M
Mark Sargent
Researcher at University of Sussex
Publications - 227
Citations - 17074
Mark Sargent is an academic researcher from University of Sussex. The author has contributed to research in topics: Galaxy & Star formation. The author has an hindex of 66, co-authored 217 publications receiving 14925 citations. Previous affiliations of Mark Sargent include ETH Zurich & DSM.
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Journal ArticleDOI
The Star Formation History of Mass-selected Galaxies in the COSMOS Field
A. Karim,A. Karim,Eva Schinnerer,A. Martinez-Sansigre,A. Martinez-Sansigre,A. Martinez-Sansigre,Mark Sargent,A. van der Wel,H. W. Rix,O. Ilbert,Vernesa Smolčić,Chris Carilli,Maurilio Pannella,Anton M. Koekemoer,Eric F. Bell,Mara Salvato +15 more
TL;DR: In this paper, the authors explore the redshift evolution of specific star formation rate (SSFR) for galaxies of different stellar mass by drawing on a deep 3.6 µm-selected sample of > 10 5 galaxies in the 2 deg 2 COSMOS field.
Journal ArticleDOI
The Herschel view of the dominant mode of galaxy growth from z = 4 to the present day
Corentin Schreiber,Maurilio Pannella,David Elbaz,Matthieu Béthermin,Hanae Inami,Mark Dickinson,Benjamin Magnelli,Tao Wang,Herve Aussel,Emanuele Daddi,Stéphanie Juneau,Xinwen Shu,Mark Sargent,Veronique Buat,Sandra M. Faber,Henry C. Ferguson,M. Giavalisco,Anton M. Koekemoer,Georgios E. Magdis,Glenn Morrison,Casey Papovich,Paola Santini,Douglas Scott +22 more
TL;DR: In this paper, the authors present an analysis of the deep Herschel images in four major extragalactic fields Goodfellow-Herschel, CANDELS, UDS, and COSMOS.
Journal ArticleDOI
The star formation history of mass-selected galaxies in the COSMOS field
Alexander Karim,Eva Schinnerer,A. Martinez-Sansigre,Mark Sargent,Arjen van der Wel,Hans-Walter Rix,Olivier Ilbert,Vernesa Smolčić,Chris Carilli,Maurilio Pannella,Anton M. Koekemoer,Eric F. Bell,Mara Salvato +12 more
TL;DR: In this paper, the authors explore the evolution of the specific star formation rate (SSFR) for 3.6um-selected galaxies of different M_* in the COSMOS field.
Journal ArticleDOI
The Evolving Interstellar Medium of Star-forming Galaxies since z = 2 as Probed by Their Infrared Spectral Energy Distributions
Georgios E. Magdis,Emanuele Daddi,Matthieu Béthermin,Mark Sargent,David Elbaz,Maurilio Pannella,Mark Dickinson,Helmut Dannerbauer,E. da Cunha,Fabian Walter,Dimitra Rigopoulou,Dimitra Rigopoulou,Vassilis Charmandaris,Ho Seong Hwang,Jeyhan S. Kartaltepe +14 more
TL;DR: In this article, the authors show that the variations of specific star formation rates (sSFRs = SFR/M*) are driven by varying gas fractions and that the hardness of the radiation field, which is proportional to the dust-mass-weighted luminosity (L IR/M dust) and the primary parameter defining the shape of the IR spectral energy distribution, is equivalent to SFE/Z.
Journal ArticleDOI
The Herschel* PEP/HerMES luminosity function - I. Probing the evolution of PACS selected Galaxies to z ≃ 4
Carlotta Gruppioni,Francesca Pozzi,Giulia Rodighiero,Ivan Delvecchio,S. Berta,Lucia Pozzetti,G. Zamorani,P. Andreani,Alessandro Cimatti,O. Ilbert,E. Le Floc'h,Dieter Lutz,Benjamin Magnelli,Lucia Marchetti,Lucia Marchetti,Pierluigi Monaco,Raanan Nordon,Seb Oliver,P. Popesso,L. Riguccini,Isaac Roseboom,Isaac Roseboom,David J. Rosario,Mark Sargent,Mattia Vaccari,Mattia Vaccari,Bruno Altieri,H. Aussel,Ángel Bongiovanni,J. Cepa,Emanuele Daddi,H. Dominguez-Sanchez,H. Dominguez-Sanchez,D. Elbaz,N. M. Foerster Schreiber,R. Genzel,Alvaro Iribarrem,M. Magliocchetti,Roberto Maiolino,Albrecht Poglitsch,A. M. Pérez García,M. Sánchez-Portal,Eckhard Sturm,Linda J. Tacconi,Ivan Valtchanov,Alexandre Amblard,V. Arumugam,M. Bethermin,James J. Bock,James J. Bock,A. Boselli,V. Buat,Denis Burgarella,N. Castro-Rodríguez,N. Castro-Rodríguez,Antonio Cava,P. Chanial,David L. Clements,A. Conley,Asantha Cooray,Asantha Cooray,C. D. Dowell,C. D. Dowell,Eli Dwek,Stephen Anthony Eales,Alberto Franceschini,Jason Glenn,Matthew Joseph Griffin,Evanthia Hatziminaoglou,Edo Ibar,K. G. Isaak,Rob Ivison,Rob Ivison,Guilaine Lagache,Louis Levenson,Louis Levenson,Nanyao Y. Lu,S. C. Madden,Bruno Maffei,G. Mainetti,H. T. Nguyen,H. T. Nguyen,B. O'Halloran,M. J. Page,P. Panuzzo,Andreas Papageorgiou,Chris Pearson,Chris Pearson,Ismael Perez-Fournon,Ismael Perez-Fournon,Michael Pohlen,Dimitra Rigopoulou,Dimitra Rigopoulou,Michael Rowan-Robinson,Benjamin L. Schulz,Douglas Scott,Nick Seymour,Nick Seymour,D. L. Shupe,Anthony J. Smith,Jamie Stevens,M. Symeonidis,Markos Trichas,K. E. Tugwell,L. Vigroux,Lian-Tao Wang,G. Wright,C. K. Xu,Michael Zemcov,Michael Zemcov,S. Bardelli,M. Carollo,Thierry Contini,O. Le Fevre,Simon J. Lilly,Vincenzo Mainieri,Alvio Renzini,Marco Scodeggio,E. Zucca +118 more
TL;DR: In this article, the authors exploit the deep and extended far-IR data sets (at 70, 100 and 160 μm) of the GPS 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 luminosity functions (LFs) up to z ∼ 4.