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1. The dust content of high-z submillimeter galaxies revealed by Herschel

Author: Francesca Pozzi, David Elbaz, Albrecht Poglitsch, M. Sanchez-Portal, Bruno Altieri, Giulia Rodighiero, Herve Aussel, Dieter Lutz, Raanan Nordon, Amélie Saintonge, Francesca Matteucci, Lijing Shao, I. Valtchanov, Ángel Bongiovanni, Andrea Cimatti, Carlotta Gruppioni, H. Dominguez-Sanchez, L. Silva, Andrea Grazian, L. Riguccini, Paola Andreani, Gian Luigi Granato, Emanuele Daddi, I. Pérez Garcia, Helmut Dannerbauer, Francesco Calura, Roberto Maiolino, S. Berta, Adriano Fontana, Antonio Cava, Linda J. Tacconi, Reinhard Genzel, J. Cepa, Georgios E. Magdis, Manuela Magliocchetti, Paola Popesso, Drew Brisbin, N. M. Förster Schreiber, Paola Santini, E. Sturm, Benjamin Magnelli, Santini P., Maiolino R., Magnelli B., Silva L., Grazian A., Altieri B., Andreani P., Aussel H., Berta S., Bongiovanni A., Brisbin D., Calura F., Cava A., Cepa J., Cimatti A., Daddi E., Dannerbauer H., Dominguez-Sanchez H., Elbaz D., Fontana A., Förster Schreiber N., Genzel R., Granato G. L., Gruppioni C., Lutz D., Magdis G., Magliocchetti M., Matteucci F., Nordon R., Pérez Garcia I., Poglitsch A., Popesso P., Pozzi F., Riguccini L., Rodighiero G., Saintonge A., Sanchez-Portal M., Shao L., Sturm E., Tacconi L., Valtchanov I., Santini, P., Maiolino, R., Magnelli, B., Silva, L., Grazian, A., Altieri, B., Andreani, P., Aussel, H., Berta, S., Bongiovanni, A., Brisbin, D., Calura, F., Cava, A., Cepa, J., Cimatti, A., Daddi, E., Dannerbauer, H., Dominguez Sanchez, H., Elbaz, D., Fontana, A., Förster Schreiber, N., Genzel, R., Granato, G. L., Gruppioni, C., Lutz, D., Magdis, G., Magliocchetti, M., Matteucci, MARIA FRANCESCA, Nordon, R., Pérez Garcia, I., Poglitsch, A., Popesso, P., Pozzi, F., Riguccini, L., Rodighiero, G., Saintonge, A., Sanchez Portal, M., Shao, L., Sturm, E., Tacconi, L., and Valtchanov, I. Affiliation
Subjects: submillimeter: galaxies, Cosmology and Nongalactic Astrophysics (astro-ph.CO), media_common.quotation_subject, galaxies [submillimeter], FOS: Physical sciences, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, infrared: galaxies, galaxies: high-redshift, galaxies: evolution, galaxies: ISM, Astrophysics::Solar and Stellar Astrophysics, evolution [galaxies], Astrophysics::Galaxy Astrophysics, media_common, Physics, Luminous infrared galaxy, Spiral galaxy, ISM [galaxies], Spectrometer, Astronomy and Astrophysics, Galaxy, Universe, galaxie [infrared], On board, Space and Planetary Science, Content (measure theory), Astrophysics::Earth and Planetary Astrophysics, high-redshift [galaxies], Order of magnitude, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: We use deep observations taken with the Photodetector Array Camera and Spectrometer (PACS), on board the Herschel satellite as part of the PACS evolutionary probe (PEP) guaranteed project along with submm ground-based observations to measure the dust mass of a sample of high-z submillimeter galaxies (SMGs). We investigate their dust content relative to their stellar and gas masses, and compare them with local star-forming galaxies. High-z SMGs are dust rich, i.e. they have higher dust-to-stellar mass ratios compared to local spiral galaxies (by a factor of 30) and also compared to local ultraluminous infrared galaxies (ULIRGs, by a factor of 6). This indicates that the large masses of gas typically hosted in SMGs have already been highly enriched with metals and dust. Indeed, for those SMGs whose gas mass is measured, we infer dust-to-gas ratios similar or higher than local spirals and ULIRGs. However, similarly to other strongly star-forming galaxies in the local Universe and at high-z, SMGs are characterized by gas metalicities lower (by a factor of a few) than local spirals, as inferred from their optical nebular lines, which are generally ascribed to infall of metal-poor gas. This is in contrast with the large dust content inferred from the far-IR and submm data. In short, the metalicity inferred from the dust mass is much higher (by more than an order of magnitude) than that inferred from the optical nebular lines. We discuss the possible explanations of this discrepancy and the possible implications for the investigation of the metalicity evolution at high-z., Comment: Accepted for publication in Astronomy & Astrophysics Letters. One reference updated
Published: 2010

2. PACS Evolutionary Probe (PEP)-A Herschel key program

Author: Ivan Valtchanov, Emanuele Daddi, J. Cepa, Roberto Maiolino, Carlotta Gruppioni, E. Le Floc'h, David Elbaz, Amélie Saintonge, Giulia Rodighiero, Antonio Cava, Andrea Grazian, S. Berta, Paola Andreani, Ángel Bongiovanni, Linda J. Tacconi, H. Dominguez-Sanchez, Bruno Altieri, Francesca Pozzi, Lijing Shao, A. M. Pérez García, M. Wetzstein, Reinhard Genzel, Martin Harwit, Albrecht Poglitsch, Andrea Cimatti, Paola Popesso, Raanan Nordon, Drew Brisbin, Georgios E. Magdis, Herve Aussel, M. Sanchez Portal, Dieter Lutz, E. Wieprecht, N. M. Förster Schreiber, Paola Santini, L. Riguccini, E. Sturm, Benjamin Magnelli, Lutz D., Poglitsch A., Altieri B., Andreani P., Aussel H., Berta S., Bongiovanni A., Brisbin D., Cava A., Cepa J., Cimatti A., Daddi E., Dominguez-Sanchez H., Elbaz D., Förster Schreiber N. M., Genzel R., Grazian A., Gruppioni C., Harwit M., Le Floc'h E., Magdis G., Magnelli B., Maiolino R., Nordon R., Pérez García A. M., Popesso P., Pozzi F., Riguccini L., Rodighiero G., Saintonge A., Sanchez Portal M., Santini P., Shao L., Sturm E., Tacconi L. J., Valtchanov I., Wetzstein M., and Wieprecht E.
Subjects: Physics, Astrofísica, Cosmology and Nongalactic Astrophysics (astro-ph.CO), Star formation, galaxie, FOS: Physical sciences, Astronomy and Astrophysics, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Galaxy, Redshift, Astronomía, Space and Planetary Science, Cosmic infrared background, infrared, Key (cryptography), Galaxy formation and evolution, Astrophysics::Earth and Planetary Astrophysics, cosmology, Astrophysics::Galaxy Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics, Data reduction
Abstract: Deep far-infrared photometric surveys studying galaxy evolution and the nature of the cosmic infrared background are a key strength of the Herschel mission. We describe the scientific motivation for the PACS Evolutionary Probe (PEP) guaranteed time key program and its role in the complement of Herschel surveys, and the field selection which includes popular multiwavelength fields such as GOODS, COSMOS, Lockman Hole, ECDFS, EGS. We provide an account of the observing strategies and data reduction methods used. An overview of first science results illustrates the potential of PEP in providing calorimetric star formation rates for high redshift galaxy populations, thus testing and superseeding previous extrapolations from other wavelengths, and enabling a wide range of galaxy evolution studies., Comment: 13 pages, 12 figures, accepted for publication in A&A
Published: 2011

3. The evolution of the dust temperatures of galaxies in the SFR\u2013

Author: B. Magnelli, D. Lutz, A. Saintonge, S. Berta, P. Santini, M. Symeonidis, B. Altieri, P. Andreani, H. Aussel, M. Bxe9thermin, J. Bock, A. Bongiovanni, J. Cepa, A. Cimatti, A. Conley, E. Daddi, D. Elbaz, N. M. Fxf6rster Schreiber, R. Genzel, R. J. Ivison, E. Le Floc’h, G. Magdis, R. Maiolino, R. Nordon, S. J. Oliver, M. Page, A. Pxe9rez Garcxeda, A. Poglitsch, P. Popesso, F. Pozzi, and et al (including L. Wang)
Published: 2014

4. The evolution of the dust temperatures of galaxies in the SFR-M-* plane up to z similar to 2

Author: Magnelli, B, Lutz, D, Saintonge, A, Berta, S, Santini, P, Symeonidis, M, Altieri, B, Andreani, P, Aussel, H, Bethermin, M, Bock, J, Bongiovanni, A, Cepa, J, Cimatti, A, Conley, A, Daddi, E, Elbaz, D, Schreiber, NMF, Genzel, R, Ivison, RJ, Le Floc'h, E, Magdis, G, Maiolino, R, Nordon, R, Oliver, SJ, Page, M, Perez Garcia, A, Poglitsch, A, Popesso, P, Pozzi, F, Riguccini, L, Rodighiero, G, Rosario, D, Roseboom, I, Sanchez-Portal, M, Scott, D, Sturm, L, Tacconi, LJ, Valtchanov, I, Wang, L, and Wuyts, S
Abstract: We study the evolution of the dust temperature of galaxies in the SFR-Mâ̂- plane up to z ~ 2 using far-infrared and submillimetre observations from the Herschel Space Observatory taken as part of the PACS Evolutionary Probe (PEP) and Herschel Multi-tiered Extragalactic Survey (HerMES) guaranteed time key programmes. Starting from a sample of galaxies with reliable star-formation rates (SFRs), stellar masses (M-) and redshift estimates, we grid the SFR-M-parameter space in several redshift ranges and estimate the mean dust temperature (Tdust) of each SFR-M--z bin. Dust temperatures are inferred using the stacked far-infrared flux densities (100-500 μm) of our SFR-M--z bins. At all redshifts, the dust temperature of galaxies smoothly increases with rest-frame infrared luminosities (LIR), specific SFRs (SSFR; i.e., SFR/M-), and distances with respect to the main sequence (MS) of the SFR-M- plane (i.e., Δlog (SSFR)MS = log [SSFR(galaxy)/SSFRMS(M-,z)]). The Tdust-SSFR and Tdust-Δlog (SSFR)MS correlations are statistically much more significant than the Tdust-LIR one. While the slopes of these three correlations are redshift-independent, their normalisations evolve smoothly from z = 0 and z ~ 2. We convert these results into a recipe to derive Tdust from SFR, M- and z, valid out to z ~ 2 and for the stellar mass and SFR range covered by our stacking analysis. The existence of a strong Tdust-Δlog (SSFR)MS correlation provides us with several pieces of information on the dust and gas content of galaxies. Firstly, the slope of the T dust-Δlog (SSFR)MS correlation can be explained by the increase in the star-formation efficiency (SFE; SFR/Mgas) with Δlog (SSFR)MS as found locally by molecular gas studies. Secondly, at fixed Δlog (SSFR)MS, the constant dust temperature observed in galaxies probing wide ranges in SFR and M- can be explained by an increase or decrease in the number of star-forming regions with comparable SFE enclosed in them. And thirdly, at high redshift, the normalisation towards hotter dust temperature of the Tdust-Δlog (SSFR)MS correlation can be explained by the decrease in the metallicities of galaxies or by the increase in the SFE of MS galaxies. All these results support the hypothesis that the conditions prevailing in the star-forming regions of MS and far-above-MS galaxies are different. MS galaxies have star-forming regions with low SFEs and thus cold dust, while galaxies situated far above the MS seem to be in a starbursting phase characterised by star-forming regions with high SFEs and thus hot dust. © 2014 ESO.
Published: 2014

5. The effect of environment on star forming galaxies at redshift 1 First insight from PACS (vol 532, A145, 2011)

Author: Popesso, P, Rodighiero, G, Saintonge, A, Santini, P, Grazian, A, Lutz, D, Brusa, M, Altieri, B, Andreani, P, Aussel, H, Berta, S, Bongiovanni, A, Cava, A, Cepa, J, Cimatti, A, Daddi, E, Dominguez, H, Elbaz, D, Schreiber, NF, Genzel, R, Gruppioni, C, Magdis, G, Maiolino, R, Magnelli, B, Nordon, R, Perez Garcia, AM, Poglitsch, A, Pozzi, F, Riguccini, L, Sanchez-Portal, M, Shao, L, Sturm, E, Tacconi, L, Valtchanov, I, Wieprecht, E, and Wetzstein, M
Published: 2011

6. GOODS-Herschel A population of 24micron dropout sources at z < 2

Author: Magdis, Georgios E., Elbaz, D., Dickinson, M., Hwang, H. S., Charmandaris, V., Armus, L., Daddi, E., Floc'h, E. Le, Aussel, H., Dannerbauer, H., Rigopoulou, D., Buat, V., Morrison, G., Mullaney, J., Lutz, D., Scott, D., Coia, D., Pope, A., Pannella, M., Altieri1, B., Burgarella, D., Bethermin, M., Dasyra, K., Kartaltepe, J., Leiton, R., Magnelli, B., Popesso, P., and Valtchanov, I.
Subjects: Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: Using extremely deep PACS 100- and 160um Herschel data from the GOODS-Herschel program, we identify 21 infrared bright galaxies previously missed in the deepest 24um surveys performed by MIPS. These MIPS dropouts are predominantly found in two redshift bins, centred at z ~0.4 and ~1.3. Their S_100/S_24 flux density ratios are similar to those of local LIRGs and ULIRGs, whose silicate absorption features at 18um (at z ~ 0.4) and 9.7um (at z ~ 1.3) are shifted into the 24um MIPS band at these redshifts. The high-z sub-sample consists of 11 infrared luminous sources, accounting for ~2% of the whole GOODS-Herschel sample and putting strong upper limits on the fraction of LIRGs/ULIRGs at 1.0 43 colour cut selects galaxies with a redshift distribution similar to that of the MIPS dropouts and when combined with a second colour cut, S_16/S_8 > 4, isolates sources at 1.0 < z < 1.7. We show that these sources have elevated specific star formation rates (sSFR) compared to main sequence galaxies at these redshifts and are likely to be compact starbursts with moderate/strong 9.7um silicate absorption features in their mid-IR spectra. Herschel data reveal that their infrared luminosities extrapolated from the 24um flux density are underestimated, on average, by a factor of ~3. These silicate break galaxies account for 16% (8%) of the ULIRG (LIRG) population in the GOODS fields, indicating a lower limit in their space density of 2.0 \times 10^(-5) Mpc^(-3). Finally, we provide estimates of the fraction of z < 2 MIPS dropout sources as a function of the 24-, 100-, 160-, 250- and 350um sensitivity limits, and conclude that previous predictions of a population of silicate break galaxies missed by the major 24um extragalactic surveys have been overestimated., Comment: Accepted for publication at A&A
Published: 2011

7. Erratum: The effect of environment on star forming galaxies at redshift 1 First insight from PACS (Astronomy and Astrophysics (2011) 532 (A145) DOI: 10.1051/0004-6361/201015672)

Author: Popesso, P, Rodighiero, G, Saintonge, A, Santini, P, Grazian, A, Lutz, D, Brusa, M, Altieri, B, Andreani, P, Aussel, H, Berta, S, Bongiovanni, A, Cava, A, Cepa, J, Cimatti, A, Daddi, E, Dominguez, H, Elbaz, D, Schreiber, NF, Genzel, R, Gruppioni, C, Magdis, G, Maiolino, R, Magnelli, B, Nordon, R, García, AMP, Poglitsch, A, Pozzi, F, Riguccini, L, Sanchez-Portal, M, Shao, L, Sturm, E, Tacconi, L, Valtchanov, I, Wieprecht, E, and Wetzstein, M
Published: 2011

8. Herschel FIR counterparts of selected Ly alpha emitters at z similar to 2.2 Fast evolution since z similar to 3 or missed obscured AGNs?

Author: Bongiovanni, A, Oteo, I, Cepa, J, Perez Garcia, AM, Sanchez-Portal, M, Ederoclite, A, Aguerri, JAL, Alfaro, EJ, Altieri, B, Andreani, P, Aparicio-Villegas, MT, Aussel, H, Benitez, N, Berta, S, Broadhurst, T, Cabrera-Cano, J, Castander, FJ, Cava, A, Cervino, M, Chulani, H, Cimatti, A, Cristobal-Hornillos, D, Daddi, E, Dominguez, H, Elbaz, D, Fernandez-Soto, A, Schreiber, NF, Genzel, R, Gomez, MF, Gonzalez Delgado, RM, Grazian, A, Gruppioni, C, Herreros, JM, Iglesias Groth, S, Infante, L, Lutz, D, Magnelli, B, Magdis, G, Maiolino, R, Marquez, I, Martinez, VJ, Masegosa, J, Moles, M, Molino, A, Nordon, R, del Olmo, A, Perea, J, Poglitsch, A, Popesso, P, Pozzi, F, Prada, F, Quintana, JM, Riguccini, L, Rodighiero, G, Saintonge, A, Sanchez, SF, Santini, P, Shao, L, Sturm, E, Tacconi, L, and Valtchanov, I
Published: 2010

9. PEP: First Herschel probe of dusty galaxy evolution up to z similar to 3

Author: Gruppioni, C, Pozzi, F, Andreani, P, Rodighiero, G, Cimatti, A, Altieri, B, Aussel, H, Berta, S, Bongiovanni, A, Brisbin, D, Cava, A, Cepa, J, Daddi, E, Dominguez-Sanchez, H, Elbaz, D, Schreiber, NF, Genzel, R, Le Floc'h, E, Lutz, D, Magdis, G, Magliocchetti, M, Magnelli, B, Maiolino, R, Nordon, R, Perez-Garcia, AM, Poglitsch, A, Popesso, P, Riguccini, L, Saintonge, A, Sanchez-Portal, M, Santini, P, Shao, L, Sturm, E, Tacconi, L, and Valtchanov, I
Abstract: Aims. We exploit the deepest existing far-infrared (FIR) data obtained so far by Herschel at 100 and 160 μm in the GOODS-N, as part of the PACS evolutionary probe (PEP) survey, to derive for the first time the evolution of the rest-frame 60-μm, 90-μm, and total IR luminosity functions (LFs) of galaxies and AGNs from z = 0 to unprecedented high redshifts (z ∼ 2-3). Methods. The PEP LFs were computed using the 1/Vmax method. The FIR sources were classified by means of a detailed broad-band SED-fitting analysis and spectral characterisation. Based on the best-fit model results, k-correction and total IR (8-1000 μm) luminosity were obtained for each source. LFs (monochromatic and total) were then derived for various IR populations separately in different redshift bins and compared to backward evolution model predictions. Results. We detect strong evolution in the LF to at least z ∼ 2. Objects with SEDs similar to local spiral galaxies are the major contributors to the star formation density (SFD) at z ≲ 0.3, then, as redshift increases, moderate SF galaxies-most likely containing a low-luminosity AGN-start dominating up to z 1.5. At z ≳ 1.5 the SFD is dominated by the contributions of starburst galaxies. In agreement with previous findings, the comoving IR LD derived from our data evolves approximately as (1 + z) 3.8±0.3 up to z ∼ 1, there being some evidence of flattening up to z ∼ 2. © 2010 ESO.
Published: 2010

10. Infrared spectroscopy of faint 15 mu m sources in the Hubble Deep Field South: First hints at the properties of the sources of the IR background

Author: Franceschini, A, Berta, S, Rigopoulou, D, Aussel, H, Cesarsky, C, Elbaz, D, Genzel, R, Moy, E, Oliver, S, Rowan-Robinson, M, and Van der Werf, P
Published: 2003

11. The star-formation rates of 1.5 < z < 2.5 massive galaxies

Author: N. M. Förster Schreiber, S. Berta, H. Dominguez, L. Riguccini, Giulia Rodighiero, Eckhard Sturm, Roberto Maiolino, Georgios E. Magdis, Lijing Shao, D. Elbaz, Benjamin Magnelli, Andrea Cimatti, E. Daddi, Raanan Nordon, Herve Aussel, P. Santini, Paola Andreani, Dieter Lutz, Andrea Grazian, A. M. Pérez García, Amélie Saintonge, Ángel Bongiovanni, I. Valtchanov, Ekkehard Wieprecht, P. Popesso, Linda J. Tacconi, Francesca Pozzi, J. Cepa, M. Wetzstein, M. Sánchez-Portal, Reinhard Genzel, Albrecht Poglitsch, Antonio Cava, Bruno Altieri, R. Nordon, D. Lutz, L. Shao, B. Magnelli, S. Berta, B. Altieri, P. Andreani, H. Aussel, A. Bongiovanni, A. Cava, J. Cepa, A. Cimatti, E. Daddi, H. Dominguez, D. Elbaz, N. M. Förster Schreiber, R. Genzel, A.Grazian, G. Magdi, R. Maiolino R., A. M. Pérez García, A. Poglitsch A., P. Popesso, F. Pozzi, L. Riguccini, and G. Rodighiero
Subjects: Physics, Luminous infrared galaxy, cosmology: observation, Star formation, Extinction (astronomy), Theoretical models, galaxies: starburst, Astronomy and Astrophysics, Astrophysics, Galaxy, Redshift, infrared: galaxies, Space and Planetary Science, Galaxy formation and evolution, galaxies: evolution, galaxies: fundamental parameter
Abstract: The star formation rate (SFR) is a key parameter in the study of galaxy evolution. The accuracy of SFR measurements at z ∼ 2 has been questioned following a disagreement between observations and theoretical models. The latter predict SFRs at this redshift that are typically a factor 4 or more lower than the measurements. We present star-formation rates based on calorimetric measurements of the far-infrared (FIR) luminosities for massive 1.5 < z < 2.5, normal star-forming galaxies (SFGs), which do not depend on extinction corrections and/or extrapolations of spectral energy distributions. The measurements are based on observations in GOODS-N with the Photodetector Array Camera and Spectrometer (PACS) onboard Herschel, as part of the PACS evolutionary probe (PEP) project, that resolve for the first time individual SFGs at these redshifts at FIR wavelengths. We compare FIR-based SFRs to the more commonly used 24 μm and UV SFRs. We find that SFRs from 24 μm alone are higher by a factor of ∼4-7.5 than the true SFRs. This overestimation depends on luminosity: gradually increasing for log L(24 μm) > 12.2 L ⊙. The SFGs and AGNs tend to exhibit the same 24 μm excess. The UV SFRs are in closer agreement with the FIR-based SFRs. Using a Calzetti UV extinction correction results in a mean excess of up to 0.3 dex and a scatter of 0.35 dex from the FIR SFRs. The previous UV SFRs are thus confirmed and the mean excess, while narrowing the gap, is insufficient to explain the discrepancy between the observed SFRs and simulation predictions. © 2010 ESO.
Published: 2010
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12. Star formation in AGN hosts in GOODS-N

Author: Bruno Altieri, Emmanouel Rovilos, Marcella Brusa, V. Mainieri, Franz E. Bauer, Reinhard Genzel, Giulia Rodighiero, Andrea Grazian, N. M. Förster Schreiber, Albrecht Poglitsch, Francesca Pozzi, Paola Santini, Amélie Saintonge, David M. Alexander, Carlotta Gruppioni, Dieter Lutz, M. Wetzstein, L. Riguccini, E. Sturm, W. N. Brandt, Emanuele Daddi, Lijing Shao, Benjamin Magnelli, Roberto Maiolino, Ángel Bongiovanni, H. Dominguez-Sanchez, Linda J. Tacconi, Georgios E. Magdis, Mara Salvato, Ivan Valtchanov, S. Berta, Raanan Nordon, A. M. Pérez García, J. Cepa, Norbert Geis, Andrea Cimatti, Paola Popesso, Antonio Cava, E. Wieprecht, Herve Aussel, M. Sanchez Portal, David Elbaz, Paola Andreani, Shao L., Lutz D., Nordon R., Maiolino R., Alexander D. M., Altieri B., Andreani P., Aussel H., Bauer F. E., Berta S., Bongiovanni A., Brandt W. N., Brusa M., Cava A., Cepa J., Cimatti A., Daddi E., Dominguez-Sanchez H., Elbaz D., Förster Schreiber N. M., Geis N., Genzel R., Grazian A., Gruppioni C., Magdis G., Magnelli B., Mainieri V., Pérez García A. M., Poglitsch A., Popesso P., Pozzi F., Riguccini L., Rodighiero G., Rovilos E., Saintonge A., Salvato M., Sanchez Portal M., Santini P., Sturm E., Tacconi L. J., Valtchanov I., Wetzstein M., and Wieprecht E.
Subjects: Physics, Cosmology and Nongalactic Astrophysics (astro-ph.CO), Star formation, Astrophysics::High Energy Astrophysical Phenomena, Conjunction (astronomy), FOS: Physical sciences, Astronomy and Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, Galaxy, Redshift, Luminosity, Space and Planetary Science, Astrophysics::Solar and Stellar Astrophysics, Astrophysics::Earth and Planetary Astrophysics, Astrophysics::Galaxy Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: Sensitive Herschel far-infrared observations can break degeneracies that were inherent to previous studies of star formation in high-z AGN hosts. Combining PACS 100 and 160um observations of the GOODS-N field with 2Msec Chandra data, we detect ~20% of X-ray AGN individually at >3sig. The host far-infrared luminosity of AGN with L2-10~10^43erg/s increases with redshift by an order of magnitude from z=0 to z~1. In contrast, there is little dependence of far-infrared luminosity on AGN luminosity, for L2-10~1. We do not find a dependence of far-infrared luminosity on X-ray obscuring column, for our sample which is dominated by L2-10, Comment: Accepted for publication in A&A Herschel issue. 4 pages, 6 figures
Published: 2010
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13. HerschelFIR counterparts of selected Lyαemitters atz~ 2.2

Author: Bongiovanni, Á., primary, Oteo, I., additional, Cepa, J., additional, Pérez García, A. M., additional, Sánchez-Portal, M., additional, Ederoclite, A., additional, Aguerri, J. A. L., additional, Alfaro, E. J., additional, Altieri, B., additional, Andreani, P., additional, Aparicio-Villegas, M. T., additional, Aussel, H., additional, Benítez, N., additional, Berta, S., additional, Broadhurst, T., additional, Cabrera-Caño, J., additional, Castander, F. J., additional, Cava, A., additional, Cerviño, M., additional, Chulani, H., additional, Cimatti, A., additional, Cristóbal-Hornillos, D., additional, Daddi, E., additional, Dominguez, H., additional, Elbaz, D., additional, Fernández-Soto, A., additional, Förster Schreiber, N., additional, Genzel, R., additional, Gómez, M. F., additional, González Delgado, R. M., additional, Grazian, A., additional, Gruppioni, C., additional, Herreros, J. M., additional, Iglesias Groth, S., additional, Infante, L., additional, Lutz, D., additional, Magnelli, B., additional, Magdis, G., additional, Maiolino, R., additional, Márquez, I., additional, Martínez, V. J., additional, Masegosa, J., additional, Moles, M., additional, Molino, A., additional, Nordon, R., additional, del Olmo, A., additional, Perea, J., additional, Poglitsch, A., additional, Popesso, P., additional, Pozzi, F., additional, Prada, F., additional, Quintana, J. M., additional, Riguccini, L., additional, Rodighiero, G., additional, Saintonge, A., additional, Sánchez, S. F., additional, Santini, P., additional, Shao, L., additional, Sturm, E., additional, Tacconi, L., additional, and Valtchanov, I., additional
Published: 2010
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14. The HerMES SPIRE submillimeter local luminosity function

Author: Vaccari, M., primary, Marchetti, L., additional, Franceschini, A., additional, Altieri, B., additional, Amblard, A., additional, Arumugam, V., additional, Auld, R., additional, Aussel, H., additional, Babbedge, T., additional, Blain, A., additional, Bock, J., additional, Boselli, A., additional, Buat, V., additional, Burgarella, D., additional, Castro-Rodríguez, N., additional, Cava, A., additional, Chanial, P., additional, Clements, D. L., additional, Conley, A., additional, Conversi, L., additional, Cooray, A., additional, Dowell, C. D., additional, Dwek, E., additional, Dye, S., additional, Eales, S., additional, Elbaz, D., additional, Farrah, D., additional, Fox, M., additional, Gear, W., additional, Glenn, J., additional, González Solares, E. A., additional, Griffin, M., additional, Halpern, M., additional, Hatziminaoglou, E., additional, Huang, J., additional, Ibar, E., additional, Isaak, K., additional, Ivison, R. J., additional, Lagache, G., additional, Levenson, L., additional, Lu, N., additional, Madden, S., additional, Maffei, B., additional, Mainetti, G., additional, Mortier, A. M. J., additional, Nguyen, H. T., additional, O'Halloran, B., additional, Oliver, S. J., additional, Omont, A., additional, Page, M. J., additional, Panuzzo, P., additional, Papageorgiou, A., additional, Pearson, C. P., additional, Pérez-Fournon, I., additional, Pohlen, M., additional, Rawlings, J. I., additional, Raymond, G., additional, Rigopoulou, D., additional, Rizzo, D., additional, Rodighiero, G., additional, Roseboom, I. G., additional, Rowan-Robinson, M., additional, Sánchez Portal, M., additional, Schulz, B., additional, Scott, D., additional, Seymour, N., additional, Shupe, D. L., additional, Smith, A. J., additional, Stevens, J. A., additional, Symeonidis, M., additional, Trichas, M., additional, Tugwell, K. E., additional, Valiante, E., additional, Valtchanov, I., additional, Vigroux, L., additional, Wang, L., additional, Ward, R., additional, Wright, G., additional, Xu, C. K., additional, and Zemcov, M., additional
Published: 2010
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15. HerMES: Far infrared properties of known AGN in the HerMES fields

Author: Hatziminaoglou, E., primary, Omont, A., additional, Stevens, J. A., additional, Amblard, A., additional, Arumugam, V., additional, Auld, R., additional, Aussel, H., additional, Babbedge, T., additional, Blain, A., additional, Bock, J., additional, Boselli, A., additional, Buat, V., additional, Burgarella, D., additional, Castro-Rodríguez, N., additional, Cava, A., additional, Chanial, P., additional, Clements, D. L., additional, Conley, A., additional, Conversi, L., additional, Cooray, A., additional, Dowell, C. D., additional, Dwek, E., additional, Dye, S., additional, Eales, S., additional, Elbaz, D., additional, Farrah, D., additional, Fox, M., additional, Franceschini, A., additional, Gear, W., additional, Glenn, J., additional, González Solares, E. A., additional, Griffin, M., additional, Halpern, M., additional, Ibar, E., additional, Isaak, K., additional, Ivison, R. J., additional, Lagache, G., additional, Levenson, L., additional, Lu, N., additional, Madden, S., additional, Maffei, B., additional, Mainetti, G., additional, Marchetti, L., additional, Mortier, A. M. J., additional, Nguyen, H. T., additional, O'Halloran, B., additional, Oliver, S. J., additional, Page, M. J., additional, Panuzzo, P., additional, Papageorgiou, A., additional, Pearson, C. P., additional, Pérez-Fournon, I., additional, Pohlen, M., additional, Rawlings, J. I., additional, Rigopoulou, D., additional, Rizzo, D., additional, Roseboom, I. G., additional, Rowan-Robinson, M., additional, Sanchez Portal, M., additional, Schulz, B., additional, Scott, D., additional, Seymour, N., additional, Shupe, D. L., additional, Smith, A. J., additional, Symeonidis, M., additional, Trichas, M., additional, Tugwell, K. E., additional, Vaccari, M., additional, Valtchanov, I., additional, Vigroux, L., additional, Wang, L., additional, Ward, R., additional, Wright, G., additional, Xu, C. K., additional, and Zemcov, M., additional
Published: 2010
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16. The far-infrared/radio correlation as probed byHerschel

Author: Ivison, R. J., primary, Magnelli, B., additional, Ibar, E., additional, Andreani, P., additional, Elbaz, D., additional, Altieri, B., additional, Amblard, A., additional, Arumugam, V., additional, Auld, R., additional, Aussel, H., additional, Babbedge, T., additional, Berta, S., additional, Blain, A., additional, Bock, J., additional, Bongiovanni, A., additional, Boselli, A., additional, Buat, V., additional, Burgarella, D., additional, Castro-Rodríguez, N., additional, Cava, A., additional, Cepa, J., additional, Chanial, P., additional, Cimatti, A., additional, Cirasuolo, M., additional, Clements, D. L., additional, Conley, A., additional, Conversi, L., additional, Cooray, A., additional, Daddi, E., additional, Dominguez, H., additional, Dowell, C. D., additional, Dwek, E., additional, Eales, S., additional, Farrah, D., additional, Förster Schreiber, N., additional, Fox, M., additional, Franceschini, A., additional, Gear, W., additional, Genzel, R., additional, Glenn, J., additional, Griffin, M., additional, Gruppioni, C., additional, Halpern, M., additional, Hatziminaoglou, E., additional, Isaak, K., additional, Lagache, G., additional, Levenson, L., additional, Lu, N., additional, Lutz, D., additional, Madden, S., additional, Maffei, B., additional, Magdis, G., additional, Mainetti, G., additional, Maiolino, R., additional, Marchetti, L., additional, Morrison, G. E., additional, Mortier, A. M. J., additional, Nguyen, H. T., additional, Nordon, R., additional, O'Halloran, B., additional, Oliver, S. J., additional, Omont, A., additional, Owen, F. N., additional, Page, M. J., additional, Panuzzo, P., additional, Papageorgiou, A., additional, Pearson, C. P., additional, Pérez-Fournon, I., additional, Pérez García, A. M., additional, Poglitsch, A., additional, Pohlen, M., additional, Popesso, P., additional, Pozzi, F., additional, Rawlings, J. I., additional, Raymond, G., additional, Rigopoulou, D., additional, Riguccini, L., additional, Rizzo, D., additional, Rodighiero, G., additional, Roseboom, I. G., additional, Rowan-Robinson, M., additional, Saintonge, A., additional, Sanchez Portal, M., additional, Santini, P., additional, Schulz, B., additional, Scott, D., additional, Seymour, N., additional, Shao, L., additional, Shupe, D. L., additional, Smith, A. J., additional, Stevens, J. A., additional, Sturm, E., additional, Symeonidis, M., additional, Tacconi, L., additional, Trichas, M., additional, Tugwell, K. E., additional, Vaccari, M., additional, Valtchanov, I., additional, Vieira, J., additional, Vigroux, L., additional, Wang, L., additional, Ward, R., additional, Wright, G., additional, Xu, C. K., additional, and Zemcov, M., additional
Published: 2010
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17. Probing the molecular interstellar medium of M82 withHerschel-SPIRE spectroscopy

Author: Panuzzo, P., primary, Rangwala, N., additional, Rykala, A., additional, Isaak, K. G., additional, Glenn, J., additional, Wilson, C. D., additional, Auld, R., additional, Baes, M., additional, Barlow, M. J., additional, Bendo, G. J., additional, Bock, J. J., additional, Boselli, A., additional, Bradford, M., additional, Buat, V., additional, Castro-Rodríguez, N., additional, Chanial, P., additional, Charlot, S., additional, Ciesla, L., additional, Clements, D. L., additional, Cooray, A., additional, Cormier, D., additional, Cortese, L., additional, Davies, J. I., additional, Dwek, E., additional, Eales, S. A., additional, Elbaz, D., additional, Fulton, T., additional, Galametz, M., additional, Galliano, F., additional, Gear, W. K., additional, Gomez, H. L., additional, Griffin, M., additional, Hony, S., additional, Levenson, L. R., additional, Lu, N., additional, Madden, S., additional, O'Halloran, B., additional, Okumura, K., additional, Oliver, S., additional, Page, M. J., additional, Papageorgiou, A., additional, Parkin, T. J., additional, Pérez-Fournon, I., additional, Pohlen, M., additional, Polehampton, E. T., additional, Rigby, E. E., additional, Roussel, H., additional, Sacchi, N., additional, Sauvage, M., additional, Schulz, B., additional, Schirm, M. R. P., additional, Smith, M. W. L., additional, Spinoglio, L., additional, Stevens, J. A., additional, Srinivasan, S., additional, Symeonidis, M., additional, Swinyard, B., additional, Trichas, M., additional, Vaccari, M., additional, Vigroux, L., additional, Wozniak, H., additional, Wright, G. S., additional, and Zeilinger, W. W., additional
Published: 2010
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18. The dust content of high-zsubmillimeter galaxies revealed byHerschel

Author: Santini, P., primary, Maiolino, R., additional, Magnelli, B., additional, Silva, L., additional, Grazian, A., additional, Altieri, B., additional, Andreani, P., additional, Aussel, H., additional, Berta, S., additional, Bongiovanni, A., additional, Brisbin, D., additional, Calura, F., additional, Cava, A., additional, Cepa, J., additional, Cimatti, A., additional, Daddi, E., additional, Dannerbauer, H., additional, Dominguez-Sanchez, H., additional, Elbaz, D., additional, Fontana, A., additional, Förster Schreiber, N., additional, Genzel, R., additional, Granato, G. L., additional, Gruppioni, C., additional, Lutz, D., additional, Magdis, G., additional, Magliocchetti, M., additional, Matteucci, F., additional, Nordon, R., additional, Pérez Garcia, I., additional, Poglitsch, A., additional, Popesso, P., additional, Pozzi, F., additional, Riguccini, L., additional, Rodighiero, G., additional, Saintonge, A., additional, Sanchez-Portal, M., additional, Shao, L., additional, Sturm, E., additional, Tacconi, L., additional, and Valtchanov, I., additional
Published: 2010
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19. HerMES: SPIRE galaxy number counts at 250, 350, and 500 μm

Author: Oliver, S. J., primary, Wang, L., additional, Smith, A. J., additional, Altieri, B., additional, Amblard, A., additional, Arumugam, V., additional, Auld, R., additional, Aussel, H., additional, Babbedge, T., additional, Blain, A., additional, Bock, J., additional, Boselli, A., additional, Buat, V., additional, Burgarella, D., additional, Castro-Rodríguez, N., additional, Cava, A., additional, Chanial, P., additional, Clements, D. L., additional, Conley, A., additional, Conversi, L., additional, Cooray, A., additional, Dowell, C. D., additional, Dwek, E., additional, Eales, S., additional, Elbaz, D., additional, Fox, M., additional, Franceschini, A., additional, Gear, W., additional, Glenn, J., additional, Griffin, M., additional, Halpern, M., additional, Hatziminaoglou, E., additional, Ibar, E., additional, Isaak, K., additional, Ivison, R. J., additional, Lagache, G., additional, Levenson, L., additional, Lu, N., additional, Madden, S., additional, Maffei, B., additional, Mainetti, G., additional, Marchetti, L., additional, Mitchell-Wynne, K., additional, Mortier, A. M. J., additional, Nguyen, H. T., additional, O'Halloran, B., additional, Omont, A., additional, Page, M. J., additional, Panuzzo, P., additional, Papageorgiou, A., additional, Pearson, C. P., additional, Pérez-Fournon, I., additional, Pohlen, M., additional, Rawlings, J. I., additional, Raymond, G., additional, Rigopoulou, D., additional, Rizzo, D., additional, Roseboom, I. G., additional, Rowan-Robinson, M., additional, Sánchez Portal, M., additional, Savage, R., additional, Schulz, B., additional, Scott, D., additional, Seymour, N., additional, Shupe, D. L., additional, Stevens, J. A., additional, Symeonidis, M., additional, Trichas, M., additional, Tugwell, K. E., additional, Vaccari, M., additional, Valiante, E., additional, Valtchanov, I., additional, Vieira, J. D., additional, Vigroux, L., additional, Ward, R., additional, Wright, G., additional, Xu, C. K., additional, and Zemcov, M., additional
Published: 2010
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20. The star-formation rates of 1.5 < z < 2.5 massive galaxies

Author: Nordon, R., primary, Lutz, D., additional, Shao, L., additional, Magnelli, B., additional, Berta, S., additional, Altieri, B., additional, Andreani, P., additional, Aussel, H., additional, Bongiovanni, A., additional, Cava, A., additional, Cepa, J., additional, Cimatti, A., additional, Daddi, E., additional, Dominguez, H., additional, Elbaz, D., additional, Förster Schreiber, N. M., additional, Genzel, R., additional, Grazian, A., additional, Magdis, G., additional, Maiolino, R., additional, Pérez García, A. M., additional, Poglitsch, A., additional, Popesso, P., additional, Pozzi, F., additional, Riguccini, L., additional, Rodighiero, G., additional, Saintonge, A., additional, Sanchez-Portal, M., additional, Santini, P., additional, Sturm, E., additional, Tacconi, L., additional, Valtchanov, I., additional, Wetzstein, M., additional, and Wieprecht, E., additional
Published: 2010
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21. SPIRE imaging of M 82: Cool dust in the wind and tidal streams

Author: Roussel, H., primary, Wilson, C. D., additional, Vigroux, L., additional, Isaak, K. G., additional, Sauvage, M., additional, Madden, S. C., additional, Auld, R., additional, Baes, M., additional, Barlow, M. J., additional, Bendo, G. J., additional, Bock, J. J., additional, Boselli, A., additional, Bradford, M., additional, Buat, V., additional, Castro-Rodriguez, N., additional, Chanial, P., additional, Charlot, S., additional, Ciesla, L., additional, Clements, D. L., additional, Cooray, A., additional, Cormier, D., additional, Cortese, L., additional, Davies, J. I., additional, Dwek, E., additional, Eales, S. A., additional, Elbaz, D., additional, Galametz, M., additional, Galliano, F., additional, Gear, W. K., additional, Glenn, J., additional, Gomez, H. L., additional, Griffin, M., additional, Hony, S., additional, Levenson, L. R., additional, Lu, N., additional, O'Halloran, B., additional, Okumura, K., additional, Oliver, S., additional, Page, M. J., additional, Panuzzo, P., additional, Papageorgiou, A., additional, Parkin, T. J., additional, Perez-Fournon, I., additional, Pohlen, M., additional, Rangwala, N., additional, Rigby, E. E., additional, Rykala, A., additional, Sacchi, N., additional, Schulz, B., additional, Schirm, M. R. P., additional, Smith, M. W. L., additional, Spinoglio, L., additional, Stevens, J. A., additional, Srinivasan, S., additional, Symeonidis, M., additional, Trichas, M., additional, Vaccari, M., additional, Wozniak, H., additional, Wright, G. S., additional, and Zeilinger, W. W., additional
Published: 2010
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22. Dissecting the cosmic infra-red background withHerschel/PEP

Author: Berta, S., primary, Magnelli, B., additional, Lutz, D., additional, Altieri, B., additional, Aussel, H., additional, Andreani, P., additional, Bauer, O., additional, Bongiovanni, A., additional, Cava, A., additional, Cepa, J., additional, Cimatti, A., additional, Daddi, E., additional, Dominguez, H., additional, Elbaz, D., additional, Feuchtgruber, H., additional, Förster Schreiber, N. M., additional, Genzel, R., additional, Gruppioni, C., additional, Katterloher, R., additional, Magdis, G., additional, Maiolino, R., additional, Nordon, R., additional, Pérez García, A. M., additional, Poglitsch, A., additional, Popesso, P., additional, Pozzi, F., additional, Riguccini, L., additional, Rodighiero, G., additional, Saintonge, A., additional, Santini, P., additional, Sanchez-Portal, M., additional, Shao, L., additional, Sturm, E., additional, Tacconi, L. J., additional, Valtchanov, I., additional, Wetzstein, M., additional, and Wieprecht, E., additional
Published: 2010
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23. Herschelunveils a puzzling uniformity of distant dusty galaxies

Author: Elbaz, D., primary, Hwang, H. S., additional, Magnelli, B., additional, Daddi, E., additional, Aussel, H., additional, Altieri, B., additional, Amblard, A., additional, Andreani, P., additional, Arumugam, V., additional, Auld, R., additional, Babbedge, T., additional, Berta, S., additional, Blain, A., additional, Bock, J., additional, Bongiovanni, A., additional, Boselli, A., additional, Buat, V., additional, Burgarella, D., additional, Castro-Rodriguez, N., additional, Cava, A., additional, Cepa, J., additional, Chanial, P., additional, Chary, R.-R., additional, Cimatti, A., additional, Clements, D. L., additional, Conley, A., additional, Conversi, L., additional, Cooray, A., additional, Dickinson, M., additional, Dominguez, H., additional, Dowell, C. D., additional, Dunlop, J. S., additional, Dwek, E., additional, Eales, S., additional, Farrah, D., additional, Förster Schreiber, N., additional, Fox, M., additional, Franceschini, A., additional, Gear, W., additional, Genzel, R., additional, Glenn, J., additional, Griffin, M., additional, Gruppioni, C., additional, Halpern, M., additional, Hatziminaoglou, E., additional, Ibar, E., additional, Isaak, K., additional, Ivison, R. J., additional, Lagache, G., additional, Le Borgne, D., additional, Le Floc'h, E., additional, Levenson, L., additional, Lu, N., additional, Lutz, D., additional, Madden, S., additional, Maffei, B., additional, Magdis, G., additional, Mainetti, G., additional, Maiolino, R., additional, Marchetti, L., additional, Mortier, A. M. J., additional, Nguyen, H. T., additional, Nordon, R., additional, O'Halloran, B., additional, Okumura, K., additional, Oliver, S. J., additional, Omont, A., additional, Page, M. J., additional, Panuzzo, P., additional, Papageorgiou, A., additional, Pearson, C. P., additional, Perez Fournon, I., additional, Pérez García, A. M., additional, Poglitsch, A., additional, Pohlen, M., additional, Popesso, P., additional, Pozzi, F., additional, Rawlings, J. I., additional, Rigopoulou, D., additional, Riguccini, L., additional, Rizzo, D., additional, Rodighiero, G., additional, Roseboom, I. G., additional, Rowan-Robinson, M., additional, Saintonge, A., additional, Sanchez Portal, M., additional, Santini, P., additional, Sauvage, M., additional, Schulz, B., additional, Scott, D., additional, Seymour, N., additional, Shao, L., additional, Shupe, D. L., additional, Smith, A. J., additional, Stevens, J. A., additional, Sturm, E., additional, Symeonidis, M., additional, Tacconi, L., additional, Trichas, M., additional, Tugwell, K. E., additional, Vaccari, M., additional, Valtchanov, I., additional, Vieira, J., additional, Vigroux, L., additional, Wang, L., additional, Ward, R., additional, Wright, G., additional, Xu, C. K., additional, and Zemcov, M., additional
Published: 2010
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24. HerMES: The SPIRE confusion limit

Author: Nguyen, H. T., primary, Schulz, B., additional, Levenson, L., additional, Amblard, A., additional, Arumugam, V., additional, Aussel, H., additional, Babbedge, T., additional, Blain, A., additional, Bock, J., additional, Boselli, A., additional, Buat, V., additional, Castro-Rodriguez, N., additional, Cava, A., additional, Chanial, P., additional, Chapin, E., additional, Clements, D. L., additional, Conley, A., additional, Conversi, L., additional, Cooray, A., additional, Dowell, C. D., additional, Dwek, E., additional, Eales, S., additional, Elbaz, D., additional, Fox, M., additional, Franceschini, A., additional, Gear, W., additional, Glenn, J., additional, Griffin, M., additional, Halpern, M., additional, Hatziminaoglou, E., additional, Ibar, E., additional, Isaak, K., additional, Ivison, R. J., additional, Lagache, G., additional, Lu, N., additional, Madden, S., additional, Maffei, B., additional, Mainetti, G., additional, Marchetti, L., additional, Marsden, G., additional, Marshall, J., additional, O'Halloran, B., additional, Oliver, S. J., additional, Omont, A., additional, Page, M. J., additional, Panuzzo, P., additional, Papageorgiou, A., additional, Pearson, C. P., additional, Perez Fournon, I., additional, Pohlen, M., additional, Rangwala, N., additional, Rigopoulou, D., additional, Rizzo, D., additional, Roseboom, I. G., additional, Rowan-Robinson, M., additional, Scott, D., additional, Seymour, N., additional, Shupe, D. L., additional, Smith, A. J., additional, Stevens, J. A., additional, Symeonidis, M., additional, Trichas, M., additional, Tugwell, K. E., additional, Vaccari, M., additional, Valtchanov, I., additional, Vigroux, L., additional, Wang, L., additional, Ward, R., additional, Wiebe, D., additional, Wright, G., additional, Xu, C. K., additional, and Zemcov, M., additional
Published: 2010
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25. TheHerschelSpace Observatory view of dust in M81

Author: Bendo, G. J., primary, Wilson, C. D., additional, Pohlen, M., additional, Sauvage, M., additional, Auld, R., additional, Baes, M., additional, Barlow, M. J., additional, Bock, J. J., additional, Boselli, A., additional, Bradford, M., additional, Buat, V., additional, Castro-Rodriguez, N., additional, Chanial, P., additional, Charlot, S., additional, Ciesla, L., additional, Clements, D. L., additional, Cooray, A., additional, Cormier, D., additional, Cortese, L., additional, Davies, J. I., additional, Dwek, E., additional, Eales, S. A., additional, Elbaz, D., additional, Galametz, M., additional, Galliano, F., additional, Gear, W. K., additional, Glenn, J., additional, Gomez, H. L., additional, Griffin, M., additional, Hony, S., additional, Isaak, K. G., additional, Levenson, L. R., additional, Lu, N., additional, Madden, S., additional, O'Halloran, B., additional, Okumura, K., additional, Oliver, S., additional, Page, M. J., additional, Panuzzo, P., additional, Papageorgiou, A., additional, Parkin, T. J., additional, Perez-Fournon, I., additional, Rangwala, N., additional, Rigby, E. E., additional, Roussel, H., additional, Rykala, A., additional, Sacchi, N., additional, Schulz, B., additional, Schirm, M. R. P., additional, Smith, M. W. L., additional, Spinoglio, L., additional, Stevens, J. A., additional, Sundar, S., additional, Symeonidis, M., additional, Trichas, M., additional, Vaccari, M., additional, Vigroux, L., additional, Wozniak, H., additional, Wright, G. S., additional, and Zeilinger, W. W., additional
Published: 2010
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26. Herschelphotometric observations of the nearby low metallicity irregular galaxy NGC 6822

Author: Galametz, M., primary, Madden, S. C., additional, Galliano, F., additional, Hony, S., additional, Sauvage, M., additional, Pohlen, M., additional, Bendo, G. J., additional, Auld, R., additional, Baes, M., additional, Barlow, M. J., additional, Bock, J. J., additional, Boselli, A., additional, Bradford, M., additional, Buat, V., additional, Castro-Rodríguez, N., additional, Chanial, P., additional, Charlot, S., additional, Ciesla, L., additional, Clements, D. L., additional, Cooray, A., additional, Cormier, D., additional, Cortese, L., additional, Davies, J. I., additional, Dwek, E., additional, Eales, S. A., additional, Elbaz, D., additional, Gear, W. K., additional, Glenn, J., additional, Gomez, H. L., additional, Griffin, M., additional, Isaak, K. G., additional, Levenson, L. R., additional, Lu, N., additional, O'Halloran, B., additional, Okumura, K., additional, Oliver, S., additional, Page, M. J., additional, Panuzzo, P., additional, Papageorgiou, A., additional, Parkin, T. J., additional, Pérez-Fournon, I., additional, Rangwala, N., additional, Rigby, E. E., additional, Roussel, H., additional, Rykala, A., additional, Sacchi, N., additional, Schulz, B., additional, Schirm, M. R. P., additional, Smith, M. W. L., additional, Spinoglio, L., additional, Stevens, J. A., additional, Sundar, S., additional, Symeonidis, M., additional, Trichas, M., additional, Vaccari, M., additional, Vigroux, L., additional, Wilson, C. D., additional, Wozniak, H., additional, Wright, G. S., additional, and Zeilinger, W. W., additional
Published: 2010
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27. HerMES: The submillimeter spectral energy distributions ofHerschel/SPIRE-detected galaxies

Author: Schulz, B., primary, Pearson, C. P., additional, Clements, D. L., additional, Altieri, B., additional, Amblard, A., additional, Arumugam, V., additional, Auld, R., additional, Aussel, H., additional, Babbedge, T., additional, Blain, A., additional, Bock, J., additional, Boselli, A., additional, Buat, V., additional, Burgarella, D., additional, Castro-Rodríguez, N., additional, Cava, A., additional, Chanial, P., additional, Conley, A., additional, Conversi, L., additional, Cooray, A., additional, Dowell, C. D., additional, Dwek, E., additional, Eales, S., additional, Elbaz, D., additional, Fox, M., additional, Franceschini, A., additional, Gear, W., additional, Giovannoli, E., additional, Glenn, J., additional, Griffin, M., additional, Halpern, M., additional, Hatziminaoglou, E., additional, Ibar, E., additional, Isaak, K., additional, Ivison, R. J., additional, Lagache, G., additional, Levenson, L., additional, Lu, N., additional, Madden, S., additional, Maffei, B., additional, Mainetti, G., additional, Marchetti, L., additional, Marsden, G., additional, Mortier, A. M. J., additional, Nguyen, H. T., additional, O'Halloran, B., additional, Oliver, S. J., additional, Omont, A., additional, Page, M. J., additional, Panuzzo, P., additional, Papageorgiou, A., additional, Pérez-Fournon, I., additional, Pohlen, M., additional, Rangwala, N., additional, Rawlings, J. I., additional, Raymond, G., additional, Rigopoulou, D., additional, Rizzo, D., additional, Roseboom, I. G., additional, Rowan-Robinson, M., additional, Sánchez Portal, M., additional, Scott, D., additional, Seymour, N., additional, Shupe, D. L., additional, Smith, A. J., additional, Stevens, J. A., additional, Symeonidis, M., additional, Trichas, M., additional, Tugwell, K. E., additional, Vaccari, M., additional, Valiante, E., additional, Valtchanov, I., additional, Vigroux, L., additional, Wang, L., additional, Ward, R., additional, Wright, G., additional, Xu, C. K., additional, and Zemcov, M., additional
Published: 2010
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28. Radial distribution of gas and dust in spiral galaxies

Author: Pohlen, M., primary, Cortese, L., additional, Smith, M. W. L., additional, Eales, S. A., additional, Boselli, A., additional, Bendo, G. J., additional, Gomez, H. L., additional, Papageorgiou, A., additional, Auld, R., additional, Baes, M., additional, Bock, J. J., additional, Bradford, M., additional, Buat, V., additional, Castro-Rodriguez, N., additional, Chanial, P., additional, Charlot, S., additional, Ciesla, L., additional, Clements, D. L., additional, Cooray, A., additional, Cormier, D., additional, Dwek, E., additional, Elbaz, D., additional, Galametz, M., additional, Galliano, F., additional, Gear, W. K., additional, Glenn, J., additional, Griffin, M., additional, Hony, S., additional, Isaak, K. G., additional, Levenson, L. R., additional, Lu, N., additional, Madden, S., additional, O'Halloran, B., additional, Okumura, K., additional, Oliver, S., additional, Page, M. J., additional, Panuzzo, P., additional, Parkin, T. J., additional, Perez-Fournon, I., additional, Rangwala, N., additional, Rigby, E. E., additional, Roussel, H., additional, Rykala, A., additional, Sacchi, N., additional, Sauvage, M., additional, Schulz, B., additional, Schirm, M. R. P., additional, Spinoglio, L., additional, Stevens, J. A., additional, Srinivasan, S., additional, Symeonidis, M., additional, Trichas, M., additional, Vaccari, M., additional, Vigroux, L., additional, Wilson, C. D., additional, Wozniak, H., additional, Wright, G. S., additional, and Zeilinger, W. W., additional
Published: 2010
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29. Star formation in AGN hosts in GOODS-N

Author: Shao, L., primary, Lutz, D., additional, Nordon, R., additional, Maiolino, R., additional, Alexander, D. M., additional, Altieri, B., additional, Andreani, P., additional, Aussel, H., additional, Bauer, F. E., additional, Berta, S., additional, Bongiovanni, A., additional, Brandt, W. N., additional, Brusa, M., additional, Cava, A., additional, Cepa, J., additional, Cimatti, A., additional, Daddi, E., additional, Dominguez-Sanchez, H., additional, Elbaz, D., additional, Förster Schreiber, N. M., additional, Geis, N., additional, Genzel, R., additional, Grazian, A., additional, Gruppioni, C., additional, Magdis, G., additional, Magnelli, B., additional, Mainieri, V., additional, Pérez García, A. M., additional, Poglitsch, A., additional, Popesso, P., additional, Pozzi, F., additional, Riguccini, L., additional, Rodighiero, G., additional, Rovilos, E., additional, Saintonge, A., additional, Salvato, M., additional, Sanchez Portal, M., additional, Santini, P., additional, Sturm, E., additional, Tacconi, L. J., additional, Valtchanov, I., additional, Wetzstein, M., additional, and Wieprecht, E., additional
Published: 2010
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30. The dust morphology of the elliptical Galaxy M 86 with SPIRE

Author: Gomez, H. L., primary, Baes, M., additional, Cortese, L., additional, Smith, M. W. L., additional, Boselli, A., additional, Ciesla, L., additional, Bendo, G. J., additional, Pohlen, M., additional, di Serego Alighieri, S., additional, Auld, R., additional, Barlow, M. J., additional, Bock, J. J., additional, Bradford, M., additional, Buat, V., additional, Castro-Rodriguez, N., additional, Chanial, P., additional, Charlot, S., additional, Clements, D. L., additional, Cooray, A., additional, Cormier, D., additional, Davies, J. I., additional, Dwek, E., additional, Eales, S., additional, Elbaz, D., additional, Galametz, M., additional, Galliano, F., additional, Gear, W. K., additional, Glenn, J., additional, Griffin, M., additional, Hony, S., additional, Isaak, K. G., additional, Levenson, L. R., additional, Lu, N., additional, Madden, S., additional, O'Halloran, B., additional, Okumura, K., additional, Oliver, S., additional, Page, M. J., additional, Panuzzo, P., additional, Papageorgiou, A., additional, Parkin, T. J., additional, Perez-Fournon, I., additional, Rangwala, N., additional, Rigby, E. E., additional, Roussel, H., additional, Rykala, A., additional, Sacchi, N., additional, Sauvage, M., additional, Schirm, M. R. P., additional, Schulz, B., additional, Spinoglio, L., additional, Srinivasan, S., additional, Stevens, J. A., additional, Symeonidis, M., additional, Trichas, M., additional, Vaccari, M., additional, Vigroux, L., additional, Wilson, C. D., additional, Wozniak, H., additional, Wright, G. S., additional, and Zeilinger, W. W., additional
Published: 2010
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31. The central region of spiral galaxies as seen byHerschel

Author: Sauvage, M., primary, Sacchi, N., additional, Bendo, G. J., additional, Boselli, A., additional, Pohlen, M., additional, Wilson, C. D., additional, Auld, R., additional, Baes, M., additional, Barlow, M. J., additional, Bock, J. J., additional, Bradford, M., additional, Buat, V., additional, Castro-Rodriguez, N., additional, Chanial, P., additional, Charlot, S., additional, Ciesla, L., additional, Clements, D. L., additional, Cooray, A., additional, Cormier, D., additional, Cortese, L., additional, Davies, J. I., additional, Dwek, E., additional, Eales, S. A., additional, Elbaz, D., additional, Galametz, M., additional, Galliano, F., additional, Gear, W. K., additional, Glenn, J., additional, Gomez, H. L., additional, Griffin, M., additional, Hony, S., additional, Isaak, K. G., additional, Levenson, L. R., additional, Lu, N., additional, Madden, S. C., additional, O'Halloran, B., additional, Okumura, K., additional, Oliver, S., additional, Page, M. J., additional, Panuzzo, P., additional, Papageorgiou, A., additional, Parkin, T. J., additional, Perez-Fournon, I., additional, Rangwala, N., additional, Rigby, E. E., additional, Roussel, H., additional, Rykala, A., additional, Schulz, B., additional, Schirm, M. R. P., additional, Smith, M. W. L., additional, Spinoglio, L., additional, Stevens, J. A., additional, Srinivasan, S., additional, Symeonidis, M., additional, Trichas, M., additional, Vaccari, M., additional, Vigroux, L., additional, Wozniak, H., additional, Wright, G. S., additional, and Zeilinger, W. W., additional
Published: 2010
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32. FIR colours and SEDs of nearby galaxies observed withHerschel

Author: Boselli, A., primary, Ciesla, L., additional, Buat, V., additional, Cortese, L., additional, Auld, R., additional, Baes, M., additional, Bendo, G. J., additional, Bianchi, S., additional, Bock, J., additional, Bomans, D. J., additional, Bradford, M., additional, Castro-Rodriguez, N., additional, Chanial, P., additional, Charlot, S., additional, Clemens, M., additional, Clements, D., additional, Corbelli, E., additional, Cooray, A., additional, Cormier, D., additional, Dariush, A., additional, Davies, J., additional, De Looze, I., additional, di Serego Alighieri, S., additional, Dwek, E., additional, Eales, S., additional, Elbaz, D., additional, Fadda, D., additional, Fritz, J., additional, Galametz, M., additional, Galliano, F., additional, Garcia-Appadoo, D. A., additional, Gavazzi, G., additional, Gear, W., additional, Giovanardi, C., additional, Glenn, J., additional, Gomez, H., additional, Griffin, M., additional, Grossi, M., additional, Hony, S., additional, Hughes, T. M., additional, Hunt, L., additional, Isaak, K., additional, Jones, A., additional, Levenson, L., additional, Lu, N., additional, Madden, S. C., additional, O'Halloran, B., additional, Okumura, K., additional, Oliver, S., additional, Page, M., additional, Panuzzo, P., additional, Papageorgiou, A., additional, Parkin, T., additional, Perez-Fournon, I., additional, Pierini, D., additional, Pohlen, M., additional, Rangwala, N., additional, Rigby, E., additional, Roussel, H., additional, Rykala, A., additional, Sabatini, S., additional, Sacchi, N., additional, Sauvage, M., additional, Schulz, B., additional, Schirm, M., additional, Smith, M. W. L., additional, Spinoglio, L., additional, Stevens, J., additional, Sundar, S., additional, Symeonidis, M., additional, Trichas, M., additional, Vaccari, M., additional, Verstappen, J., additional, Vigroux, L., additional, Vlahakis, C., additional, Wilson, C., additional, Wozniak, H., additional, Wright, G., additional, Xilouris, E. M., additional, Zeilinger, W., additional, and Zibetti, S., additional
Published: 2010
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33. First results from HerMES on the evolution of the submillimetre luminosity function

Author: Eales, S. A., primary, Raymond, G., additional, Roseboom, I. G., additional, Altieri, B., additional, Amblard, A., additional, Arumugam, V., additional, Auld, R., additional, Aussel, H., additional, Babbedge, T., additional, Blain, A., additional, Bock, J., additional, Boselli, A., additional, Brisbin, D., additional, Buat, V., additional, Burgarella, D., additional, Castro-Rodríguez, N., additional, Cava, A., additional, Chanial, P., additional, Clements, D. L., additional, Conley, A., additional, Conversi, L., additional, Cooray, A., additional, Dowell, C. D., additional, Dwek, E., additional, Dye, S., additional, Elbaz, D., additional, Farrah, D., additional, Fox, M., additional, Franceschini, A., additional, Gear, W., additional, Glenn, J., additional, González Solares, E. A., additional, Griffin, M., additional, Harwit, M., additional, Hatziminaoglou, E., additional, Huang, J., additional, Ibar, E., additional, Isaak, K., additional, Ivison, R. J., additional, Lagache, G., additional, Levenson, L., additional, Lonsdale, C. J., additional, Lu, N., additional, Madden, S., additional, Maffei, B., additional, Mainetti, G., additional, Marchetti, L., additional, Morrison, G. E., additional, Mortier, A. M. J., additional, Nguyen, H. T., additional, O'Halloran, B., additional, Oliver, S. J., additional, Omont, A., additional, Owen, F. N., additional, Page, M. J., additional, Pannella, M., additional, Panuzzo, P., additional, Papageorgiou, A., additional, Pearson, C. P., additional, Pérez-Fournon, I., additional, Pohlen, M., additional, Rawlings, J. I., additional, Rigopoulou, D., additional, Rizzo, D., additional, Rowan-Robinson, M., additional, Sánchez Portal, M., additional, Schulz, B., additional, Scott, D., additional, Seymour, N., additional, Shupe, D. L., additional, Smith, A. J., additional, Stevens, J. A., additional, Strazzullo, V., additional, Symeonidis, M., additional, Trichas, M., additional, Tugwell, K. E., additional, Vaccari, M., additional, Valtchanov, I., additional, Vigroux, L., additional, Wang, L., additional, Ward, R., additional, Wright, G., additional, Xu, C. K., additional, and Zemcov, M., additional
Published: 2010
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34. Mapping the interstellar medium in galaxies withHerschel/SPIRE

Author: Eales, S. A., primary, Smith, M. W. L., additional, Wilson, C. D., additional, Bendo, G. J., additional, Cortese, L., additional, Pohlen, M., additional, Boselli, A., additional, Gomez, H. L., additional, Auld, R., additional, Baes, M., additional, Barlow, M. J., additional, Bock, J. J., additional, Bradford, M., additional, Buat, V., additional, Castro-Rodríguez, N., additional, Chanial, P., additional, Charlot, S., additional, Ciesla, L., additional, Clements, D. L., additional, Cooray, A., additional, Cormier, D., additional, Davies, J. I., additional, Dwek, E., additional, Elbaz, D., additional, Galametz, M., additional, Galliano, F., additional, Gear, W. K., additional, Glenn, J., additional, Griffin, M., additional, Hony, S., additional, Isaak, K. G., additional, Levenson, L. R., additional, Lu, N., additional, Madden, S., additional, O'Halloran, B., additional, Okumura, K., additional, Oliver, S., additional, Page, M. J., additional, Panuzzo, P., additional, Papageorgiou, A., additional, Parkin, T. J., additional, Pérez-Fournon, I., additional, Rangwala, N., additional, Rigby, E. E., additional, Roussel, H., additional, Rykala, A., additional, Sacchi, N., additional, Sauvage, M., additional, Schulz, B., additional, Schirm, M. R. P., additional, Spinoglio, L., additional, Srinivasan, S., additional, Stevens, J. A., additional, Symeonidis, M., additional, Trichas, M., additional, Vaccari, M., additional, Vigroux, L., additional, Wozniak, H., additional, Wright, G. S., additional, and Zeilinger, W. W., additional
Published: 2010
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35. Herschelphotometric observations of the low metallicity dwarf galaxy NGC 1705

Author: O'Halloran, B., primary, Galametz, M., additional, Madden, S. C., additional, Auld, R., additional, Baes, M., additional, Barlow, M. J., additional, Bendo, G. J., additional, Bock, J. J., additional, Boselli, A., additional, Bradford, M., additional, Buat, V., additional, Castro-Rodriguez, N., additional, Chanial, P., additional, Charlot, S., additional, Ciesla, L., additional, Clements, D. L., additional, Cormier, D., additional, Cooray, A., additional, Cortese, L., additional, Davies, J. I., additional, Dwek, E., additional, Eales, S. A., additional, Elbaz, D., additional, Galliano, F., additional, Gear, W. K., additional, Glenn, J., additional, Gomez, H. L., additional, Hony, S., additional, Isaak, K. G., additional, Levenson, L. R., additional, Lu, N., additional, Okumura, K., additional, Oliver, S., additional, Page, M. J., additional, Panuzzo, P., additional, Papageorgiou, A., additional, Parkin, T. J., additional, Perez-Fournon, I., additional, Pohlen, M., additional, Rangwala, N., additional, Rigby, E. E., additional, Roussel, H., additional, Rykala, A., additional, Sacchi, N., additional, Sauvage, M., additional, Schulz, B., additional, Schirm, M. R. P., additional, Smith, M. W. L., additional, Spinoglio, L., additional, Srinivasan, S., additional, Stevens, J. A., additional, Symeonidis, M., additional, Trichas, M., additional, Vaccari, M., additional, Vigroux, L., additional, Wilson, C. D., additional, Wozniak, H., additional, Wright, G. S., additional, and Zeilinger, W. W., additional
Published: 2010
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36. HerMES: Halo occupation number and bias properties of dusty galaxies from angular clustering measurements

Author: Cooray, A., primary, Amblard, A., additional, Wang, L., additional, Arumugam, V., additional, Auld, R., additional, Aussel, H., additional, Babbedge, T., additional, Blain, A., additional, Bock, J., additional, Boselli, A., additional, Buat, V., additional, Burgarella, D., additional, Castro-Rodriguez, N., additional, Cava, A., additional, Chanial, P., additional, Clements, D. L., additional, Conley, A., additional, Conversi, L., additional, Dowell, C. D., additional, Dwek, E., additional, Eales, S., additional, Elbaz, D., additional, Farrah, D., additional, Fox, M., additional, Franceschini, A., additional, Gear, W., additional, Glenn, J., additional, Griffin, M., additional, Halpern, M., additional, Hatziminaoglou, E., additional, Ibar, E., additional, Isaak, K., additional, Ivison, R. J., additional, Khostovan, A. A., additional, Lagache, G., additional, Levenson, L., additional, Lu, N., additional, Madden, S., additional, Maffei, B., additional, Mainetti, G., additional, Marchetti, L., additional, Marsden, G., additional, Mitchell-Wynne, K., additional, Mortier, A. M. J., additional, Nguyen, H. T., additional, O'Halloran, B., additional, Oliver, S. J., additional, Omont, A., additional, Page, M. J., additional, Panuzzo, P., additional, Papageorgiou, A., additional, Pearson, C. P., additional, Perez Fournon, I., additional, Pohlen, M., additional, Rawlings, J. I., additional, Raymond, G., additional, Rigopoulou, D., additional, Rizzo, D., additional, Roseboom, I. G., additional, Rowan-Robinson, M., additional, Schulz, B., additional, Scott, D., additional, Serra, P., additional, Seymour, N., additional, Shupe, D. L., additional, Smith, A. J., additional, Stevens, J. A., additional, Symeonidis, M., additional, Trichas, M., additional, Tugwell, K. E., additional, Vaccari, M., additional, Valtchanov, I., additional, Vieira, J. D., additional, Vigroux, L., additional, Ward, R., additional, Wright, G., additional, Xu, C. K., additional, and Zemcov, M., additional
Published: 2010
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37. Herscheldeep far-infrared counts through Abell 2218 cluster-lens

Author: Altieri, B., primary, Berta, S., additional, Lutz, D., additional, Kneib, J.-P., additional, Metcalfe, L., additional, Andreani, P., additional, Aussel, H., additional, Bongiovanni, A., additional, Cava, A., additional, Cepa, J., additional, Ciesla, L., additional, Cimatti, A., additional, Daddi, E., additional, Dominguez, H., additional, Elbaz, D., additional, Förster Schreiber, N. M., additional, Genzel, R., additional, Gruppioni, C., additional, Magnelli, B., additional, Magdis, G., additional, Maiolino, R., additional, Nordon, R., additional, Pérez García, A. M., additional, Poglitsch, A., additional, Popesso, P., additional, Pozzi, F., additional, Richard, J., additional, Riguccini, L., additional, Rodighiero, G., additional, Saintonge, A., additional, Santini, P., additional, Sanchez-Portal, M., additional, Shao, L., additional, Sturm, E., additional, Tacconi, L. J., additional, Valtchanov, I., additional, Wetzstein, M., additional, and Wieprecht, E., additional
Published: 2010
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38. PEP: FirstHerschelprobe of dusty galaxy evolution up to z ~ 3

Author: Gruppioni, C., primary, Pozzi, F., additional, Andreani, P., additional, Rodighiero, G., additional, Cimatti, A., additional, Altieri, B., additional, Aussel, H., additional, Berta, S., additional, Bongiovanni, A., additional, Brisbin, D., additional, Cava, A., additional, Cepa, J., additional, Daddi, E., additional, Dominguez-Sanchez, H., additional, Elbaz, D., additional, Förster Schreiber, N., additional, Genzel, R., additional, Le Floc'h, E., additional, Lutz, D., additional, Magdis, G., additional, Magliocchetti, M., additional, Magnelli, B., additional, Maiolino, R., additional, Nordon, R., additional, Peréz-García, A. M., additional, Poglitsch, A., additional, Popesso, P., additional, Riguccini, L., additional, Saintonge, A., additional, Sanchez-Portal, M., additional, Santini, P., additional, Shao, L., additional, Sturm, E., additional, Tacconi, L., additional, and Valtchanov, I., additional
Published: 2010
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39. Far-infrared properties of submillimeter and optically faint radio galaxies

Author: Magnelli, B., primary, Lutz, D., additional, Berta, S., additional, Altieri, B., additional, Andreani, P., additional, Aussel, H., additional, Castañeda, H., additional, Cava, A., additional, Cepa, J., additional, Cimatti, A., additional, Daddi, E., additional, Dannerbauer, H., additional, Dominguez, H., additional, Elbaz, D., additional, Förster Schreiber, N., additional, Genzel, R., additional, Grazian, A., additional, Gruppioni, C., additional, Magdis, G., additional, Maiolino, R., additional, Nordon, R., additional, Pérez Fournon, I., additional, Pérez García, I., additional, Poglitsch, A., additional, Popesso, P., additional, Pozzi, F., additional, Riguccini, L., additional, Rodighiero, G., additional, Saintonge, A., additional, Santini, P., additional, Sanchez-Portal, M., additional, Shao, L., additional, Sturm, E., additional, Tacconi, L., additional, Valtchanov, I., additional, Wieprecht, E., additional, and Wiezorrek, E., additional
Published: 2010
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40. Herschel-SPIRE observations of the disturbed galaxy NGC 4438

Author: Cortese, L., primary, Bendo, G. J., additional, Boselli, A., additional, Davies, J. I., additional, Gomez, H. L., additional, Pohlen, M., additional, Auld, R., additional, Baes, M., additional, Bock, J. J., additional, Bradford, M., additional, Buat, V., additional, Castro-Rodriguez, N., additional, Chanial, P., additional, Charlot, S., additional, Ciesla, L., additional, Clements, D. L., additional, Cooray, A., additional, Cormier, D., additional, Dwek, E., additional, Eales, S. A., additional, Elbaz, D., additional, Galametz, M., additional, Galliano, F., additional, Gear, W. K., additional, Glenn, J., additional, Griffin, M., additional, Hony, S., additional, Isaak, K. G., additional, Levenson, L. R., additional, Lu, N., additional, Madden, S., additional, O'Halloran, B., additional, Okumura, K., additional, Oliver, S., additional, Page, M. J., additional, Panuzzo, P., additional, Papageorgiou, A., additional, Parkin, T. J., additional, Perez-Fournon, I., additional, Rangwala, N., additional, Rigby, E. E., additional, Roussel, H., additional, Rykala, A., additional, Sacchi, N., additional, Sauvage, M., additional, Schulz, B., additional, Schirm, M. R. P., additional, Smith, M. W. L., additional, Spinoglio, L., additional, Stevens, J. A., additional, Srinivasan, S., additional, Symeonidis, M., additional, Trichas, M., additional, Vaccari, M., additional, Vigroux, L., additional, Wilson, C. D., additional, Wozniak, H., additional, Wright, G. S., additional, and Zeilinger, W. W., additional
Published: 2010
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41. The firstHerschelview of the mass-SFR link in high-zgalaxies

Author: Rodighiero, G., primary, Cimatti, A., additional, Gruppioni, C., additional, Popesso, P., additional, Andreani, P., additional, Altieri, B., additional, Aussel, H., additional, Berta, S., additional, Bongiovanni, A., additional, Brisbin, D., additional, Cava, A., additional, Cepa, J., additional, Daddi, E., additional, Dominguez-Sanchez, H., additional, Elbaz, D., additional, Fontana, A., additional, Förster Schreiber, N., additional, Franceschini, A., additional, Genzel, R., additional, Grazian, A., additional, Lutz, D., additional, Magdis, G., additional, Magliocchetti, M., additional, Magnelli, B., additional, Maiolino, R., additional, Mancini, C., additional, Nordon, R., additional, Perez Garcia, A. M., additional, Poglitsch, A., additional, Santini, P., additional, Sanchez-Portal, M., additional, Pozzi, F., additional, Riguccini, L., additional, Saintonge, A., additional, Shao, L., additional, Sturm, E., additional, Tacconi, L., additional, Valtchanov, I., additional, Wetzstein, M., additional, and Wieprecht, E., additional
Published: 2010
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42. TheHerschelSpace Observatory view of dust in M81

Author: Marc Sauvage, N. Lu, Pierre Chanial, Walter Kieran Gear, L. Vigroux, Pasquale Panuzzo, M. Symeonidis, Herve Wozniak, Diane Cormier, George J. Bendo, B. O'Halloran, James J. Bock, M. J. Barlow, Werner W. Zeilinger, Jamie Stevens, Mattia Vaccari, E. E. Rigby, Stephane Charlot, Helene Roussel, David L. Clements, Luca Cortese, Naseem Rangwala, T. J. Parkin, Michael Pohlen, N. Castro-Rodriguez, Matthew Joseph Griffin, Matthew Smith, Sacha Hony, S. Sundar, Maud Galametz, Alessandro Boselli, A. Cooray, Gillian S. Wright, Christine D. Wilson, M. Bradford, Haley Louise Gomez, Stephen Anthony Eales, Koryo Okumura, Andreas Papageorgiou, Eli Dwek, Maximilien R. P. Schirm, Laure Ciesla, Kate Gudrun Isaak, Maarten Baes, N. Sacchi, Suzanne C. Madden, L. R. Levenson, Benjamin L. Schulz, Markos Trichas, Seb Oliver, V. Buat, Ismael Perez-Fournon, Mat Page, Jason Glenn, Robbie Richard Auld, D. Elbaz, Frédéric Galliano, L. Spinoglio, A. Rykala, Jonathan Ivor Davies, Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Institut d'Astrophysique de Paris (IAP), Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Observatoire astronomique de Strasbourg (ObAS), and Université de Strasbourg (UNISTRA)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)
Subjects: galaxies: spiral, Cosmology and Nongalactic Astrophysics (astro-ph.CO), Active galactic nucleus, TELESCOPE, H-ALPHA, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, THINGS, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, STAR-FORMATION RATES, individual: M81 [galaxies], galaxies: individual: M81, Bulge, Astrophysics::Solar and Stellar Astrophysics, Surface brightness, FIELD, Astrophysics::Galaxy Astrophysics, QB, Physics, Spiral galaxy, [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph], ISM [galaxies], Spectral density, Astronomy and Astrophysics, Radius, Space observatory, GALAXIES, SPITZER, Stars, spiral [galaxies], Physics and Astronomy, [SDU]Sciences of the Universe [physics], Space and Planetary Science, Astrophysics::Earth and Planetary Astrophysics, EMISSION, galaxies: ISM, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: We use Herschel Space Observatory data to place observational constraints on the peak and Rayleigh-Jeans slope of dust emission observed at 70-500 microns in the nearby spiral galaxy M81. We find that the ratios of wave bands between 160 and 500 microns are primarily dependent on radius but that the ratio of 70 to 160 micron emission shows no clear dependence on surface brightness or radius. These results along with analyses of the spectral energy distributions imply that the 160-500 micron emission traces 15-30 K dust heated by evolved stars in the bulge and disc whereas the 70 micron emission includes dust heated by the active galactic nucleus and young stars in star forming regions., Accepted for A & A Herschel special issue
Published: 2010
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43. Probing the molecular interstellar medium of M82 withHerschel-SPIRE spectroscopy

Author: B. O'Halloran, Jonathan Ivor Davies, M. Bradford, Naseem Rangwala, Marc Sauvage, Koryo Okumura, N. Lu, Pierre Chanial, L. Spinoglio, Sundar Srinivasan, Laure Ciesla, N. Castro-Rodriguez, Sacha Hony, Walter Kieran Gear, Gillian S. Wright, Mat Page, N. Sacchi, James J. Bock, M. Symeonidis, A. Cooray, V. Buat, Stephane Charlot, Kate Gudrun Isaak, Diane Cormier, Pasquale Panuzzo, T. Fulton, Jason Glenn, E. E. Rigby, Maximilien R. P. Schirm, George J. Bendo, Frédéric Galliano, M. J. Barlow, Michael Pohlen, Edward Polehampton, Haley Louise Gomez, Ismael Perez-Fournon, T. J. Parkin, B. Swinyard, Werner W. Zeilinger, Seb Oliver, Stephen Anthony Eales, Markos Trichas, Robbie Richard Auld, D. Elbaz, Matthew Smith, Alessandro Boselli, Maud Galametz, L. Vigroux, Helene Roussel, David L. Clements, Luca Cortese, Herve Wozniak, Eli Dwek, A. Rykala, Christine D. Wilson, L. R. Levenson, Benjamin L. Schulz, Jamie Stevens, Maarten Baes, Andreas Papageorgiou, Mattia Vaccari, Matthew Joseph Griffin, Suzanne C. Madden, Laboratoire d'Astrophysique de Marseille (LAM), and Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)
Subjects: Cosmology and Nongalactic Astrophysics (astro-ph.CO), Astrophysics::High Energy Astrophysical Phenomena, Fourier transform spectrometers, FOS: Physical sciences, galaxies [submillimeter], LINE, Flux, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, STARBURST GALAXY M82, 01 natural sciences, 0103 physical sciences, Spectroscopy, TEMPERATURE, NUCLEUS, 010303 astronomy & astrophysics, molecules [ISM], Astrophysics::Galaxy Astrophysics, QB, Physics, ISM [galaxies], [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph], starburst [galaxies], 010308 nuclear & particles physics, Turbulence, CLOUDS, Astronomy and Astrophysics, THERMAL BALANCE, Dissipation, Galaxy, CO, Interstellar medium, Spire, Physics and Astronomy, GAS, 13. Climate action, Space and Planetary Science, TURBULENCE, individual: M82 [galaxies], EMISSION, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: We present the observations of the starburst galaxy M82 taken with the Herschel SPIRE Fourier Transform Spectrometer. The spectrum (194-671 {\mu}m) shows a prominent CO rotational ladder from J = 4-3 to 13-12 emitted by the central region of M82. The fundamental properties of the gas are well constrained by the high J lines observed for the first time. Radiative transfer modeling of these high-S/N 12CO and 13CO lines strongly indicates a very warm molecular gas component at ~500 K and pressure of ~3x10^6 K cm^-3, in good agreement with the H_2 rotational lines measurements from Spitzer and ISO. We suggest that this warm gas is heated by dissipation of turbulence in the interstellar medium (ISM) rather than X-rays or UV flux from the straburst. This paper illustrates the promise of the SPIRE FTS for the study of the ISM of nearby galaxies., Comment: 5 pages, 4 figures, Accepted for publication on the A&A Herschel Special Issue
Published: 2010
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44. Radial distribution of gas and dust in spiral galaxies

Author: M. Pohlen, L. Cortese, M. W. L. Smith, S. A. Eales, A. Boselli, G. J. Bendo, H. L. Gomez, A. Papageorgiou, R. Auld, M. Baes, J. J. Bock, M. Bradford, V. Buat, N. Castro-Rodriguez, P. Chanial, S. Charlot, L. Ciesla, D. L. Clements, A. Cooray, D. Cormier, E. Dwek, D. Elbaz, M. Galametz, F. Galliano, W. K. Gear, J. Glenn, M. Griffin, S. Hony, K. G. Isaak, L. R. Levenson, N. Lu, S. Madden, B. O'Halloran, K. Okumura, S. Oliver, M. J. Page, P. Panuzzo, T. J. Parkin, I. Perez-Fournon, N. Rangwala, E. E. Rigby, H. Roussel, A. Rykala, N. Sacchi, M. Sauvage, B. Schulz, M. R. P. Schirm, L. Spinoglio, J. A. Stevens, S. Srinivasan, M. Symeonidis, M. Trichas, M. Vaccari, L. Vigroux, C. D. Wilson, H. Wozniak, G. S. Wright, W. W. Zeilinger, Laboratoire d'Astrophysique de Marseille (LAM), and Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)
Subjects: Metallicity, nuclei [galaxies], galaxies [submillimeter], Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, Spatial distribution, galaxies [infrared], 01 natural sciences, law.invention, law, 0103 physical sciences, fundamental parameters [galaxies], Astrophysics::Solar and Stellar Astrophysics, DUST EMISSION, Variation (astronomy), 010303 astronomy & astrophysics, Astrophysics::Galaxy Astrophysics, Physics, Spiral galaxy, [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph], 010308 nuclear & particles physics, Astronomy and Astrophysics, Radius, Photometer, Virgo Cluster, Galaxy, spiral [galaxies], Physics and Astronomy, Space and Planetary Science, Astrophysics::Earth and Planetary Astrophysics
Abstract: With appropriate spatial resolution, images of spiral galaxies in thermal infrared (similar to 10 mu m and beyond) often reveal a bright central component, distinct from the stellar bulge, superimposed on a disk with prominent spiral arms. ISO and Spitzer studies have shown that much of the scatter in the mid-infrared colors of spiral galaxies is related to changes in the relative importance of these two components, rather than to other modifications, such as the morphological type or star formation rate, that affect the properties of the galaxy as a whole. With the Herschel imaging capability from 70 to 500 mu m, we revisit this two-component approach at longer wavelengths, to see if it still provides a working description of the brightness distribution of galaxies, and to determine its implications on the interpretation of global far-infrared properties of galaxies. We quantify the luminosity of the central component by both a decomposition of the radial surface brightness profile and a direct extraction in 2D. We find the central component contribution is variable within the three galaxies in our sample, possibly connected more directly to the presence of a bar than to the morphological type. The central component's relative contribution is at its maximum in the mid-infrared range and drops around 160 mu m to reach a constant value beyond 200 mu m. The central component contains a greater fraction of hot dust than the disk component, and while the colors of the central components are scattered, colors of the disk components are more homogenous from one galaxy to the next.
Published: 2010
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45. Quasar induced galaxy formation: a new paradigm?

Author: Elbaz, D., Jahnke, K., Pantin, E., Le Borgne, D., Letawe, G., Elbaz, D., Jahnke, K., Pantin, E., Le Borgne, D., and Letawe, G.
Abstract: Aims. We discuss observational evidence that quasars play a key role in the formation of galaxies, starting from the detailed study of the quasar HE0450-2958 and extending the discussion to a series of converging evidence that radio jets may trigger galaxy formation.
Published: 2009
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46. Cosmic star-formation history from a non-parametric inversion of infrared galaxy counts*

Author: Le Borgne, D., Elbaz, D., Ocvirk, P., Pichon, C., Le Borgne, D., Elbaz, D., Ocvirk, P., and Pichon, C.
Abstract: Aims. This paper aims at providing new conservative constraints on the cosmic star-formation (SF) history from the empirical modeling of recent observations in the mid and far infrared.
Published: 2009
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47. Observations and modeling of a clumpy galaxy at z= 1.6*

Author: Bournaud, F., Daddi, E., Elmegreen, B. G., Elmegreen, D. M., Nesvadba, N., Vanzella, E., Di Matteo, P., Le Tiran, L., Lehnert, M., Elbaz, D., Bournaud, F., Daddi, E., Elmegreen, B. G., Elmegreen, D. M., Nesvadba, N., Vanzella, E., Di Matteo, P., Le Tiran, L., Lehnert, M., and Elbaz, D.
Abstract: We investigate the properties of a clump-cluster galaxy at redshift 1.57. In optical observations, the morphology of this galaxy is dominated by eight star-forming clumps, and its photometric properties are typical of most clump-cluster and chain galaxies. Its complex asymmetrical morphology has led to the suggestion that this system is a group merger of several initially separate proto-galaxies. We performed Hαintegral field spectroscopy of this system using SINFONI on VLT UT4. These observations reveal a large-scale velocity gradient throughout the system, but with large local kinematic disturbances. Using a numerical model of gas-rich disk fragmentation, we find that clump interactions and migration can explain the observed disturbed rotation. On the other hand, the global rotation would not be expected for a multiply merging system. We also find that this system follows the relations of stellar mass versus metallicity, star formation rate, and size that are expected for a disk at this redshift. Furthermore, the galaxy exhibits a disk-like radial metallicity gradient. A formation scenario of internal disk fragmentation is therefore the most likely one. A red and metallic central concentration appears to be a bulge in this proto-spiral clumpy galaxy. A chain galaxy at redshift 2.07 in the same field also shows disk-like rotation. Such systems are likely progenitors of present-day bright spiral galaxies, which shape their exponential disks through clump migration and disruption, a process that in turn fuels their bulges. Our results show that disturbed morphologies and kinematics are not necessarily signs of galaxy mergers and interactions, but may instead be produced by the internal evolution of primordial disks.
Published: 2008
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48. The spatial clustering of mid-IR selected star forming galaxies at z~ 1 in the GOODS fields

Author: Gilli, R., Daddi, E., Chary, R., Dickinson, M., Elbaz, D., Giavalisco, M., Kitzbichler, M., Stern, D., Vanzella, E., Gilli, R., Daddi, E., Chary, R., Dickinson, M., Elbaz, D., Giavalisco, M., Kitzbichler, M., Stern, D., and Vanzella, E.
Abstract: We present the first spatial clustering measurements of $z\sim1$, 24 μm-selected, star forming galaxies in the Great Observatories Origins Deep Survey (GOODS). The sample under investigation includes 495 objects in GOODS-South and 811 objects in GOODS-North selected down to flux densities of $f_{24}>20\,\mu$Jy and $z_{\rm AB}<23.5$mag, for which spectroscopic redshifts are available. The median redshift, IR luminosity and star formation rate (SFR) of the sample are $z\sim 0.8$, $L_{\rm IR}\sim4.4\times10^{10}$$L_{\odot}$, and ${\it SFR}\sim 7.6\,M_{\odot}$yr-1, respectively. We measure the projected correlation function $w(r_{\rm p})$on scales of $r_{\rm p}=0.06{-}10\,h^{-1}$Mpc, from which we derive a best fit comoving correlation length of $r_0 = 4.0\pm0.4\,h^{-1}$Mpc and slope of $\gamma=1.5\pm0.1$for the whole $f_{24}>20\,\mu$Jy sample after combining the two fields. We find indications of a larger correlation length for objects of higher luminosity, with Luminous Infrared Galaxies (LIRGs, $L_{\rm IR}>10^{11}\,L_{\odot}$) reaching $r_0\sim 5.1\,h^{-1}$Mpc. This would imply that galaxies with larger SFRs are hosted in progressively more massive halos, reaching minimum halo masses of ~$3\times10^{12}~M_\odot$for LIRGs. We compare our measurements with the predictions from semi-analytic models based on the Millennium simulation. The variance in the models is used to estimate the errors in our GOODS clustering measurements, which are dominated by cosmic variance. The measurements from the two GOODS fields are found to be consistent within the errors. On scales of the GOODS fields, the real sources appear more strongly clustered than objects in the Millennium-simulation based catalogs, if the selection function is applied consistently. This suggests that star formation at $z\sim0.5{-}1$is being hosted in more massive halos and denser environments than currently predicted by galaxy formation models. Mid-IR selected sources appear also to be more strongly clustered than optically selected ones at similar redshifts in deep surveys like the DEEP2 Galaxy Redshift Survey and the VIMOS-VLT Deep Survey (VVDS), although the significance of this result is $\la$$3\sigma$when accounting for cosmic variance. We find that LIRGs at $z\sim1$are consistent with being the direct descendants of Lyman Break Galaxies and UV-selected galaxies at $z\sim2{-}3$, both in term of number densities and clustering properties, which would suggest long lasting star-formation activity in galaxies over cosmological timescales. The local descendants of $z\sim0.5{-}1$star forming galaxies are not luminous IR galaxies but are more likely to be normal, $L
Published: 2007
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49. The reversal of the star formation-density relation in the distant universe

Author: Elbaz, D., Daddi, E., Le Borgne, D., Dickinson, M., Alexander, D. M., Chary, R.-R., Starck, J.-L., Brandt, W. N., Kitzbichler, M., MacDonald, E., Nonino, M., Popesso, P., Stern, D., Vanzella, E., Elbaz, D., Daddi, E., Le Borgne, D., Dickinson, M., Alexander, D. M., Chary, R.-R., Starck, J.-L., Brandt, W. N., Kitzbichler, M., MacDonald, E., Nonino, M., Popesso, P., Stern, D., and Vanzella, E.
Abstract: Aims.We study the relationship between the local environment of galaxies and their star formation rate (SFR) in the Great Observatories Origins Deep Survey, GOODS, at $z\sim1$.
Published: 2007
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50. New spectroscopic redshifts from the CDFS and a test of the cosmological relevance of the GOODS-South field*

Author: Ravikumar, C. D., Puech, M., Flores, H., Proust, D., Hammer, F., Lehnert, M., Rawat, A., Amram, P., Balkowski, C., Burgarella, D., Cassata, P., Cesarsky, C., Cimatti, A., Combes, F., Daddi, E., Dannerbauer, H., di Serego Alighieri, S., Elbaz, D., Guiderdoni, B., Kembhavi, A., Liang, Y. C., Pozzetti, L., Vergani, D., Vernet, J., Wozniak, H., Zheng, X. Z., Ravikumar, C. D., Puech, M., Flores, H., Proust, D., Hammer, F., Lehnert, M., Rawat, A., Amram, P., Balkowski, C., Burgarella, D., Cassata, P., Cesarsky, C., Cimatti, A., Combes, F., Daddi, E., Dannerbauer, H., di Serego Alighieri, S., Elbaz, D., Guiderdoni, B., Kembhavi, A., Liang, Y. C., Pozzetti, L., Vergani, D., Vernet, J., Wozniak, H., and Zheng, X. Z.
Abstract: Context.This paper prepares a series of papers analysing the Intermediate MAss Galaxy Evolution Sequence (IMAGES) up to a redshift of one. Intermediate mass galaxies ($M_{\rm J} \leq -20.3$) are selected from the Chandra Deep Field South (CDFS) for which we identify a serious lack of spectroscopically determined redshifts.
Published: 2007
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