A WFC3 Grism Emission Line Redshift Catalog In The GOODS-South Field
dc.contributor.utaustinauthor | Finkelstein, Steven L. | en_US |
dc.creator | Morris, Aaron M. | en_US |
dc.creator | Kocevski, Dale D. | en_US |
dc.creator | Trump, Jonathan R. | en_US |
dc.creator | Weiner, Benjamin J. | en_US |
dc.creator | Hathi, Nimish P. | en_US |
dc.creator | Barro, Guillermo | en_US |
dc.creator | Dahlen, Tomas | en_US |
dc.creator | Faber, Sandra M. | en_US |
dc.creator | Finkelstein, Steven L. | en_US |
dc.creator | Fontana, Adriano | en_US |
dc.creator | Ferguson, Henry C. | en_US |
dc.creator | Grogin, Norman A. | en_US |
dc.creator | Grutzbauch, Ruth | en_US |
dc.creator | Guo, Yicheng C. | en_US |
dc.creator | Hsu, Li-Ting | en_US |
dc.creator | Koekemoer, Anton M. | en_US |
dc.creator | Koo, David C. | en_US |
dc.creator | Mobasher, Bahram | en_US |
dc.creator | Pforr, Janine | en_US |
dc.creator | Salvato, Mara | en_US |
dc.creator | Wiklind, Tommy | en_US |
dc.creator | Wuyts, Stijn | en_US |
dc.date.accessioned | 2016-04-22T19:47:37Z | |
dc.date.available | 2016-04-22T19:47:37Z | |
dc.date.issued | 2015-06 | en |
dc.description.abstract | We combine Hubble Space Telescope (HST)/Wide Field Camera3 (WFC3) imaging and G141 grism observations from the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CANDELS) and 3D-HST surveys to produce a catalog of grism spectroscopic redshifts for galaxies in the CANDELS/GOODS-South field. The WFC3/G141 grism spectra cover a wavelength range of 1.1 <= lambda <= 1.7 mu m with a resolving power of R similar to 130 for point sources, thus providing rest-frame optical spectra for galaxies out to z similar to 3.5. The catalog is selected in the H-band (F160W) and includes both galaxies with and without previously published spectroscopic redshifts. Grism spectra are extracted for all H-band detected galaxies with H <= 24 and a CANDELS photometric redshift z(phot) >= 0.6. The resulting spectra are visually inspected to identify emission lines, and redshifts are determined using cross-correlation with empirical spectral templates. To establish the accuracy of our redshifts, we compare our results against high-quality spectroscopic redshifts from the literature. Using a sample of 411 control galaxies, this analysis yields a precision of sigma(NMAD) = 0.0028 for the grism-derived redshifts, which is consistent with the accuracy reported by the 3D-HST team. Our final catalog covers an area of 153 arcmin(2) and contains 1019 redshifts for galaxies in GOODS-S. Roughly 60% (608/1019) of these redshifts are for galaxies with no previously published spectroscopic redshift. These new redshifts span a range of 0.677 <= z <= 3.456 and have a median redshift of z = 1.282. The catalog contains a total of 234 new redshifts for galaxies at z > 1.5. In addition, we present 20 galaxy pair candidates identified for the first time using the grism redshifts in our catalog, including four new galaxy pairs at z similar to 2, nearly doubling the number of such pairs previously identified. | en_US |
dc.description.department | Astronomy | en_US |
dc.description.sponsorship | NASA NAS5-26555 | en_US |
dc.description.sponsorship | NSF 0808133 | en_US |
dc.description.sponsorship | HST-AR 12822.03A | en_US |
dc.identifier | doi:10.15781/T2XF7K | |
dc.identifier.citation | Morris, Aaron M., Dale D. Kocevski, Jonathan R. Trump, Benjamin J. Weiner, Nimish P. Hathi, Guillermo Barro, Tomas Dahlen et al. >A WFC3 Grism Emission Line Redshift Catalog in the GOODS-South Field.> The Astronomical Journal, Vol. 149, No. 6 (Jun., 2015): 178. | en_US |
dc.identifier.doi | 10.1088/0004-6256/149/6/178 | en_US |
dc.identifier.issn | 0004-6256 | en_US |
dc.identifier.uri | http://hdl.handle.net/2152/34502 | |
dc.language.iso | English | en_US |
dc.relation.ispartofserial | Astronomical 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.subject | catalogs | en_US |
dc.subject | galaxies: high-redshift | en_US |
dc.subject | techniques: spectroscopic | en_US |
dc.subject | hubble-space-telescope | en_US |
dc.subject | origins deep survey | en_US |
dc.subject | extragalactic legacy | en_US |
dc.subject | survey | en_US |
dc.subject | star-forming galaxies | en_US |
dc.subject | greater-than 1 | en_US |
dc.subject | photometric redshift | en_US |
dc.subject | optical spectroscopy | en_US |
dc.subject | quiescent galaxies | en_US |
dc.subject | nuclear activity | en_US |
dc.subject | data | en_US |
dc.subject | reduction | en_US |
dc.subject | astronomy & astrophysics | en_US |
dc.title | A WFC3 Grism Emission Line Redshift Catalog In The GOODS-South Field | en_US |
dc.type | Article | en_US |
Access full-text files
Original bundle
1 - 1 of 1