| 000 | 03178nam a22005055i 4500 | ||
|---|---|---|---|
| 001 | 978-3-540-31641-1 | ||
| 003 | DE-He213 | ||
| 005 | 20161121230951.0 | ||
| 007 | cr nn 008mamaa | ||
| 008 | 100805s2005 gw | s |||| 0|eng d | ||
| 020 |
_a9783540316411 _9978-3-540-31641-1 |
||
| 024 | 7 |
_a10.1007/b96746 _2doi |
|
| 050 | 4 | _aQB1-991 | |
| 050 | 4 | _aQB460-466 | |
| 050 | 4 | _aQB980-991 | |
| 072 | 7 |
_aPGC _2bicssc |
|
| 072 | 7 |
_aSCI004000 _2bisacsh |
|
| 072 | 7 |
_aSCI005000 _2bisacsh |
|
| 082 | 0 | 4 |
_a520 _223 |
| 245 | 1 | 0 |
_aMultiwavelength Mapping of Galaxy Formation and Evolution _h[electronic resource] : _bProceedings of the ESO Workshop Held at Venice, Italy, 13-16 October 2003 / _cedited by Alvio Renzini, Ralf Bender. |
| 264 | 1 |
_aBerlin, Heidelberg : _bSpringer Berlin Heidelberg, _c2005. |
|
| 300 |
_aXXVI, 490 p. _bonline resource. |
||
| 336 |
_atext _btxt _2rdacontent |
||
| 337 |
_acomputer _bc _2rdamedia |
||
| 338 |
_aonline resource _bcr _2rdacarrier |
||
| 347 |
_atext file _bPDF _2rda |
||
| 490 | 1 |
_aESO Astrophysics Symposia, _x1431-2433 |
|
| 505 | 0 | _aThe Dawn of Galaxies -- Evolution of X-Ray Selected AGN -- Clustering of Submillimetre-Selected Galaxies -- Star-Forming Galaxies in the 'Redshift Desert' -- The Near-Infrared View of Galaxy Evolution -- Galaxy Formation and Evolution since z=1 -- Exploring the Reionization Epoch with HST and JWST -- Chemo-Photometric Models of Ring Galaxies -- The Cosmic Evolution of Quasar Hosts -- Stellar Populations in Spiral Galaxies -- The Cosmological Evolution of Quasar Black-Hole Masses -- Radio Observations of the Subaru/XMM-Newton Deep Survey Field. | |
| 520 | _aThe possibilities of astronomical observation have dramatically increased over the last decade. Major satellites, like the Hubble Space Telescope, Chandra and XMM Newton, are complemented by numerous large ground-based observatories, from 8m-10m optical telescopes to sub-mm and radio facilities. As a result, observational astronomy has access to virtually the whole electromagnetic spectrum of galaxies, even at high redshifts. Theoretical models of galaxy formation and cosmological evolution now face a serious challenge to match the plethora of observational data. In October 2003, over 170 astronomers from 15 countries met for a 4-day workshop to extensively illustrate and discuss all major observational projects and ongoing theoretical efforts to model galaxy formation and evolution. This volume contains the complete proceedings of this meeting and is therefore a unique and timely overview of the current state of research in this rapidly evolving field. | ||
| 650 | 0 | _aPhysics. | |
| 650 | 0 | _aAstronomy. | |
| 650 | 0 | _aAstrophysics. | |
| 650 | 0 | _aCosmology. | |
| 650 | 1 | 4 | _aPhysics. |
| 650 | 2 | 4 | _aAstronomy, Astrophysics and Cosmology. |
| 700 | 1 |
_aRenzini, Alvio. _eeditor. |
|
| 700 | 1 |
_aBender, Ralf. _eeditor. |
|
| 710 | 2 | _aSpringerLink (Online service) | |
| 773 | 0 | _tSpringer eBooks | |
| 776 | 0 | 8 |
_iPrinted edition: _z9783540256656 |
| 830 | 0 |
_aESO Astrophysics Symposia, _x1431-2433 |
|
| 856 | 4 | 0 | _uhttp://dx.doi.org/10.1007/b96746 |
| 912 | _aZDB-2-PHA | ||
| 950 | _aPhysics and Astronomy (Springer-11651) | ||
| 999 |
_c506578 _d506578 |
||