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Observing evolution in star-forming galaxies in x-rays
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Ptak, Andrew |
| Copyright Year | 2011 |
| Description | The Chandra Deep Fields (CDFs) have reached flux limits where normal/starburst galaxies are significant contributors to the X-ray number counts (approximately 40% at F _{0.5-2.0} = 1 x 10(^)-17). Based on these results and current theoretical models of X-ray binary evolution we will discuss expectations for observing galaxy evolution in X-rays in IXO deep surveys. With the high sensitivity of IXO (particularly approximately 5" resolution constant across the WFI FOV and high effective area) IXO surveys should detect large numbers of galaxies which will allow evolution to be studied in multiple redshift bins. High spatial resolution will also drive the need to minimize source confusion below F _{0.5-2.0 keV} = 10^{-17} ergs/s/cm^2. In addition to detecting starburst galaxies individually, stacking will be used to constrain their properties on average, particularly Lyman-break galaxies at z greater than 2. We will also discuss challenges in segregating galaxies from obscured AGN in IXO deep fields and expectations proposed survey X-ray missions. |
| File Size | 43635 |
| Page Count | 1 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_20110008026 |
| Archival Resource Key | ark:/13960/t86h9jh6p |
| Language | English |
| Publisher Date | 2011-03-14 |
| Access Restriction | Open |
| Subject Keyword | Astronomy Red Shift Active Galactic Nuclei Sensitivity X Rays Star Formation Starburst Galaxies Mathematical Models Spatial Resolution Ntrs Nasa Technical Reports ServerĀ (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |