scholarly journals GOODS-Herschel: identification of the individual galaxies responsible for the 80–290μm cosmic infrared background

2015 ◽  
Vol 579 ◽  
pp. A93 ◽  
Author(s):  
R. Leiton ◽  
D. Elbaz ◽  
K. Okumura ◽  
H. S. Hwang ◽  
G. Magdis ◽  
...  
2017 ◽  
Vol 95 (10) ◽  
Author(s):  
Masahiro Kawasaki ◽  
Alexander Kusenko ◽  
Lauren Pearce ◽  
Louis Yang

2006 ◽  
Vol 2 (14) ◽  
pp. 266-266
Author(s):  
Asantha R. Cooray

AbstractWe discuss anisotropies in the near-IR background between 1 to a few microns. This background is expected to contain a signature of primordial galaxies. We have measured fluctuations of resolved galaxies with Spitzer imaging data and we are developing a rocket-borne instrument (the Cosmic Infrared Background ExpeRiment, or CIBER) to search for signatures of primordial galaxy formation in the cosmic near-infrared extra-galactic background.


2010 ◽  
Author(s):  
Asantha Cooray ◽  
Jamie Bock ◽  
Mitsunobu Kawada ◽  
Brian Keating ◽  
Dae-Hee Lee ◽  
...  

2011 ◽  
Author(s):  
Michael Zemcov ◽  
Toshiaki Arai ◽  
John Battle ◽  
James Bock ◽  
Asantha Cooray ◽  
...  

1998 ◽  
Vol 508 (1) ◽  
pp. 25-43 ◽  
Author(s):  
M. G. Hauser ◽  
R. G. Arendt ◽  
T. Kelsall ◽  
E. Dwek ◽  
N. Odegard ◽  
...  

1996 ◽  
Author(s):  
Edward L. Wright ◽  
Michael Werner ◽  
George Rieke

2000 ◽  
Vol 174 ◽  
pp. 100-106
Author(s):  
S. Nishiura

AbstractThe compact group of galaxies “Seyfert’s Sextet” shows irregularly shaped soft X-ray morphology. In order to understand its origin, we have obtained a deep optical (VR + I) image of the group. Our image shows that a faint envelope surrounds the member galaxies. We find that optical and soft X-ray images are significantly similar in morphology. This similarity provides direct morphological evidence that the dark matter in Seyfert’s Sextet was originally associated with the individual galaxies and is now spreading out around the group.


Sign in / Sign up

Export Citation Format

Share Document