J
J.M. Gales
Researcher at Goddard Space Flight Center
Publications - 4
Citations - 1941
J.M. Gales is an academic researcher from Goddard Space Flight Center. The author has contributed to research in topics: Galactic plane & Micrometre. The author has an hindex of 3, co-authored 4 publications receiving 1695 citations.
Papers
More filters
Journal ArticleDOI
The Cosmic Microwave Background spectrum from the full COBE FIRAS data set
TL;DR: In this article, the Far-InfraRed Absolute Spectrophotometer (FIRAS) on board the COBE (COsmic Background Explorer) is used to measure the difference between the cosmic microwave background and a precise blackbody spectrum.
Journal ArticleDOI
Morphology of the interstellar cooling lines detected by cobe
Charles L. Bennett,Dale J. Fixsen,Gary Hinshaw,John C. Mather,S. H. Moseley,Edward L. Wright,R. E. Eplee,J.M. Gales,Tilak Hewagama,R. B. Isaacman,Richard A. Shafer,Kevin R. Turpie +11 more
TL;DR: In this article, the results of an unbiased survey of far-infrared emission from the COBE satellite were reported, which includes emission lines from 158 micrometer C(+), 122 and 205 micrometers N(+), 370 and 609 micromer C(0), and CO J = 2 goes to 1 through J = 5 goes to 4.
Journal ArticleDOI
The Cosmic Microwave Background Spectrum from the Full COBE/FIRAS Data Set
TL;DR: In this paper, the Far InfraRed Absolute Spectrophotometer (FIRAS) on board the COBE (COsmic Background Explorer) was used to measure the difference between the cosmic microwave background and a precise blackbody spectrum.
Journal ArticleDOI
Morphology of the Interstellar Cooling Lines Detected by COBE
Charles L. Bennett,Dale J. Fixsen,Gary Hinshaw,John C. Mather,S. H. Moseley,Edward L. Wright,R. E. Eplee,J.M. Gales,Tilak Hewagama,R. B. Isaacman,Richard A. Shafer,Kevin R. Turpie +11 more
TL;DR: In this paper, the results of an unbiased survey of the far-infrared emission from the COBE satellite were reported, which includes emission lines from 158 um C+, 122 um and 205 um N+, 370 um and 609 um C, and CO J=2-1 through 5-4.