The Herschel PEP/HerMES luminosity function - I. Probing the evolution of PACS selected Galaxies to z ≃ 4. Gruppioni, C., Pozzi, F., Rodighiero, G., Delvecchio, I., Berta, S., Pozzetti, L., Zamorani, G., Andreani, P., Cimatti, A., Ilbert, O., Le Floc'h, E., Lutz, D., Magnelli, B., Marchetti, L., Monaco, P., Nordon, R., Oliver, S., Popesso, P., Riguccini, L., Roseboom, I., Rosario, D. J., Sargent, M., Vaccari, M., Altieri, B., Aussel, H., Bongiovanni, A., Cepa, J., Daddi, E., Domínguez-Sánchez, H., Elbaz, D., Förster Schreiber, N., Genzel, R., Iribarrem, A., Magliocchetti, M., Maiolino, R., Poglitsch, A., Pérez García, A., Sanchez-Portal, M., Sturm, E., Tacconi, L., Valtchanov, I., Amblard, A., Arumugam, V., Bethermin, M., Bock, J., Boselli, A., Buat, V., Burgarella, D., Castro-Rodríguez, N., Cava, A., Chanial, P., Clements, D. L., Conley, A., Cooray, A., Dowell, C. D., Dwek, E., Eales, S., Franceschini, A., Glenn, J., Griffin, M., Hatziminaoglou, E., Ibar, E., Isaak, K., Ivison, R. J., Lagache, G., Levenson, L., Lu, N., Madden, S., Maffei, B., Mainetti, G., Nguyen, H. T., O'Halloran, B., Page, M. J., Panuzzo, P., Papageorgiou, A., Pearson, C. P., Pérez-Fournon, I., Pohlen, M., Rigopoulou, D., Rowan-Robinson, M., Schulz, B., Scott, D., Seymour, N., Shupe, D. L., Smith, A. J., Stevens, J. A., Symeonidis, M., Trichas, M., Tugwell, K. E., Vigroux, L., Wang, L., Wright, G., Xu, C. K., Zemcov, M., Bardelli, S., Carollo, M., Contini, T., Le Févre, O., Lilly, S., Mainieri, V., Renzini, A., Scodeggio, M., & Zucca, E. Monthly Notices of the Royal Astronomical Society, 432:23–52, June, 2013. ![The Herschel PEP/HerMES luminosity function - I. Probing the evolution of PACS selected Galaxies to z ≃ 4 [link]](https://bibbase.org/img/filetypes/link.svg "link")
Paper doi abstract bibtex We exploit the deep and extended far-IR data sets (at 70, 100 and 160 μm) of the Herschel Guaranteed Time Observation (GTO) PACS Evolutionary Probe (PEP) Survey, in combination with the Herschel Multi-tiered Extragalactic Survey data at 250, 350 and 500 μm, to derive the evolution of the rest-frame 35-, 60-, 90- and total infrared (IR) luminosity functions (LFs) up to z ∼ 4. We detect very strong luminosity evolution for the total IR LF (LIR ∝ (1 + z)3.55 ± 0.10 up to z ∼ 2, and ∝ (1 + z)1.62 ± 0.51 at 2 \textless z ≲ 4) combined with a density evolution (∝(1 + z)-0.57 ± 0.22 up to z ∼ 1 and ∝ (1 + z)-3.92 ± 0.34 at 1 \textless z ≲ 4). In agreement with previous findings, the IR luminosity density (ρIR) increases steeply to z ∼ 1, then flattens between z ∼ 1 and z ∼ 3 to decrease at z ≳ 3. Galaxies with different spectral energy distributions, masses and specific star formation rates (SFRs) evolve in very different ways and this large and deep statistical sample is the first one allowing us to separately study the different evolutionary behaviours of the individual IR populations contributing to ρIR. Galaxies occupying the well-established SFR-stellar mass main sequence (MS) are found to dominate both the total IR LF and ρIR at all redshifts, with the contribution from off-MS sources (≥0.6 dex above MS) being nearly constant (∼20 per cent of the total ρIR) and showing no significant signs of increase with increasing z over the whole 0.8 \textless z \textless 2.2 range. Sources with mass in the range 10 ≤ log(M/M⊙) ≤ 11 are found to dominate the total IR LF, with more massive galaxies prevailing at the bright end of the high-z (≳2) LF. A two-fold evolutionary scheme for IR galaxies is envisaged: on the one hand, a starburst-dominated phase in which the Super Massive Black Holes (SMBH) grows and is obscured by dust (possibly triggered by a major merging event), is followed by an AGN-dominated phase, then evolving towards a local elliptical. On the other hand, moderately star-forming galaxies containing a low-luminosity AGN have various properties suggesting they are good candidates for systems in a transition phase preceding the formation of steady spiral galaxies.
@article{gruppioni_herschel_2013,
title = {The {Herschel} {PEP}/{HerMES} luminosity function - {I}. {Probing} the evolution of {PACS} selected {Galaxies} to z ≃ 4},
volume = {432},
issn = {0035-8711},
url = {http://adsabs.harvard.edu/abs/2013MNRAS.432...23G},
doi = {10.1093/mnras/stt308},
abstract = {We exploit the deep and extended far-IR data sets (at 70, 100 and 160
μm) of the Herschel Guaranteed Time Observation (GTO) PACS
Evolutionary Probe (PEP) Survey, in combination with the Herschel
Multi-tiered Extragalactic Survey data at 250, 350 and 500 μm, to
derive the evolution of the rest-frame 35-, 60-, 90- and total infrared
(IR) luminosity functions (LFs) up to z ∼ 4. We detect very strong
luminosity evolution for the total IR LF (LIR ∝ (1 +
z)3.55 ± 0.10 up to z ∼ 2, and ∝ (1 +
z)1.62 ± 0.51 at 2 {\textless} z ≲ 4) combined with a
density evolution (∝(1 + z)-0.57 ± 0.22 up to z
∼ 1 and ∝ (1 + z)-3.92 ± 0.34 at 1 {\textless} z
≲ 4). In agreement with previous findings, the IR luminosity
density (ρIR) increases steeply to z ∼ 1, then
flattens between z ∼ 1 and z ∼ 3 to decrease at z ≳ 3.
Galaxies with different spectral energy distributions, masses and
specific star formation rates (SFRs) evolve in very different ways and
this large and deep statistical sample is the first one allowing us to
separately study the different evolutionary behaviours of the individual
IR populations contributing to ρIR. Galaxies occupying
the well-established SFR-stellar mass main sequence (MS) are found to
dominate both the total IR LF and ρIR at all redshifts,
with the contribution from off-MS sources (≥0.6 dex above MS) being
nearly constant (∼20 per cent of the total ρIR) and
showing no significant signs of increase with increasing z over the
whole 0.8 {\textless} z {\textless} 2.2 range. Sources with mass in the range 10 ≤
log(M/M⊙) ≤ 11 are found to dominate the total IR LF,
with more massive galaxies prevailing at the bright end of the high-z
(≳2) LF. A two-fold evolutionary scheme for IR galaxies is
envisaged: on the one hand, a starburst-dominated phase in which the
Super Massive Black Holes (SMBH) grows and is obscured by dust (possibly
triggered by a major merging event), is followed by an AGN-dominated
phase, then evolving towards a local elliptical. On the other hand,
moderately star-forming galaxies containing a low-luminosity AGN have
various properties suggesting they are good candidates for systems in a
transition phase preceding the formation of steady spiral galaxies.},
urldate = {2020-05-13},
journal = {Monthly Notices of the Royal Astronomical Society},
author = {Gruppioni, C. and Pozzi, F. and Rodighiero, G. and Delvecchio, I. and Berta, S. and Pozzetti, L. and Zamorani, G. and Andreani, P. and Cimatti, A. and Ilbert, O. and Le Floc'h, E. and Lutz, D. and Magnelli, B. and Marchetti, L. and Monaco, P. and Nordon, R. and Oliver, S. and Popesso, P. and Riguccini, L. and Roseboom, I. and Rosario, D. J. and Sargent, M. and Vaccari, M. and Altieri, B. and Aussel, H. and Bongiovanni, A. and Cepa, J. and Daddi, E. and Domínguez-Sánchez, H. and Elbaz, D. and Förster Schreiber, N. and Genzel, R. and Iribarrem, A. and Magliocchetti, M. and Maiolino, R. and Poglitsch, A. and Pérez García, A. and Sanchez-Portal, M. and Sturm, E. and Tacconi, L. and Valtchanov, I. and Amblard, A. and Arumugam, V. and Bethermin, M. and Bock, J. and Boselli, A. and Buat, V. and Burgarella, D. and Castro-Rodríguez, N. and Cava, A. and Chanial, P. and Clements, D. L. and Conley, A. and Cooray, A. and Dowell, C. D. and Dwek, E. and Eales, S. and Franceschini, A. and Glenn, J. and Griffin, M. and Hatziminaoglou, E. and Ibar, E. and Isaak, K. and Ivison, R. J. and Lagache, G. and Levenson, L. and Lu, N. and Madden, S. and Maffei, B. and Mainetti, G. and Nguyen, H. T. and O'Halloran, B. and Page, M. J. and Panuzzo, P. and Papageorgiou, A. and Pearson, C. P. and Pérez-Fournon, I. and Pohlen, M. and Rigopoulou, D. and Rowan-Robinson, M. and Schulz, B. and Scott, D. and Seymour, N. and Shupe, D. L. and Smith, A. J. and Stevens, J. A. and Symeonidis, M. and Trichas, M. and Tugwell, K. E. and Vigroux, L. and Wang, L. and Wright, G. and Xu, C. K. and Zemcov, M. and Bardelli, S. and Carollo, M. and Contini, T. and Le Févre, O. and Lilly, S. and Mainieri, V. and Renzini, A. and Scodeggio, M. and Zucca, E.},
month = jun,
year = {2013},
keywords = {cosmology: observations, galaxies: active, galaxies: evolution, galaxies: luminosity function, galaxies: starburst, infrared: galaxies, mass function},
pages = {23--52},
}
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{"_id":"FswfW3526mJDAQgm7","bibbaseid":"gruppioni-pozzi-rodighiero-delvecchio-berta-pozzetti-zamorani-andreani-etal-theherschelpephermesluminosityfunctioniprobingtheevolutionofpacsselectedgalaxiestoz4-2013","author_short":["Gruppioni, C.","Pozzi, F.","Rodighiero, G.","Delvecchio, I.","Berta, S.","Pozzetti, L.","Zamorani, G.","Andreani, P.","Cimatti, A.","Ilbert, O.","Le Floc'h, E.","Lutz, D.","Magnelli, B.","Marchetti, L.","Monaco, P.","Nordon, R.","Oliver, S.","Popesso, P.","Riguccini, L.","Roseboom, I.","Rosario, D. J.","Sargent, M.","Vaccari, M.","Altieri, B.","Aussel, H.","Bongiovanni, A.","Cepa, J.","Daddi, E.","Domínguez-Sánchez, H.","Elbaz, D.","Förster Schreiber, N.","Genzel, R.","Iribarrem, A.","Magliocchetti, M.","Maiolino, R.","Poglitsch, A.","Pérez García, A.","Sanchez-Portal, M.","Sturm, E.","Tacconi, L.","Valtchanov, I.","Amblard, A.","Arumugam, V.","Bethermin, M.","Bock, J.","Boselli, A.","Buat, V.","Burgarella, D.","Castro-Rodríguez, N.","Cava, A.","Chanial, P.","Clements, D. L.","Conley, A.","Cooray, A.","Dowell, C. D.","Dwek, E.","Eales, S.","Franceschini, A.","Glenn, J.","Griffin, M.","Hatziminaoglou, E.","Ibar, E.","Isaak, K.","Ivison, R. J.","Lagache, G.","Levenson, L.","Lu, N.","Madden, S.","Maffei, B.","Mainetti, G.","Nguyen, H. T.","O'Halloran, B.","Page, M. J.","Panuzzo, P.","Papageorgiou, A.","Pearson, C. P.","Pérez-Fournon, I.","Pohlen, M.","Rigopoulou, D.","Rowan-Robinson, M.","Schulz, B.","Scott, D.","Seymour, N.","Shupe, D. L.","Smith, A. J.","Stevens, J. A.","Symeonidis, M.","Trichas, M.","Tugwell, K. E.","Vigroux, L.","Wang, L.","Wright, G.","Xu, C. K.","Zemcov, M.","Bardelli, S.","Carollo, M.","Contini, T.","Le Févre, O.","Lilly, S.","Mainieri, V.","Renzini, A.","Scodeggio, M.","Zucca, E."],"bibdata":{"bibtype":"article","type":"article","title":"The Herschel PEP/HerMES luminosity function - I. Probing the evolution of PACS selected Galaxies to z ≃ 4","volume":"432","issn":"0035-8711","url":"http://adsabs.harvard.edu/abs/2013MNRAS.432...23G","doi":"10.1093/mnras/stt308","abstract":"We exploit the deep and extended far-IR data sets (at 70, 100 and 160 μm) of the Herschel Guaranteed Time Observation (GTO) PACS Evolutionary Probe (PEP) Survey, in combination with the Herschel Multi-tiered Extragalactic Survey data at 250, 350 and 500 μm, to derive the evolution of the rest-frame 35-, 60-, 90- and total infrared (IR) luminosity functions (LFs) up to z ∼ 4. We detect very strong luminosity evolution for the total IR LF (LIR ∝ (1 + z)3.55 ± 0.10 up to z ∼ 2, and ∝ (1 + z)1.62 ± 0.51 at 2 \\textless z ≲ 4) combined with a density evolution (∝(1 + z)-0.57 ± 0.22 up to z ∼ 1 and ∝ (1 + z)-3.92 ± 0.34 at 1 \\textless z ≲ 4). In agreement with previous findings, the IR luminosity density (ρIR) increases steeply to z ∼ 1, then flattens between z ∼ 1 and z ∼ 3 to decrease at z ≳ 3. Galaxies with different spectral energy distributions, masses and specific star formation rates (SFRs) evolve in very different ways and this large and deep statistical sample is the first one allowing us to separately study the different evolutionary behaviours of the individual IR populations contributing to ρIR. Galaxies occupying the well-established SFR-stellar mass main sequence (MS) are found to dominate both the total IR LF and ρIR at all redshifts, with the contribution from off-MS sources (≥0.6 dex above MS) being nearly constant (∼20 per cent of the total ρIR) and showing no significant signs of increase with increasing z over the whole 0.8 \\textless z \\textless 2.2 range. Sources with mass in the range 10 ≤ log(M/M⊙) ≤ 11 are found to dominate the total IR LF, with more massive galaxies prevailing at the bright end of the high-z (≳2) LF. A two-fold evolutionary scheme for IR galaxies is envisaged: on the one hand, a starburst-dominated phase in which the Super Massive Black Holes (SMBH) grows and is obscured by dust (possibly triggered by a major merging event), is followed by an AGN-dominated phase, then evolving towards a local elliptical. On the other hand, moderately star-forming galaxies containing a low-luminosity AGN have various properties suggesting they are good candidates for systems in a transition phase preceding the formation of steady spiral galaxies.","urldate":"2020-05-13","journal":"Monthly Notices of the Royal Astronomical 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observations, galaxies: active, galaxies: evolution, galaxies: luminosity function, galaxies: starburst, infrared: galaxies, mass function","pages":"23–52","bibtex":"@article{gruppioni_herschel_2013,\n\ttitle = {The {Herschel} {PEP}/{HerMES} luminosity function - {I}. {Probing} the evolution of {PACS} selected {Galaxies} to z ≃ 4},\n\tvolume = {432},\n\tissn = {0035-8711},\n\turl = {http://adsabs.harvard.edu/abs/2013MNRAS.432...23G},\n\tdoi = {10.1093/mnras/stt308},\n\tabstract = {We exploit the deep and extended far-IR data sets (at 70, 100 and 160 \nμm) of the Herschel Guaranteed Time Observation (GTO) PACS\nEvolutionary Probe (PEP) Survey, in combination with the Herschel\nMulti-tiered Extragalactic Survey data at 250, 350 and 500 μm, to\nderive the evolution of the rest-frame 35-, 60-, 90- and total infrared\n(IR) luminosity functions (LFs) up to z ∼ 4. We detect very strong\nluminosity evolution for the total IR LF (LIR ∝ (1 +\nz)3.55 ± 0.10 up to z ∼ 2, and ∝ (1 +\nz)1.62 ± 0.51 at 2 {\\textless} z ≲ 4) combined with a\ndensity evolution (∝(1 + z)-0.57 ± 0.22 up to z\n∼ 1 and ∝ (1 + z)-3.92 ± 0.34 at 1 {\\textless} z\n≲ 4). In agreement with previous findings, the IR luminosity\ndensity (ρIR) increases steeply to z ∼ 1, then\nflattens between z ∼ 1 and z ∼ 3 to decrease at z ≳ 3.\nGalaxies with different spectral energy distributions, masses and\nspecific star formation rates (SFRs) evolve in very different ways and\nthis large and deep statistical sample is the first one allowing us to\nseparately study the different evolutionary behaviours of the individual\nIR populations contributing to ρIR. Galaxies occupying\nthe well-established SFR-stellar mass main sequence (MS) are found to\ndominate both the total IR LF and ρIR at all redshifts,\nwith the contribution from off-MS sources (≥0.6 dex above MS) being\nnearly constant (∼20 per cent of the total ρIR) and\nshowing no significant signs of increase with increasing z over the\nwhole 0.8 {\\textless} z {\\textless} 2.2 range. Sources with mass in the range 10 ≤\nlog(M/M⊙) ≤ 11 are found to dominate the total IR LF,\nwith more massive galaxies prevailing at the bright end of the high-z\n(≳2) LF. A two-fold evolutionary scheme for IR galaxies is\nenvisaged: on the one hand, a starburst-dominated phase in which the\nSuper Massive Black Holes (SMBH) grows and is obscured by dust (possibly\ntriggered by a major merging event), is followed by an AGN-dominated\nphase, then evolving towards a local elliptical. On the other hand,\nmoderately star-forming galaxies containing a low-luminosity AGN have\nvarious properties suggesting they are good candidates for systems in a\ntransition phase preceding the formation of steady spiral galaxies.},\n\turldate = {2020-05-13},\n\tjournal = {Monthly Notices of the Royal Astronomical Society},\n\tauthor = {Gruppioni, C. and Pozzi, F. and Rodighiero, G. and Delvecchio, I. and Berta, S. and Pozzetti, L. and Zamorani, G. and Andreani, P. and Cimatti, A. and Ilbert, O. and Le Floc'h, E. and Lutz, D. and Magnelli, B. and Marchetti, L. and Monaco, P. and Nordon, R. and Oliver, S. and Popesso, P. and Riguccini, L. and Roseboom, I. and Rosario, D. J. and Sargent, M. and Vaccari, M. and Altieri, B. and Aussel, H. and Bongiovanni, A. and Cepa, J. and Daddi, E. and Domínguez-Sánchez, H. and Elbaz, D. and Förster Schreiber, N. and Genzel, R. and Iribarrem, A. and Magliocchetti, M. and Maiolino, R. and Poglitsch, A. and Pérez García, A. and Sanchez-Portal, M. and Sturm, E. and Tacconi, L. and Valtchanov, I. and Amblard, A. and Arumugam, V. and Bethermin, M. and Bock, J. and Boselli, A. and Buat, V. and Burgarella, D. and Castro-Rodríguez, N. and Cava, A. and Chanial, P. and Clements, D. L. and Conley, A. and Cooray, A. and Dowell, C. D. and Dwek, E. and Eales, S. and Franceschini, A. and Glenn, J. and Griffin, M. and Hatziminaoglou, E. and Ibar, E. and Isaak, K. and Ivison, R. J. and Lagache, G. and Levenson, L. and Lu, N. and Madden, S. and Maffei, B. and Mainetti, G. and Nguyen, H. T. and O'Halloran, B. and Page, M. J. and Panuzzo, P. and Papageorgiou, A. and Pearson, C. P. and Pérez-Fournon, I. and Pohlen, M. and Rigopoulou, D. and Rowan-Robinson, M. and Schulz, B. and Scott, D. and Seymour, N. and Shupe, D. L. and Smith, A. J. and Stevens, J. A. and Symeonidis, M. and Trichas, M. and Tugwell, K. E. and Vigroux, L. and Wang, L. and Wright, G. and Xu, C. K. and Zemcov, M. and Bardelli, S. and Carollo, M. and Contini, T. and Le Févre, O. and Lilly, S. and Mainieri, V. and Renzini, A. and Scodeggio, M. and Zucca, E.},\n\tmonth = jun,\n\tyear = {2013},\n\tkeywords = {cosmology: observations, galaxies: active, galaxies: evolution, galaxies: luminosity function, galaxies: starburst, infrared: galaxies, mass function},\n\tpages = {23--52},\n}\n\n","author_short":["Gruppioni, C.","Pozzi, F.","Rodighiero, G.","Delvecchio, I.","Berta, S.","Pozzetti, L.","Zamorani, G.","Andreani, P.","Cimatti, A.","Ilbert, O.","Le Floc'h, E.","Lutz, D.","Magnelli, B.","Marchetti, L.","Monaco, P.","Nordon, R.","Oliver, S.","Popesso, P.","Riguccini, L.","Roseboom, I.","Rosario, D. J.","Sargent, M.","Vaccari, M.","Altieri, B.","Aussel, H.","Bongiovanni, A.","Cepa, J.","Daddi, E.","Domínguez-Sánchez, H.","Elbaz, D.","Förster Schreiber, N.","Genzel, R.","Iribarrem, A.","Magliocchetti, M.","Maiolino, R.","Poglitsch, A.","Pérez García, A.","Sanchez-Portal, M.","Sturm, E.","Tacconi, L.","Valtchanov, I.","Amblard, A.","Arumugam, V.","Bethermin, M.","Bock, J.","Boselli, A.","Buat, V.","Burgarella, D.","Castro-Rodríguez, N.","Cava, A.","Chanial, P.","Clements, D. L.","Conley, A.","Cooray, A.","Dowell, C. D.","Dwek, E.","Eales, S.","Franceschini, A.","Glenn, J.","Griffin, M.","Hatziminaoglou, E.","Ibar, E.","Isaak, K.","Ivison, R. J.","Lagache, G.","Levenson, L.","Lu, N.","Madden, S.","Maffei, B.","Mainetti, G.","Nguyen, H. T.","O'Halloran, B.","Page, M. J.","Panuzzo, P.","Papageorgiou, A.","Pearson, C. P.","Pérez-Fournon, I.","Pohlen, M.","Rigopoulou, D.","Rowan-Robinson, M.","Schulz, B.","Scott, D.","Seymour, N.","Shupe, D. L.","Smith, A. J.","Stevens, J. A.","Symeonidis, M.","Trichas, M.","Tugwell, K. E.","Vigroux, L.","Wang, L.","Wright, G.","Xu, C. K.","Zemcov, M.","Bardelli, S.","Carollo, M.","Contini, T.","Le Févre, O.","Lilly, S.","Mainieri, V.","Renzini, A.","Scodeggio, M.","Zucca, E."],"key":"gruppioni_herschel_2013","id":"gruppioni_herschel_2013","bibbaseid":"gruppioni-pozzi-rodighiero-delvecchio-berta-pozzetti-zamorani-andreani-etal-theherschelpephermesluminosityfunctioniprobingtheevolutionofpacsselectedgalaxiestoz4-2013","role":"author","urls":{"Paper":"http://adsabs.harvard.edu/abs/2013MNRAS.432...23G"},"keyword":["cosmology: observations","galaxies: active","galaxies: evolution","galaxies: luminosity function","galaxies: starburst","infrared: galaxies","mass function"],"metadata":{"authorlinks":{}}},"bibtype":"article","biburl":"https://bibbase.org/zotero/polyphant","dataSources":["7gvjSdWrEu7z5vjjj"],"keywords":["cosmology: observations","galaxies: active","galaxies: evolution","galaxies: luminosity function","galaxies: starburst","infrared: galaxies","mass function"],"search_terms":["herschel","pep","hermes","luminosity","function","probing","evolution","pacs","selected","galaxies","gruppioni","pozzi","rodighiero","delvecchio","berta","pozzetti","zamorani","andreani","cimatti","ilbert","le floc'h","lutz","magnelli","marchetti","monaco","nordon","oliver","popesso","riguccini","roseboom","rosario","sargent","vaccari","altieri","aussel","bongiovanni","cepa","daddi","domínguez-sánchez","elbaz","förster schreiber","genzel","iribarrem","magliocchetti","maiolino","poglitsch","pérez garcía","sanchez-portal","sturm","tacconi","valtchanov","amblard","arumugam","bethermin","bock","boselli","buat","burgarella","castro-rodríguez","cava","chanial","clements","conley","cooray","dowell","dwek","eales","franceschini","glenn","griffin","hatziminaoglou","ibar","isaak","ivison","lagache","levenson","lu","madden","maffei","mainetti","nguyen","o'halloran","page","panuzzo","papageorgiou","pearson","pérez-fournon","pohlen","rigopoulou","rowan-robinson","schulz","scott","seymour","shupe","smith","stevens","symeonidis","trichas","tugwell","vigroux","wang","wright","xu","zemcov","bardelli","carollo","contini","le févre","lilly","mainieri","renzini","scodeggio","zucca"],"title":"The Herschel PEP/HerMES luminosity function - I. Probing the evolution of PACS selected Galaxies to z ≃ 4","year":2013}