A 1200-μm MAMBO survey of ELAIS N2 and the Lockman Hole - I. Maps, sources and number counts

By T. Greve, R. Ivison, F. Bertoldi, J. Stevens, J. Dunlop, D. Lutz, C. L. C. IfA, Edinburgh, Atc, Mpifr and 5 more. 2004

167 citations recorded by the source corpus.

The definitive version is available at www.blackwell-synergy.com '.--Copyright Blackwell Publishing. DOI : 10.1111/j.1365-2966.2004.08235.x

Subfields: Astronomy and Astrophysics, Instrumentation

View Paper: https://www.semanticscholar.org/paper/0c847e700d99c916465619168fdf94bc744a1c93

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DUSTY INFRARED GALAXIES: Sources of the Cosmic Infrared Background (2005, methodology): “Fifteen-meter submillime- ter telescopes are limited by the confusion at 1.2 mJy at 850 µm and at 0.5 mJy at 1.2 mm. Ongoing surveys (Smail et al. 2002; Greve et al. 2004) already reach or are about to reach these levels.”
Cosmic evolution of submillimeter galaxies and their contribution to stellar mass assembly (2009, background): “Lots of studies have addressed the issue of characterizing the nature of SMGs (Egami et al., 2004; Greve et al., 2004, 2005; Smail et al., 2004; Swinbank et al., 2004, 2006, 2008; Takagi et al., 2004; Alexander et al., 2005; Borys et al., 2005; Kovács et al., 2006; Laurent et al., 2006; Pope et…”
A Redshift Survey of the Submillimeter Galaxy Population (2004, methodology): “Greve et al. (2004) and Ivison et al. (2005), have recently suggested that the fraction of bright SMGs, robustly confirmed at both 850µm and 1200µm, which are detected in the radio may be even higher – ∼80%.”
AN ALMA SURVEY OF SUBMILLIMETER GALAXIES IN THE EXTENDED CHANDRA DEEP FIELD SOUTH: SOURCE CATALOG AND MULTIPLICITY (2013, methodology): “…sources have used telescopes such as the JCMT, IRAM 30m, and APEX single dishes equipped with the SCUBA, MAMBO, and LABOCA bolometer arrays (Smail et al. 1997; Barger et al. 1998; Hughes et al. 1998; Eales et al. 1999; Bertoldi et al. 2000; Greve et al. 2004; Coppin et al. 2006; Weiß et al. 2009).”
COSBO: The MAMBO 1.2 Millimeter Imaging Survey of the COSMOS Field (2007, methodology): “To partially correct for this effect, we follow the approach of Greve et al. (2004): we produced maps from our data with randomized (i.e., wrong) array parameters.”
SHARC-2 350 μm Observations of Distant Submillimeter-selected Galaxies (2006, methodology): “In principle, this may be attempted on an individual basis, since several galaxies haveMAMBO (Greve et al. 2004) and/or Bolocam (Laurent et al. 2005) detections at longerwavelengths, providing justification for a three-parameter fit.”
Dusty Star Forming Galaxies at High Redshift (2014, background): “Some small deep fields have already been obtained, particularly in a 5 × 5 arcmin portion of GOODS-N to 120 µJy/beam RMS (Staguhn et al., 2013) with more, wider-field pointings being planned in fields like COSMOS.”
An interferometric CO survey of luminous submillimetre galaxies (2005, background): “…receivers to attempt to determine accurate continuum positions and fluxes or, in cases where a higher-J CO line would coincide with the 1.3-mm band, 1 This source was denoted MM J16371+4053 in Greve et al. (2004b) to search for emission from this transition, e.g. SMM J04431+0210 (Neri et al. 2003).”
Evidence for a Population of High-Redshift Submillimeter Galaxies from Interferometric Imaging (2007, background): “…with the Submillimeter Common– User Bolometric Array (SCUBA; Holland et al. 1999) on the James Clerk Maxwell Telescope (JCMT), and later surveys at millimeter wavelengths (Greve et al. 2004; Dannerbauer et al. 2004; Carilli et al. 2005; Schlaerth et al. 2005; Laurent et al. 2005; Bertoldi et…”
EVIDENCE FOR A CLUMPY, ROTATING GAS DISK IN A SUBMILLIMETER GALAXY AT z = 4 (2012, background): “…galaxies (SMGs; Blain et al. 2002) are dusty, gas–rich, high–z galaxies that were revealed in the first extragalactic surveys using SCUBA and MAMBO (e.g., Smail et al. 1997; Hughes et al. 1998; Barger et al. 1998; Eales et al. 1999; Blain et al. 1999; Bertoldi et al. 2000; Greve et al. 2004).”
Molecular Gas at High Redshift (2005, background): “The large linewidths of the SMG population (Greve et al. 2004a) are a good indication that the total mass of some of these early galaxies is large but most of these have unknown morphology and do not have size measurements.”
Testing the evolutionary link between submillimetre galaxies and quasars: CO observations of QSOs at z∼ 2 (2008, methodology): “The final sample comprises 10 submm-detected QSOs with similar fluxes to the SMG sample (Greve et al. 2005; > ∼ 5mJy at 850 µm, assuming 850 µm/1.2 mm colours typical of SMGs; Greve et al. 2004), with a median of 10mJy.”
A deep ALMA image of the Hubble Ultra Deep Field (2016, unknown): “…surveys with the JCMT (e.g. Scott et al. 2002, 2006; Coppin et al. 2006; Austermann et al. 2010; Geach et al. 2013), IRAM (Dannerbauer et al. 2004; Greve et al. 2004; Lindner et al. 2011), APEX (Weiss et al. 2009; Smolcic et al. 2012), ASTE (Scott et al. 2008, 2010; Hatsukade et al. 2010, 2011),…”
MOST SUBMILLIMETER GALAXIES ARE MAJOR MERGERS (2010, unknown): “…carried out with SCUBA (Holland et al. 1999) and MAMBO (Kreysa et al. 1998) revealed a high-redshift (z∼ 1-3.5) population of sub-millimetre-luminous (S850µm ≥ 5 mJy) galaxies (SMGs hereafter; see e.g. Greve et al. 2004; Coppin et al. 2005; Chapman et al. 2005; Pope et al. 2005; Weiss et al. 2009).”