P
Perry B. Hacking
Researcher at Jet Propulsion Laboratory
Publications - 39
Citations - 2016
Perry B. Hacking is an academic researcher from Jet Propulsion Laboratory. The author has contributed to research in topics: Galaxy & Luminous infrared galaxy. The author has an hindex of 19, co-authored 39 publications receiving 1975 citations. Previous affiliations of Perry B. Hacking include California Institute of Technology.
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Journal ArticleDOI
SWIRE: The SIRTF Wide‐Area Infrared Extragalactic Survey
Carol J. Lonsdale,Harding E. Smith,M. Rowan-Robinson,Jason Surace,David L. Shupe,Cong Xu,Sebastian Oliver,Deborah L. Padgett,Fan Fang,Tim Conrow,Alberto Franceschini,Nick Gautier,Matthew Joseph Griffin,Perry B. Hacking,Frank J. Masci,Glenn Morrison,J. O'Linger,Frazer N. Owen,Ismael Perez-Fournon,Marguerite Pierre,R. C. Puetter,Gordon J. Stacey,Sandra Castro,Maria del Carmen Polletta,Duncan Farrah,Thomas H. Jarrett,Dave Frayer,Brian Siana,Tom Babbedge,Simon Dye,M. Fox,Eduardo Gonzalez-Solares,Malcolm Salaman,Stefano Berta,James J. Condon,Herve Dole,Steve Serjeant +36 more
TL;DR: The SIRTF Wide Area Infrared Extragalactic Survey (SWIRE) as discussed by the authors is a legacy program of the International Astronomical Union (IAU) that has been used to trace the evolution of galaxies, star forming and active galactic nuclei.
Journal ArticleDOI
A high-redshift IRAS galaxy with huge luminosity―hidden quasar or protogalaxy?
Michael Rowan-Robinson,Tom Broadhurst,Andy Lawrence,Richard G. McMahon,Carol J. Lonsdale,S. J. Oliver,A. N. Taylor,Perry B. Hacking,Perry B. Hacking,Tim Conrow,Tim Conrow,Will Saunders,Rowan Ellis,George Efstathiou,James J. Condon +14 more
TL;DR: In this article, the authors found an emission-line galaxy at a redshift of 2.286, and with the enormous far-infrared luminosity of 3 × 10^(14) times that of the Sun.
Journal ArticleDOI
The remarkable infrared galaxy ARP 220 = IC 4553
B. T. Soifer,G. Neugebauer,George Helou,C. J. Lonsdale,Perry B. Hacking,W. Rice,J. R. Houck,F. J. Low,M. Rowan-Robinson +8 more
TL;DR: The infrared-to-blue luminosity ratio of this galaxy is - 80, which is the largest value of the ratio for galaxies in the UGC catalog, and places it in the range of the "unidentified" infrared sources recently reported by Houck et al. in the IRAS all-sky survey as discussed by the authors.
Journal ArticleDOI
Emission Features and Source Counts of Galaxies in Mid-Infrared
Cong Xu,Perry B. Hacking,Fan Fang,David L. Shupe,Carol J. Lonsdale,Nanyao Y. Lu,George Helou,Gordon J. Stacey,Matthew L. N. Ashby +8 more
TL;DR: In this paper, the authors incorporated the newest ISO results on the mid-infrared spectral energy distribution (SED) of galaxies into models for the number counts and redshift distributions of MIR surveys.
Journal ArticleDOI
The ultraviolet-to-radio continuum of the ultraluminous galaxy IRAS F10214+4724.
M. Rowan-Robinson,Andreas Efstathiou,Andy Lawrence,S. J. Oliver,A. N. Taylor,Tom Broadhurst,Richard G. McMahon,C. R. Benn,James J. Condon,Carol J. Lonsdale,Perry B. Hacking,Tim Conrow,W. S. Saunders,D. L. Clements,Richard S. Ellis,Ian Robson +15 more
TL;DR: In this paper, the authors present new observations and theoretical models for the continuous ultraviolet-to-radio spectrum of the ultraluminous protogalaxy candidate IRAS F 10214 + 4724.