High precision X-ray log N - log S distributions : implications for the obscured AGN population.
dc.contributor.author | Mateos, S. | |
dc.contributor.author | Treister, Ezequiel | |
dc.contributor.author | Warwick, R. S. | |
dc.contributor.author | Carrera, F J. | |
dc.contributor.author | Stewart, G. C. | |
dc.contributor.author | Ebrero, J. | |
dc.contributor.author | Della Ceca, R. | |
dc.contributor.author | Caccianiga, A. | |
dc.contributor.author | Gilli, R. | |
dc.contributor.author | Page, M. J. | |
dc.contributor.author | Tedds, J. A. | |
dc.contributor.author | Watson, M. G. | |
dc.contributor.author | Lamer, G. | |
dc.contributor.author | Saxton, R. D. | |
dc.contributor.author | Brunner, H. | |
dc.contributor.author | Page, C. G. | |
dc.date.accessioned | 2019-05-24T15:19:34Z | |
dc.date.available | 2019-05-24T15:19:34Z | |
dc.date.issued | 2008 | |
dc.date.updated | 2019-05-24T15:17:00Z | |
dc.fuente.origen | ORCID | |
dc.identifier.doi | 10.1051/0004-6361:200810004 | |
dc.identifier.issn | 1432-0746 | |
dc.identifier.uri | https://ui.adsabs.harvard.edu/#abs/2008A&A...492...51M | |
dc.identifier.uri | https://repositorio.uc.cl/handle/11534/22899 | |
dc.issue.numero | No. 1 | |
dc.pagina.final | 69 | |
dc.pagina.inicio | 51 | |
dc.relation.isformatof | Astronomy and Astrophysics, vol. 492, no. 1 (oct. 2008), pp. 51-69. | |
dc.revista | Astronomy & Astrophysics | es_ES |
dc.subject | Surveys | es_ES |
dc.subject | X-rays: general | es_ES |
dc.subject | Cosmology: observations | es_ES |
dc.subject | Galaxies: active | es_ES |
dc.subject.ddc | 520 | |
dc.subject.dewey | Astronomía | es_ES |
dc.title | High precision X-ray log N - log S distributions : implications for the obscured AGN population. | es_ES |
dc.type | artículo | |
dc.volumen | Vol. 492 | |
sipa.codpersvinculados | 1031846 |
Files
Original bundle
1 - 1 of 1
Loading...
- Name:
- High precision X-ray log N-log S distributions implications for the obscured AGN population.pdf
- Size:
- 1.54 MB
- Format:
- Adobe Portable Document Format
- Description: