G
Glen Petitpas
Researcher at Harvard University
Publications - 140
Citations - 7169
Glen Petitpas is an academic researcher from Harvard University. The author has contributed to research in topics: Galaxy & Submillimeter Array. The author has an hindex of 47, co-authored 134 publications receiving 6701 citations. Previous affiliations of Glen Petitpas include McMaster University & Smithsonian Institution.
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Journal ArticleDOI
A dust-obscured massive maximum-starburst galaxy at a redshift of 6.34
Dominik Riechers,Dominik Riechers,Charles M. Bradford,Charles M. Bradford,David L. Clements,C. D. Dowell,C. D. Dowell,Ismael Perez-Fournon,Ismael Perez-Fournon,Rob Ivison,Rob Ivison,Carrie Bridge,A. Conley,Hai Fu,Joaquin Vieira,Julie Wardlow,J. A. Calanog,Asantha Cooray,Asantha Cooray,Peter Hurley,R. Neri,Julia Kamenetzky,James E. Aguirre,Bruno Altieri,V. Arumugam,Dominic J. Benford,Matthieu Béthermin,Matthieu Béthermin,James J. Bock,James J. Bock,Denis Burgarella,A. Cabrera-Lavers,A. Cabrera-Lavers,Scott Chapman,Peter Timothy Cox,James Dunlop,L. Earle,Duncan Farrah,P. Ferrero,P. Ferrero,Alberto Franceschini,Raphael Gavazzi,Jason Glenn,E. A. González Solares,Mark Gurwell,Mark Halpern,Evanthia Hatziminaoglou,A. Hyde,Edo Ibar,Attila Kovács,Attila Kovács,M. Krips,Roxana Lupu,P. R. Maloney,P. Martinez-Navajas,P. Martinez-Navajas,Hideo Matsuhara,Eric J. Murphy,B. J. Naylor,H. T. Nguyen,H. T. Nguyen,Seb Oliver,Alain Omont,M. J. Page,Glen Petitpas,Naseem Rangwala,Isaac Roseboom,Isaac Roseboom,Douglas Scott,Anthony J. Smith,Johannes Staguhn,Johannes Staguhn,Alina Streblyanska,Alina Streblyanska,Alasdair Thomson,Ivan Valtchanov,Marco P. Viero,Lin Wang,Michael Zemcov,Michael Zemcov,Jonas Zmuidzinas,Jonas Zmuidzinas +81 more
TL;DR: Despite the overall downturn in cosmic star formation towards the highest redshifts, it seems that environments mature enough to form the most massive, intense starbursts existed at least as early as 880 million years after the Big Bang.
Journal ArticleDOI
Birth of a relativistic outflow in the unusual γ-ray transient Swift J164449.3+573451
B. A. Zauderer,Edo Berger,Alicia M. Soderberg,Abraham Loeb,Ramesh Narayan,Dale A. Frail,Glen Petitpas,Andreas Brunthaler,Ryan Chornock,John M. Carpenter,Guy G. Pooley,Kunal Mooley,Shrinivas R. Kulkarni,Raffaella Margutti,D. B. Fox,Ehud Nakar,Nimesh A. Patel,Nikolaus H. Volgenau,T. L. Culverhouse,Michael Bietenholz,Michael Bietenholz,Michael P. Rupen,Walter Max-Moerbeck,Anthony C. S. Readhead,Joseph L. Richards,Martin C. Shepherd,Shaye Storm,Charles L. H. Hull +27 more
TL;DR: It is concluded that the tidal disruption of a star naturally explains the observed high-energy properties and radio luminosity and the inferred rate of such events, and the weaker beaming in the radio-frequency spectrum relative to γ-rays or X-rays suggests that radio searches may uncover similar events out to redshifts of z ≈ 6.
Journal ArticleDOI
Luminous infrared galaxies with the submillimeter array. i. survey overview and the central gas to dust ratio
Christine D. Wilson,Christine D. Wilson,Glen Petitpas,Daisuke Iono,Andrew J. Baker,Alison B. Peck,Melanie Krips,B. E. Warren,J. Golding,Adam Atkinson,Lee Armus,Thomas J. Cox,Paul T. P. Ho,Paul T. P. Ho,Mika Juvela,Satoki Matsushita,J. Christopher Mihos,Ylva Pihlström,Min S. Yun +18 more
TL;DR: In this paper, the authors used the Submillimeter Array of 14 nearby luminous and ultraluminous infrared galaxies to measure an average gas-to-dust mass ratio of 120 ± 28 (rms deviation 109) in the central regions of these galaxies.
Journal ArticleDOI
Evidence for a Population of High-Redshift Submillimeter Galaxies from Interferometric Imaging
Joshua D. Younger,Giovanni G. Fazio,Jiasheng Huang,Min S. Yun,Grant W. Wilson,Matthew L. N. Ashby,Mark Gurwell,Kamson Lai,Alison B. Peck,Glen Petitpas,David J. Wilner,Daisuke Iono,Kotaro Kohno,Ryohei Kawabe,David H. Hughes,Itziar Aretxaga,T. M. A. Webb,Alejo Martinez-Sansigre,Sungeun Kim,Kimberly S. Scott,Jason E. Austermann,Thushara Perera,James D. Lowenthal,Eva Schinnerer,Vernesa Smolčić +24 more
TL;DR: In this article, the authors used the Submillimeter Array to image a flux-limited sample of seven submillimeter galaxies, selected by the AzTEC camera on the JCMT at 1.1 mm, in the COSMOS field at 890 μ m with ~2'' resolution.
Journal ArticleDOI
Luminous infrared galaxies with the submillimeter array. ii. comparing the co (3-2) sizes and luminosities of local and high-redshift luminous infrared galaxies
Daisuke Iono,Christine D. Wilson,Min S. Yun,Andrew J. Baker,Glen Petitpas,Alison B. Peck,Melanie Krips,Thomas J. Cox,Satoki Matsushita,J. Christopher Mihos,Ylva Pihlström +10 more
TL;DR: In this article, a detailed comparison of the CO (3-2) emitting molecular gas between a local sample of luminous infrared galaxies (U/LIRGs) and a high-redshift sample that comprises submm selected galaxies (SMGs), quasars, and Lyman Break Galaxies (LBGs).