G. W. Wilson
University of Massachusetts Amherst
62 Papers
2.4K Citations
G. W. Wilson is an academic researcher from University of Massachusetts Amherst. The author has contributed to research in topics: Galaxy & Redshift. The author has an hindex of 28, co-authored 62 publications.
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Papers
GOODS–Herschel: an infrared main sequence for star-forming galaxies
David Elbaz,Mark Dickinson,Ho Seong Hwang,Tanio Díaz-Santos,Georgios E. Magdis,Benjamin Magnelli,D. Le Borgne,Frédéric Galliano,Maurilio Pannella,P. Chanial,Lee Armus,Vassilis Charmandaris,Vassilis Charmandaris,Emanuele Daddi,Herve Aussel,P. Popesso,Jeyhan S. Kartaltepe,Bruno Altieri,Ivan Valtchanov,D. Coia,Helmut Dannerbauer,Kalliopi Dasyra,Roger Leiton,Roger Leiton,Joseph M. Mazzarella,David M. Alexander,V. Buat,Denis Burgarella,R.-R. Chary,Roberto Gilli,Rob Ivison,Rob Ivison,Stéphanie Juneau,E. Le Floc'h,Dieter Lutz,G. E. Morrison,James Mullaney,Eric J. Murphy,Alexandra Pope,Douglas Scott,Mark Brodwin,Daniela Calzetti,C. Cesarsky,Stéphane Charlot,Herve Dole,Peter Eisenhardt,Henry C. Ferguson,N. M. Förster Schreiber,Dave Frayer,Mauro Giavalisco,Minh Huynh,Anton M. Koekemoer,Casey Papovich,Naveen A. Reddy,Christian Surace,Harry I. Teplitz,Min S. Yun,G. W. Wilson +57 more
TL;DR: In this paper, the authors examined the infrared (IR) 3-500μm spectral energy distributions (SEDs) of galaxies at 0 < z < 2.5, supplemented by a local reference sample from IRAS, ISO, Spitzer, and AKARI data.
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GOODS-Herschel: an infrared main sequence for star-forming galaxies
David Elbaz,Mark Dickinson,Ho Seong Hwang,Tanio Díaz-Santos,Georgios E. Magdis,Benjamin Magnelli,D. Le Borgne,Frédéric Galliano,Maurilio Pannella,P. Chanial,Lee Armus,Vassilis Charmandaris,Emanuele Daddi,Herve Aussel,P. Popesso,Jeyhan S. Kartaltepe,Bruno Altieri,Ivan Valtchanov,D. Coia,Helmut Dannerbauer,Kalliopi Dasyra,Roger Leiton,Joseph M. Mazzarella,V. Buat,Denis Burgarella,Roberto Gilli,Rob Ivison,Stéphanie Juneau,E. LeFloch,Dieter Lutz,G. E. Morrison,James Mullaney,Eric J. Murphy,Alexandra Pope,Douglas Scott,David M. Alexander,Mark Brodwin,Daniela Calzetti,C. J. Cesarsky,Stéphane Charlot,H. Dole,Peter Eisenhardt,Henry C. Ferguson,N. Foerster-Schreiber,Dave Frayer,Mauro Giavalisco,Minh Huynh,Anton M. Koekemoer,Casey Papovich,Naveen A. Reddy,Christian Surace,Harry Teplitz,Min S. Yun,G. W. Wilson +53 more
TL;DR: In this article, deep far-IR observations obtained with Herschel and examined the 3-500um SEDs of galaxies at 0 3x10^10 Lsun kpc^-2 and a high specific SFR (i.e., SBs).
AzTEC millimetre survey of the COSMOS field – III. Source catalogue over 0.72 deg2 and plausible boosting by large-scale structure
Itziar Aretxaga,G. W. Wilson,E. Aguilar,Stacey Alberts,Kimberly S. Scott,Nick Scoville,M. S. Yun,Jason E. Austermann,T. P. Downes,Hajime Ezawa,B. Hatsukade,David H. Hughes,Ryohei Kawabe,Kotaro Kohno,T. Oshima,Thushara Perera,Yoichi Tamura,Milagros Zeballos +17 more
TL;DR: In this paper, the authors presented a 0.72 deg^2 contiguous 1.1-mm survey in the central area of the Cosmological Evolution Survey field carried out to a 1σ ≈ 1.26 mJy beam^(−1) depth with the AzTEC camera mounted on the 10m Atacama Submillimeter Telescope Experiment.
Deep 1.1 mm-wavelength imaging of the GOODS-S field by AzTEC/ASTE – II. Redshift distribution and nature of the submillimetre galaxy population
M. S. Yun,Kimberly S. Scott,Yicheng Guo,Itziar Aretxaga,Mauro Giavalisco,Jason E. Austermann,Peter Capak,Yuxi Chen,Hajime Ezawa,Bunyo Hatsukade,David H. Hughes,Daisuke Iono,Seth Johnson,Ryohei Kawabe,Kotaro Kohno,James D. Lowenthal,Neal A. Miller,G. E. Morrison,T. Oshima,Thushara Perera,Mara Salvato,John D. Silverman,Yoichi Tamura,Christina C. Williams,G. W. Wilson +24 more
TL;DR: The results of the counterpart identification and a detailed analysis of the physical properties of the 48 sources discovered in our deep 1.1-mm wavelength imaging survey of the Great Observatories Origins Deep Survey-South (GOODS-S) field using the AzTEC instrument on the Atacama Submillimeter Telescope Experiment were reported in this article.
The Atacama Cosmology Telescope: a measurement of the 600 < ℓ < 8000 cosmic microwave background power spectrum at 148 GHz
Joseph W. Fowler,Viviana Acquaviva,Viviana Acquaviva,Peter A. R. Ade,Paula Aguirre,Mandana Amiri,John W. Appel,L. F. Barrientos,Elia S. Battistelli,Elia S. Battistelli,J. R. Bond,Ben Brown,B. Burger,Jay Chervenak,Sudeep Das,Sudeep Das,Mark J. Devlin,Simon Dicker,William B. Doriese,Jo Dunkley,Jo Dunkley,Rolando Dünner,Thomas Essinger-Hileman,R. P. Fisher,Amir Hajian,Mark Halpern,Matthew Hasselfield,C. Hernández-Monteagudo,Gene C. Hilton,Matt Hilton,Adam D. Hincks,Renée Hlozek,Kevin M. Huffenberger,David H. Hughes,John P. Hughes,Leopoldo Infante,Kent D. Irwin,Raul Jimenez,J. B. Juin,Madhuri Kaul,Jacob Klein,Arthur Kosowsky,Judy M. Lau,Judy M. Lau,Michele Limon,Michele Limon,Michele Limon,Y-T. Lin,Y-T. Lin,Y-T. Lin,Robert H. Lupton,Tobias A. Marriage,Danica Marsden,Krista Martocci,Philip Daniel Mauskopf,Felipe Menanteau,Kavilan Moodley,H. Moseley,Calvin B. Netterfield,Michael D. Niemack,Michael D. Niemack,M. R. Nolta,L. A. Page,L. P. Parker,Bruce Partridge,Hernan Quintana,B. Reid,B. Reid,Neelima Sehgal,Neelima Sehgal,Jonathan Sievers,David N. Spergel,Suzanne T. Staggs,Daniel S. Swetz,Daniel S. Swetz,Eric R. Switzer,Robert Thornton,Robert Thornton,Hy Trac,Hy Trac,Carole Tucker,Licia Verde,Ryan Warne,G. W. Wilson,Edward J. Wollack,Yue Zhao +85 more
TL;DR: In this paper, the angular power spectrum of the cosmic microwave background (CMB) radiation observed at 148 GHz was measured using maps with 14 angular resolution made with data from the Atacama Cosmology Telescope (ACT).