S
S. P. Willner
Researcher at Harvard University
Publications - 138
Citations - 10847
S. P. Willner is an academic researcher from Harvard University. The author has contributed to research in topics: Galaxy & Luminous infrared galaxy. The author has an hindex of 50, co-authored 138 publications receiving 10446 citations.
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Journal ArticleDOI
The Infrared Array Camera (IRAC) for the Spitzer Space Telescope
Giovanni G. Fazio,Joseph L. Hora,Lori E. Allen,M. L. N. Ashby,Pauline Barmby,Lynne K. Deutsch,Lynne K. Deutsch,J.-S. Huang,S. C. Kleiner,Massimo Marengo,S. T. Megeath,Gary J. Melnick,Michael A. Pahre,Brian M. Patten,J. Polizotti,Howard A. Smith,R. S. Taylor,Zhong Wang,S. P. Willner,William F. Hoffmann,Judy Pipher,William J. Forrest,C. W. McMurty,Craig R. McCreight,Mark E. McKelvey,Robert E. McMurray,David G. Koch,Samuel H. Moseley,R. G. Arendt,John Eric Mentzell,Catherine T. Marx,P. Losch,P. Mayman,W. Eichhorn,Danny J. Krebs,Murzy D. Jhabvala,Daniel Y. Gezari,D. J. Fixsen,J. Flores,K. Shakoorzadeh,R. Jungo,Claef Hakun,Lois G. Workman,Gabriel Karpati,R. Kichak,R. Whitley,S. Mann,Eric V. Tollestrup,Peter Eisenhardt,Daniel Stern,Varoujan Gorjian,Bidushi Bhattacharya,Sean Carey,Brant O. Nelson,William J. Glaccum,Mark Lacy,Patrick J. Lowrance,Seppo Laine,William T. Reach,J. A. Stauffer,Jason Surace,Gillian Wilson,Edward L. Wright,Alan W. Hoffman,George Domingo,Martin Cohen +65 more
TL;DR: The Infrared Array Camera (IRAC) is one of three focal plane instruments on the Spitzer Space Telescope as mentioned in this paper, which is a four-channel camera that obtains simultaneous broadband images at 3.6, 4.5, 5.8, and 8.0 m.
Mid-Infrared Selection of Active Galaxies
Daniel Stern,Peter Eisenhardt,V. Gorjian,Christopher S. Kochanek,Daniel J. Eisenstein,Pauline Barmby,Mark Brodwin,Michael J. I. Brown,Nelson Caldwell,R. Cool,Arjun Dey,Paul J. Green,Buell T. Jannuzi,S. S. Murray,Michael A. Pahre,S. P. Willner +15 more
Journal ArticleDOI
UBVRI Light Curves of 44 Type Ia Supernovae
Saurabh Jha,Saurabh Jha,Robert P. Kirshner,Peter Challis,Peter M. Garnavich,Thomas Matheson,Alicia M. Soderberg,Genevieve J. Graves,Malcolm Hicken,João Alves,Héctor G. Arce,Zoltan Balog,Pauline Barmby,Elizabeth J. Barton,Perry Berlind,Ann Bragg,Cesar Briceno,Warren R. Brown,J. H. Buckley,Nelson Caldwell,Michael L. Calkins,B. J. Carter,Kristi Dendy Concannon,R. Hank Donnelly,Kristoffer A. Eriksen,Daniel G. Fabricant,Emilio E. Falco,Fabrizio Fiore,Michael R. Garcia,Mercedes Gomez,Norman A. Grogin,Ted Groner,Paul J. Groot,Karl E. Haisch,Lee Hartmann,Carl Hergenrother,Matthew J. Holman,John P. Huchra,Ray Jayawardhana,D. Jerius,Sheila J. Kannappan,Dong-Woo Kim,Jan T. Kleyna,Christopher S. Kochanek,Daniel M. Koranyi,M. Krockenberger,Charles J. Lada,Kevin Luhman,Jane Luu,Lucas M. Macri,J. Mader,Andisheh Mahdavi,Massimo Marengo,Brian G. Marsden,Brian McLeod,Brian R. McNamara,S. Thomas Megeath,Dan Moraru,A. Mossman,August Muench,J. A. Muñoz,James Muzerolle,Orlando Naranjo,Kristin Nelson-Patel,Michael A. Pahre,Brian M. Patten,J. Peters,Wayne Peters,John C. Raymond,Kenneth J. Rines,Rudolph E. Schild,Gregory J. Sobczak,Timothy Spahr,John R. Stauffer,Robert P. Stefanik,Andrew Szentgyorgyi,Eric V. Tollestrup,Petri Vaisanen,Alexey Vikhlinin,Zhong Wang,S. P. Willner,Scott J. Wolk,Joseph Zajac,Ping Zhao,Krzysztof Z. Stanek +84 more
TL;DR: In this article, the authors present UBVRI photometry of 44 Type Ia supernovae (SNe Ia) observed from 1997 to 2001 as part of a continuing monitoring campaign at the Fred Lawrence Whipple Observatory of the Harvard-Smithsonian Center for Astrophysics.
Journal ArticleDOI
A Significant Population of Very Luminous Dust-Obscured Galaxies at Redshift z ~ 2
Arjun Dey,B. T. Soifer,Vandana Desai,Kate Brand,Emeric LeFloc'h,Michael J. I. Brown,Buell T. Jannuzi,Lee Armus,Shane Bussmann,Mark Brodwin,C. Bian,Peter Eisenhardt,Sarah J.U. Higdon,Daniel W. Weedman,S. P. Willner +14 more
TL;DR: In this paper, a simple method for selecting high-z population based solely on the ratio of the observed mid-IR 24um to optical R-band flux density was presented, revealing a significant population of high-redshift z~2 dust-obscured galaxies (DOGs) with large midIR to UV luminosity ratios.
Journal ArticleDOI
Number Counts at 3 μm < λ < 10 μm from the Spitzer Space Telescope
Giovanni G. Fazio,M. L. N. Ashby,Pauline Barmby,Joseph L. Hora,J.-S. Huang,Michael A. Pahre,Zhong Wang,S. P. Willner,R. G. Arendt,Samuel H. Moseley,Mark Brodwin,Peter Eisenhardt,Daniel Stern,E. V. Tollestrup,Edward L. Wright +14 more
TL;DR: In this paper, galaxy counts at 3.6 and 4.5μm were shown to follow the expectations of a Euclidean world model down to ~16.5 mag.