COSBO: The MAMBO 1.2 Millimeter Imaging Survey of the COSMOS Field

By F. Bertoldi, C. Carilli, M. Aravena, E. Schinnerer, H. Voss, V. Smolčić, K. Jahnke, N. Scoville, A. Blain, K. Menten and 13 more. 2007

146 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/1787b962f135379ecff9ad33e6d8881724bbaeb5

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In Astronomy and Astrophysics

1. D. M. Alexander
2. L. Hernquist
3. P. Hopkins
4. D. Narayanan
5. E. Daddi
6. P. Capak
7. R. Somerville
8. A. Koekemoer

Citations in the corpus

• AN ALMA SURVEY OF SUBMILLIMETER GALAXIES IN THE EXTENDED CHANDRA DEEP FIELD SOUTH: THE REDSHIFT DISTRIBUTION AND EVOLUTION OF SUBMILLIMETER GALAXIES (2013, background): “…(e.g. Ivison et al. 1998, 2000), as deep 1.4 GHz radio imaging with the Very Large Array (VLA) provides the sub-arcsecond resolution required to accurately locate the counterpart to the submm emission (Ivison et al. 2002, 2004, 2007; Bertoldi et al. 2007; Biggs et al. 2011; Lindner et al. 2011).”
• THE CHANDRA COSMOS SURVEY. I. OVERVIEW AND POINT SOURCE CATALOG (2009, background): “…on this same central sub-field of COSMOS: the z-COSMOS Deep spectroscopic survey (to B∼25, Lilly et al. 2007), the deep VLA survey (6 µJy rms, Schinnerer et al. 2009, in preparation), and several – 6 – millimeter and sub-millimeter surveys (MAMBO, Bertoldi et al. 2007 and AzTEC, Scott et al. 2008).”
• SUBMILLIMETER GALAXIES AS PROGENITORS OF COMPACT QUIESCENT GALAXIES (2014, background): “…(AzTEC, LABOCA, MAMBO, SMA, CARMA, PdBI) and FIR (Spitzer MIPS, Herschel PACS and SPIRE) observations of the COSMOS field (Sanders et al. 2007; Lutz et al. 2011; Oliver et al. 2012; Scott et al. 2008; Aretxaga et al. 2011; Bertoldi et al. 2007; Younger et al. 2007, 2008; Smolčić et al. 2012a,b).”
• THE VLA-COSMOS SURVEY. IV. DEEP DATA AND JOINT CATALOG (2010, methodology): “…al. 2007; Capak et al. 2007), optical HST (Scoville et al. 2007a; Koekemoer et al. 2007), midto far-infrared Spitzer (Sanders et al. 2007), millimeter (Bertoldi et al. 2007; Scott et al. 2008) and radio VLA (Schinnerer et al. 2004, 2007) imaging to extensive optical spectroscopy using the…”
• EXTRAGALACTIC MILLIMETER-WAVE SOURCES IN SOUTH POLE TELESCOPE SURVEY DATA: SOURCE COUNTS, CATALOG, AND STATISTICS FOR AN 87 SQUARE-DEGREE FIELD (2009, background): “…in surveys of blank fields, but only over a total area on the order of a square degree (Scott et al. 2002; Borys et al. 2003; Greve et al. 2004; Laurent et al. 2005; Coppin et al. 2006; Bertoldi et al. 2007; Perera et al. 2008; Scott et al. 2008; Austermann et al. 2010; Weiß et al. 2009).”
• AzTEC millimetre survey of the COSMOS field – I. Data reduction and source catalogue (2008, background): “This AzTEC map has no overlap with the MAMBO/COSMOS survey (Bertoldi et al. 2007) and only a small amount of overlap with the shallower Bolocam survey (J. Aguirre, private communication).”
• A Herschel view of the far-infrared properties of submillimetre galaxies (2012, methodology): “The optical counterpart of MAMBO11 without any spectroscopic redshift estimate (MAMBO11W) has a photometric redshift supporting the assumption of an interacting system (Bertoldi et al. 2007).”
• The VLA-COSMOS 3 GHz Large Project: Continuum data and source catalog release (2017, background): “…multiwavelength X-ray to mm photometry (Scoville et al. 2007; Koekemoer et al. 2007; Hasinger et al. 2007; Capak et al. 2007; Sanders et al. 2007; Bertoldi et al. 2007; Elvis et al. 2009; Ilbert et al. 2013; McCracken et al. 2012; Scott et al. 2008; Aretxaga et al. 2011; Smolčić et al. 2012;…”
• The LABOCA survey of the Extended Chandra Deep Field South: A photometric redshift survey of submillimetre galaxies (2010, background): “…identified through statistical arguments and physical correlations based on radio, mid- or near-IR emission (e.g. Ivison et al. 1998, 2000, 2005; Smail et al. 1999; Pope et al. 2005; Bertoldi et al. 2007; Hainline et al. 2009; Biggs et al. 2011), but these locate only ∼60–80 per cent of SMGs.”
• Dusty Star Forming Galaxies at High Redshift (2014, background): “10 illustrates the changing resolution over a single patch of sky in the COSMOS field from optical i-band through to 1.4 GHz radio continuum.”
• Evidence for a Population of High-Redshift Submillimeter Galaxies from Interferometric Imaging (2007, background): “Furthermore, their ubiquity in both this (70% of sources with S/N > 5 at 1.1 mm) and other (50% of sources with S/N > 4 at 1.2 mm; Bertoldi et al. 2007) millimeter surveys further suggest that they contribute significantly to the observed millimeter/submillimeter number counts, and that the median…”
• Deep Spitzer 24 μm COSMOS Imaging. I. The Evolution of Luminous Dusty Galaxies—Confronting the Models (2009, background): “2mm observations of COSMOS (Frayer et al., submitted; Bertoldi et al. 2007) or with the future coverage of this field with forthcoming facilities like Herschel will provide an even more detailed picture of the history of the EBL over the whole range of IR wavelengths.”
• THE STAR FORMATION HISTORY OF MASS-SELECTED GALAXIES IN THE COSMOS FIELD (2010, methodology): “In addition to observations of the whole or parts of the COSMOS field in the X-ray (Hasinger et al. 2007; Elvis et al. 2009) and millimeter (Bertoldi et al. 2007; Scott et al. 2008), imaging by Spitzer in the midto far-IR (Sanders et al. 2007) as well as interferometric radio data (Schinnerer et…”
• Characterization of Scuba-2 450 μm and 850 μm selected galaxies in the COSMOS field (2013, background): “There is only one long-wavelength submillimeter source detected in this area: 850.05 in our sample, as well as COSBO3, detected at 1.2 mm (Bertoldi et al. 2007), and AzTEC/C6, detected at 1.1 mm (Aretxaga et al. 2011).”
• zCOSMOS – 10k-bright spectroscopic sample - The bimodality in the galaxy stellar mass function: exploring its evolution with redshift (2009, background): “…MIR and FIR (S-COSMOS with Spitzer, Sanders et al. 2007), in combination with a multiwavelength dataset from radio (with VLA, Schinnerer et al. 2007), millimetre (with MAMBO-2 at the IRAM telescope, Bertoldi et al. 2007), to X-rays (with XMM, Hasinger et al. 2007, and Chandra, Elvis et al. 2009).”