Open AccessJournal Article
The cosmic star formation history
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In this article, a model for calculating the cosmic star formation rate density history in a hierarchical A Cold Dark Matter (ACDM) universe is presented and compared with the model presented in this paper.Abstract:
Resumen en: A model for calculating the cosmic star formation rate density history in a hierarchical A Cold Dark Matter (ACDM) universe is presented and compared wit...read more
Citations
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Journal ArticleDOI
Constraining the galaxy–halo connection over the last 13.3 Gyr: star formation histories, galaxy mergers and structural properties
Aldo Rodríguez-Puebla,Aldo Rodríguez-Puebla,Joel R. Primack,Vladimir Avila-Reese,S. M. Faber +4 more
TL;DR: In this article, the stellar-to-halo mass relation (SHMR) at 0-10 degrees of freedom was determined to match the evolution of the galaxy stellar mass function, the SFR-M_*$ relation, and the cosmic star formation rate.
Journal ArticleDOI
The ALPINE-ALMA [CII] survey. Survey strategy, observations, and sample properties of 118 star-forming galaxies at 4 < z < 6
O. Le Fevre,M. Bethermin,Andreas L. Faisst,G. C. Jones,Peter Capak,Peter Capak,Paolo Cassata,John D. Silverman,Daniel Schaerer,Daniel Schaerer,Lin Yan,Ricardo Amorín,S. Bardelli,Médéric Boquien,Andrea Cimatti,Miroslava Dessauges-Zavadsky,Mauro Giavalisco,Nimish P. Hathi,Y. Fudamoto,Y. Fudamoto,Seiji Fujimoto,Michele Ginolfi,Carlotta Gruppioni,Shoubaneh Hemmati,Edo Ibar,Anton M. Koekemoer,Y. Khusanova,G. Lagache,Brian C. Lemaux,F. Loiacono,Roberto Maiolino,Chiara Mancini,Desika Narayanan,L. Morselli,H. Mendez-Hernandez,Pascal Oesch,Francesca Pozzi,M. Romano,Dominik Riechers,Dominik Riechers,Nick Scoville,Margherita Talia,L. A. M. Tasca,R. Thomas,Sune Toft,Livia Vallini,D. Vergani,Fabian Walter,G. Zamorani,E. Zucca +49 more
TL;DR: The ALMA-ALPINE [CII] survey (A2C2S) aims at characterizing the properties of a sample of normal star-forming galaxies (SFGs).
Journal ArticleDOI
Strong dependence of Type Ia supernova standardization on the local specific star formation rate
Mickael Rigault,V. Brinnel,Greg Aldering,P. Antilogus,Cecilia Aragon,Stephen Bailey,C. Baltay,K. Barbary,S. Bongard,Kyle Boone,Kyle Boone,C. Buton,M. Childress,N. Chotard,Y. Copin,S. Dixon,Parker Fagrelius,Parker Fagrelius,U. Feindt,Dominique Fouchez,E. Gangler,Brian Hayden,Wolfgang Hillebrandt,Dale Andrew Howell,Dale Andrew Howell,A. G. Kim,Marek Kowalski,D. Kuesters,P.-F. Leget,S. Lombardo,Q. Lin,Jakob Nordin,Reynald Pain,Emmanuel Pecontal,R. Pereira,Saul Perlmutter,Saul Perlmutter,David Rabinowitz,K. Runge,David Rubin,David Rubin,C. Saunders,G. Smadja,Caroline Sofiatti,Caroline Sofiatti,Nao Suzuki,Nao Suzuki,S. Taubenberger,S. Taubenberger,Charling Tao,R. C. Thomas +50 more
TL;DR: In this article, a large sample of nearby Type Ia supernovae (SN Ia) is classified into those that are located in predominantly younger or older environments, based on the specific star formation rate measured within a projected distance of 1 kpc from each SN location.
Journal ArticleDOI
Constraining the primordial black hole scenario with Bayesian inference and machine learning: The GWTC-2 gravitational wave catalog
Kaze W. K. Wong,Gabriele Franciolini,Valerio De Luca,Vishal Baibhav,Emanuele Berti,Paolo Pani,Antonio Riotto +6 more
TL;DR: The authors constrain primordial black hole formation models within a hierarchical Bayesian inference framework based on deep learning techniques, finding best-fit values for distinctive features of these models, including the PBH initial mass function, the fraction of PBHs in dark matter, and the accretion efficiency.
Journal ArticleDOI
The ALPINE-ALMA [CII] survey. Little to no evolution in the [CII]-SFR relation over the last 13 Gyr
Daniel Schaerer,Michele Ginolfi,M. Bethermin,Y. Fudamoto,Pascal Oesch,O. Le Fevre,Andreas L. Faisst,Peter Capak,Paolo Cassata,John D. Silverman,Lin Yan,G. C. Jones,Ricardo Amorín,S. Bardelli,Médéric Boquien,A. Cimatti,Miroslava Dessauges-Zavadsky,M. Giavalisco,Nimish P. Hathi,Seiji Fujimoto,E. Ibar,Anton M. Koekemoer,G. Lagache,Brian Lemaux,F. Loiacono,Roberto Maiolino,D. Narayanan,L. Morselli,H. Mendez-Hernandez,Francesca Pozzi,Dominik Riechers,Margherita Talia,S. Toft,Livia Vallini,D. Vergani,G. Zamorani,E. Zucca +36 more
TL;DR: In this article, a weak dependence of the SFR on the Lyman-alpha equivalent width of the [CII] 158 micron line was found for the ALPINE sources, which suggests no or little evolution of the L([CII])-SFR relation over the last 13 Gyr of cosmic time.
References
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Journal ArticleDOI
Formation of the first three gravitational-wave observations through isolated binary evolution
Simon Stevenson,Alejandro Vigna-Gómez,Ilya Mandel,Jim W. Barrett,Coenraad J. Neijssel,David T S Perkins,Selma E. de Mink +6 more
TL;DR: The rapid binary population synthesis code COMPAS is used to show that all three events can be explained by a single evolutionary channel—classical isolated binary evolution via mass transfer including a common envelope phase.
Journal ArticleDOI
Constraining the galaxy–halo connection over the last 13.3 Gyr: star formation histories, galaxy mergers and structural properties
Aldo Rodríguez-Puebla,Aldo Rodríguez-Puebla,Joel R. Primack,Vladimir Avila-Reese,S. M. Faber +4 more
TL;DR: In this article, the stellar-to-halo mass relation (SHMR) at 0-10 degrees of freedom was determined to match the evolution of the galaxy stellar mass function, the SFR-M_*$ relation, and the cosmic star formation rate.
Journal ArticleDOI
The ALPINE-ALMA [CII] survey. Survey strategy, observations, and sample properties of 118 star-forming galaxies at 4 < z < 6
O. Le Fevre,M. Bethermin,Andreas L. Faisst,G. C. Jones,Peter Capak,Peter Capak,Paolo Cassata,John D. Silverman,Daniel Schaerer,Daniel Schaerer,Lin Yan,Ricardo Amorín,S. Bardelli,Médéric Boquien,Andrea Cimatti,Miroslava Dessauges-Zavadsky,Mauro Giavalisco,Nimish P. Hathi,Y. Fudamoto,Y. Fudamoto,Seiji Fujimoto,Michele Ginolfi,Carlotta Gruppioni,Shoubaneh Hemmati,Edo Ibar,Anton M. Koekemoer,Y. Khusanova,G. Lagache,Brian C. Lemaux,F. Loiacono,Roberto Maiolino,Chiara Mancini,Desika Narayanan,L. Morselli,H. Mendez-Hernandez,Pascal Oesch,Francesca Pozzi,M. Romano,Dominik Riechers,Dominik Riechers,Nick Scoville,Margherita Talia,L. A. M. Tasca,R. Thomas,Sune Toft,Livia Vallini,D. Vergani,Fabian Walter,G. Zamorani,E. Zucca +49 more
TL;DR: The ALMA-ALPINE [CII] survey (A2C2S) aims at characterizing the properties of a sample of normal star-forming galaxies (SFGs).
Journal ArticleDOI
The ALPINE-ALMA [CII] survey: data processing, catalogs, and statistical source properties
Matthieu Béthermin,Y. Fudamoto,Michele Ginolfi,F. Loiacono,Y. Khusanova,Peter Capak,Peter Capak,Paolo Cassata,Andreas L. Faisst,O. Le Fèvre,Daniel Schaerer,Daniel Schaerer,John D. Silverman,Lin Yan,Ricardo Amorín,S. Bardelli,Médéric Boquien,Andrea Cimatti,Iary Davidzon,Iary Davidzon,Miroslava Dessauges-Zavadsky,Seiji Fujimoto,Carlotta Gruppioni,Nimish P. Hathi,Edo Ibar,G. C. Jones,Anton M. Koekemoer,Guilaine Lagache,Brian C. Lemaux,C. Moreau,Pascal Oesch,Pascal Oesch,Francesca Pozzi,Dominik A. Riechers,Dominik A. Riechers,Margherita Talia,Sune Toft,Livia Vallini,Daniela Vergani,G. Zamorani,E. Zucca +40 more
TL;DR: The Atacama Large Millimeter Array (ALMA) Large Program to Investigate [C II] at Early times (ALPINE) targets the 158 μm line and the far-infrared continuum in 118 spectroscopically confirmed star-forming galaxies as mentioned in this paper.
Journal ArticleDOI
Strong dependence of Type Ia supernova standardization on the local specific star formation rate
Mickael Rigault,V. Brinnel,Greg Aldering,P. Antilogus,Cecilia Aragon,Stephen Bailey,C. Baltay,K. Barbary,S. Bongard,Kyle Boone,Kyle Boone,C. Buton,M. Childress,N. Chotard,Y. Copin,S. Dixon,Parker Fagrelius,Parker Fagrelius,U. Feindt,Dominique Fouchez,E. Gangler,Brian Hayden,Wolfgang Hillebrandt,Dale Andrew Howell,Dale Andrew Howell,A. G. Kim,Marek Kowalski,D. Kuesters,P.-F. Leget,S. Lombardo,Q. Lin,Jakob Nordin,Reynald Pain,Emmanuel Pecontal,R. Pereira,Saul Perlmutter,Saul Perlmutter,David Rabinowitz,K. Runge,David Rubin,David Rubin,C. Saunders,G. Smadja,Caroline Sofiatti,Caroline Sofiatti,Nao Suzuki,Nao Suzuki,S. Taubenberger,S. Taubenberger,Charling Tao,R. C. Thomas +50 more
TL;DR: In this article, a large sample of nearby Type Ia supernovae (SN Ia) is classified into those that are located in predominantly younger or older environments, based on the specific star formation rate measured within a projected distance of 1 kpc from each SN location.