G
Gordon J. Stacey
Researcher at Cornell University
Publications - 255
Citations - 12430
Gordon J. Stacey is an academic researcher from Cornell University. The author has contributed to research in topics: Galaxy & Star formation. The author has an hindex of 55, co-authored 246 publications receiving 11784 citations. Previous affiliations of Gordon J. Stacey include Max Planck Society & Ames Research Center.
Papers
More filters
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
SWIRE: The SIRTF Wide-area InfraRed Extragalactic Survey
Carol J. Lonsdale,Harding E. Smith,M. Rowan-Robinson,Jason Surace,David L. Shupe,Cong Xu,Seb Oliver,Deborah Padgett,Fan Fang,Alberto Franceschini,Nick Gautier,Matthew Joseph Griffin,Frank J. Masci,Glenn Morrison,JoAnn O'Linger,Ismael Perez-Fournon,Marguerite Pierre,Richard C. Puetter,Gordon J. Stacey +18 more
TL;DR: The SIRTF Wide-area InfraRed Extragalactic Survey (SWIRE) as discussed by the authors is the largest survey to date to trace the evolution of galaxies, star-forming galaxies, evolved stellar populations, and AGN.
Journal ArticleDOI
The 158 micron forbidden C II line - A measure of global star formation activity in galaxies
Gordon J. Stacey,Norbert Geis,Reinhard Genzel,J. B. Lugten,Albrecht Poglitsch,Amiel Sternberg,Charles H. Townes +6 more
TL;DR: In this paper, some 158 micron (CII) fine structure line observations from a sample of fourteen gas rich galaxies are reported. And the results confirm and generalize previous basic results that the (cII) line is bright amounting to approximately 0.1 to 1 percent of the Far Infra Red (FIR) luminosity of the nuclear regions of galaxies.
Journal ArticleDOI
Far-Infrared Spectroscopy of Normal Galaxies: Physical Conditions in the Interstellar Medium
Sangeeta Malhotra,Michael J. Kaufman,Michael J. Kaufman,David Hollenbach,George Helou,Robert H. Rubin,J. Brauher,Daniel A. Dale,N. Y. Lu,S. D. Lord,Gordon J. Stacey,Alessandra Contursi,Deidre A. Hunter,Harriet L. Dinerstein +13 more
TL;DR: In this paper, the authors present measurements by the Infrared Space Observatory Long Wavelength Spectrometer of seven lines from neutral and ionized ISM of 60 normal, star-forming galaxies.
Journal ArticleDOI
Far Infrared Spectroscopy of Normal Galaxies: Physical Conditions in the Interstellar Medium
Sangeeta Malhotra,Michael J. Kaufman,D. J. Hollenbach,George Helou,Robert H. Rubin,J. Brauher,Daniel A. Dale,N. Y. Lu,S. D. Lord,Gordon J. Stacey,A. Contursi +10 more
TL;DR: The most important cooling lines of the neutral interstellar medium (ISM) lie in the far-infrared (FIR) as discussed by the authors, and the results of the measurements by the Infrared Space Observatory Long Wavelength Spectrometer of seven lines from neutral and ionized ISM of 60 normal, star-forming galaxies.