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Herschel-ATLAS: Blazars in the science demonstration phase field

Astronomy and Astrophysics 518:3 (2010)

Authors:

J González-Nuevo, G De Zotti, P Andreani, EJ Barton, F Bertoldi, M Birkinshaw, L Bonavera, S Buttiglione, J Cooke, A Cooray, G Danese, L Dunne, S Eales, L Fan, MJ Jarvis, HR Klöckner, E Hatziminaoglou, D Herranz, DH Hughes, A Lapi, A Lawrence, L Leeuw, M Lopez-Caniego, M Massardi, T Mauch, MJ Michałowski, M Negrello, S Rawlings, G Rodighiero, S Samui, S Serjeant, JD Vieira, G White, A Amblard, R Auld, M Baes, DG Bonfield, D Burgarella, A Cava, DL Clements, A Dariush, S Dye, D Frayer, J Fritz, E Ibar, RJ Ivison, G Lagache, S Maddox, E Pascale, M Pohlen, E Rigby, B Sibthorpe, DJB Smith, P Temi, M Thompson, I Valtchanov, A Verma

Abstract:

To investigate the poorly constrained sub-mm counts and spectral properties of blazars we searched for these in the Herschel-ATLAS (H-ATLAS) science demonstration phase (SDP) survey catalog. We cross-matched 500 μm sources brighter than 50 mJy with the FIRST radio catalogue. We found two blazars, both previously known. Our study is among the first blind blazar searches at sub-mm wavelengths, i.e., in the spectral regime where little is still known about the blazar SEDs, but where the synchrotron peak of the most luminous blazars is expected to occur. Our early results are consistent with educated extrapolations of lower frequency counts and question indications of substantial spectral curvature downwards and of spectral upturns at mm wavelengths. One of the two blazars is identified with a Fermi/LAT γ-ray source and a WMAP source. The physical parameters of the two blazars are briefly discussed. These observations demonstrate that the H-ATLAS survey will provide key information about the physics of blazars and their contribution to sub-mm counts. © 2010 ESO.
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Herschel-ATLAS: Dust temperature and redshift distribution of SPIRE and PACS detected sources using submillimetre colours

Astronomy and Astrophysics 518:1 (2010)

Authors:

A Amblard, A Cooray, P Serra, P Temi, E Barton, M Negrello, R Auld, M Baes, IK Baldry, S Bamford, A Blain, J Bock, D Bonfield, D Burgarella, S Buttiglione, E Cameron, A Cava, D Clements, S Croom, A Dariush, G De Zotti, S Driver, J Dunlop, L Dunne, S Dye, S Eales, D Frayer, J Fritz, JP Gardner, J Gonzalez-Nuevo, D Herranz, D Hill, A Hopkins, DH Hughes, E Ibar, RJ Ivison, M Jarvis, DH Jones, L Kelvin, G Lagache, L Leeuw, J Liske, M Lopez-Caniego, J Loveday, S Maddox, M Michałowski, P Norberg, H Parkinson, JA Peacock, C Pearson, E Pascale, M Pohlen, C Popescu, M Prescott, A Robotham, E Rigby, G Rodighiero, S Samui, A Sansom, D Scott, S Serjeant, R Sharp, B Sibthorpe, DJB Smith, MA Thompson, R Tuffs, I Valtchanov, E Van Kampen, P Van Der Werf, A Verma, J Vieira, C Vlahakis

Abstract:

We present colour-colour diagrams of detected sources in the Herschel-ATLAS science demonstration field from 100 to 500 μm using both PACS and SPIRE. We fit isothermal modified black bodies to the spectral energy distribution (SED) to extract the dust temperature of sources with counterparts in Galaxy And Mass Assembly (GAMA) or SDSS surveys with either a spectroscopic or a photometric redshift. For a subsample of 330 sources detected in at least three FIR bands with a significance greater than 3σ, we find an average dust temperature of (28±8) K. For sources with no known redshift, we populate the colour-colour diagram with a large number of SEDs generated with a broad range of dust temperatures and emissivity parameters, and compare to colours of observed sources to establish the redshift distribution of this sample. For another subsample of 1686 sources with fluxes above 35 mJy at 350 μm and detected at 250 and 500 μm with a significance greater than 3σ, we find an average redshift of 2.2±0.6. © 2010 ESO.
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Herschel-ATLAS: Dust temperature and redshift distribution of SPIRE and PACS detected sources using submillimetre colours

Astronomy and Astrophysics 518:1 (2010)

Authors:

A Amblard, A Cooray, P Serra, P Temi, E Barton, M Negrello, R Auld, M Baes, IK Baldry, S Bamford, A Blain, J Bock, D Bonfield, D Burgarella, S Buttiglione, E Cameron, A Cava, D Clements, S Croom, A Dariush, G De Zotti, S Driver, J Dunlop, L Dunne, S Dye, S Eales, D Frayer, J Fritz, JP Gardner, J Gonzalez-Nuevo, D Herranz, D Hill, A Hopkins, DH Hughes, E Ibar, RJ Ivison, M Jarvis, DH Jones, L Kelvin, G Lagache, L Leeuw, J Liske, M Lopez-Caniego, J Loveday, S Maddox, M Michałowski, P Norberg, H Parkinson, JA Peacock, C Pearson, E Pascale, M Pohlen, C Popescu, M Prescott, A Robotham, E Rigby, G Rodighiero, S Samui, A Sansom, D Scott, S Serjeant, R Sharp, B Sibthorpe, DJB Smith, MA Thompson, R Tuffs, I Valtchanov, E Van Kampen, P Van Der Werf, A Verma, J Vieira, C Vlahakis

Abstract:

We present colour-colour diagrams of detected sources in the Herschel-ATLAS science demonstration field from 100 to 500 μm using both PACS and SPIRE. We fit isothermal modified black bodies to the spectral energy distribution (SED) to extract the dust temperature of sources with counterparts in Galaxy And Mass Assembly (GAMA) or SDSS surveys with either a spectroscopic or a photometric redshift. For a subsample of 330 sources detected in at least three FIR bands with a significance greater than 3σ, we find an average dust temperature of (28±8) K. For sources with no known redshift, we populate the colour-colour diagram with a large number of SEDs generated with a broad range of dust temperatures and emissivity parameters, and compare to colours of observed sources to establish the redshift distribution of this sample. For another subsample of 1686 sources with fluxes above 35 mJy at 350 μm and detected at 250 and 500 μm with a significance greater than 3σ, we find an average redshift of 2.2±0.6. © 2010 ESO.
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Herschel-ATLAS: Evolution of the 250 μm luminosity function out to z = 0.5

Astronomy and Astrophysics 518:1 (2010)

Authors:

S Dye, L Dunne, S Eales, DJB Smith, A Amblard, R Auld, M Baes, IK Baldry, S Bamford, AW Blain, DG Bonfield, M Bremer, D Burgarella, S Buttiglione, E Cameron, A Cava, DL Clements, A Cooray, S Croom, A Dariush, G De Zotti, S Driver, JS Dunlop, D Frayer, J Fritz, JP Gardner, HL Gomez, J Gonzalez-Nuevo, D Herranz, D Hill, A Hopkins, E Ibar, RJ Ivison, MJ Jarvis, DH Jones, L Kelvin, G Lagache, L Leeuw, J Liske, M Lopez-Caniego, J Loveday, S Maddox, MJ Michałowski, M Negrello, P Norberg, MJ Page, H Parkinson, E Pascale, JA Peacock, M Pohlen, C Popescu, M Prescott, D Rigopoulou, A Robotham, E Rigby, G Rodighiero, S Samui, D Scott, S Serjeant, R Sharp, B Sibthorpe, P Temi, MA Thompson, R Tuffs, I Valtchanov, PP Van Der Werf, E Van Kampen, A Verma

Abstract:

We have determined the luminosity function of 250 μm-selected galaxies detected in the ∼14 deg2science demonstration region of the Herschel-ATLAS project out to a redshift of z = 0.5. Our findings very clearly show that the luminosity function evolves steadily out to this redshift. By selecting a sub-group of sources within a fixed luminosity interval where incompleteness effects are minimal, we have measured a smooth increase in the comoving 250 μm luminosity density out to z = 0.2 where it is 3.6+1.4-0.9times higher than the local value. © 2010 ESO.
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Herschel-ATLAS: Extragalactic number counts from 250 to 500 microns

Astronomy and Astrophysics 518:1 (2010)

Authors:

DL Clements, E Rigby, S Maddox, L Dunne, A Mortier, C Pearson, A Amblard, R Auld, M Baes, D Bonfield, D Burgarella, S Buttiglione, A Cava, A Cooray, A Dariush, G De Zotti, S Dye, S Eales, D Frayer, J Fritz, JP Gardner, J Gonzalez-Nuevo, D Herranz, E Ibar, R Ivison, MJ Jarvis, G Lagache, L Leeuw, M Lopez-Caniego, M Negrello, E Pascale, M Pohlen, G Rodighiero, S Samui, S Serjeant, B Sibthorpe, D Scott, DJB Smith, P Temi, M Thompson, I Valtchanov, P Van Der Werf, A Verma

Abstract:

Aims. The Herschel-ATLAS survey (H-ATLAS) will be the largest area survey to be undertaken by the Herschel Space Observatory. It will cover 550 sq. deg. of extragalactic sky at wavelengths of 100, 160, 250, 350 and 500 μm when completed, reaching flux limits (5σ) from 32 to 145 mJy. We here present galaxy number counts obtained for SPIRE observations of the first ∼14 sq. deg. observed at 250, 350 and 500 μm. Methods. Number counts are a fundamental tool in constraining models of galaxy evolution. We use source catalogs extracted from the H-ATLAS maps as the basis for such an analysis. Correction factors for completeness and flux boosting are derived by applying our extraction method to model catalogs and then applied to the raw observational counts. Results. We find a steep rise in the number counts at flux levels of 100-200 mJy in all three SPIRE bands, consistent with results from BLAST. The counts are compared to a range of galaxy evolution models. None of the current models is an ideal fit to the data but all ascribe the steep rise to a population of luminous, rapidly evolving dusty galaxies at moderate to high redshift. © 2010 ESO.
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