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Related papers: Ultradeep Ks Imaging in the GOODS-N

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We present the first spatial clustering measurements of z~1, 24um-selected, star forming galaxies in the Great Observatories Origins Deep Survey (GOODS). The sample under investigation includes 495 objects in GOODS-South and 811 objects in…

Astrophysics · Physics 2009-11-13 R. Gilli , E. Daddi , R. Chary , M. Dickinson , D. Elbaz , M. Giavalisco , M. Kitzbichler , D. Stern , E. Vanzella

We analyze very deep HST, VLT and Spitzer photometry of galaxies at 2<z<3.5 in the Hubble Deep Field South. The sample is selected from the deepest public K-band imaging currently available. We show that the rest-frame U-V vs V-J…

We present a multi-wavelength study of a 3.6 $\mu$m-selected galaxy sample in the Extended Groth strip. The sample is complete for galaxies with stellar mass $>10^{9.5}$ \Msun and redshift $0.4<z<1.2$. In this redshift range, the IRAC 3.6…

(Abridge) We study statistical intrinsic shape of star-forming BzK galaxies (sBzK galaxies) at z~2 in both rest-frame UV and rest-frame optical wavelengths. The sBzK galaxies are selected down to K(AB)=24.0 mag in the GOODS-South and SXDS…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-11 Suraphong Yuma , Kouji Ohta , Kiyoto Yabe

We have analysed the rest-frame far infrared (FIR) properties of a sample of massive (Mstar > 10^11Msun) galaxies at 2<z<3 in the GOODS (Great Observatories Origins Deep Survey) North field using the Spectral and Photometric Imaging…

Infrared (IR), sub-millimetre (sub-mm) and millimetre (mm) databases contain a huge quantity of high quality data. However, a large part of these data are photometric, and are thought not to be useful to derive a quantitative information on…

The IRAC mapping of the NMBS-II fields program is an imaging survey at 3.6 and 4.5$\mu$m with the Spitzer Infrared Array Camera (IRAC). The observations cover three Canada-France-Hawaii Telescope Legacy Survey Deep (CFHTLS-D) fields,…

In this paper we present a deep and homogeneous i-band selected multi-waveband catalogue in the COSMOS field covering an area of about 0.7 square-degree. Our catalogue with a formal 50 percent completeness limit for point sources of i~26.7…

Astrophysics · Physics 2009-11-13 A. Gabasch , Y. Goranova , U. Hopp , S. Noll , M. Pannella

Using deep near-infrared Keck/MOSFIRE observations, we analyze the rest-optical spectra of eight star-forming galaxies in the COSMOS and GOODS-N fields. We reach integration times of $\sim$10 hours in the deepest bands, pushing the limits…

We present a library of high-resolution (R $\equiv$ $\lambda$/$\Delta$$\lambda$ $\sim$ 45,000) and high signal-to-noise ratio (S/N $\geq$ 200) near-infrared spectra for stars of a wide range of spectral types and luminosity classes. The…

We present the results of spectroscopic observations in the GOODS-N field completed using DEIMOS on the Keck II telescope as part of the DEEP3 Galaxy Redshift Survey. Observations of 370 unique targets down to a limiting magnitude of R =…

We present a pilot study of the stellar populations of 8 AGN hosts at z~1 and compare to (1) lower redshift samples and (2) a sample of nonactive galaxies of similar redshift. We utilize K' images in the GOODS South field obtained with the…

Astrophysics · Physics 2015-05-13 S. Mark Ammons , Jason Melbourne , Claire E. Max , David C. Koo , David J. V. Rosario

The largest K-band flux-limited sample of luminous quasars to date has been constructed from the UKIDSS Large Area Survey Early Data Release, covering an effective area of 12.8 deg^2. Exploiting the K-band excess of all quasars with respect…

Astrophysics · Physics 2009-11-13 Natasha Maddox , Paul C. Hewett , S. J. Warren , S. M. Croom

Context. This is the third paper of a series devoted to the WIde-field Nearby Galaxy-cluster Survey (WINGS).WINGS is a long term project aimed at gathering wide-field, multiband imaging and spectroscopy of galaxies in a complete sample of…

Cosmology and Nongalactic Astrophysics · Physics 2009-08-11 T. Valentinuzzi , D. Woods , G. Fasano , M. Riello , M. D'Onofrio , J. Varela , D. Bettoni , A. Cava , W. J. Couch , A. Dressler , J. Fritz , M. Moles , A. Omizzolo , B. M. Poggianti , P. Kjaergaard

We describe the Dark Energy Survey (DES) Deep Fields, a set of images and associated multi-wavelength catalogue ($ugrizJHKs$) built from Dark Energy Camera (DECam) and Visible and Infrared Survey Telescope for Astronomy (VISTA) data. The…

Cosmology and Nongalactic Astrophysics · Physics 2022-02-17 W. G. Hartley , A. Choi , A. Amon , R. A. Gruendl , E. Sheldon , I. Harrison , G. M. Bernstein , I. Sevilla-Noarbe , B. Yanny , K. Eckert , H. T. Diehl , A. Alarcon , M. Banerji , K. Bechtol , R. Buchs , S. Cantu , C. Conselice , J. Cordero , C. Davis , T. M. Davis , S. Dodelson , A. Drlica-Wagner , S. Everett , A. Ferté , D. Gruen , K. Honscheid , M. Jarvis , M. D. Johnson , N. Kokron , N. MacCrann , J. Myles , A. B. Pace , A. Palmese , F. Paz-Chinchón , M. E. S. Pereira , A. A. Plazas , J. Prat , M. Rodriguez-Monroy , E. S. Rykoff , S. Samuroff , C. Sánchez , L. F. Secco , F. Tarsitano , A. Tong , M. A. Troxel , Z. Vasquez , K. Wang , C. Zhou , T. M. C. Abbott , M. Aguena , S. Allam , J. Annis , D. Bacon , E. Bertin , S. Bhargava , D. Brooks , D. L. Burke , A. Carnero Rosell , M. Carrasco Kind , J. Carretero , F. J. Castander , M. Costanzi , M. Crocce , L. N. da Costa , J. De Vicente , J. DeRose , S. Desai , J. P. Dietrich , T. F. Eifler , J. Elvin-Poole , I. Ferrero , B. Flaugher , P. Fosalba , J. García-Bellido , E. Gaztanaga , D. W. Gerdes , J. Gschwend , G. Gutierrez , S. R. Hinton , D. L. Hollowood , D. Huterer , D. J. James , S. Kent , E. Krause , K. Kuehn , N. Kuropatkin , O. Lahav , H. Lin , M. A. G. Maia , M. March , J. L. Marshall , P. Martini , P. Melchior , F. Menanteau , R. Miquel , J. J. Mohr , R. Morgan , E. Neilsen , R. L. C. Ogando , S. Pandey , A. K. Romer , A. Roodman , M. Sako , E. Sanchez , V. Scarpine , S. Serrano , M. Smith , M. Soares-Santos , E. Suchyta , M. E. C. Swanson , G. Tarle , D. Thomas , C. To , T. N. Varga , A. R. Walker , W. Wester , R. D. Wilkinson , J. Zuntz

Spitzer IRAC selection is a powerful tool for identifying luminous AGN. For deep IRAC data, however, the AGN selection wedges currently in use are heavily contaminated by star-forming galaxies, especially at high redshift. Using the large…

We present ultra-deep J and Ks imaging observations covering a 30' * 30' area of the Extended Chandra Deep Field-South (ECDFS) carried out by our Taiwan ECDFS Near-Infrared Survey (TENIS). The median 5-sigma limiting magnitudes for all…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-11 Bau-Ching Hsieh , Wei-Hao Wang , Chih-Chiang Hsieh , Lihwai Lin , Haojing Yan , Jeremy Lim , Paul T. P. Ho

We use the GOODS-MUSIC sample, a catalog of ~3000 Ks-selected galaxies based on VLT and HST observation of the GOODS-South field with extended multi-wavelength coverage (from 0.3 to 8 micron) and accurate estimates of the photometric…