The Multiwavelength Survey By Yale-Chile (MUSYC) Wide K-Band Imaging, Photometric Catalogs, Clustering, And Physical Properties Of Galaxies At Z Similar To 2
dc.contributor.utaustinauthor | Blanc, Guillermo A. | en_US |
dc.creator | Blanc, Guillermo A. | en_US |
dc.creator | Lira, Paulina | en_US |
dc.creator | Barrientos, L. Felipe | en_US |
dc.creator | Aguirre, Paula | en_US |
dc.creator | Francke, Harod | en_US |
dc.creator | Taylor, Edward N. | en_US |
dc.creator | Quadri, Ryan | en_US |
dc.creator | Marchesini, Danilo | en_US |
dc.creator | Infante, Leopoldo | en_US |
dc.creator | Gawiser, Eric | en_US |
dc.creator | Hall, Patrick B. | en_US |
dc.creator | Willis, Jon P. | en_US |
dc.creator | Herrera, David | en_US |
dc.creator | Maza, Jose | en_US |
dc.date.accessioned | 2016-04-28T19:34:59Z | |
dc.date.available | 2016-04-28T19:34:59Z | |
dc.date.issued | 2008-07 | en |
dc.description.abstract | We present K-band imaging of two similar to 30' x 30' fields covered by the Multiwavelength Survey by Yale-Chile (MUSYC) Wide NIR Survey. The SDSS 1030+05 and Cast 1255 fields were imaged with the Infrared Side Port Imager (ISPI) on the 4 m Blanco telescope at the Cerro Tololo Inter-American Observatory (CTIO) to a 5 sigma point-source limiting depth of K similar to 20 (Vega). Combining these data with the MUSYC optical UBVRIz imaging, we created multiband K-selected source catalogs for both fields. These catalogs, together with the MUSYC K-band catalog of the Extended Chandra Deep Field South (ECDF-S) field, were used to select K 20 BzK galaxies over an area of 0.71 deg(2). This is the largest area ever surveyed for BzK galaxies. We present number counts, redshift distributions, and stellar masses for our sample of 3261 BzK galaxies (2502 star-forming [sBzK] and 759 passively evolving [pBzK]), as well as reddening and star formation rate estimates for the star-forming BzK systems. We also present two-point angular correlation functions and spatial correlation lengths for both sBzK and pBzK galaxies and show that previous estimates of the correlation function of these galaxies were affected by cosmic variance due to the small areas surveyed. We have measured correlation lengths r(0) of 8.89 +/- 2.03 and 10.82 +/- 1.72 Mpc for sBzK and pBzK galaxies, respectively. This is the first reported measurement of the spatial correlation function of passive BzK galaxies. In the Lambda CDM scenario of galaxy formation, these correlation lengths at z similar to 2 translate into minimum masses of similar to 4 x 10(12) and similar to 9 x 10(12) M(circle dot) for the dark matter halos hosting sBzK and pBzK galaxies, respectively. The clustering properties of the galaxies in our sample are consistent with their being the descendants of bright Lyman break galaxies at z similar to 3, and the progenitors of present-day > 1L* galaxies. | en_US |
dc.description.department | Astronomy | en_US |
dc.description.sponsorship | en_US | |
dc.identifier | doi:10.15781/T2VZ3M | |
dc.identifier.Filename | 2008_07_multiwavelength.pdf | en_US |
dc.identifier.citation | Blanc, Guillermo A., Paulina Lira, L. Felipe Barrientos, Paula Aguirre, Harold Francke, Edward N. Taylor, Ryan Quadri et al. "The Multiwavelength Survey by Yale-Chile (MUSYC): Wide K-Band Imaging, Photometric Catalogs, Clustering, and Physical Properties of Galaxies at z~ 2." The Astrophysical Journal, Vol. 681, No. 2 (Jul., 2008): 1099. | en_US |
dc.identifier.doi | 10.1086/588018 | en_US |
dc.identifier.issn | 0004-637X | en_US |
dc.identifier.uri | http://hdl.handle.net/2152/34812 | |
dc.language.iso | English | en_US |
dc.relation.ispartof | en_US | |
dc.relation.ispartofserial | Astrophysical Journal | en_US |
dc.rights | Administrative deposit of works to Texas ScholarWorks: This works author(s) is or was a University faculty member, student or staff member; this article is already available through open access or the publisher allows a PDF version of the article to be freely posted online. The library makes the deposit as a matter of fair use (for scholarly, educational, and research purposes), and to preserve the work and further secure public access to the works of the University. | en_US |
dc.rights.restriction | Open | en_US |
dc.subject | catalogs | en_US |
dc.subject | galaxies : evolution | en_US |
dc.subject | galaxies : high-redshift | en_US |
dc.subject | galaxies : | en_US |
dc.subject | statistics | en_US |
dc.subject | large-scale structure of universe | en_US |
dc.subject | surveys | en_US |
dc.subject | star-forming galaxies | en_US |
dc.subject | deep-field-south | en_US |
dc.subject | ly-alpha emitters | en_US |
dc.subject | high-redshift galaxies | en_US |
dc.subject | lyman break galaxies | en_US |
dc.subject | dark-matter haloes | en_US |
dc.subject | luminosity functions | en_US |
dc.subject | spectroscopic confirmation | en_US |
dc.subject | stellar populations | en_US |
dc.subject | emitting galaxies | en_US |
dc.subject | astronomy & astrophysics | en_US |
dc.title | The Multiwavelength Survey By Yale-Chile (MUSYC) Wide K-Band Imaging, Photometric Catalogs, Clustering, And Physical Properties Of Galaxies At Z Similar To 2 | en_US |
dc.type | Article | en_US |