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764 results on '"Le Floc'h E."'

201. Sociétés paysannes, transitions agraires et dynamiques écologiques dans le sud-ouest de Madagascar : actes de l'atelier CNRE IRD

Author

Rakotoarimanana, Vonjison, Le Floc'h, E., Grouzis, Michel, Razanaka, S. (ed.), Grouzis, Michel (ed.), Milleville, Pierre (ed.), Moizo, Bernard (ed.), and Aubry, C. (ed.)

Subjects
PROTECTION DE L'ECOSYSTEME, BIOLOGIE VEGETALE, BIOMASSE, ANALYSE DIACHRONIQUE, STRATE HERBACEE, FLORISTIQUE, PATURAGE, PLUVIOMETRIE, ETUDE D'IMPACT, FEU, SAVANE, PRODUCTION VEGETALE, parasitic diseases, HERBACEE, human activities, METHODOLOGIE
Published
2001

202. Sociétés paysannes, transitions agraires et dynamiques écologiques dans le sud-ouest de Madagascar : actes de l'atelier CNRE IRD

Author

Grouzis, Michel, Razanaka, S., Le Floc'h, E., Leprun, Jean-Claude, Rakotomalala, R. (collab.), Rakotondramanana, Modeste (collab.), Razanaka, S. (ed.), Grouzis, Michel (ed.), Milleville, Pierre (ed.), Moizo, Bernard (ed.), and Aubry, C. (ed.)

Subjects
FORET, ECHANTILLONNAGE, SOL, ECOSYSTEME, FLORISTIQUE, SAVANE, JACHERE, FLORE DU SOL, FACTEUR EDAPHIQUE, FACTEUR BIOTIQUE, FORET DENSE SECHE, BIOMASSE EPIGEE, VEGETATION, DEFORESTATION, METHODOLOGIE
Published
2001

203. A redshift survey of herschel far-infrared selected starbursts and implications for obscured star formation

Author

Casey, C., Berta, S., Béthermin, M., Bock, J., Bridge, C., Budynkiewicz, J., Burgarella, D., Chapin, E., Chapman, S., Clements, D., Conley, A., Conselice, C., Cooray, A., Farrah, D., Hatziminaoglou, E., Ivison, R., Le Floc'h, E., Lutz, D., Magdis, G., Magnelli, B., Oliver, S., Page, M., Pozzi, F., Rigopoulou, D., Riguccini, L., Roseboom, I., Sanders, D., Scott, D., Seymour, Nick, Valtchanov, I., Vieira, J., Viero, M., Wardlow, J., Casey, C., Berta, S., Béthermin, M., Bock, J., Bridge, C., Budynkiewicz, J., Burgarella, D., Chapin, E., Chapman, S., Clements, D., Conley, A., Conselice, C., Cooray, A., Farrah, D., Hatziminaoglou, E., Ivison, R., Le Floc'h, E., Lutz, D., Magdis, G., Magnelli, B., Oliver, S., Page, M., Pozzi, F., Rigopoulou, D., Riguccini, L., Roseboom, I., Sanders, D., Scott, D., Seymour, Nick, Valtchanov, I., Vieira, J., Viero, M., and Wardlow, J.

Abstract

We present Keck spectroscopic observations and redshifts for a sample of 767 Herschel-SPIRE selected galaxies (HSGs) at 250, 350, and 500 μm, taken with the Keck I Low Resolution Imaging Spectrometer and the Keck II DEep Imaging Multi-Object Spectrograph. The redshift distribution of these SPIRE sources from the Herschel Multitiered Extragalactic Survey peaks at z = 0.85, with 731 sources at z < 2 and a tail of sources out to z ~ 5. We measure more significant disagreement between photometric and spectroscopic redshifts ( Δz/(1 + z spec) = 0.29) than is seen in non-infrared selected samples, likely due to enhanced star formation rates and dust obscuration in infrared-selected galaxies. The infrared data are used to directly measure integrated infrared luminosities and dust temperatures independent of radio or 24 μm flux densities. By probing the dust spectral energy distribution (SED) at its peak, we estimate that the vast majority (72%-83%) of z < 2 Herschel-selected galaxies would drop out of traditional submillimeter surveys at 0.85-1 mm. We find that dust temperature traces infrared luminosity, due in part to the SPIRE wavelength selection biases, and partially from physical effects.As a result, we measure no significant trend in SPIRE color with redshift; if dust temperature were independent of luminosity or redshift, a trend in SPIRE color would be expected. Composite infrared SEDs are constructed as a function of infrared luminosity, showing the increase in dust temperature with luminosity, and subtle change in near-infrared and mid-infrared spectral properties. Moderate evolution in the far-infrared (FIR)/radio correlation is measured for this partially radio-selected sample, with q IR∝(1 + z)–0.30 ± 0.02 at z < 2. We estimate the luminosity function and implied star formation rate density contribution of HSGs at z < 1.6 and find overall agreement with work based on 24 μm extrapolations of the LIRG, ULIRG, and total infrared contributions. This work signific

Published
2012

204. HerMES: Deep number counts at 250 µm, 350 µm and 500 µm in the COSMOS and GOODS-N fields and the build-up of the cosmic infrared background

Author

Béthermin, M., Le Floc'H, E., Ilbert, O., Conley, A., Lagache, G., Amblard, A., Arumugam, V., Aussel, H., Berta, S., Bock, J., Boselli, A., Buat, V., Casey, C., Castro-Rodríguez, N., Cava, A., Clements, D., Cooray, A., Dowell, C., Eales, S., Farrah, D., Franceschini, A., Glenn, J., Griffin, M., Hatziminaoglou, E., Heinis, S., Ibar, E., Ivison, R., Kartaltepe, J., Levenson, L., Magdis, G., Marchetti, L., Marsden, G., Nguyen, H., O'Halloran, B., Oliver, S., Omont, A., Page, M., Panuzzo, P., Papageorgiou, A., Pearson, C., Pérez-Fournon, I., Pohlen, M., Rigopoulou, D., Roseboom, I., Rowan-Robinson, M., Salvato, M., Schulz, B., Scott, D., Seymour, Nick, Shupe, D., Smith, A., Symeonidis, M., Trichas, M., Tugwell, K., Vaccari, M., Valtchanov, I., Vieira, J., Viero, M., Wang, L., Xu, C., Zemcov, M., Béthermin, M., Le Floc'H, E., Ilbert, O., Conley, A., Lagache, G., Amblard, A., Arumugam, V., Aussel, H., Berta, S., Bock, J., Boselli, A., Buat, V., Casey, C., Castro-Rodríguez, N., Cava, A., Clements, D., Cooray, A., Dowell, C., Eales, S., Farrah, D., Franceschini, A., Glenn, J., Griffin, M., Hatziminaoglou, E., Heinis, S., Ibar, E., Ivison, R., Kartaltepe, J., Levenson, L., Magdis, G., Marchetti, L., Marsden, G., Nguyen, H., O'Halloran, B., Oliver, S., Omont, A., Page, M., Panuzzo, P., Papageorgiou, A., Pearson, C., Pérez-Fournon, I., Pohlen, M., Rigopoulou, D., Roseboom, I., Rowan-Robinson, M., Salvato, M., Schulz, B., Scott, D., Seymour, Nick, Shupe, D., Smith, A., Symeonidis, M., Trichas, M., Tugwell, K., Vaccari, M., Valtchanov, I., Vieira, J., Viero, M., Wang, L., Xu, C., and Zemcov, M.

Abstract

Aims. The Spectral and Photometric Imaging REceiver (SPIRE) onboard the Herschel space telescope has provided confusion limited maps of deep fields at 250 μm, 350 μm, and 500 μm, as part of the Herschel Multi-tiered Extragalactic Survey (HerMES). Unfortunately, due to confusion, only a small fraction of the cosmic infrared background (CIB) can be resolved into individually-detected sources. Our goal is to produce deep galaxy number counts and redshift distributions below the confusion limit at SPIRE wavelengths (~20 mJy), which we then use to place strong constraints on the origins of the cosmic infrared background and on models of galaxy evolution. Methods. We individually extracted the bright SPIRE sources (>20 mJy) in the COSMOS field with a method using the positions, the flux densities, and the redshifts of the 24 μm sources as a prior, and derived the number counts and redshift distributions of the bright SPIRE sources. For fainter SPIRE sources (<20 mJy), we reconstructed the number counts and the redshift distribution below the confusion limit using the deep 24 μm catalogs associated with photometric redshift and information provided by the stacking of these sources into the deep SPIRE maps of the GOODS-N and COSMOS fields. Finally, by integrating all these counts, we studied the contribution of the galaxies to the CIB as a function of their flux density and redshift.Results. Through stacking, we managed to reconstruct the source counts per redshift slice down to ~2 mJy in the three SPIRE bands, which lies about a factor 10 below the 5σ confusion limit. Our measurements place tight constraints on source population models. None of the pre-existing models are able to reproduce our results at better than 3-σ. Finally, we extrapolate our counts to zero flux density in order to derive an estimate of the total contribution of galaxies to the CIB, finding 10.1-2.3+2.6 nW m-2 sr-1, 6.5-1.6+1.7 nW m-2 sr-1, and 2.8-0.8+0.9 nW m-2 sr-1 at 250 μm, 350 μm, and 500 μm, r

Published
2012

205. A redshift survey of Herschel far-infrared selected starbursts and implications for obscured star formation

Author

Casey, C. M., Berta, S., Bethermin, M., Bock, J., Bridge, C. R., Budynkiewicz, J., Burgarella, D., Chapin, E., Chapman, S. C., Clements, D. L., Conley, A., Conselice, C. J., Cooray, A., Farrah, D., Hatziminaoglou, E., Ivison, R. J., Le Floc'h, E., Lutz, D., Magdis, G. E., Magnelli, B., Oliver, S. J., Page, M. J., Pozzi, F., Rigopoulou, D., Riguccini, L., Roseboom, I. G., Sanders, D. B., Scott, D., Seymour, N., Valtchanov, I., Vieira, J. D., Viero, M., Wardlow, J., Casey, C. M., Berta, S., Bethermin, M., Bock, J., Bridge, C. R., Budynkiewicz, J., Burgarella, D., Chapin, E., Chapman, S. C., Clements, D. L., Conley, A., Conselice, C. J., Cooray, A., Farrah, D., Hatziminaoglou, E., Ivison, R. J., Le Floc'h, E., Lutz, D., Magdis, G. E., Magnelli, B., Oliver, S. J., Page, M. J., Pozzi, F., Rigopoulou, D., Riguccini, L., Roseboom, I. G., Sanders, D. B., Scott, D., Seymour, N., Valtchanov, I., Vieira, J. D., Viero, M., and Wardlow, J.

Abstract

We present Keck spectroscopic observations and redshifts for a sample of 767 Herschel-SPIRE selected galaxies (HSGs) at 250, 350, and 500 mu m, taken with the Keck I Low Resolution Imaging Spectrometer and the Keck II DEep Imaging Multi-Object Spectrograph. The redshift distribution of these SPIRE sources from the Herschel Multitiered Extragalactic Survey peaks at z = 0.85, with 731 sources at z < 2 and a tail of sources out to z similar to 5. We measure more significant disagreement between photometric and spectroscopic redshifts ( = 0.29) than is seen in non-infrared selected samples, likely due to enhanced star formation rates and dust obscuration in infrared-selected galaxies. The infrared data are used to directly measure integrated infrared luminosities and dust temperatures independent of radio or 24 mu m flux densities. By probing the dust spectral energy distribution (SED) at its peak, we estimate that the vast majority (72%-83%) of z < 2 Herschel-selected galaxies would drop out of traditional submillimeter surveys at 0.85-1 mm. We find that dust temperature traces infrared luminosity, due in part to the SPIRE wavelength selection biases, and partially from physical effects. As a result, we measure no significant trend in SPIRE color with redshift; if dust temperature were independent of luminosity or redshift, a trend in SPIRE color would be expected. Composite infrared SEDs are constructed as a function of infrared luminosity, showing the increase in dust temperature with luminosity, and subtle change in near-infrared and mid-infrared spectral properties. Moderate evolution in the far-infrared (FIR)/radio correlation is measured for this partially radio-selected sample, with q(IR) proportional to (1 + z)(-0.30 +/- 0.02) at z < 2. We estimate the luminosity function and implied star formation rate density contribution of HSGs at z < 1.6 and find overall agreement with work based on 24 mu m extrapolations of the LIRG, ULIRG, and tota

Published
2012
Full Text
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206. A Population of z > 2 Far-Infrared Herschel-Spire-Selected Starbursts

Author

Casey, C. M., Berta, S., Bethermin, M., Bock, J., Bridge, C. R., Burgarella, D., Chapin, E., Chapman, S. C., Clements, D. L., Conley, A., Conselice, C. J., Cooray, A., Farrah, D., Hatziminaoglou, E., Ivison, R. J., Le Floc'h, E., Lutz, D., Magdis, G. E., Magnelli, B., Oliver, S. J., Page, M. J., Pozzi, F., Rigopoulou, D., Riguccini, L., Roseboom, I. G., Sanders, D. B., Scott, D., Seymour, N., Valtchanov, I., Vieira, J. D., Viero, M., Wardlow, J., Casey, C. M., Berta, S., Bethermin, M., Bock, J., Bridge, C. R., Burgarella, D., Chapin, E., Chapman, S. C., Clements, D. L., Conley, A., Conselice, C. J., Cooray, A., Farrah, D., Hatziminaoglou, E., Ivison, R. J., Le Floc'h, E., Lutz, D., Magdis, G. E., Magnelli, B., Oliver, S. J., Page, M. J., Pozzi, F., Rigopoulou, D., Riguccini, L., Roseboom, I. G., Sanders, D. B., Scott, D., Seymour, N., Valtchanov, I., Vieira, J. D., Viero, M., and Wardlow, J.

Abstract

We present spectroscopic observations for a sample of 36 Herschel-Spire 250-500 mu m selected galaxies (HSGs) at 2 < z < 5 from the Herschel Multi-tiered Extragalactic Survey. Redshifts are confirmed as part of a large redshift survey of Herschel-Spire-selected sources covering similar to 0.93 deg(2) in six extragalactic legacy fields. Observations were taken with the Keck I Low Resolution Imaging Spectrometer and the Keck II DEep Imaging Multi-Object Spectrograph. Precise astrometry, needed for spectroscopic follow-up, is determined by identification of counterparts at 24 mu m or 1.4 GHz using a cross-identification likelihood matching method. Individual source luminosities range from log(L-IR/L-circle dot) = 12.5-13.6 (corresponding to star formation rates (SFRs) 500-9000M(circle dot) yr(-1), assuming a Salpeter initial mass function), constituting some of the most intrinsically luminous, distant infrared galaxies discovered thus far. We present both individual and composite rest-frame ultraviolet spectra and infrared spectral energy distributions. The selection of these HSGs is reproducible and well characterized across large areas of the sky in contrast to most z > 2 HyLIRGs in the literature, which are detected serendipitously or via tailored surveys searching only for high-z HyLIRGs; therefore, we can place lower limits on the contribution of HSGs to the cosmic star formation rate density (SFRD) at (7 +/- 2) x 10(-3) M-circle dot yr(-1) h(3) Mpc(-3) at z similar to 2.5, which is > 10% of the estimated total SFRD of the universe from optical surveys. The contribution at z similar to 4 has a lower limit of 3 x 10(-3) M-circle dot yr(-1) h(3) Mpc(-3), greater than or similar to 20% of the estimated total SFRD. This highlights the importance of extremely infrared-luminous galaxies with high SFRs to the buildup of stellar mass, even at the earliest epochs.

Published
2012
Full Text
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207. A redshift survey of Herschel far-infrared selected starbursts and implications for obscured star formation

Author

Physics, Casey, C. M., Berta, S., Bethermin, M., Bock, J., Bridge, C. R., Budynkiewicz, J., Burgarella, D., Chapin, E., Chapman, S. C., Clements, D. L., Conley, A., Conselice, C. J., Cooray, A., Farrah, D., Hatziminaoglou, E., Ivison, R. J., Le Floc'h, E., Lutz, D., Magdis, G. E., Magnelli, B., Oliver, S. J., Page, M. J., Pozzi, F., Rigopoulou, D., Riguccini, L., Roseboom, I. G., Sanders, D. B., Scott, D., Seymour, N., Valtchanov, I., Vieira, J. D., Viero, M., Wardlow, J., Physics, Casey, C. M., Berta, S., Bethermin, M., Bock, J., Bridge, C. R., Budynkiewicz, J., Burgarella, D., Chapin, E., Chapman, S. C., Clements, D. L., Conley, A., Conselice, C. J., Cooray, A., Farrah, D., Hatziminaoglou, E., Ivison, R. J., Le Floc'h, E., Lutz, D., Magdis, G. E., Magnelli, B., Oliver, S. J., Page, M. J., Pozzi, F., Rigopoulou, D., Riguccini, L., Roseboom, I. G., Sanders, D. B., Scott, D., Seymour, N., Valtchanov, I., Vieira, J. D., Viero, M., and Wardlow, J.

Abstract

We present Keck spectroscopic observations and redshifts for a sample of 767 Herschel-SPIRE selected galaxies (HSGs) at 250, 350, and 500 mu m, taken with the Keck I Low Resolution Imaging Spectrometer and the Keck II DEep Imaging Multi-Object Spectrograph. The redshift distribution of these SPIRE sources from the Herschel Multitiered Extragalactic Survey peaks at z = 0.85, with 731 sources at z < 2 and a tail of sources out to z similar to 5. We measure more significant disagreement between photometric and spectroscopic redshifts ( = 0.29) than is seen in non-infrared selected samples, likely due to enhanced star formation rates and dust obscuration in infrared-selected galaxies. The infrared data are used to directly measure integrated infrared luminosities and dust temperatures independent of radio or 24 mu m flux densities. By probing the dust spectral energy distribution (SED) at its peak, we estimate that the vast majority (72%-83%) of z < 2 Herschel-selected galaxies would drop out of traditional submillimeter surveys at 0.85-1 mm. We find that dust temperature traces infrared luminosity, due in part to the SPIRE wavelength selection biases, and partially from physical effects. As a result, we measure no significant trend in SPIRE color with redshift; if dust temperature were independent of luminosity or redshift, a trend in SPIRE color would be expected. Composite infrared SEDs are constructed as a function of infrared luminosity, showing the increase in dust temperature with luminosity, and subtle change in near-infrared and mid-infrared spectral properties. Moderate evolution in the far-infrared (FIR)/radio correlation is measured for this partially radio-selected sample, with q(IR) proportional to (1 + z)(-0.30 +/- 0.02) at z < 2. We estimate the luminosity function and implied star formation rate density contribution of HSGs at z < 1.6 and find overall agreement with work based on 24 mu m extrapolations of the LIRG, ULIRG, and tota

Published
2012

208. A Population of z > 2 Far-Infrared Herschel-Spire-Selected Starbursts

Author

Physics, Casey, C. M., Berta, S., Bethermin, M., Bock, J., Bridge, C. R., Burgarella, D., Chapin, E., Chapman, S. C., Clements, D. L., Conley, A., Conselice, C. J., Cooray, A., Farrah, D., Hatziminaoglou, E., Ivison, R. J., Le Floc'h, E., Lutz, D., Magdis, G. E., Magnelli, B., Oliver, S. J., Page, M. J., Pozzi, F., Rigopoulou, D., Riguccini, L., Roseboom, I. G., Sanders, D. B., Scott, D., Seymour, N., Valtchanov, I., Vieira, J. D., Viero, M., Wardlow, J., Physics, Casey, C. M., Berta, S., Bethermin, M., Bock, J., Bridge, C. R., Burgarella, D., Chapin, E., Chapman, S. C., Clements, D. L., Conley, A., Conselice, C. J., Cooray, A., Farrah, D., Hatziminaoglou, E., Ivison, R. J., Le Floc'h, E., Lutz, D., Magdis, G. E., Magnelli, B., Oliver, S. J., Page, M. J., Pozzi, F., Rigopoulou, D., Riguccini, L., Roseboom, I. G., Sanders, D. B., Scott, D., Seymour, N., Valtchanov, I., Vieira, J. D., Viero, M., and Wardlow, J.

Abstract

We present spectroscopic observations for a sample of 36 Herschel-Spire 250-500 mu m selected galaxies (HSGs) at 2 < z < 5 from the Herschel Multi-tiered Extragalactic Survey. Redshifts are confirmed as part of a large redshift survey of Herschel-Spire-selected sources covering similar to 0.93 deg(2) in six extragalactic legacy fields. Observations were taken with the Keck I Low Resolution Imaging Spectrometer and the Keck II DEep Imaging Multi-Object Spectrograph. Precise astrometry, needed for spectroscopic follow-up, is determined by identification of counterparts at 24 mu m or 1.4 GHz using a cross-identification likelihood matching method. Individual source luminosities range from log(L-IR/L-circle dot) = 12.5-13.6 (corresponding to star formation rates (SFRs) 500-9000M(circle dot) yr(-1), assuming a Salpeter initial mass function), constituting some of the most intrinsically luminous, distant infrared galaxies discovered thus far. We present both individual and composite rest-frame ultraviolet spectra and infrared spectral energy distributions. The selection of these HSGs is reproducible and well characterized across large areas of the sky in contrast to most z > 2 HyLIRGs in the literature, which are detected serendipitously or via tailored surveys searching only for high-z HyLIRGs; therefore, we can place lower limits on the contribution of HSGs to the cosmic star formation rate density (SFRD) at (7 +/- 2) x 10(-3) M-circle dot yr(-1) h(3) Mpc(-3) at z similar to 2.5, which is > 10% of the estimated total SFRD of the universe from optical surveys. The contribution at z similar to 4 has a lower limit of 3 x 10(-3) M-circle dot yr(-1) h(3) Mpc(-3), greater than or similar to 20% of the estimated total SFRD. This highlights the importance of extremely infrared-luminous galaxies with high SFRs to the buildup of stellar mass, even at the earliest epochs.

Published
2012

209. The Herschel Multi-tiered Extragalactic Survey: HerMES

Author

Oliver, S., Bock, J., Altieri, B., Amblard, A., Arumugam, V., Aussel, H., Babbedge, T., Beelen, A., Bethermin, M., Blain, A., Boselli, A., Bridge, C., Brisbin, D., Buat, V., Burgarella, D., Castro-Rodriguez, N., Cava, A., Chania, P., Cirasuolo, M., Clements, D., Conley, A., Conversi, L., Cooray, A., Dowell, C., Dubois, E., Dwek, E., Dye, S., Eales, S., Elbaz, D., Farrah, D., Feltre, A., Ferrero, P., Fiolet, N., Fox, M., Franceschini, A., Gear, W., Giovannoli, E., Glenn, J., Gong, Y., Solares, E., Griffin, M., Halpern, M., Harwit, M., Hatziminaoglou, E., Heinis, S., Hurley, P., Hwang, H., Hyde, A., Ibar, E., Ilbert, O., Isaak, K., Ivison, R., Lagache, G., Le Floc'h, E., Levenson, L., Lo Faro, B., Lu, N., Madden, S., Maffei, B., Magdis, G., Mainetti, G., Marchetti, L., Marsden, G., Marshall, J., Mortier, A., Nguyen, H., O'Halloran, B., Omont, A., Page, M., Panuzzo, P., Papageorgiou, A., Patel, H., Pearson, C., Perez-Fournon, I., Pohlen, M., Rawlings, J., Raymond, G., Rigopoulou, D., Riguccini, L., Rizzo, D., Rodighiero, G., Roseboom, I., Rowan-Robinson, M., Portal, M., Schulz, B., Scott, D., Seymour, Nick, Shupe, D., Smith, A., Stevens, J., Symeonidis, M., Trichas, M., Tugwell, K., Vaccari, M., Valtchanov, I., Vieira, J., Viero, M., Vigroux, L., Wang, L., Ward, R., Wardlow, J., Wright, G., Xu, C., Zemcov, M., Oliver, S., Bock, J., Altieri, B., Amblard, A., Arumugam, V., Aussel, H., Babbedge, T., Beelen, A., Bethermin, M., Blain, A., Boselli, A., Bridge, C., Brisbin, D., Buat, V., Burgarella, D., Castro-Rodriguez, N., Cava, A., Chania, P., Cirasuolo, M., Clements, D., Conley, A., Conversi, L., Cooray, A., Dowell, C., Dubois, E., Dwek, E., Dye, S., Eales, S., Elbaz, D., Farrah, D., Feltre, A., Ferrero, P., Fiolet, N., Fox, M., Franceschini, A., Gear, W., Giovannoli, E., Glenn, J., Gong, Y., Solares, E., Griffin, M., Halpern, M., Harwit, M., Hatziminaoglou, E., Heinis, S., Hurley, P., Hwang, H., Hyde, A., Ibar, E., Ilbert, O., Isaak, K., Ivison, R., Lagache, G., Le Floc'h, E., Levenson, L., Lo Faro, B., Lu, N., Madden, S., Maffei, B., Magdis, G., Mainetti, G., Marchetti, L., Marsden, G., Marshall, J., Mortier, A., Nguyen, H., O'Halloran, B., Omont, A., Page, M., Panuzzo, P., Papageorgiou, A., Patel, H., Pearson, C., Perez-Fournon, I., Pohlen, M., Rawlings, J., Raymond, G., Rigopoulou, D., Riguccini, L., Rizzo, D., Rodighiero, G., Roseboom, I., Rowan-Robinson, M., Portal, M., Schulz, B., Scott, D., Seymour, Nick, Shupe, D., Smith, A., Stevens, J., Symeonidis, M., Trichas, M., Tugwell, K., Vaccari, M., Valtchanov, I., Vieira, J., Viero, M., Vigroux, L., Wang, L., Ward, R., Wardlow, J., Wright, G., Xu, C., and Zemcov, M.

Abstract

The Herschel Multi-tiered Extragalactic Survey (HerMES) is a legacy programme designed to map a set of nested fields totalling ~380deg 2. Fields range in size from 0.01 to ~20deg 2, using the Herschel-Spectral and Photometric Imaging Receiver (SPIRE) (at 250, 350 and 500µm) and the Herschel-Photodetector Array Camera and Spectrometer (PACS) (at 100 and 160µm), with an additional wider component of 270deg 2 with SPIRE alone. These bands cover the peak of the redshifted thermal spectral energy distribution from interstellar dust and thus capture the reprocessed optical and ultraviolet radiation from star formation that has been absorbed by dust, and are critical for forming a complete multiwavelength understanding of galaxy formation and evolution. The survey will detect of the order of 100000 galaxies at 5s in some of the best-studied fields in the sky. Additionally, HerMES is closely coordinated with the PACS Evolutionary Probe survey. Making maximum use of the full spectrum of ancillary data, from radio to X-ray wavelengths, it is designed to facilitate redshift determination, rapidly identify unusual objects and understand the relationships between thermal emission from dust and other processes. Scientific questions HerMES will be used to answer include the total infrared emission of galaxies, the evolution of the luminosity function, the clustering properties of dusty galaxies and the properties of populations of galaxies which lie below the confusion limit through lensing and statistical techniques. This paper defines the survey observations and data products, outlines the primary scientific goals of the HerMES team, and reviews some of the early results. © 2012 The Authors. Monthly Notices of the Royal Astronomical Society © 2012 RAS.

Published
2012

210. A mid-IR study of Hickson compact groups II. Multiwavelength analysis of the complete GALEX-Spitzer sample

Author

Bitsakis, T., Charmandaris, Vassilis, da Cunha, Elisabete, Díaz-Santos, T., Le Floc’h, E., Magdis, G., Bitsakis, T., Charmandaris, Vassilis, da Cunha, Elisabete, Díaz-Santos, T., Le Floc’h, E., and Magdis, G.

Abstract

We present a comprehensive study of the impact of the environment of compact galaxy groups on the evolution of their members using a multiwavelength analysis from the ultraviolet to the infrared, for a sample of 32 Hickson compact groups (HCGs) containing 135 galaxies. Fitting the spectral energy distributions (SEDs) of all galaxies with the state-of-the-art model of da Cunha et al. (2008, MNRAS, 388, 1595) we can accurately calculate their mass, SFR, and extinction, as well as estimate their infrared luminosity and dust content. We compare our findings with samples of field galaxies, early-stage interacting pairs, and cluster galaxies with similar data. We find that classifying the groups as dynamically “old” or “young”, depending on whether at least one quarter of their members are early-type systems, is physical and consistent with past classifications of HCGs based on their atomic gas content. Dynamically “old” groups are more compact and display higher velocity dispersions than “young” groups. Late-type galaxies in dynamically “young” groups have specific star formation rates (sSFRs), NUV-r, and mid-infrared colors that are similar to those of field and early-stage, interacting pair spirals. Late-type galaxies in dynamically “old” groups have redder NUV-r colors, because they have likely experienced several tidal encounters in the past, thereby building up their stellar mass, and display lower sSFRs. We identify several late-type galaxies that have sSFRs and colors similar to those of elliptical galaxies, since they lost part of their gas due to numerous interactions with other group members. Also, 25% of the elliptical galaxies in these groups have bluer UV/optical colors than normal ellipticals in the field, probably due to star formation as they accreted gas from other galaxies of the group or via merging of dwarf companions. Finally, our SED modeling suggests that in 13 groups, ten of which are dynamically “old”, there is diffuse cold dust in the intragroup

Published
2011

211. Galaxies in X-ray groups. I: Robust membership assignment and the impact of group environments on quenching

Author

George, M R, Leauthaud, A, Bundy, K, Finoguenov, A, Tinker, J, Lin, Y T, Mei, S, Kneib, J-P, Aussel, H, Behroozi, P S, Busha, M T, Capak, P, Coccato, L, Covone, G, Faure, C, Fiorenza, S L, Ilbert, O, Le Floc'h, E, Koekemoer, A M, Tanaka, M, Wechsler, R H, Wolk, M, George, M R, Leauthaud, A, Bundy, K, Finoguenov, A, Tinker, J, Lin, Y T, Mei, S, Kneib, J-P, Aussel, H, Behroozi, P S, Busha, M T, Capak, P, Coccato, L, Covone, G, Faure, C, Fiorenza, S L, Ilbert, O, Le Floc'h, E, Koekemoer, A M, Tanaka, M, Wechsler, R H, and Wolk, M

Abstract

Understanding the mechanisms that lead dense environments to host galaxies with redder colors, more spheroidal morphologies, and lower star formation rates than field populations remains an important problem. As most candidate processes ultimately depend on host halo mass, accurate characterizations of the local environment, ideally tied to halo mass estimates and spanning a range in halo mass and redshift, are needed. In this work, we present and test a rigorous, probabilistic method for assigning galaxies to groups based on precise photometric redshifts and X-ray-selected groups drawn from the COSMOS field. The groups have masses in the range 1013 <~ M 200c/M ☉ <~ 1014 and span redshifts 0 < z < 1. We characterize our selection algorithm via tests on spectroscopic subsamples, including new data obtained at the Very Large Telescope, and by applying our method to detailed mock catalogs. We find that our group member galaxy sample has a purity of 84% and completeness of 92% within 0.5{R_{200c}}. We measure the impact of uncertainties in redshifts and group centering on the quality of the member selection with simulations based on current data as well as future imaging and spectroscopic surveys. As a first application of our new group member catalog which will be made publicly available, we show that member galaxies exhibit a higher quenched fraction compared to the field at fixed stellar mass out to z ~ 1, indicating a significant relationship between star formation and environment at group scales. We also address the suggestion that dusty star-forming galaxies in such groups may impact the high-l power spectrum of the cosmic microwave background and find that such a population cannot explain the low power seen in recent Sunyaev-Zel'dovich measurements.

Published
2011

212. Herschel reveals a Tdust-unbiased selection of z~ 2 ultraluminous infrared galaxies

Author

Magdis, G., Elbaz, D., Hwang, H., Amblard, A., Arumugam, V., Aussel, H., Blain, A., Bock, J., Boselli, A., Buat, V., Castro-Rodríguez, N., Cava, A., Chanial, P., Clements, D., Conley, A., Conversi, L., Cooray, A., Dowell, C., Dwek, E., Eales, S., Farrah, D., Franceschini, A., Glenn, J., Griffin, M., Halpern, M., Hatziminaoglou, E., Huang, J., Ibar, E., Isaak, K., Le Floc'h, E., Lagache, G., Levenson, L., Lonsdale, C., Lu, N., Madden, S., Maffei, B., Mainetti, G., Marchetti, L., Morrison, G., Nguyen, H., O'Halloran, B., Oliver, S., Omont, A., Owen, F., Page, M., Pannella, M., Panuzzo, P., Papageorgiou, A., Pearson, C., Pérez-Fournon, I., Pohlen, M., Rigopoulou, D., Rizzo, D., Roseboom, I., Rowan-Robinson, M., Schulz, B., Scott, D., Seymour, Nick, Shupe, D., Smith, A., Stevens, J., Strazzullo, V., Symeonidis, M., Trichas, M., Tugwell, K., Vaccari, M., Valtchanov, I., Vigroux, L., Wang, L., Wright, G., Xu, C., Zemcov, M., Magdis, G., Elbaz, D., Hwang, H., Amblard, A., Arumugam, V., Aussel, H., Blain, A., Bock, J., Boselli, A., Buat, V., Castro-Rodríguez, N., Cava, A., Chanial, P., Clements, D., Conley, A., Conversi, L., Cooray, A., Dowell, C., Dwek, E., Eales, S., Farrah, D., Franceschini, A., Glenn, J., Griffin, M., Halpern, M., Hatziminaoglou, E., Huang, J., Ibar, E., Isaak, K., Le Floc'h, E., Lagache, G., Levenson, L., Lonsdale, C., Lu, N., Madden, S., Maffei, B., Mainetti, G., Marchetti, L., Morrison, G., Nguyen, H., O'Halloran, B., Oliver, S., Omont, A., Owen, F., Page, M., Pannella, M., Panuzzo, P., Papageorgiou, A., Pearson, C., Pérez-Fournon, I., Pohlen, M., Rigopoulou, D., Rizzo, D., Roseboom, I., Rowan-Robinson, M., Schulz, B., Scott, D., Seymour, Nick, Shupe, D., Smith, A., Stevens, J., Strazzullo, V., Symeonidis, M., Trichas, M., Tugwell, K., Vaccari, M., Valtchanov, I., Vigroux, L., Wang, L., Wright, G., Xu, C., and Zemcov, M.

Abstract

Using Herschel Photodetector Array Camera (PACS) and Spectral and Photometric Imaging Receiver (SPIRE) observations of Lockman Hole-North and Great Observatories Origins Deep Survey-North (GOODS-N) as part of the Herschel Multi-tiered Extragalactic Survey (HerMES) project, we explore the far-infrared (IR) properties of a sample of mid-IR-selected starburst-dominated ultraluminous infrared galaxies (ULIRGs) at z~ 2. The selection of the sample is based on the detection of the stellar bump that appears in the spectral energy distribution of star-forming galaxies at 1.6 µm. We derive robust estimates of infrared luminosities (LIR) and dust temperatures (Td) of the population and find that while the luminosities in our sample span less than an order of magnitude (12.24 = log(LIR/L·) = 12.94), they cover a wide range of dust temperatures (25 =Td= 62 K). Galaxies in our sample range from those that are as cold as high-z submillimetre galaxies (SMGs) to those that are as warm as optically faint radio galaxies (OFRGs) and local ULIRGs. Nevertheless, our sample has median Td= 42.3 K, filling the gap between SMGs and OFRGs, bridging the two populations. We demonstrate that a significant fraction of our sample would be missed from ground-based (sub)mm surveys (850-1200 µm), showing that the latter introduce a bias towards the detection of colder sources. We conclude that Herschel observations confirm the existence of high-z ULIRGs warmer than SMGs, show that the mid-IR selection of high-z ULIRGs is not Td dependent, reveal a large dispersion in Td of high-z ULIRGs and provide the means to characterize the bulk of the ULIRG population, free from selection biases introduced by ground-based (sub)mm surveys. © 2010 The Authors. Journal compilation © 2010 RAS.

Published
2010

213. The evolution of the dust temperatures of galaxies in the SFR–M∗plane up toz ~ 2

Author

Magnelli, B., primary, Lutz, D., additional, Saintonge, A., additional, Berta, S., additional, Santini, P., additional, Symeonidis, M., additional, Altieri, B., additional, Andreani, P., additional, Aussel, H., additional, Béthermin, M., additional, Bock, J., additional, Bongiovanni, A., additional, Cepa, J., additional, Cimatti, A., additional, Conley, A., additional, Daddi, E., additional, Elbaz, D., additional, Förster Schreiber, N. M., additional, Genzel, R., additional, Ivison, R. J., additional, Le Floc’h, E., additional, Magdis, G., additional, Maiolino, R., additional, Nordon, R., additional, Oliver, S. J., additional, Page, M., additional, Pérez García, A., additional, Poglitsch, A., additional, Popesso, P., additional, Pozzi, F., additional, Riguccini, L., additional, Rodighiero, G., additional, Rosario, D., additional, Roseboom, I., additional, Sanchez-Portal, M., additional, Scott, D., additional, Sturm, E., additional, Tacconi, L. J., additional, Valtchanov, I., additional, Wang, L., additional, and Wuyts, S., additional

Published
2014
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214. zCOSMOS 20k: satellite galaxies are the main drivers of environmental effects in the galaxy population at least to z ∼ 0.7

Author

Kovač, K., primary, Lilly, S. J., additional, Knobel, C., additional, Bschorr, T. J., additional, Peng, Y., additional, Carollo, C. M., additional, Contini, T., additional, Kneib, J.-P., additional, Le Févre, O., additional, Mainieri, V., additional, Renzini, A., additional, Scodeggio, M., additional, Zamorani, G., additional, Bardelli, S., additional, Bolzonella, M., additional, Bongiorno, A., additional, Caputi, K., additional, Cucciati, O., additional, de la Torre, S., additional, de Ravel, L., additional, Franzetti, P., additional, Garilli, B., additional, Iovino, A., additional, Kampczyk, P., additional, Lamareille, F., additional, Le Borgne, J.-F., additional, Le Brun, V., additional, Maier, C., additional, Mignoli, M., additional, Oesch, P., additional, Pello, R., additional, Montero, E. Perez, additional, Presotto, V., additional, Silverman, J., additional, Tanaka, M., additional, Tasca, L., additional, Tresse, L., additional, Vergani, D., additional, Zucca, E., additional, Aussel, H., additional, Koekemoer, A. M., additional, Le Floc'h, E., additional, Moresco, M., additional, and Pozzetti, L., additional

Published
2013
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215. The incidence of obscuration in active galactic nuclei

Author

Merloni, A., primary, Bongiorno, A., additional, Brusa, M., additional, Iwasawa, K., additional, Mainieri, V., additional, Magnelli, B., additional, Salvato, M., additional, Berta, S., additional, Cappelluti, N., additional, Comastri, A., additional, Fiore, F., additional, Gilli, R., additional, Koekemoer, A., additional, Le Floc'h, E., additional, Lusso, E., additional, Lutz, D., additional, Miyaji, T., additional, Pozzi, F., additional, Riguccini, L., additional, Rosario, D. J., additional, Silverman, J., additional, Symeonidis, M., additional, Treister, E., additional, Vignali, C., additional, and Zamorani, G., additional

Published
2013
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216. THE ROLE OF GALAXY INTERACTION IN THE SFR-M*RELATION: CHARACTERIZING MORPHOLOGICAL PROPERTIES OFHerschel-SELECTED GALAXIES AT 0.2 < 1.5

Author

Hung, Chao-Ling, primary, Sanders, D. B., additional, Casey, C. M., additional, Lee, N., additional, Barnes, J. E., additional, Capak, P., additional, Kartaltepe, J. S., additional, Koss, M., additional, Larson, K. L., additional, Le Floc'h, E., additional, Lockhart, K., additional, Man, A. W. S., additional, Mann, A. W., additional, Riguccini, L., additional, Scoville, N., additional, and Symeonidis, M., additional

Published
2013
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217. Reversal or no reversal: the evolution of the star formation rate–density relation up to z ∼ 1.6

Author

Ziparo, F., primary, Popesso, P., additional, Finoguenov, A., additional, Biviano, A., additional, Wuyts, S., additional, Wilman, D., additional, Salvato, M., additional, Tanaka, M., additional, Nandra, K., additional, Lutz, D., additional, Elbaz, D., additional, Dickinson, M., additional, Altieri, B., additional, Aussel, H., additional, Berta, S., additional, Cimatti, A., additional, Fadda, D., additional, Genzel, R., additional, Le Floc'h, E., additional, Magnelli, B., additional, Nordon, R., additional, Poglitsch, A., additional, Pozzi, F., additional, Portal, M. Sanchez, additional, Tacconi, L., additional, Bauer, F. E., additional, Brandt, W. N., additional, Cappelluti, N., additional, Cooper, M. C., additional, and Mulchaey, J. S., additional

Published
2013
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218. Erratum: The Herschel★ PEP/HerMES Luminosity Function – I. Probing the Evolution of PACS selected Galaxies to z ≃ 4

Author

Gruppioni, C., primary, Pozzi, F., additional, Rodighiero, G., additional, Delvecchio, I., additional, Berta, S., additional, Pozzetti, L., additional, Zamorani, G., additional, Andreani, P., additional, Cimatti, A., additional, Ilbert, O., additional, Le Floc'h, E., additional, Lutz, D., additional, Magnelli, B., additional, Marchetti, L., additional, Monaco, P., additional, Nordon, R., additional, Oliver, S., additional, Popesso, P., additional, Riguccini, L., additional, Roseboom, I., additional, Rosario, D. J., additional, Sargent, M., additional, Vaccari, M., additional, Altieri, B., additional, Aussel, H., additional, Bongiovanni, A., additional, Cepa, J., additional, Daddi, E., additional, Domínguez-Sánchez, H., additional, Elbaz, D., additional, Schreiber, N. Förster, additional, Genzel, R., additional, Iribarrem, A., additional, Magliocchetti, M., additional, Maiolino, R., additional, Poglitsch, A., additional, García, A. Pérez, additional, Sanchez-Portal, M., additional, Sturm, E., additional, Tacconi, L., additional, Valtchanov, I., additional, Amblard, A., additional, Arumugam, V., additional, Bethermin, M., 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, Cooray, A., additional, Dowell, C. D., additional, Dwek, E., additional, Eales, S., additional, Franceschini, A., additional, Glenn, J., additional, Griffin, 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, Nguyen, H. T., additional, O'Halloran, B., additional, Page, M. J., additional, Panuzzo, P., additional, Papageorgiou, A., additional, Pearson, C. P., additional, Pérez-Fournon, I., additional, Pohlen, M., additional, Rigopoulou, D., additional, Rowan-Robinson, 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, Vigroux, L., additional, Wang, L., additional, Wright, G., additional, Xu, C. K., additional, Zemcov, M., additional, Bardelli, S., additional, Carollo, M., additional, Contini, T., additional, Le Févre, O., additional, Lilly, S., additional, Mainieri, V., additional, Renzini, A., additional, Scodeggio, M., additional, and Zucca, E., additional

Published
2013
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219. Encoding of the infrared excess in theNUVrKcolor diagram for star-forming galaxies

Author

Arnouts, S., primary, Le Floc’h, E., additional, Chevallard, J., additional, Johnson, B. D., additional, Ilbert, O., additional, Treyer, M., additional, Aussel, H., additional, Capak, P., additional, Sanders, D. B., additional, Scoville, N., additional, McCracken, H. J., additional, Milliard, B., additional, Pozzetti, L., additional, and Salvato, M., additional

Published
2013
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220. Spot the difference

Author

Moresco, M., primary, Pozzetti, L., additional, Cimatti, A., additional, Zamorani, G., additional, Bolzonella, M., additional, Lamareille, F., additional, Mignoli, M., additional, Zucca, E., additional, Lilly, S. J., additional, Carollo, C. M., additional, Contini, T., additional, Kneib, J.-P., additional, Le Fèvre, O., additional, Mainieri, V., additional, Renzini, A., additional, Scodeggio, M., additional, Bardelli, S., additional, Bongiorno, A., additional, Caputi, K., additional, Cucciati, O., additional, de la Torre, S., additional, de Ravel, L., additional, Franzetti, P., additional, Garilli, B., additional, Iovino, A., additional, Kampczyk, P., additional, Knobel, C., additional, Kovač, K., additional, Le Borgne, J.-F., additional, Le Brun, V., additional, Maier, C., additional, Pelló, R., additional, Peng, Y., additional, Perez-Montero, E., additional, Presotto, V., additional, Silverman, J. D., additional, Tanaka, M., additional, Tasca, L., additional, Tresse, L., additional, Vergani, D., additional, Barnes, L., additional, Bordoloi, R., additional, Cappi, A., additional, Diener, C., additional, Koekemoer, A. M., additional, Le Floc’h, E., additional, López-Sanjuan, C., additional, McCracken, H. J., additional, Nair, P., additional, Oesch, P., additional, Scarlata, C., additional, Scoville, N., additional, and Welikala, N., additional

Published
2013
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223. Lyman Break and ultraviolet-selected galaxies at z ∼ 1 – II. PACS 100 μm/160 μm FIR detections★

Author

Oteo, I., primary, Magdis, G., additional, Bongiovanni, Á., additional, Pérez-García, A. M., additional, Cepa, J., additional, Cedrés, B., additional, Ederoclite, A., additional, Sánchez-Portal, M., additional, Aguerri, J. A. L., additional, Alfaro, E. J., additional, Altieri, B., additional, Andreani, P., additional, Aparicio-Villegas, T., additional, Aussel, H., additional, Benítez, N., additional, Berta, S., additional, Broadhurst, T., additional, Cabrera-Caño, J., additional, Castander, F. J., additional, Cerviño, M., additional, Cimatti, A., additional, Cristobal-Hornillos, D., additional, Daddi, E., additional, Elbaz, D., additional, Fernandez-Soto, A., additional, Schreiber, N. Förster, additional, Genzel, R., additional, Gonzalez-Delgado, R. M., additional, Husillos, C., additional, Infante, L., additional, Le Floc'h, E., additional, Lutz, D., additional, Magnelli, B., additional, Maiolino, R., additional, Márquez, I., additional, Martínez, V. J., additional, Masegosa, J., additional, Matute, I., additional, Moles, M., additional, Molino, A., additional, Olmo, A. del, additional, Perea, J., additional, Pérez-Martínez, R., additional, Pintos-Castro, I., additional, Poglitsch, A., additional, Polednikova, J., additional, Popesso, P., additional, Pović, M., additional, Pozzi, F., additional, Prada, F., additional, Quintana, J. M., additional, Riguccini, L., additional, Sturm, E., additional, Tacconi, L., additional, Valtchanov, I., additional, and Viironen, K., additional

Published
2013
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224. Herschel reveals the obscured star formation in HiZELS H emitters at z = 1.47

Author

Ibar, E., primary, Sobral, D., additional, Best, P. N., additional, Ivison, R. J., additional, Smail, I., additional, Arumugam, V., additional, Berta, S., additional, Bethermin, M., additional, Bock, J., additional, Cava, A., additional, Conley, A., additional, Farrah, D., additional, Geach, J., additional, Ikarashi, S., additional, Kohno, K., additional, Le Floc'h, E., additional, Lutz, D., additional, Magdis, G., additional, Magnelli, B., additional, Marsden, G., additional, Oliver, S. J., additional, Page, M. J., additional, Pozzi, F., additional, Riguccini, L., additional, Schulz, B., additional, Seymour, N., additional, Smith, A. J., additional, Symeonidis, M., additional, Wang, L., additional, Wardlow, J., additional, and Zemcov, M., additional

Published
2013
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225. Mass assembly in quiescent and star-forming galaxies sincez≃ 4 from UltraVISTA

Author

Ilbert, O., primary, McCracken, H. J., additional, Le Fèvre, O., additional, Capak, P., additional, Dunlop, J., additional, Karim, A., additional, Renzini, M. A., additional, Caputi, K., additional, Boissier, S., additional, Arnouts, S., additional, Aussel, H., additional, Comparat, J., additional, Guo, Q., additional, Hudelot, P., additional, Kartaltepe, J., additional, Kneib, J. P., additional, Krogager, J. K., additional, Le Floc’h, E., additional, Lilly, S., additional, Mellier, Y., additional, Milvang-Jensen, B., additional, Moutard, T., additional, Onodera, M., additional, Richard, J., additional, Salvato, M., additional, Sanders, D. B., additional, Scoville, N., additional, Silverman, J. D., additional, Taniguchi, Y., additional, Tasca, L., additional, Thomas, R., additional, Toft, S., additional, Tresse, L., additional, Vergani, D., additional, Wolk, M., additional, and Zirm, A., additional

Published
2013
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226. HerschelPEP/HerMES: the redshift evolution (0 ≤z≤ 4) of dust attenuation and of the total (UV+IR) star formation rate density

Author

Burgarella, D., primary, Buat, V., additional, Gruppioni, C., additional, Cucciati, O., additional, Heinis, S., additional, Berta, S., additional, Béthermin, M., additional, Bock, J., additional, Cooray, A., additional, Dunlop, J. S., additional, Farrah, D., additional, Franceschini, A., additional, Le Floc’h, E., additional, Lutz, D., additional, Magnelli, B., additional, Nordon, R., additional, Oliver, S. J., additional, Page, M. J., additional, Popesso, P., additional, Pozzi, F., additional, Riguccini, L., additional, Vaccari, M., additional, and Viero, M., additional

Published
2013
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227. The Herschel-PEP survey: evidence for downsizing in the hosts of dusty star-forming systems

Author

Magliocchetti, M., primary, Popesso, P., additional, Rosario, D., additional, Lutz, D., additional, Aussel, H., additional, Berta, S., additional, Altieri, B., additional, Andreani, P., additional, Cepa, J., additional, Castañeda, H., additional, Cimatti, A., additional, Elbaz, D., additional, Genzel, R., additional, Grazian, A., additional, Gruppioni, C., additional, Ilbert, O., additional, Le Floc’h, E., additional, Magnelli, B., additional, Maiolino, R., additional, Nordon, R., additional, Poglitsch, A., additional, Pozzi, F., additional, Riguccini, L., additional, Rodighiero, G., additional, Sanchez-Portal, M., additional, Santini, P., additional, Förster Schreiber, N. M., additional, Sturm, E., additional, Tacconi, L., additional, and Valtchanov, I., additional

Published
2013
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228. The Herschel★ PEP/HerMES luminosity function – I. Probing the evolution of PACS selected Galaxies to z ≃ 4

Author

Gruppioni, C., primary, Pozzi, F., additional, Rodighiero, G., additional, Delvecchio, I., additional, Berta, S., additional, Pozzetti, L., additional, Zamorani, G., additional, Andreani, P., additional, Cimatti, A., additional, Ilbert, O., additional, Le Floc’h, E., additional, Lutz, D., additional, Magnelli, B., additional, Marchetti, L., additional, Monaco, P., additional, Nordon, R., additional, Oliver, S., additional, Popesso, P., additional, Riguccini, L., additional, Roseboom, I., additional, Rosario, D. J., additional, Sargent, M., additional, Vaccari, M., additional, Altieri, B., additional, Aussel, H., additional, Bongiovanni, A., additional, Cepa, J., additional, Daddi, E., additional, Domínguez-Sánchez, H., additional, Elbaz, D., additional, Förster Schreiber, N., additional, Genzel, R., additional, Iribarrem, A., additional, Magliocchetti, M., additional, Maiolino, R., additional, Poglitsch, A., additional, Pérez García, A., additional, Sanchez-Portal, M., additional, Sturm, E., additional, Tacconi, L., additional, Valtchanov, I., additional, Amblard, A., additional, Arumugam, V., additional, Bethermin, M., 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, Cooray, A., additional, Dowell, C. D., additional, Dwek, E., additional, Eales, S., additional, Franceschini, A., additional, Glenn, J., additional, Griffin, 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, Nguyen, H. T., additional, O’Halloran, B., additional, Page, M. J., additional, Panuzzo, P., additional, Papageorgiou, A., additional, Pearson, C. P., additional, Pérez-Fournon, I., additional, Pohlen, M., additional, Rigopoulou, D., additional, Rowan-Robinson, 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, Vigroux, L., additional, Wang, L., additional, Wright, G., additional, Xu, C. K., additional, Zemcov, M., additional, Bardelli, S., additional, Carollo, M., additional, Contini, T., additional, Le Févre, O., additional, Lilly, S., additional, Mainieri, V., additional, Renzini, A., additional, Scodeggio, M., additional, and Zucca, E., additional

Published
2013
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229. Panchromatic spectral energy distributions ofHerschelsources

Author

Berta, S., primary, Lutz, D., additional, Santini, P., additional, Wuyts, S., additional, Rosario, D., additional, Brisbin, D., additional, Cooray, A., additional, Franceschini, A., additional, Gruppioni, C., additional, Hatziminaoglou, E., additional, Hwang, H. S., additional, Le Floc’h, E., additional, Magnelli, B., additional, Nordon, R., additional, Oliver, S., additional, Page, M. J., additional, Popesso, P., additional, Pozzetti, L., additional, Pozzi, F., additional, Riguccini, L., additional, Rodighiero, G., additional, Roseboom, I., additional, Scott, D., additional, Symeonidis, M., additional, Valtchanov, I., additional, Viero, M., additional, and Wang, L., additional

Published
2013
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230. HELP: XID+, the probabilistic de-blender for Herschel SPIRE maps.

Author

Hurley, P. D., Oliver, S., Betancourt, M., Clarke, C., Cowley, W. I., Duivenvoorden, S., Farrah, D., Griffin, M., Lacey, C., Le Floc'h, E., Papadopoulos, A., Sargent, M., Scudder, J. M., Vaccari, M., Valtchanov, I., and Wang, L.

Subjects
ASTRONOMICAL photometry, SPECTRAL imaging, BAYESIAN analysis, PROBABILITY theory, METAPHYSICAL cosmology
Abstract

We have developed a new prior-based source extraction tool, XID+, to carry out photometry in the Herschel SPIRE (Spectral and Photometric Imaging Receiver) maps at the positions of known sources. XID+ is developed using a probabilistic Bayesian framework that provides a natural framework in which to include prior information, and uses the Bayesian inference tool Stan to obtain the full posterior probability distribution on flux estimates. In this paper, we discuss the details of XID+ and demonstrate the basic capabilities and performance by running it on simulated SPIRE maps resembling the COSMOS field, and comparing to the current prior-based source extraction tool DESPHOT. Not only we show that XID+ performs better on metrics such as flux accuracy and flux uncertainty accuracy, but we also illustrate how obtaining the posterior probability distribution can help overcome some of the issues inherent with maximum-likelihood-based source extraction routines. We run XID+ on the COSMOS SPIRE maps from Herschel Multi-Tiered Extragalactic Survey using a 24-µm catalogue as a positional prior, and a uniform flux prior ranging from 0.01 to 1000 mJy. We show the marginalized SPIRE colour--colour plot and marginalized contribution to the cosmic infrared background at the SPIRE wavelengths. XID+ is a core tool arising from the Herschel Extragalactic Legacy Project (HELP) and we discuss how additional work within HELP providing prior information on fluxes can and will be utilized. The software is available at https://github.com/H-E-L-P/XID_plus.We also provide the data product for COSMOS. We believe this is the first time that the full posterior probability of galaxy photometry has been provided as a data product. [ABSTRACT FROM AUTHOR]

Published
2017
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231. Planck's Dusty GEMS II. Extended [CII] emission and absorption in the Garnet at z = 3.4 seen with ALMA.

Author

Nesvadba, N., Kneissl, R., Cañameras, R., Boone, F., Falgarone, E., Frye, B., Gerin, M., Koenig, S., Lagache, G., Le Floc'h, E., Malhotra, S., and Scott, D.

Subjects
GARNET, REDSHIFT, GALAXY formation, GALACTIC evolution, INTERSTELLAR medium, STARBURSTS
Abstract

We present spatially resolved ALMA [CII] observations of the bright (flux density S350 = 400 mJy at 350 μm), gravitationally lensed, starburst galaxy PLCK G045.1+61.1 at z = 3.427, the “Garnet”. This source is part of our set of “Planck’s Dusty GEMS”, discovered with the Planck’s all-sky survey. Two emission-line clouds with a relative velocity offset of ~600 km s-1 extend towards north-east and south-west, respectively, of a small, intensely star-forming clump with a star-formation intensity of 220 M⊙ yr-1 kpc-2, akin to maximal starbursts. [CII] is also seen in absorption, with a redshift of +350 km s-1 relative to the brightest CO component. [CII] absorption has previously only been found in the Milky Way along sightlines toward bright high-mass star-forming regions, and this is the first detection in another galaxy. Similar to Galactic environments, the [CII] absorption feature is associated with [CI] emission, implying that this is diffuse gas shielded from the UV radiation of the clump, and likely at large distances from the clump. Since absorption can only be seen in front of a continuum source, the gas in this structure can definitely be attributed to gas flowing towards the clump. The absorber could be part of a cosmic filament or merger debris being accreted onto the galaxy. We discuss our results also in light of the on-going debate of the origin of the [CII] deficit in dusty star-forming galaxies. [ABSTRACT FROM AUTHOR]

Published
2016
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232. Populations et environnement dans les pays du Sud

Author

Floret, C., Le Floc'h, E., Pontanier, Roger, Gendreau, Francis (ed.), Gubry, Patrick (ed.), and Véron, J. (ed.)

Subjects
DESERTIFICATION, ANTHROPISATION, PATURAGE, GESTION DE L'ENVIRONNEMENT, EAU DU SOL, DEGRADATION DE L'ENVIRONNEMENT, VEGETATION, AGRICULTURE INTENSIVE, PRESSION DEMOGRAPHIQUE, DONNEES STATISTIQUES
Published
1996

234. Des arbres et des arbustes spontanés de l'Adrar des Iforas (Mali)

Author

Ag Sidiyene, Ehya, Le Floc'h, E. (collab.), and Bernus, Edmond (collab.)

Subjects
VEGETATION SPONTANEE, PROTECTION DE L'ECOSYSTEME, ARBUSTE, VOCABULAIRE, ETHNOBOTANIQUE, NOM VERNACULAIRE, LIGNEUX, ESPECE MENACEE, ARBRE, PHYTOGEOGRAPHIE, FOURRAGE, ECONOMIE PASTORALE, ETHNOLINGUISTIQUE, FLORE
Abstract

Enclavé dans le Sahara, le massif montagneux de l'Adrar bénéficie d'un climat mixte, saharien et sahélien, et abrite une flore particulière. Cet ouvrage énumère cinquante espèces ligneuses dont certaines ne sont plus représentées que par un ou deux individus. Il précise le vocabulaire qui s'y raporte et présente leurs usages et leur intérêt pastoral. L'étude constitue un précieux témoignage sur la nature de l'Adrar des Iforas et la culture touarègue, alors que l'environnement de cette région est fragilisé par l'isolement, les sécheresses constantes et l'avancement progressif de la désertification. (Résumé d'auteur)

Published
1996

235. Accreting supermassive black holes in the COSMOS field and the connection to their host galaxies

Author

Bongiorno, A., primary, Merloni, A., additional, Brusa, M., additional, Magnelli, B., additional, Salvato, M., additional, Mignoli, M., additional, Zamorani, G., additional, Fiore, F., additional, Rosario, D., additional, Mainieri, V., additional, Hao, H., additional, Comastri, A., additional, Vignali, C., additional, Balestra, I., additional, Bardelli, S., additional, Berta, S., additional, Civano, F., additional, Kampczyk, P., additional, Le Floc'h, E., additional, Lusso, E., additional, Lutz, D., additional, Pozzetti, L., additional, Pozzi, F., additional, Riguccini, L., additional, Shankar, F., additional, and Silverman, J., additional

Published
2012
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237. GOODS-Herschel: radio-excess signature of hidden AGN activity in distant star-forming galaxies

Author

Del Moro, A., primary, Alexander, D. M., additional, Mullaney, J. R., additional, Daddi, E., additional, Pannella, M., additional, Bauer, F. E., additional, Pope, A., additional, Dickinson, M., additional, Elbaz, D., additional, Barthel, P. D., additional, Garrett, M. A., additional, Brandt, W. N., additional, Charmandaris, V., additional, Chary, R. R., additional, Dasyra, K., additional, Gilli, R., additional, Hickox, R. C., additional, Hwang, H. S., additional, Ivison, R. J., additional, Juneau, S., additional, Le Floc’h, E., additional, Luo, B., additional, Morrison, G. E., additional, Rovilos, E., additional, Sargent, M. T., additional, and Xue, Y. Q., additional

Published
2012
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238. A REDSHIFT SURVEY OFHERSCHELFAR-INFRARED SELECTED STARBURSTS AND IMPLICATIONS FOR OBSCURED STAR FORMATION

Author

Casey, C. M., primary, Berta, S., additional, Béthermin, M., additional, Bock, J., additional, Bridge, C., additional, Budynkiewicz, J., additional, Burgarella, D., additional, Chapin, E., additional, Chapman, S. C., additional, Clements, D. L., additional, Conley, A., additional, Conselice, C. J., additional, Cooray, A., additional, Farrah, D., additional, Hatziminaoglou, E., additional, Ivison, R. J., additional, le Floc'h, E., additional, Lutz, D., additional, Magdis, G., additional, Magnelli, B., additional, Oliver, S. J., additional, Page, M. J., additional, Pozzi, F., additional, Rigopoulou, D., additional, Riguccini, L., additional, Roseboom, I. G., additional, Sanders, D. B., additional, Scott, Douglas, additional, Seymour, N., additional, Valtchanov, I., additional, Vieira, J. D., additional, Viero, M., additional, and Wardlow, J., additional

Published
2012
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239. The dominant role of mergers in the size evolution of massive early-type galaxies sincez ~ 1

Author

López-Sanjuan, C., primary, Le Fèvre, O., additional, Ilbert, O., additional, Tasca, L. A. M., additional, Bridge, C., additional, Cucciati, O., additional, Kampczyk, P., additional, Pozzetti, L., additional, Xu, C. K., additional, Carollo, C. M., additional, Contini, T., additional, Kneib, J.-P., additional, Lilly, S. J., additional, Mainieri, V., additional, Renzini, A., additional, Sanders, D., additional, Scodeggio, M., additional, Scoville, N. Z., additional, Taniguchi, Y., additional, Zamorani, G., additional, Aussel, H., additional, Bardelli, S., additional, Bolzonella, M., additional, Bongiorno, A., additional, Capak, P., additional, Caputi, K., additional, de la Torre, S., additional, de Ravel, L., additional, Franzetti, P., additional, Garilli, B., additional, Iovino, A., additional, Knobel, C., additional, Kovač, K., additional, Lamareille, F., additional, Le Borgne, J.-F., additional, Le Brun, V., additional, Le Floc’h, E., additional, Maier, C., additional, McCracken, H. J., additional, Mignoli, M., additional, Pelló, R., additional, Peng, Y., additional, Pérez-Montero, E., additional, Presotto, V., additional, Ricciardelli, E., additional, Salvato, M., additional, Silverman, J. D., additional, Tanaka, M., additional, Tresse, L., additional, Vergani, D., additional, Zucca, E., additional, Barnes, L., additional, Bordoloi, R., additional, Cappi, A., additional, Cimatti, A., additional, Coppa, G., additional, Koekemoer, A., additional, Liu, C. T., additional, Moresco, M., additional, Nair, P., additional, Oesch, P., additional, Schawinski, K., additional, and Welikala, N., additional

Published
2012
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240. COSMIC EVOLUTION OF STAR FORMATION ENHANCEMENT IN CLOSE MAJOR-MERGER GALAXY PAIRS SINCEz= 1

Author

Xu, C. K., primary, Shupe, D. L., additional, Béthermin, M., additional, Aussel, H., additional, Berta, S., additional, Bock, J., additional, Bridge, C., additional, Conley, A., additional, Cooray, A., additional, Elbaz, D., additional, Franceschini, A., additional, Le Floc'h, E., additional, Lu, N., additional, Lutz, D., additional, Magnelli, B., additional, Marsden, G., additional, Oliver, S. J., additional, Pozzi, F., additional, Riguccini, L., additional, Schulz, B., additional, Scoville, N., additional, Vaccari, M., additional, Vieira, J. D., additional, Wang, L., additional, and Zemcov, M., additional

Published
2012
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241. NO CLEAR SUBMILLIMETER SIGNATURE OF SUPPRESSED STAR FORMATION AMONG X-RAY LUMINOUS ACTIVE GALACTIC NUCLEI

Author

Harrison, C. M., primary, Alexander, D. M., additional, Mullaney, J. R., additional, Altieri, B., additional, Coia, D., additional, Charmandaris, V., additional, Daddi, E., additional, Dannerbauer, H., additional, Dasyra, K., additional, Del Moro, A., additional, Dickinson, M., additional, Hickox, R. C., additional, Ivison, R. J., additional, Kartaltepe, J., additional, Le Floc'h, E., additional, Leiton, R., additional, Magnelli, B., additional, Popesso, P., additional, Rovilos, E., additional, Rosario, D., additional, and Swinbank, A. M., additional

Published
2012
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242. Impact of a river flash flood on microbial carbon and nitrogen production in a Mediterranean Lagoon (Thau Lagoon, France)

Author

Fouilland, E., primary, Trottet, A., additional, Bancon-Montigny, C., additional, Bouvy, M., additional, Le Floc'h, E., additional, Gonzalez, J.-L., additional, Hatey, E., additional, Mas, S., additional, Mostajir, B., additional, Nouguier, J., additional, Pecqueur, D., additional, Rochelle-Newall, E., additional, Rodier, C., additional, Roques, C., additional, Salles, C., additional, Tournoud, M.-G., additional, and Vidussi, F., additional

Published
2012
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243. SPECTRAL ENERGY DISTRIBUTIONS OF TYPE 1 ACTIVE GALACTIC NUCLEI IN THE COSMOS SURVEY. I. THEXMM-COSMOS SAMPLE

Author

Elvis, M., primary, Hao, H., additional, Civano, F., additional, Brusa, M., additional, Salvato, M., additional, Bongiorno, A., additional, Capak, P., additional, Zamorani, G., additional, Comastri, A., additional, Jahnke, K., additional, Lusso, E., additional, Mainieri, V., additional, Trump, J. R., additional, Ho, L. C., additional, Aussel, H., additional, Cappelluti, N., additional, Cisternas, M., additional, Frayer, D., additional, Gilli, R., additional, Hasinger, G., additional, Huchra, J. P., additional, Impey, C. D., additional, Koekemoer, A. M., additional, Lanzuisi, G., additional, Le Floc'h, E., additional, Lilly, S. J., additional, Liu, Y., additional, McCarthy, P., additional, McCracken, H. J., additional, Merloni, A., additional, Roeser, H.-J., additional, Sanders, D. B., additional, Sargent, M., additional, Scoville, N., additional, Schinnerer, E., additional, Schiminovich, D., additional, Silverman, J., additional, Taniguchi, Y., additional, Vignali, C., additional, Urry, C. M., additional, Zamojski, M. A., additional, and Zatloukal, M., additional

Published
2012
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244. Bolometric luminosities and Eddington ratios of X-ray selected active galactic nuclei in theXMM-COSMOS survey

Author

Lusso, E., primary, Comastri, A., additional, Simmons, B. D., additional, Mignoli, M., additional, Zamorani, G., additional, Vignali, C., additional, Brusa, M., additional, Shankar, F., additional, Lutz, D., additional, Trump, J. R., additional, Maiolino, R., additional, Gilli, R., additional, Bolzonella, M., additional, Puccetti, S., additional, Salvato, M., additional, Impey, C. D., additional, Civano, F., additional, Elvis, M., additional, Mainieri, V., additional, Silverman, J. D., additional, Koekemoer, A. M., additional, Bongiorno, A., additional, Merloni, A., additional, Berta, S., additional, Le Floc'h, E., additional, Magnelli, B., additional, Pozzi, F., additional, and Riguccini, L., additional

Published
2012
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245. TheHerschelMulti-tiered Extragalactic Survey: HerMES

Author

Oliver, S. J., primary, Bock, J., additional, Altieri, B., additional, Amblard, A., additional, Arumugam, V., additional, Aussel, H., additional, Babbedge, T., additional, Beelen, A., additional, Béthermin, M., additional, Blain, A., additional, Boselli, A., additional, Bridge, C., additional, Brisbin, D., additional, Buat, V., additional, Burgarella, D., additional, Castro-Rodríguez, N., additional, Cava, A., additional, Chanial, P., additional, Cirasuolo, M., additional, Clements, D. L., additional, Conley, A., additional, Conversi, L., additional, Cooray, A., additional, Dowell, C. D., additional, Dubois, E. N., additional, Dwek, E., additional, Dye, S., additional, Eales, S., additional, Elbaz, D., additional, Farrah, D., additional, Feltre, A., additional, Ferrero, P., additional, Fiolet, N., additional, Fox, M., additional, Franceschini, A., additional, Gear, W., additional, Giovannoli, E., additional, Glenn, J., additional, Gong, Y., additional, González Solares, E. A., additional, Griffin, M., additional, Halpern, M., additional, Harwit, M., additional, Hatziminaoglou, E., additional, Heinis, S., additional, Hurley, P., additional, Hwang, H. S., additional, Hyde, A., additional, Ibar, E., additional, Ilbert, O., additional, Isaak, K., additional, Ivison, R. J., additional, Lagache, G., additional, Le Floc'h, E., additional, Levenson, L., additional, Faro, B. Lo, additional, Lu, N., additional, Madden, S., additional, Maffei, B., additional, Magdis, G., additional, Mainetti, G., additional, Marchetti, L., additional, Marsden, G., additional, Marshall, J., 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, Patel, H., additional, Pearson, C. P., additional, Pérez-Fournon, I., additional, Pohlen, M., 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, Sánchez Portal, M., additional, Schulz, B., additional, Scott, Douglas, 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, Viero, M., additional, Vigroux, L., additional, Wang, L., additional, Ward, R., additional, Wardlow, J., additional, Wright, G., additional, Xu, C. K., additional, and Zemcov, M., additional

Published
2012
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246. HerMES: deep number counts at 250 μm, 350 μm and 500 μm in the COSMOS and GOODS-N fields and the build-up of the cosmic infrared background

Author

Béthermin, M., primary, Le Floc’h, E., additional, Ilbert, O., additional, Conley, A., additional, Lagache, G., additional, Amblard, A., additional, Arumugam, V., additional, Aussel, H., additional, Berta, S., additional, Bock, J., additional, Boselli, A., additional, Buat, V., additional, Casey, C. M., additional, Castro-Rodríguez, N., additional, Cava, A., additional, Clements, D. L., additional, Cooray, A., additional, Dowell, C. D., additional, Eales, S., additional, Farrah, D., additional, Franceschini, A., additional, Glenn, J., additional, Griffin, M., additional, Hatziminaoglou, E., additional, Heinis, S., additional, Ibar, E., additional, Ivison, R. J., additional, Kartaltepe, J. S., additional, Levenson, L., additional, Magdis, G., additional, Marchetti, L., additional, Marsden, G., 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, Rigopoulou, D., additional, Roseboom, I. G., additional, Rowan-Robinson, M., additional, Salvato, 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, Vieira, J. D., additional, Viero, M., additional, Wang, L., additional, Xu, C. K., additional, and Zemcov, M., additional

Published
2012
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248. PHYSICAL PROPERTIES OF Lyα EMITTERS ATz∼ 0.3 FROM UV-TO-FIR MEASUREMENTS

Author

Oteo, I., primary, Bongiovanni, A., additional, Pérez García, A. M., additional, Cepa, J., additional, Ederoclite, A., additional, Sánchez-Portal, M., additional, Pintos-Castro, I., additional, Pérez-Martínez, R., additional, Lutz, D., additional, Altieri, B., additional, Andreani, P., additional, Aussel, H., additional, Berta, S., additional, Cimatti, A., additional, Daddi, E., additional, Elbaz, D., additional, Förster Schreiber, N., additional, Genzel, R., additional, Le Floc'h, E., additional, Magnelli, B., additional, Maiolino, R., additional, Poglitsch, A., additional, Popesso, P., additional, Pozzi, F., additional, Riguccini, L., additional, Sturm, E., additional, Tacconi, L., additional, and Valtchanov, I., additional

Published
2012
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249. Enhanced star formation rates in AGN hosts with respect to inactive galaxies from PEP-Herschelobservations

Author

Santini, P., primary, Rosario, D. J., additional, Shao, L., additional, Lutz, D., 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, Cepa, J., additional, Cimatti, A., additional, Daddi, E., additional, Elbaz, D., additional, Fontana, A., additional, Förster Schreiber, N. M., additional, Genzel, R., additional, Grazian, A., additional, Le Floc’h, E., additional, Magnelli, B., additional, Mainieri, V., additional, Nordon, R., additional, Pérez Garcia, A. M., additional, Poglitsch, A., additional, Popesso, P., additional, Pozzi, F., additional, Riguccini, L., additional, Rodighiero, G., additional, Salvato, M., additional, Sanchez-Portal, M., additional, Sturm, E., additional, Tacconi, L. J., additional, Valtchanov, I., additional, and Wuyts, S., additional

Published
2012
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250. AHerschelview of the far-infrared properties of submillimetre galaxies

Author

Magnelli, B., primary, Lutz, D., additional, Santini, P., additional, Saintonge, A., additional, Berta, S., additional, Albrecht, M., additional, Altieri, B., additional, Andreani, P., additional, Aussel, H., additional, Bertoldi, F., additional, Béthermin, M., additional, Bongiovanni, A., additional, Capak, P., additional, Chapman, S., additional, Cepa, J., additional, Cimatti, A., additional, Cooray, A., additional, Daddi, E., additional, Danielson, A. L. R., additional, Dannerbauer, H., additional, Dunlop, J. S., additional, Elbaz, D., additional, Farrah, D., additional, Förster Schreiber, N. M., additional, Genzel, R., additional, Hwang, H. S., additional, Ibar, E., additional, Ivison, R. J., additional, Le Floc’h, E., additional, Magdis, G., additional, Maiolino, R., additional, Nordon, R., additional, Oliver, S. J., additional, Pérez García, A., additional, Poglitsch, A., additional, Popesso, P., additional, Pozzi, F., additional, Riguccini, L., additional, Rodighiero, G., additional, Rosario, D., additional, Roseboom, I., additional, Salvato, M., additional, Sanchez-Portal, M., additional, Scott, D., additional, Smail, I., additional, Sturm, E., additional, Swinbank, A. M., additional, Tacconi, L. J., additional, Valtchanov, I., additional, Wang, L., additional, and Wuyts, S., additional

Published
2012
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