J/ApJ/821/123 z∼4-7 Lyman break galaxies in Hubble deep fields (Harikane+, 2016)

Evolution of stellar-to-halo mass ratio at z=0-7 identified by clustering analysis with the Hubble legacy imaging and early Subaru/Hyper Suprime-Cam survey data. Harikane Y., Ouchi M., Ono Y., More S., Saito S., Lin Y.-T., Coupon J., Shimasaku K., Shibuya T., Price P.A., Lin L., Hsieh B.-C., Ishigaki M., Komiyama Y., Silverman J., Takata T., Tamazawa H., Toshikawa J. <Astrophys. J., 821, 123-123 (2016)> =2016ApJ...821..123H 2016ApJ...821..123H (SIMBAD/NED BibCode)
ADC_Keywords: Photometry, HST ; Galaxies, IR ; Surveys Keywords: galaxies: evolution; galaxies: formation; galaxies: high-redshift Abstract: We present clustering analysis results from 10381 Lyman break galaxies (LBGs) at z∼4-7, identified in the Hubble legacy deep imaging and new complimentary large-area Subaru/Hyper Suprime-Cam data. We measure the angular correlation functions of these LBGs at z∼4, 5, 6, and 7 and fit these measurements using halo occupation distribution (HOD) models that provide an estimate of halo masses, Mh~(1-20)x1011M. Our Mh estimates agree with those obtained by previous clustering studies in a UV-magnitude versus Mh plane and allow us to calculate stellar-to-halo mass ratios (SHMRs) of LBGs. By comparison with the z∼0 SHMR, we identify evolution of the SHMR from z∼0 to z∼4 and from z∼4 to z∼7 at the >98% confidence levels. The SHMR decreases by a factor of ∼2 from z∼0 to 4 and increases by a factor of ∼4 from z∼4 to 7 at the dark matter halo mass of Mh∼1011M_☉. We compare our SHMRs with results of a hydrodynamic simulation and a semianalytic model and find that these theoretical studies do not predict the SHMR increase from z∼4 to 7. We obtain the baryon conversion efficiency (BCE) of LBGs at z∼4 and find that the BCE increases with increasing dark matter halo mass. Finally, we compare our clustering+HOD estimates with results from abundance matching techniques and conclude that the Mh estimates of the clustering+HOD analyses agree with those of the simple abundance matching within a factor of 3, and that the agreement improves when using more sophisticated abundance matching techniques that include subhalos, incompleteness, and/or evolution in the star formation and stellar mass functions. Description: We use 10 deep optical-near-IR imaging data sets of the Hubble Ultra Deep Field (HUDF), Great Observatories Origins Deep Survey (GOODS)-North-Deep, GOODS-North-Wide, GOODS-South-Deep, GOODS-South-Wide, Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CANDELS)-All-Wavelength Extended Groth Strip International Survey (AEGIS), CANDELS-Cosmological Evolution Survey (COSMOS), CANDELS-Ultra Deep Survey (UDS), Hubble Frontier Field (HFF)-Abell2744P, and HFF-MACS0416P that are taken with ACS and WFC3 on the HST. The total area of the Hubble data is ∼600arcmin2. The typical FWHMs of the PSFs of ACS and WFC3 images are 0.1" and 0.2", respectively. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table3.dat 161 9651 Catalog of Lyman break galaxies (LBGs) in the Hubble data -------------------------------------------------------------------------------- See also: II/318 : GOODS Source Catalogs release r2.0z (Giavalisco+ 2008) J/A+A/590/A31 : ASTRODEEP Frontier Fields Catalogues (Merlin+, 2016) J/ApJ/814/95 : Star formation rate of 4≲z≲8 galaxies (Finkelstein+, 2015) J/ApJS/219/15 : Morphologies of z=0-10 galaxies with HST data (Shibuya+, 2015) J/ApJS/218/33 : Spitzer-CANDELS catalog within 5 deep fields (Ashby+, 2015) J/ApJ/803/34 : z∼4-10 galaxies from HST legacy fields (Bouwens+, 2015) J/ApJS/214/24 : 3D-HST+CANDELS catalog (Skelton+, 2014) J/ApJS/207/24 : GOODS-S CANDELS multiwavelength catalog (Guo+, 2013) J/ApJS/206/10 : CANDELS multiwavelength catalog (Galametz+, 2013) J/MNRAS/430/425 : VLT LBG Redshift Survey. III. (Bielby+, 2013) J/ApJS/203/24 : Structural param. of galaxies in CANDELS (van der Wel+, 2012) J/ApJ/750/99 : The Pan-STARRS1 photometric system (Tonry+, 2012) J/ApJ/742/3 : Photometric catalogs for ECDF-S and CDF-N (Rafferty+, 2011) J/ApJS/187/251 : Ultradeep Ks imaging in the GOODS-N (Wang+, 2010) J/ApJ/703/2033 : Lyman-break galaxies (LBG) in the HUDF (Rafelski+, 2009) J/ApJ/697/1369 : GOODS Ks-selected multiwavelength compilations (Bundy+, 2009) J/AJ/132/1729 : Hubble Ultra Deep Field BVI-dropout sources (Beckwith+, 2006) J/AJ/132/926 : Galaxies in the Hubble Ultra Deep Field (Coe+, 2006) J/ApJ/519/1 : Lyman-break galaxies at z≳4 (Steidel+, 1999) http://candels.ucolick.org/ : CANDELS home page http://archive.stsci.edu/prepds/xdf/ : Hubble eXtreme Deep Field (XDF) page http://3dhst.research.yale.edu/ : 3D-HST home page http://www.stsci.edu/hst/campaigns/frontier-fields/ : HST Frontier Fields page http://www.sdss.org/dr12/ : SDSS-DR12 home page Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 14 A14 --- ID Catalog identifier (1) 16- 28 F13.9 deg RAdeg Right Ascension in decimal degrees (J2000) 30- 42 F13.9 deg DEdeg Declination in decimal degrees (J2000) 44 A1 --- l_Bmag The 1σ limit flag on Bmag 45- 49 F5.2 mag Bmag [25.9/31.8]? The HST/ACS B band (435nm) AB magnitude (2) 51- 54 F4.2 mag e_Bmag [0.01/6]? Uncertainty in Bmag 56 A1 --- l_Vmag The 1σ limit flag on Vmag 57- 61 F5.2 mag Vmag [24.4/32.3]The HST/ACS V band (606nm) AB magnitude (2) 63- 66 F4.2 mag e_Vmag [0/5]? Uncertainty in Vmag 68 A1 --- l_imag The 1σ limit flag on imag 69- 73 F5.2 mag imag [23.2/31.9]? The HST/ACS i band (775nm) AB magnitude (2) 75- 78 F4.2 mag e_imag [0/7]? Uncertianty in imag 80 A1 --- l_Imag The 1σ limit flag on Imag 81- 85 F5.2 mag Imag [21.5/32.3] The HST/ACS I band (814nm) AB magnitude (2) 87- 90 F4.2 mag e_Imag [0/3.4]? Uncertainty in Imag 92 A1 --- l_zmag The 1σ limit flag on zmag 93- 97 F5.2 mag zmag [22.9/31.4]? The HST/ACS z band (850nm) AB magnitude (2) 99-102 F4.2 mag e_zmag [0/3]? Uncertainty in zmag 104 A1 --- l_Ymag The 1σ limit flag on Ymag 105-109 F5.2 mag Ymag [19.3/31.2]? HST/WFC3 Y band (1050nm) AB magnitude (2) 111-114 F4.2 mag e_Ymag [0/3]? Uncertainty in Ymag 116 A1 --- l_Jmag The 1σ limit flag on Jmag 117-121 F5.2 mag Jmag [21.7/31.7] The HST/WFC3 J band (1250nm) AB magnitude (2) 123-126 F4.2 mag e_Jmag [0/4]? Uncertainty in Jmag 128 A1 --- l_H14mag The 1σ limit flag on H14mag 129-133 F5.2 mag H14mag [25.4/31.6]? The HST/WFC3 H band (1400nm) AB magnitude (2) 135-138 F4.2 mag e_H14mag [0/3]? Uncertainty in H14mag 140 A1 --- l_H16mag The 1σ limit flag on H16mag 141-145 F5.2 mag H16mag [21.8/31.7] The HST/WFC3 H band (1600nm) AB magnitude (2) 147-150 F4.2 mag e_H16mag [0/3]? Uncertainty in H16mag 152-156 F5.2 mag Coadd [21.8/30.6]? IR coadd image AB magnitude (3) 158-161 F4.2 mag e_Coadd [0/0.3]? Uncertainty in Coadd -------------------------------------------------------------------------------- Note (1): zNaaaaaaNNNNN format with zN the approximative redshift (between 4 and 7) and aaaaaa the field as described in table 4: ----------------------------------------------------------- Field Area 5σ Number arcmin2 Depth of LBGs ----------------------------------------------------------- aeg = CANDELS-AEGIS 174.9 28.0 510 uds = CANDELS-UDS 129.3 27.9 400 cos = CANDELS-COSMOS 122.0 27.9 455 gdnw = GOODS-N-Wide 58.2 28.1 1123 gdnd = GOODS-N-Deep 57.4 28.6 2534 gdsd = GOODS-S-Deep 52.7 29.0 3082 gdsw = GOODS-S-Wide 30.4 28.3 734 xdf = HUDF 3.7 30.6 614 m0416p = HFF-MACS0416P 3.8 29.5 129 a2744p = HFF-Abell2744P 3.1 29.3 70 ----------------------------------------------------------- Note (2): All magnitudes listed are measured in 0.35-diameter circular apertures. Note (3): Coadd image of Ymag, Jmag, H14mag, and H16mag bands. -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Prepared by [AAS], Emmanuelle Perret [CDS] 28-Jul-2016
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line