PACS Evolutionary Probe (PEP) – a Herschel key program
Dieter Lutz,Albrecht Poglitsch,Bruno Altieri,Paola Andreani,Paola Andreani,Herve Aussel,S. Berta,Ángel Bongiovanni,Ángel Bongiovanni,Drew Brisbin,Antonio Cava,J. Cepa,J. Cepa,Andrea Cimatti,Emanuele Daddi,H. Dominguez-Sanchez,David Elbaz,N. M. Förster Schreiber,Reinhard Genzel,Andrea Grazian,Carlotta Gruppioni,Martin Harwit,E. Le Floc'h,Georgios E. Magdis,Benjamin Magnelli,Roberto Maiolino,Raanan Nordon,A. M. Pérez García,A. M. Pérez García,Paola Popesso,Francesca Pozzi,L. Riguccini,Giulia Rodighiero,Amélie Saintonge,M. Sanchez Portal,Paola Santini,Lijing Shao,E. Sturm,Linda J. Tacconi,Ivan Valtchanov,M. Wetzstein,E. Wieprecht +41 more
TLDR
The PACS Evolutionary Probe (PEP) guaranteed time key program as discussed by the authors has been used in the entire set of Herschel surveys, and the field selection that includes popular multi-wavelength fields such as GOODS, COSMOS, Lockman Hole, ECDFS, and EGS.Abstract:
Deep far-infrared photometric surveys studying galaxy evolution and the nature of the cosmic infrared background are a key strength of the Herschel mission. We describe the scientific motivation for the PACS Evolutionary Probe (PEP) guaranteed time key program and its role within the entire set of Herschel surveys, and the field selection that includes popular multiwavelength fields such as GOODS, COSMOS, Lockman Hole, ECDFS, and EGS. We provide an account of the observing strategies and data reduction methods used. An overview of first science results illustrates the potential of PEP in providing calorimetric star formation rates for high-redshift galaxy populations, thus testing and superseding previous extrapolations from other wavelengths, and enabling a wide range of galaxy evolution studies.read more
Citations
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Book ChapterDOI
The Neogene Period
TL;DR: An Astronomically Tuned Neogene Time Scale (ATNTS2012) is presented in this article, as an update of ATNTS2004 in GTS2004, and the numerical ages are identical or almost so.
Journal ArticleDOI
The COSMOS2015 Catalog: Exploring the 1 < z < 6 Universe with Half a Million Galaxies
Clotilde Laigle,H. J. McCracken,O. Ilbert,Bau-Ching Hsieh,I. Davidzon,Peter Capak,Guenther Hasinger,John D. Silverman,Christophe Pichon,Jean Coupon,Herve Aussel,D. Le Borgne,Karina Caputi,Paolo Cassata,Yu-Yen Chang,Francesca Civano,James Dunlop,Johan P. U. Fynbo,Jeyhan S. Kartaltepe,Anton M. Koekemoer,O. Le Fèvre,E. Le Floc'h,Alexie Leauthaud,Simon J. Lilly,Lihwai Lin,Stefano Marchesi,Bo Milvang-Jensen,Mara Salvato,David B. Sanders,N. Z. Scoville,Vernesa Smolčić,M. Stockmann,Yoshiaki Taniguchi,Lidia Tasca,Sune Toft,Mattia Vaccari,Johannes Zabl +36 more
TL;DR: The COSMOS2015(24) catalog as mentioned in this paper contains precise photometric redshifts and stellar masses for more than half a million objects over the 2deg(2) COSmOS field, which is highly optimized for the study of galaxy evolution and environments in the early universe.
Journal ArticleDOI
The Lesser Role of Starbursts in Star Formation at z = 2
Giulia Rodighiero,Emanuele Daddi,Ivano Baronchelli,Andrea Cimatti,Alvio Renzini,Herve Aussel,P. Popesso,Dieter Lutz,Paola Andreani,S. Berta,Antonio Cava,David Elbaz,A. Feltre,Adriano Fontana,N. M. Förster Schreiber,Alberto Franceschini,Reinhard Genzel,Andrea Grazian,Carlotta Gruppioni,O. Ilbert,E. Le Floc'h,Georgios E. Magdis,Georgios E. Magdis,M. Magliocchetti,Benjamin Magnelli,Roberto Maiolino,H. J. McCracken,Raanan Nordon,Albrecht Poglitsch,P. Santini,Francesca Pozzi,L. Riguccini,Linda J. Tacconi,Stijn Wuyts,G. Zamorani +34 more
TL;DR: In this article, the relative contribution of star formation rate (SFR)-driven and starburst-driven galaxies to the global SFR density in the redshift interval 1.5 1000 M ☉ yr-1 was quantified.
Journal ArticleDOI
The Herschel Multi-tiered Extragalactic Survey: HerMES
Seb Oliver,James J. Bock,James J. Bock,Bruno Altieri,Alexandre Amblard,V. Arumugam,Herve Aussel,Tom Babbedge,Alexandre Beelen,Matthieu Béthermin,Matthieu Béthermin,Andrew Blain,Alessandro Boselli,C. Bridge,Drew Brisbin,V. Buat,Denis Burgarella,N. Castro-Rodríguez,N. Castro-Rodríguez,Antonio Cava,P. Chanial,Michele Cirasuolo,David L. Clements,A. Conley,L. Conversi,Asantha Cooray,Asantha Cooray,C. D. Dowell,C. D. Dowell,Elizabeth Dubois,Eli Dwek,Simon Dye,Stephen Anthony Eales,David Elbaz,Duncan Farrah,A. Feltre,P. Ferrero,P. Ferrero,N. Fiolet,N. Fiolet,M. Fox,Alberto Franceschini,Walter Kieran Gear,E. Giovannoli,Jason Glenn,Yan Gong,E. A. González Solares,Matthew Joseph Griffin,Mark Halpern,Martin Harwit,Evanthia Hatziminaoglou,Sebastien Heinis,Peter Hurley,Ho Seong Hwang,A. Hyde,Edo Ibar,O. Ilbert,K. G. Isaak,Rob Ivison,Rob Ivison,Guilaine Lagache,E. Le Floc'h,L. R. Levenson,L. R. Levenson,B. Lo Faro,Nanyao Y. Lu,S. C. Madden,Bruno Maffei,Georgios E. Magdis,G. Mainetti,Lucia Marchetti,G. Marsden,J. Marshall,J. Marshall,A. M. J. Mortier,Hien Nguyen,Hien Nguyen,B. O'Halloran,Alain Omont,Mat Page,P. Panuzzo,Andreas Papageorgiou,H. Patel,Chris Pearson,Chris Pearson,Ismael Perez-Fournon,Ismael Perez-Fournon,Michael Pohlen,Jonathan Rawlings,Gwenifer Raymond,Dimitra Rigopoulou,Dimitra Rigopoulou,L. Riguccini,D. Rizzo,Giulia Rodighiero,Isaac Roseboom,Isaac Roseboom,Michael Rowan-Robinson,M. Sanchez Portal,Benjamin L. Schulz,Douglas Scott,Nick Seymour,Nick Seymour,D. L. Shupe,A. J. Smith,Jamie Stevens,M. Symeonidis,Markos Trichas,K. E. Tugwell,Mattia Vaccari,Ivan Valtchanov,Joaquin Vieira,Marco P. Viero,L. Vigroux,Lifan Wang,Robyn L. Ward,Julie Wardlow,G. Wright,C. K. Xu,Michael Zemcov,Michael Zemcov +120 more
TL;DR: The Herschel Multi-tiered Extragalactic Survey (HerMES) is a legacy program designed to map a set of nested fields totalling ∼380deg^2 as mentioned in this paper.
Journal ArticleDOI
GALAXY STRUCTURE AND MODE OF STAR FORMATION IN THE SFR-MASS PLANE FROM z ∼ 2.5 TO z ∼ 0.1
Stijn Wuyts,Natascha M. Förster Schreiber,Arjen van der Wel,Benjamin Magnelli,Yicheng Guo,Reinhard Genzel,Dieter Lutz,Herve Aussel,Guillermo Barro,Stefano Berta,Antonio Cava,Javier Graciá-Carpio,Nimish P. Hathi,Kuang-Han Huang,Dale D. Kocevski,Anton M. Koekemoer,Kyoung-Soo Lee,Emeric Le Floc'h,Elizabeth J. McGrath,Raanan Nordon,Paola Popesso,Francesca Pozzi,L. Riguccini,Giulia Rodighiero,Amélie Saintonge,Linda J. Tacconi +25 more
TL;DR: In this article, the dependence of galaxy structure (size and Sersic index) and mode of star formation (ΣSFR and SFRIR/SFRUV) on the position of galaxies in the star formation rate (SFR) versus mass diagram is analyzed.
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TL;DR: The Spectral and Photometric Imaging REceiver (SPIRE) is the Herschel Space Observatory's sub-millimetre camera and spectrometer as discussed by the authors, which is used for image and spectroscopic data acquisition.
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