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

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

[1]  F. Bertoldi,et al.  The Faint Counterparts of MAMBO Millimeter Sources near the New Technology Telescope Deep Field , 2004 .

[2]  I. Smail,et al.  Submitted to ApJ Preprint typeset using L ATEX style emulateapj v. 6/22/04 CLUSTERING OF SUBMILLIMETER-SELECTED GALAXIES , 2004 .

[3]  R. Bender,et al.  Multiwavelength mapping of galaxy formation and evolution , 2003 .

[4]  C. Carilli,et al.  SCUBA observations of the sources detected in the MAMBO 1200-μm survey , 2003 .

[5]  M. Halpern,et al.  The Hubble Deep Field North SCUBA Super-map—I. Submillimetre maps, sources and number counts , 2003, astro-ph/0305444.

[6]  S. C. Chapman,et al.  A median redshift of 2.4 for galaxies bright at submillimetre wavelengths , 2003, Nature.

[7]  L. Dunne,et al.  A Census of Metals at High and Low Redshift and the Connection Between Submillimetre Sources and Spheroid Formation , 2002, astro-ph/0210260.

[8]  The ELAIS deep X-ray survey - I. Chandra source catalogue and first results , 2002, astro-ph/0207622.

[9]  J. Dunlop,et al.  Submillimetre observations of the Hubble Deep Field and Flanking Fields , 2002, astro-ph/0201502.

[10]  S. Lilly,et al.  The Canada-UK Deep Submillimeter Survey. VI. The 3 Hour Field , 2002, astro-ph/0201180.

[11]  S. Chapman,et al.  Submillimetre and far-infrared spectral energy distributions of galaxies: the luminosity-temperature relation and consequences for photometric redshifts , 2002, astro-ph/0209450.

[12]  J. Dunlop,et al.  Deep radio imaging of the SCUBA 8-mJy survey fields: submillimetre source identifications and redshift distribution , 2002, astro-ph/0206432.

[13]  C. Carilli,et al.  Properties of Millimeter Galaxies: Constraints from K-Band Blank Fields , 2002, astro-ph/0201104.

[14]  J. Dunlop,et al.  The SCUBA 8-mJy survey - I. Submillimetre maps, sources and number counts , 2001, astro-ph/0107446.

[15]  R. J. Ivison,et al.  The nature of faint submillimetre-selected galaxies , 2001 .

[16]  A. Efstathiou,et al.  The SCUBA 8-mJy survey - II: Multiwavelength analysis of bright sub-mm sources , 2001 .

[17]  C. Baugh,et al.  The clustering evolution of the galaxy distribution , 2001, astro-ph/0103092.

[18]  Mark Dickinson,et al.  Clustering Segregation with Ultraviolet Luminosity in Lyman Break Galaxies at z~3 and Its Implications , 2000, astro-ph/0012249.

[19]  J. Dunlop.  Sub-mm clues to elliptical galaxy formation , 2000, astro-ph/0011077.

[20]  Loretta Dunne,et al.  The Canada-UK Deep Submillimeter Survey. IV. The Survey of the 14 Hour Field , 2000, astro-ph/0009154.

[21]  D. Clements,et al.  The SCUBA Local Universe Galaxy Survey — I. First measurements of the submillimetre luminosity and dust mass functions , 2000, astro-ph/0002234.

[22]  Jean-Paul Kneib,et al.  The diversity of SCUBA-selected galaxies , 2000 .

[23]  C. L. Carilli,et al.  The Scatter in the Relationship between Redshift and the Radio-to-Submillimeter Spectral Index , 1999, astro-ph/9910316.

[24]  R. J. Ivison,et al.  Radio Constraints on the Identifications and Redshifts of Submillimeter Galaxies , 1999, astro-ph/9907083.

[25]  Andrew W. Blain.  Dust temperature and the submillimetre—radio flux density ratio as a redshift indicator for distant galaxies , 1999 .

[26]  D. B. Sanders,et al.  Resolving the Submillimeter Background: The 850 Micron Galaxy Counts , 1999, astro-ph/9904126.

[27]  C. L. Carilli,et al.  The Radio-to-Submillimeter Spectral Index as a Redshift Indicator , 1998, astro-ph/9812251.

[28]  Eugene E. Haller,et al.  Bolometer array development at the Max-Planck-Institut fuer Radioastronomie , 1998, Astronomical Telescopes and Instrumentation.

[29]  E. L. Wright,et al.  The COBE Diffuse Infrared Background Experiment Search for the Cosmic Infrared Background. I. Limits and Detections , 1998, astro-ph/9806167.

[30]  C. Bennett,et al.  The Spectrum of the Extragalactic Far-Infrared Background from the COBE FIRAS Observations , 1998, astro-ph/9803021.

[31]  Rob Ivison,et al.  A hyperluminous galaxy at z = 2.8 found in a deep submillimetre survey , 1997, astro-ph/9712161.

[32]  I. Smail,et al.  A Deep Submillimeter Survey of Lensing Clusters: A New Window on Galaxy Formation and Evolution , 1997, astro-ph/9708135.

[33]  S. Eales,et al.  The implications of large dust masses at high redshifts: a first look at galactic evolution in the submillimetre waveband , 1996 .

[34]  Peter Coles,et al.  Cosmology: The Origin and Evolution of Cosmic Structure , 1995 .

[35]  Malcolm Longair,et al.  Millimetre background radiation and galaxy formation , 1993 .

[36]  A. Szalay,et al.  Bias and variance of angular correlation functions , 1993 .

[37]  R. Ellis,et al.  The 60-μ and far-infrared luminosity functions of IRAS galaxies , 1990 .

[38]  Christopher A. Tout,et al.  Nearest neighbour analysis of random distributions on a sphere , 1989 .

[39]  P. I. Nelson,et al.  Statistical methods for astronomical data with upper limits. I - Univariate distributions , 1985 .