G
Grant R. Tremblay
Researcher at Harvard University
Publications - 198
Citations - 11622
Grant R. Tremblay is an academic researcher from Harvard University. The author has contributed to research in topics: Galaxy & Radio galaxy. The author has an hindex of 39, co-authored 179 publications receiving 9011 citations. Previous affiliations of Grant R. Tremblay include Rochester Institute of Technology & Space Telescope Science Institute.
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Journal ArticleDOI
Raining in MKW 3 s: A Chandra-MUSE Analysis of X-Ray Cold Filaments around 3CR 318.1
A. Jimenez-Gallardo,Francesco Massaro,B. Balmaverde,Alessandro Paggi,Alessandro Capetti,William R. Forman,R. P. Kraft,Ranieri D. Baldi,V. H. Mahatma,C. Mazzucchelli,V. Missaglia,F. Ricci,Giacomo Venturi,Stefi A. Baum,Elisabetta Liuzzo,C. P. O'Dea,M. A. Prieto,H. J. A. Röttgering,E. Sani,William B. Sparks,Grant R. Tremblay,R. J. van Weeren,B. Wilkes,Jeremy J. Harwood,Pasquale Mazzotta,Joanna Kuraszkiewicz +25 more
TL;DR: In this paper, the accepted manuscript version of an article which has been published in final form at https://doi.org/10.3847/2041-8213/abf6db
Posted Content
Understanding the circumgalactic medium is critical for understanding galaxy evolution
Molly S. Peeples,Peter Behroozi,Rongmon Bordoloi,Alyson Brooks,James S. Bullock,Joseph N. Burchett,Hsiao-Wen Chen,John Chisholm,Charlotte Christensen,Alison L. Coil,Lauren Corlies,Aleksandar M. Diamond-Stanic,Megan Donahue,Claude André Faucher-Giguère,Henry C. Ferguson,Drummond Fielding,Andrew J. Fox,David M. French,Steven R. Furlanetto,Mario Gennaro,Karoline M. Gilbert,Erika T. Hamden,Nimish P. Hathi,Matthew Hayes,Alaina Henry,J. Christopher Howk,Cameron Hummels,Dušan Kereš,Evan N. Kirby,Anton M. Koekemoer,Ting-Wen Lan,Lauranne Lanz,David R. Law,Nicolas Lehner,Jennifer M. Lotz,Crystal L. Martin,Kristen B. W. McQuinn,Matthew McQuinn,Ferah Munshi,S. Peng Oh,John M. O'Meara,Brian W. O'Shea,Camilla Pacifici,J. E. G. Peek,Marc Postman,Moire K. M. Prescott,Mary E. Putman,Eliot Quataert,Marc Rafelski,Joseph Ribaudo,Kate Rowlands,Kate H. R. Rubin,Brett Salmon,Claudia Scarlata,Alice E. Shapley,Raymond C. Simons,Gregory F. Snyder,Jonathan Stern,Allison L. Strom,Erik Tollerud,Paul Torrey,Grant R. Tremblay,Todd M. Tripp,Jason Tumlinson,Sarah Tuttle,Frank C. van den Bosch,G. Mark Voit,Q. Daniel Wang,Jessica K. Werk,Benjamin F. Williams,Dennis Zaritsky,Yong Zheng +71 more
TL;DR: In this article, the authors outline connections between the CGM and galactic star formation histories, internal kinematics, chemical evolution, quenching, satellite evolution, dark matter halo occupation, and the reionization of the larger scale intergalactic medium in light of the advances that will be made on these topics in the 2020s.
Posted Content
The First IFU Spectroscopic View of Shocked Cluster Galaxies
TL;DR: In this paper, the authors presented the first spatially resolved spectroscopic view of 5 H$\alpha$ emitting galaxies located in the wake of shock fronts in the low redshift (z~0.2), massive (~2$\times10^{15}$ M$_\odot$), post-core passage merging cluster, CIZA J2242.8+5301 (nicknamed the ''Sausage').
Journal ArticleDOI
Using Machine Learning to Determine Morphologies of z < 1 AGN Host Galaxies in the Hyper Suprime-Cam Wide Survey
Chuan Tian,C. Megan Urry,Aritra Ghosh,Ryan Ofman,Tonima Tasnim Ananna,C. Auge,Nico Cappelluti,Meredith Powell,David B. Sanders,Kevin Schawinski,Dominic Stark,Grant R. Tremblay +11 more
TL;DR: In this paper , the authors used PSFGAN to decouple host galaxy light from the central point source, then invoked the Galaxy Morphology Network (GaMorNet) to estimate whether the host galaxy is disk-dominated, bulge-dominated or indeterminate.
Posted Content
The Close AGN Reference Survey (CARS): Locating the [O III] wing component in luminous local Type 1 AGN
M. Singha,Bernd Husemann,Tanya Urrutia,C. P. O'Dea,J. Scharwächter,Massimo Gaspari,Francoise Combes,Rebecca Nevin,Bryan A. Terrazas,Miguel A. Pérez-Torres,Tom Rose,Timothy A. Davis,Grant R. Tremblay,Justus Neumann,I. Smirnova-Pinchukova,Stefi A. Baum +15 more
TL;DR: In this paper, the authors measured <100 pc offsets in the spatial location of the outflow from the AGN nucleus using the spectro-astrometry technique for these sources and concluded that [O III] wing emission can be compact or extended in an unbiased luminous AGN sample, where both cases are likely to appear.