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1
Secrets of the Hoary Deep: A Personal History of Modern ...
“The Chandra Deep Field South: The 1 million second exposure.” Astrophysical Journal 566:667–674. 4. P. Tozzi and the CDFS Team. 2001. “New results of x-ray and optical survey of the Chandra Deep Field South: The 300,000 seconds ...
2
Extragalactic Astronomy and Cosmology: An Introduction - Page 599
5.4.3) CBI – Cosmic Background Imager (Sect.8.6.5) CCAT – Cerro Chajnantor Atacama Telescope (Chap. 11) CCD – Charge Coupled Device CDF – Chandra Deep Field (Sect. 9.2.1) CDM – Cold Dark Matter (Sect. 7.4.1) CERN – Conseil ...
3
Physics of Active Galactic Nuclei at all Scales - Page 187
Some Deep X-ray Surveys with Chandra and XMM-Newton Survey Name Exposure Representative Reference or Note Chandra Chandra Deep Field-North 1950 ks D.M. Alexander et al., 2003, AJ, 126, 539 Chandra Deep Field-South 940 ks ...
Danielle Alloin, Rachel Johnson, Paulina Lira, 2006
4
Modern Multivariate Statistical Techniques: Regression, ... - Page 217
Variables used to analyze 3,^38 galaxies from the Chandra Deep Field South area of the sky. The variables are divided into r = 23 X -variables and s = 6 Y -variables. X-variables UjMag, BjMag, VjMag, usMag, gsMag, rsMag. UbMag, BbMag ...
5
Growing Black Holes: Accretion in a Cosmological Context: ...
I present here the first estimates of the spatial correlation function of X-ray selected AGN in the 2Msec Chandra Deep Field North (CDFN) and IMsec Chandra Deep Field South (CDFS). The AGN clustering amplitude, measured for sources with ...
Andrea Merloni, Sergei V. Nayakshin, Rashid A. Sunyaev, 2005
6
Statistical Challenges in Modern Astronomy V - Page 501
Chapter 52 Applying the Background-Source Separation Algorithm to Chandra Deep Field South Data F. Guglielmetti, H. B ̈ohringer, R. Fischer, P. Rosati, and P. Tozzi Abstract A probabilistic two-component mixture model allows one to ...
Eric D. Feigelson, Jogesh Babu, 2012
7
New X-ray results, the next generation of X-ray ...
The Chandra Deep Field North Survey. XIV. X-ray detected obscured AGNs and starburst galaxies in the bright subinm source population. Astron. J., in press, 2003a. Alexander, D.M., Bauer, F.E., Brandt, W.N., et al. The Chandra Deep Field ...
C. Done, COSPAR. Scientific Assembly, 2004
8
The Evolution of Galaxies: III — From Simple Approaches to ...
2001, The chandra deep field north survey: VII. X-ray emission from Lyman break galaxies, Astrophys. J. 558, L5–8,. Ghosh, K. and White, N.: 2001, X-ray probes of cosmic star formation history, Astrophys. J. 559, L97–100. Hornschemeier ...
G. Hensler, G. Stasinska, S. Harfst, 2013
9
Astrophysics Update - Page 178
(2002) The 60//m Extragalactic Background Radiation Intensity, Dust-Enshrouded Active Galactic Nuclei and the Assembly of Groups and Clusters of Galaxies MNRAS 333 222 Brandt WN (2001) The Chandra Deep Field North Survey. V. 1 Ms ...
10
Lighthouses of the Universe: The Most Luminous Celestial ... - Page 573
The lMsec observation of the Chandra Deep Field South (CDFS) has almost entirely resolved into single sources the hard X-ray background as measured by the HEAO-1 A2 experiment. The main population of sources, as determined by the ...
Marat Gilfanov, Rashid Sunyaev, Eugene Churazov, 2002
