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Related papers: Active and passive galaxies at z~2: Rest-frame opt…

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[abridged] New near-infrared surveys, using the HST, offer an unprecedented opportunity to study rest-frame optical galaxy morphologies at z>1 and to calibrate automated morphological parameters that will play a key role in classifying…

We present the results of a comparative study of the rest-frame optical and rest-frame ultraviolet morphological properties of 117 star-forming galaxies (SFGs), including BX, BzK, and Lyman break galaxies with B<24.5, and 15 passive…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-20 N. A. Bond , E. Gawiser , A. M. Koekemoer

We present deep and high-resolution HST/NIC2 F160W imaging at 1.6micron of six z~2 star-forming galaxies with existing near-IR integral field spectroscopy from SINFONI at the VLT. The unique combination of rest-frame optical imaging and…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-20 N. M. Förster Schreiber , A. E. Shapley , D. K. Erb , R. Genzel , C. C. Steidel , N. Bouché , G. Cresci , R. Davies

We study the structural evolution of massive galaxies by linking progenitors and descendants at a constant cumulative number density of n_c=1.4x10^{-4} Mpc^{-3} to z~3. Structural parameters were measured by fitting Sersic profiles to high…

We follow up emission line galaxies identified through the near-infrared slitless HST/WFC3 WISP survey with VLT/FORS2 optical spectroscopy. Over 4 WISP fields, we targetted 85 of 138 line emission objects at $0.4<z<2$ identified in WFC3…

From a search of a portion of the sky covered by the SDSS and UKIDSS databases, we have located 2 galaxies at z~0.5 that have properties similar to those of the luminous passive compact galaxies found at z~2.5. From Keck moderate-resolution…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-14 Alan Stockton , Hsin-Yi Shih , Kirsten Larson

We present the analysis of HST $J$- and $H$-band imaging for 29 galaxies on the star-forming main sequence at $z\sim2$, which have Adaptive Optics VLT SINFONI integral field spectroscopy from our SINS/zC-SINF program. The SINFONI H$\alpha$…

We report on a complete sample of 7 luminous early-type galaxies in the Hubble Ultra Deep Field (UDF) with spectroscopic redshifts between 1.39 and 2.47 and to K<23 AB. Using the BzK selection criterion we have pre-selected a set of objects…

In a systematic search over 11 cluster fields from Cluster Lensing And Supernova survey with Hubble (CLASH) we identify ten passively evolving massive galaxies at redshift z~2.We derive the stellar properties of these galaxies using HST…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-12 Lulu Fan , Yang Chen , Xinzhong Er , Jinrong Li , Lin Lin , Xu Kong

Using a simple two-color selection based on $g$-, $z$-, and $K$-band photometry, we pick out 1609 star-forming galaxies (sgzKs) and 422 passively evolving galaxies (pgzKs) at z\sim2$ from a $K$-band-selected sample ($K_{\rm AB} < 22.0$) in…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-04 Guanwen Fang , Xu Kong , Yang Chen , Xuanbin Lin

We present Hubble Space Telescope Wide Field Camera 3 slitless grism spectroscopy of 28 emission-line galaxies at z~2, in the GOODS-S region of the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CANDELS). The high…

We present the analysis of the deepest near-UV image obtained with HST using the WFPC2(F300W) as part of the parallel observations of the Ultra Deep Field campaign. The U-band 10sigma limiting magnitude measured over 0.2 arcsec square is…

Astrophysics · Physics 2016-08-30 Duilia. F. de Mello , Y. Wadadekar , T. Dahlen , S. Casertano , J. P. Gardner

(Abridged) The formation of massive spheroidal galaxies is studied on a visually classified sample of 910 galaxies extracted from the ACS/HST images of the GOODS North and South fields (0.4<z<.5). Three key observables are considered:…

Astrophysics of Galaxies · Physics 2014-11-18 Ignacio Ferreras , Thorsten Lisker , Anna Pasquali , Sugata Kaviraj

We use the ultra-deep HUDF09 and the deep ERS data from the HST WFC3/IR camera, along with the wide area Spitzer/IRAC data from GOODS-S to derive SEDs of star-forming galaxies from the rest-frame UV to the optical over a wide luminosity…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-03 Valentino Gonzalez , Rychard Bouwens , Ivo Labbe , Garth Illingworth , Pascal Oesch , Marijn Franx , Dan Magee

We present evidence for very high gas fractions and extended molecular gas reservoirs in normal, near-infrared selected (BzK) galaxies at z~1.5, based on multi-configuration CO[2-1] observations obtained at the IRAM PdBI. Six of the six…

Cosmology and Nongalactic Astrophysics · Physics 2014-11-20 E. Daddi , F. Bournaud , F. Walter , H. Dannerbauer , C. Carilli , M. Dickinson , D. Elbaz , G. E. Morrison , D. Riechers , M. Onodera , F. Salmi , M. Krips , D. Stern

Using the extensive multi-wavelength data in the GOODS-North field, we construct and draw comparisons between samples of optical and near-IR selected star-forming and passively evolving galaxies at redshifts 1.4<z<2.6. We find overlap at…

Galaxy formation models invoke the presence of strong feedback mechanisms that regulate the growth of massive galaxies at high redshifts. In this paper we aim to: (1) confirm spectroscopically the redshifts of a sample of massive galaxies…

Cosmology and Nongalactic Astrophysics · Physics 2014-04-23 W. Karman , K. I. Caputi , S. C. Trager , O. Almaini , M. Cirasuolo

Spectroscopic redshifts have been measured for 9 K-band luminous galaxies at 1.7 < z < 2.3, selected with Ks < 20 in the "K20 survey" region of the Great Observatories Origins Deep Survey area. Star formation rates (SFRs) of ~100-500…

We investigate rest-frame near-infrared (NIR) morphologies of a sample of 139 galaxies with M_{s} >= 1 x 10^{10} M_{sun} at z=0.8-1.2 in the GOODS-North field using our deep NIR imaging data (MOIRCS Deep Survey, MODS). We focus on Luminous…

A substantial population of high redshift early-type galaxies is detected in very deep UBVRIJHK images towards the HDF-South. Four elliptical profile galaxies are identified in the redshift range z=1-2, all with very red SEDs, implying ages…

Astrophysics · Physics 2009-10-31 Narciso Benitez , Tom Broadhurst , Rychard Bouwens , Joseph Silk , Piero Rosati