-band, corrected to total (f_H) (1) 925- 945 F21.17 0.3631uJy e_FH [0.05/5.4]?=-99 FH uncertainty (e_H) 947- 949 F3.1 --- w_FH [0/1] Weight corresponding to FH, median normalized (w_H) 951- 975 F25.19 0.3631uJy FK [-0.4/76653]?=-99 Aperture flux in UKIRT/WFCAM Ks-band, corrected to total (f_K) (1) 977- 997 F21.17 0.3631uJy e_FK [0.06/3.4]?=-99 FK uncertainty (e_K) 999-1002 F4.2 --- w_FK [0/1.3] Weight corresponding to FK, median normalized (w_K) 1004-1028 F25.19 0.3631uJy FKsHI [-4.4/11697]?=-99 Aperture flux in K-band (2.1524um), corrected to total (f_KsHI) (1) 1030-1050 F21.17 0.3631uJy e_FKsHI [0.08/4.3]?=-99 FKsHI uncertainty (e_KsHI) 1052-1055 F4.2 --- w_FKsHI [0/1.5] Weight corresponding to FKsHI, median normalized (w_KsHI) 1057-1071 F15.9 0.3631uJy F125W [-0.6/72981]?=-99 Aperture flux in HST/WFC3 F125W-band, corrected to total (f_F125W) (1) 1073-1083 F11.7 0.3631uJy e_F125W [0.01/1.8]?=-99 F125W uncertainty (e_F125W) 1085-1088 F4.2 --- w_F125W [0/9.8] Weight corresponding to F125W, median normalized (w_F125W) 1090-1104 F15.9 0.3631uJy F140W [-0.6/46628]?=-99 Aperture flux in HST/WFC3 F140W-band, corrected to total (f_F140W) (1) 1106-1118 F13.7 0.3631uJy e_F140W [0.05/3.2]?=-99 F140W uncertainty (e_F140W) 1120-1123 F4.2 --- w_F140W [0/3] Weight corresponding to F140W, median normalized (w_F140W) 1125-1136 E12.9 0.3631uJy F160W [-0.7/79691]?=-99 Aperture flux in HST/WFC3 F160W-band, corrected to total (f_F160W) (1) 1138-1150 F13.7 0.3631uJy e_F160W [0.02/1.7]?=-99 F160W uncertainty (e_F160W) 1152-1155 F4.2 --- w_F160W [0/4] Weight corresponding to F160W, median normalized (w_F160W) 1157-1179 E23.20 0.3631uJy F606W [-0.8/2933]?=-99 Aperture flux in HST/ACS F606W-band, corrected to total (f_F606W) (1) 1181-1204 F24.18 0.3631uJy e_F606W [0.02/1.5]?=-99 F606W uncertainty (e_F606W) 1206-1209 F4.2 --- w_F606W [0/2.5] Weight corresponding to F606W, median normalized (w_F606W) 1211-1235 F25.19 0.3631uJy F814W [-0.3/3425]?=-99 Aperture flux in HST/ACS F606W-band, corrected to total (f_F814W) (1) 1237-1260 F24.18 0.3631uJy e_F814W [0.02/1.6]?=-99 F814W uncertainty (e_F814W) 1262-1265 F4.2 --- w_F814W [0/2.6] Weight corresponding to F814W, median normalized (w_F814W) 1267-1289 E23.20 0.3631uJy FY [-1/6983]?=-99 Aperture flux in VLT/HAWK-I Y-band, corrected to total (f_Y) (1) 1291-1315 F25.19 0.3631uJy e_FY [0/1.2]?=-99 FY uncertainty (e_Y) 1317-1321 F5.2 --- w_FY [0/]?=99.99 Weight corresponding to FY, median normalized (w_Y) 1323-1344 E22.19 0.3631uJy F3.6 [-35/18245]?=-99 Aperture flux in Spitzer/IRAC 3.6um-band, corrected to total (f_IRAC_36) (1) 1346-1366 F21.17 0.3631uJy e_F3.6 [-5/6.5]?=-99 F3.6 uncertainty (e_IRAC_36) 1368-1374 F7.2 --- w_F3.6 [0.4/1.3]?=-99 Weight corresponding to 3.6um, median normalized (w_IRAC_36) 1376-1401 F26.20 0.3631uJy F4.5 [-27/18083]?=-99 Aperture flux in Spitzer/IRAC 4.5um-band, corrected to total (f_IRAC_45) (1) 1403-1424 F22.18 0.3631uJy e_F4.5 [-6/7.3]?=-99 F4.5 uncertainty (e_IRAC_45) 1426-1432 F7.2 --- w_F4.5 [0.4/1.3]?=-99 Weight corresponding to 4.5um, median normalized (w_IRAC_45) 1434-1456 E23.20 0.3631uJy F5.8 [-672/16511]?=-99 Aperture flux in Spitzer/IRAC 5.8um-band, corrected to total (f_IRAC_58) (1) 1458-1479 F22.16 0.3631uJy e_F5.8 [-672/86] F5.8 uncertainty (e_IRAC_58) 1481-1485 F5.1 --- w_F5.8 [1]?=-99 Weight corresponding to 5.8um, median normalized (w_IRAC_58) 1487-1512 F26.20 0.3631uJy F8.0 [-672/21089]?=-99 Aperture flux in Spitzer/IRAC 8.0um-band, corrected to total (f_IRAC_80) (1) 1514-1535 F22.16 0.3631uJy e_F8.0 [-791/109] F8.0 uncertainty (e_IRAC_80) 1537-1541 F5.1 --- w_F8.0 [1]?=-99 Weight corresponding to 8.0um, median normalized (w_IRAC_80) 1543-1545 F3.1 --- wminOpt [1] Minimum weight of groundbased optical filters (wmin_optical) 1547-1550 F4.2 --- wminHST1 [0/1] Minimum weight of HST optical filters (wmin_hst_optical) 1552-1555 F4.2 --- wminfs [0/2.5] Minimum weight of FourStar filters (wmin_fs) 1557-1560 F4.2 --- wminjhk [0/1.8] Minimum weight of broadband J, H, and K filters (wmin_jhk) 1562-1565 F4.2 --- wminHST2 [0/1] Minimum weight of HST near-IR filters (wmin_hst) 1567-1569 F3.1 --- wminIRAC [0/1] Minimum weight of Spitzer/IRAC filters (wmin_irac) 1571-1574 F4.2 --- wminAll [0.3/1.8] Minimum weight of all filters (wmin_all) 1576 I1 --- Star [0/1] 1=source is likely a star (G1) 1578 I1 --- Nghb [0/1] 1=near a bright star (nearstar) (G2) 1580 I1 --- Use [0/1] 1=selected (use) (G3) 1582-1594 F13.6 --- SNR [1.5/266262] Signal-to-noise (=FKsapD/e_FKsapD) (snr) 1596-1602 F7.3 --- zspec [0.06/6.2]?=-99 Spectroscopic redshift (z_spec) (G5) -------------------------------------------------------------------------------- Note (1): (convolved) aperture flux in filter [] within a 1.2" diameter circular aperture, corrected to total (Fap[]=F[]/KsR) CDFS passband parameters as in table 4: -------------------------------------------------------------- Filter lam_C_ FWHM Zeropoint Offset Galactic (um) (arcsec) (AB mag) extinction (G6) (AB mag) (AB mag) -------------------------------------------------------------- u 0.3828 1.06 24.905 -0.268 -0.089 B 0.4408 0.91 24.803 -0.123 -0.074 V 0.5470 0.93 24.870 -0.072 -0.058 R 0.6508 0.96 24.914 -0.038 -0.049 i 0.7656 0.98 24.986 0.021 -0.035 z 0.9060 0.99 24.974 0.001 -0.027 J_1_ 1.0540 0.55 26.121 -0.036 -0.022 J_2_ 1.1448 0.53 26.408 -0.029 -0.019 J_3_ 1.2802 0.51 26.481 -0.019 -0.015 H_s_ 1.5544 0.49 26.591 -0.000 -0.011 H_l_ 1.7020 0.51 26.448 -0.036 -0.010 Ks 2.1538 0.44 26.804 -0.067 -0.006 J 1.2502 0.91 30.863 -0.052 -0.015 H 1.6360 0.89 31.262 -0.108 -0.010 K 2.2060 0.86 31.825 -0.059 -0.006 F125W 1.2471 0.26 26.214 -0.000 -0.016 F140W 1.3924 0.26 26.439 -0.000 -0.013 F160W 1.5396 0.26 25.935 -0.000 -0.011 F606W 0.5893 0.20 26.383 -0.054 -0.054 F814W 0.8057 0.23 25.926 0.015 -0.033 Y 1.0207 0.58 27.004 0.026 -0.022 KsHI 2.1748 0.46 27.520 0.026 -0.006 IRAC_36 3.5569 1.70 21.539 -0.042 0.000 IRAC_45 4.5020 1.70 21.556 -0.025 0.000 IRAC_58 5.7450 1.90 21.458 -0.123 0.000 IRAC_80 7.9158 2.00 21.522 -0.059 0.000 -------------------------------------------------------------- In UDS the additional filters are CFHT/MegaCam/U (O. Almaini 2016, in preparation; S. Foucaud 2016, in preparation), Subaru/Surpime-Cam/B, V, R, i, z (Furusawa+ 2008ASPC..399..131F), UKIRT/WFCAM/J, H, Ks (O. Almaini 2016, in preparation), HST/WFC3/F125W, F140W, F160W and HST/ACSF606W, F814W (Grogin+ 2011ApJS..197...35G; Koekemoer+ 2011ApJS..197...36K; Brammer+ 2012ApJS..200...13B) and VLT/HAWK-I/Y (Fontana+ 2014, J/A+A/570/A11). KsHI comes from a combined VLT/HAWKI and Magellan/FOURSTAR image. -------------------------------------------------------------------------------- Global notes: Note (G1): This flag is set to 1 if the source is likely to be a star, to 0 otherwise. Note (G2): This flag is set to 1 if the source is located within r(")<10-(m-16) of a bright star with m the apparent magnitude of the star and m<17.5 in J1, J2, J3, J or Ks. Note (G3): Sources that pass the following criteria are set to 1: * star = 0 * nearstar = 0 * snr>=5 * wminfs>0.1 (A minimum exposure time of at least 0.1xthe median exposure in the FourStar bands) * wminOpt>0 (coverage in all optical bands) * not a catastrophic EAZY fit: {chi}^2^(reduced)<=1000 * not a catastrophic FAST fit, i.e., a finite and positive stellar mass estimate above 10^6^M_{sun}_ * consistent flux ratios between similar bands of different instruments, namely the J-, H-, and K-bands of FourStar and VISTA, and F814W- and groundbased I-bands * no 5{sigma} detection at wavelengths bluer than the restframe 912{AA} Lyman limit * not at z<0.1 Note (G4): Source Extractor internal flags. Flags contains, coded in decimal, all the extraction flags as a sum of powers of 2: 1 = The object has neighbours, bright and close enough to significantly bias the MAG AUTO photometry, or bad pixels 2 = The object was originally blended with another one. 4 = At least one pixel of the object is saturated (or very close to). 8 = The object is truncated (too close to an image boundary). 16 = Object's aperture data are incomplete or corrupted. Note (G5): Spectroscopic redshifts were sourced from the 3D-HST catalogs (Skelton+ 2014, J/ApJS/214/24), who in turn use the zCOSMOS catalogs (Lilly+ 2007, J/ApJS/172/70), MMT/Hectospec data (Fabricant+ 2005PASP..117.1411F; Mink+ 2007ASPC..376..249M), the FIREWORKS catalog (Wuyts+ 2008, J/ApJ/682/985), and a variety of UDS sources (Yamada+ 2005ApJ...634..861Y; Simpson+ 2006MNRAS.373L..21S; Geach+ 2007MNRAS.381.1369G; van Breukelen+ 2007MNRAS.382..971V; Ouchi+ 2008, J/ApJS/176/301; Smail+ 2008MNRAS.389..407S; Ono+ 2010MNRAS.402.1580O; Simpson+ 2012, J/MNRAS/421/3060; M. Akiyama et al., in preparation). Additionally, we crossmatch and identify additional sources from the MOSDEF survey (Kriek+ 2015ApJS..218...15K) and the VIMOS Ultra-Deep Survey (VUDS) Le Fevre+ (2015A&A...576A..79L). All sources were matched to ZFOURGE to within 1.0". Redshifts from the 3D-HST catalogues are limited to those with the highest quality flags in both the COSMOS and CDFS fields. For the UDS field, there is a mix of reliable and less reliable redshifts ranging from "flag not provided" to "multiple reliable features". More details can be found in Skelton+ (2014, J/ApJS/214/24). For MOSDEF, spectroscopic redshifts are limited to those considered "robust" in Kriek+ (2015ApJS..218...15K), i.e., a secure identification and measurement of emission lines in the 1D spectra. For VUDS, spectroscopic redshifts are limited to those rated a level 2 or higher, i.e., 75-100% probability of redshift to be correct. Note (G6): Zeropoints are effective zeropoints. These have galactic extinction and EAZY zeropoint corrections incorporated, such that Zeropoint = zeropoint_I + Eazy Offset + galactic extinction, with zeropoint_I representing the photometrically derived zeropoint of image I based on standard stars. -------------------------------------------------------------------------------- History: Downloaded from: http://zfourge.tamu.edu/DR2016/data.html Updated versions (June 2017) and complementary data sent by the author Acknowledgements: Caroline Straatman [Max Planck Institute for Astronomy in Heidelberg]; straatman [at] mpia-hd.mpg.de ================================================================================ (End) Caroline Straatman [MPIA], Emmanuelle Perret [CDS] 03-Mar-2017