THE VLA-COSMOS SURVEY. IV. DEEP DATA AND JOINT CATALOG

By E. Schinnerer, M. Sargent, M. Bondi, V. Smolčić, A. Datta, C. Carilli, F. Bertoldi, A. Blain, P. Ciliegi, A. Koekemoer and 1 more. 2010

181 citations recorded by the source corpus.

In the context of the VLA-COSMOS Deep project, additional VLA A array observations at 1.4 GHz were obtained for the central degree of the COSMOS field and combined with the existing data from the VLA-COSMOS Large project. A newly constructed Deep mosaic with a resolution of 2.″5 was used to search for sources down to 4σ with 1σ ≈ 12 μJy beam−1 in the central 50′ × 50′. This new catalog is combined with the catalog from the Large project (obtained at 1.″5 × 1.″4 resolution) to construct a new Joint catalog. All sources listed in the new Joint catalog have peak flux densities of ⩾5σ at 1.″5 and/or 2.″5 resolution to account for the fact that a significant fraction of sources at these low flux levels are expected to be slightly resolved at 1.″5 resolution. All properties listed in the Joint catalog, such as peak flux density, integrated flux density, and source size, are determined in the 2.″5 resolution Deep image. In addition, the Joint catalog contains 43 newly identified multi-component sources.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/a939a22dee797ea5271eb0f850543b9bbed7620a

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In Astronomy and Astrophysics

1. D. M. Alexander
2. P. Hopkins
3. L. Hernquist
4. P. V. van Dokkum
5. M. Franx
6. R. Somerville
7. E. Daddi
8. R. Dav'e

In Nuclear and High Energy Physics

1. D. M. Alexander
2. R. Ivison
3. I. Smail
4. W. N. Brandt
5. S. Chapman
6. C. Carilli
7. A. Merloni
8. F. Walter

Citations in the corpus

• An ALMA survey of submillimetre galaxies in the Extended Chandra Deep Field South: high-resolution 870 μm source counts (2012, methodology): “The recipes we follow to determine the full uncertainty for elliptical source fits in the presence of correlated noise in radio maps have been motivated by Condon (1997) (see also Windhorst et al. 1984; Hopkins et al. 2003, Schinnerer et al. 2004, 2010; Karim et al. 2011).”
• The bright end of the galaxy luminosity function at z≃7: before the onset of mass quenching? (2013, methodology): “In the radio, the COSMOS field is covered by the Very Large Array (VLA)-COSMOS survey (Schinnerer et al. 2010), with a sensitivity of 12µJy per beam.”
• X-shooter reveals powerful outflows in z ∼ 1.5 X-ray selected obscured quasi-stellar objects (2014, methodology): “…from H12, for which a radio detection was imposed to conduct the Integral Field Unit (IFU) follow-up, only 40% of our objects (all those detected also in PACS) are detected in the radio band at 1.4 GHz in the Very Large Array (VLA) observations of the COSMOS field (Schinnerer et al. 2010).”
• A PUBLIC Ks-SELECTED CATALOG IN THE COSMOS/UltraVISTA FIELD: PHOTOMETRY, PHOTOMETRIC REDSHIFTS, AND STELLAR POPULATION PARAMETERS, (2013, methodology): “It contains X-ray data from XMM − Newton (Hasinger et al. 2007), and Chandra (Elvis et al. 2009), UV imaging from the GALEX satellite (Martin et al. 2005), extensive optical broad-band and optical mediumband imaging from the CFHT and Subaru telescopes (Taniguchi et al. 2007; Capak et al. 2007), mid-”
• AN ALMA SURVEY OF SUBMILLIMETER GALAXIES IN THE EXTENDED CHANDRA DEEP FIELD SOUTH: SOURCE CATALOG AND MULTIPLICITY (2013, background): “(See also Windhorst et al. 1984; Hopkins et al. 2003; Schinnerer et al. 2004, 2010; Karim et al. 2011).”
• THE CHANDRA COSMOS LEGACY SURVEY: OVERVIEW AND POINT SOURCE CATALOG (2016, background): “, 260h of Herschel (Lutz et al. 2011), 750 hrs of JVLA (Schinnerer et al. 2004, 2007, 2010 and Smolcic et al. 2014 and in prep.)”
• Evolution of Interstellar Medium, Star Formation, and Accretion at High Redshift (2017, background): “In short, we begin with a prior catalog that contains all COSMOS sources detected in the Spitzer 24µm and VLA 1.4 GHz catalogs (Le Floc’h et al. 2009; Schinnerer et al. 2010), which have excellent astrometry.”
• EVIDENCE FOR WIDE-SPREAD ACTIVE GALACTIC NUCLEUS-DRIVEN OUTFLOWS IN THE MOST MASSIVE z ∼ 1–2 STAR-FORMING GALAXIES (2014, methodology): “Some of the fields from which the samples are drawn have VLA 20 cm radio catalogs from VLA-COSMOS (Schinnerer et al. 2010), AEGIS-20 (Ivison et al. 2007), GOODS-N (Morrison et al. 2010), ECDF-S (Miller et al. 2013), and SXDF (Simpson et al. 2006).”
• THE STAR FORMATION HISTORY OF MASS-SELECTED GALAXIES IN THE COSMOS FIELD (2010, methodology): “Hence we correlated our sample with the latest version of the VLA-COSMOS catalog (Schinnerer et al. 2010) and excluded those objects showing radio-derived SFRs more than twice as large as the SED-derived values.”
• Panchromatic spectral energy distributions of Herschel sources (2013, background): “All three are known X-ray sources (Luo et al. 2008, 2010; Brusa et al. 2010; Cappelluti et al. 2009) and two are detected at radio frequencies (Miller et al. 2008; Schinnerer et al. 2010).”
• The VLA-COSMOS 3 GHz Large Project: Continuum data and source catalog release (2017, methodology): “13 we compare the corrected spectral indices from MSMF with those derived from the cataloged flux densities at 3 GHz and 1.4 GHz (joint catalog, Schinnerer et al. 2010).”