Herschel-ATLAS: Extragalactic number counts from 250 to 500 microns
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S. Maddox | S. Serjeant | E. Pascale | M. Jarvis | J. Gardner | D. Clements | G. Zotti | D. Herranz | G. Lagache | D. Scott | M. Baes | J. González-Nuevo | M. López-Caniego | L. Dunne | D. Frayer | C. Pearson | P. D. Werf | S. Eales | R. Ivison | D. Bonfield | A. Verma | R. Auld | A. Cooray | M. Pohlen | E. Rigby | I. Valtchanov | A. Dariush | M. Negrello | B. Sibthorpe | D. Burgarella | E. Ibar | D.J.B. Smith | A. Amblard | A. Cava | A. Mortier | G. Rodighiero | S. Dye | L. Leeuw | S. Buttiglione | J. Fritz | P. Temi | M. Thompson | S. Samui | L. Leeuw | M. Thompson | D. Scott | P. Werf | D. Scott
[1] S. Ott,et al. Herschel Space Observatory - An ESA facility for far-infrared and submillimetre astronomy , 2010, 1005.5331.
[2] S. J. Liu,et al. Herschel : the first science highlights Special feature L etter to the E ditor The Herschel-SPIRE instrument and its in-flight performance , 2010 .
[3] H. Roussel,et al. In-flight calibration of the Herschel-SPIRE instrument , 2010, 1005.5073.
[4] S. Maddox,et al. Herschel-ATLAS: The angular correlation function of submillimetre galaxies at high and low redshift , 2010, 1005.2406.
[5] S. Maddox,et al. The Herschel ATLAS , 2009, 0910.4279.
[6] S. Bamford,et al. GAMA: towards a physical understanding of galaxy formation , 2009, 0910.5123.
[7] CEA-Saclay,et al. Deep Spitzer 24 μm COSMOS Imaging. I. The Evolution of Luminous Dusty Galaxies—Confronting the Models , 2009, 0909.4303.
[8] Padova,et al. Predictions for Herschel from Λ-cold dark matter: unveiling the cosmic star formation history , 2009, 0909.1567.
[9] Sophia A. Khan,et al. Submillimetre surveys: the prospects for Herschel , 2009, 0906.4120.
[10] James J. Bock,et al. SUBMILLIMETER NUMBER COUNTS FROM STATISTICAL ANALYSIS OF BLAST MAPS , 2009, 0906.0981.
[11] Chris Pearson,et al. The Herschel-SPIRE photometer data processing pipeline , 2008, Astronomical Telescopes + Instrumentation.
[12] L. Miller,et al. A semi-empirical simulation of the extragalactic radio continuum sky for next generation radio telescopes , 2008, 0805.3413.
[13] D. L. Clements,et al. The SCUBA Half‐Degree Extragalactic Survey (SHADES) – VIII. The nature of faint submillimetre galaxies in SHADES, SWIRE and SXDF surveys , 2008, 0803.0475.
[14] J. Dunlop,et al. The SCUBA HAlf Degree Extragalactic Survey (SHADES) – VII. Optical/IR photometry and stellar masses of submillimetre galaxies , 2008, 0802.0497.
[15] Padova,et al. Galaxy evolution in the infrared: comparison of a hierarchical galaxy formation model with Spitzer data , 2007, 0704.1562.
[16] Thomas Henning,et al. The Photodetector Array Camera and Spectrometer (PACS) for the Herschel Space Observatory , 2004, Astronomical Telescopes + Instrumentation.
[17] Dominic J. Benford,et al. First Constraints on Source Counts at 350 μm , 2007, 0704.2210.
[18] C. Baccigalupi,et al. Astrophysical and cosmological information from large-scale submillimetre surveys of extragalactic sources , 2007, astro-ph/0703210.
[19] W. Percival,et al. The SCUBA half-degree extragalactic survey - II. Submillimetre maps, catalogue and number counts , 2006, astro-ph/0609039.
[20] D. Padgett,et al. Spitzer 70 and 160 μm Observations of the Extragalactic First Look Survey , 2005, astro-ph/0509649.
[21] Philip R. Goode,et al. Rapid Change of δ Spot Structure Associated with Seven Major Flares , 2005 .
[22] Alessandro Bressan,et al. Can the faint submillimetre galaxies be explained in the Λ cold dark matter model , 2005 .
[23] I. Smail,et al. A Redshift Survey of the Submillimeter Galaxy Population , 2004, astro-ph/0412573.
[24] D. Mesa,et al. Predictions for high-frequency radio surveys of extragalactic sources , 2004, astro-ph/0410709.
[25] S. Serjeant,et al. The local submillimetre luminosity functions and predictions from Spitzer to Herschel , 2004, astro-ph/0409498.
[26] M. Irwin,et al. ImpZ: a new photometric redshift code for galaxies and quasars , 2004, astro-ph/0406296.
[27] Orsay,et al. The 24 Micron Source Counts in Deep Spitzer Space Telescope Surveys , 2004, astro-ph/0406035.
[28] G. Rieke,et al. POLYCYCLIC AROMATIC HYDROCARBON CONTRIBUTION TO THE INFRARED OUTPUT ENERGY OF THE UNIVERSE AT z 2 , 2004, astro-ph/0406016.
[29] G. Granato,et al. A Physical Model for the Coevolution of QSOs and Their Spheroidal Hosts , 2003, astro-ph/0307202.
[30] S. Serjeant,et al. The Local sub-mm luminosity functions and predictions from Spitzer to Herschel , 2004 .
[31] C. Baccigalupi,et al. Gravitational lensing of extended high-redshift sources by dark matter haloes , 2002 .
[32] Michael G. Hauser,et al. THE COSMIC INFRARED BACKGROUND: Measurements and Implications ⁄ , 2001 .
[33] Loretta Dunne,et al. The Canada-UK Deep Submillimeter Survey. IV. The Survey of the 14 Hour Field , 2000, astro-ph/0009154.
[34] C. Baugh,et al. The Infrared Side of Galaxy Formation. I. The Local Universe in the Semianalytical Framework , 2000, astro-ph/0001308.
[35] J. Dunlop,et al. High-redshift star formation in the Hubble Deep Field revealed by a submillimetre-wavelength survey , 1998, Nature.
[36] C. Bennett,et al. The Spectrum of the Extragalactic Far-Infrared Background from the COBE FIRAS Observations , 1998, astro-ph/9803021.
[37] I. Smail,et al. A Deep Submillimeter Survey of Lensing Clusters: A New Window on Galaxy Formation and Evolution , 1997, astro-ph/9708135.
[38] David W. Hogg,et al. Deep Optical Galaxy Counts with the Keck Telescope , 1995, astro-ph/9506095.
[39] P. Napier. National Radio Astronomy Observatory , 1992 .
[40] Martin Ryle,et al. An Examination of the Steady-state Model in the Light of Some Recent Observations of Radio Sources , 1961 .