Publications
320 results found
Brisbin D, Harwit M, Altieri B, et al., 2010, The Deep SPIRE HerMES Survey: spectral energy distributions and their astrophysical indications at high redshift, MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, Vol: 409, Pages: 66-74, ISSN: 0035-8711
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- Citations: 8
Roseboom IG, Oliver SJ, Kunz M, et al., 2010, The <i>Herschel</i> Multi-Tiered Extragalactic Survey: source extraction and cross-identifications in confusion-dominated SPIRE images, MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, Vol: 409, Pages: 48-65, ISSN: 0035-8711
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- Citations: 152
Magdis GE, Elbaz D, Hwang HS, et al., 2010, <i>Herschel</i> reveals a <i>T<sub>dust</sub></i>-unbiased selection of <i>z</i> ∼ 2 ultraluminous infrared galaxies, MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, Vol: 409, Pages: 22-28, ISSN: 0035-8711
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- Citations: 63
Rowan-Robinson M, Roseboom IG, Vaccari M, et al., 2010, Cold dust and young starbursts: spectral energy distributions of <i>Herschel</i> SPIRE sources from the HerMES survey, MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, Vol: 409, Pages: 2-11, ISSN: 0035-8711
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- Citations: 43
Buat V, Giovannoli E, Burgarella D, et al., 2010, Measures of star formation rates from infrared (<i>Herschel</i>) and UV (<i>GALEX</i>) emissions of galaxies in the HerMES fields, MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, Vol: 409, Pages: L1-L6, ISSN: 0035-8711
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- Citations: 52
Cava A, Rodighiero G, Perez-Fournon I, et al., 2010, HerMES: SPIRE detection of high-redshift massive compact galaxies in GOODS-N field, MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, Vol: 409, Pages: L19-L24, ISSN: 0035-8711
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- Citations: 14
Glenn J, Conley A, Bethermin M, et al., 2010, HerMES: deep galaxy number counts from a <i>P</i>(<i>D</i>) fluctuation analysis of SPIRE Science Demonstration Phase observations, MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, Vol: 409, Pages: 109-121, ISSN: 0035-8711
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- Citations: 92
Rigopoulou D, Magdis G, Ivison RJ, et al., 2010, HerMES: <i>Herschel</i>-SPIRE observations of Lyman break galaxies, MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, Vol: 409, Pages: L7-L12, ISSN: 0035-8711
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- Citations: 21
Hwang HS, Elbaz D, Magdis G, et al., 2010, Evolution of dust temperature of galaxies through cosmic time as seen by <i>Herschel</i>, MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, Vol: 409, Pages: 75-82, ISSN: 0035-8711
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- Citations: 143
Levenson L, Marsden G, Zemcov M, et al., 2010, HerMES: SPIRE Science Demonstration Phase maps, MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, Vol: 409, Pages: 83-91, ISSN: 0035-8711
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- Citations: 53
Chapman SC, Ivison RJ, Roseboom IG, et al., 2010, <i>Herschel</i>-SPIRE, far-infrared properties of millimetre-bright and -faint radio galaxies, MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, Vol: 409, Pages: L13-L18, ISSN: 0035-8711
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- Citations: 54
Tauber JA, Mandolesi N, Puget J-L, et al., 2010, <i>Planck</i> pre-launch status: The <i>Planck</i> mission, ASTRONOMY & ASTROPHYSICS, Vol: 520, ISSN: 0004-6361
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- Citations: 276
Rowan-Robinson M, Wang L, 2010, Hyper luminous infrared galaxies from IIFSCz, MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, Vol: 406, Pages: 720-728, ISSN: 0035-8711
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- Citations: 19
Georgakakis A, Rowan-Robinson M, Nandra K, et al., 2010, Infrared Excess sources: Compton thick QSOs, low-luminosity Seyferts or starbursts?, MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, Vol: 406, Pages: 420-433, ISSN: 0035-8711
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- Citations: 29
Elbaz D, Hwang HS, Magnelli B, et al., 2010, <i>Herschel</i> unveils a puzzling uniformity of distant dusty galaxies, ASTRONOMY & ASTROPHYSICS, Vol: 518, ISSN: 0004-6361
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- Citations: 171
Cooray A, Amblard A, Wang L, et al., 2010, HerMES: Halo occupation number and bias properties of dusty galaxies from angular clustering measurements, ASTRONOMY & ASTROPHYSICS, Vol: 518, ISSN: 0004-6361
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- Citations: 66
Ivison RJ, Swinbank AM, Swinyard B, et al., 2010, <i>Herschel</i> and SCUBA-2 imaging and spectroscopy of a bright, lensed submillimetre galaxy at <i>z</i>=2.3, ASTRONOMY & ASTROPHYSICS, Vol: 518, ISSN: 0004-6361
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- Citations: 162
Oliver SJ, Wang L, Smith AJ, et al., 2010, HerMES: SPIRE galaxy number counts at 250, 350, and 500 μm, ASTRONOMY & ASTROPHYSICS, Vol: 518, ISSN: 0004-6361
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- Citations: 177
Eales SA, Raymond G, Roseboom IG, et al., 2010, First results from HerMES on the evolution of the submillimetre luminosity function, ASTRONOMY & ASTROPHYSICS, Vol: 518, ISSN: 0004-6361
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- Citations: 45
Nguyen HT, Schulz B, Levenson L, et al., 2010, HerMES: The SPIRE confusion limit, ASTRONOMY & ASTROPHYSICS, Vol: 518, ISSN: 0004-6361
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- Citations: 246
Ivison RJ, Magnelli B, Ibar E, et al., 2010, The far-infrared/radio correlation as probed by <i>Herschel</i>, ASTRONOMY & ASTROPHYSICS, Vol: 518, ISSN: 0004-6361
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- Citations: 173
Vaccari M, Marchetti L, Franceschini A, et al., 2010, The HerMES SPIRE submillimeter local luminosity function, ASTRONOMY & ASTROPHYSICS, Vol: 518, ISSN: 0004-6361
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- Citations: 51
Schulz B, Pearson CP, Clements DL, et al., 2010, HerMES: The submillimeter spectral energy distributions of <i>Herschel</i>/SPIRE-detected galaxies, ASTRONOMY & ASTROPHYSICS, Vol: 518, ISSN: 0004-6361
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- Citations: 7
Griffin MJ, Abergel A, Abreu A, et al., 2010, The <i>Herschel</i>-SPIRE instrument and its in-flight performance, ASTRONOMY & ASTROPHYSICS, Vol: 518, ISSN: 0004-6361
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- Citations: 1703
Hatziminaoglou E, Omont A, Stevens JA, et al., 2010, HerMES: Far infrared properties of known AGN in the HerMES fields, ASTRONOMY & ASTROPHYSICS, Vol: 518, ISSN: 0004-6361
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- Citations: 137
Trichas M, Rowan-Robinson M, Georgakakis A, et al., 2010, Spectroscopic identifications of SWIRE sources in ELAIS-N1, MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, Vol: 405, Pages: 2243-2252, ISSN: 0035-8711
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- Citations: 20
Oliver S, Frost M, Farrah D, et al., 2010, Specific star formation and the relation to stellar mass from 0 < <i>z</i> < 2 as seen in the far-infrared at 70 and 160 <i>μ</i>m, MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, Vol: 405, Pages: 2279-2294, ISSN: 0035-8711
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- Citations: 103
Rodighiero G, Vaccari M, Franceschini A, et al., 2010, Mid- and far-infrared luminosity functions and galaxy evolution from multiwavelength <i>Spitzer</i> observations up to <i>z</i> ∼ 2.5, ASTRONOMY & ASTROPHYSICS, Vol: 515, ISSN: 0004-6361
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- Citations: 163
Coppin K, Pope A, Menendez-Delmestre K, et al., 2010, Mid-infrared spectroscopy of candidate active galactic nuclei-dominated submillimeter galaxies, Astrophysical Journal, Vol: 713, Pages: 503-519, ISSN: 0004-637X
Spitzer spectroscopy has revealed that sime80% of submm galaxies (SMGs) are starburst (SB)-dominated in the mid-infrared. Here we focus on the remaining sime20% that show signs of harboring powerful active galactic nuclei (AGNs). We have obtained Spitzer-InfraRed Spectrograph spectroscopy of a sample of eight SMGs that are candidates for harboring powerful AGNs on the basis of IRAC color selection (S 8 μm/S 4.5 μm>2, i.e., likely power-law mid-infrared spectral energy distributions). SMGs with an AGN dominating (gsim50%) their mid-infrared emission could represent the "missing link" sources in an evolutionary sequence involving a major merger. First of all, we detect polycyclic aromatic hydrocarbon (PAH) features in all of the SMGs, indicating redshifts from 2.5 to 3.4, demonstrating the power of the mid-infrared to determine redshifts for these optically faint dusty galaxies. Second, we see signs of both star formation (from the PAH features) and AGN activity (from continuum emission) in our sample: 62% of the sample are AGN-dominated in the mid-infrared with a median AGN content of 56%, compared with <30% on average for typical SMGs, revealing that our IRAC color selection has successfully singled out sources with proportionately more AGN emission than typical SB-dominated SMGs. However, we find that only about 10% of these AGNs dominate the bolometric emission of the SMG when the results are extrapolated to longer infrared wavelengths, implying that AGNs are not a significant power source to the SMG population overall, even when there is evidence in the mid-infrared for substantial AGN activity. When existing samples of mid-infrared AGN-dominated SMGs are considered, we find that S 8 μm/S 4.5 μm>1.65 works well at selecting mid-infrared energetically dominant AGNs in SMGs, implying a duty cycle of ~15% if all SMGs go through a subsequent mid-infrared AGN-dominated phase in the proposed evolutionary sequence.
Wang L, Rowan-Robinson M, 2010, The Imperial IRAS-FSC Redshift Catalogue: luminosity functions, evolution and galaxy bias, MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, Vol: 401, Pages: 35-46, ISSN: 0035-8711
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- Citations: 16
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