| dc.creator | Manolis Plionis | |
| dc.date | 2008 | |
| dc.date.accessioned | 2023-07-25T16:22:53Z | |
| dc.date.available | 2023-07-25T16:22:53Z | |
| dc.identifier | http://inaoe.repositorioinstitucional.mx/jspui/handle/1009/1052 | |
| dc.identifier.uri | https://repositorioslatinoamericanos.uchile.cl/handle/2250/7806252 | |
| dc.description | We have analysed the angular clustering of X-ray selected active galactic nuclei (AGN) in different flux-limited sub-samples of the Chandra Deep Field North (CDF-N) and South (CDF-S) surveys. We find a strong dependence of the clustering strength on the sub-sample flux-limit, a fact which explains most of the disparate clustering results of different XMM and Chandra surveys. Using Limber’s equation, we find that the inverted CDF-N and CDF-S spatial clustering lengths are consistent with direct spatial clustering measures found in the literature, while at higher flux-limits the clustering length increases considerably; for example, at fx, limit ∼10 ¯¹⁵ˉ erg s¯¹ cm¯² we obtain r₀ ≃ 17 ± 5 axxnd 18 ± 3 h−1 Mpc, for the CDF-N and CDF-S, respectively. We show that the observed flux-limit clustering trend hints towards an X-ray luminosity dependent clustering of X-ray selected, z ∼ 1, AGNs. | |
| dc.format | application/pdf | |
| dc.language | eng | |
| dc.publisher | The astrophysical journal | |
| dc.relation | citation:Plionis, M., et al., (2008). Luminosity dependent X-ray AGN clustering?, The astrophysical journal, Vol.674(1):L5-L8 | |
| dc.rights | info:eu-repo/semantics/openAccess | |
| dc.rights | http://creativecommons.org/licenses/by-nc-nd/4.0 | |
| dc.subject | info:eu-repo/classification/cti/1 | |
| dc.subject | info:eu-repo/classification/cti/21 | |
| dc.subject | info:eu-repo/classification/cti/21 | |
| dc.title | Luminosity dependent X-ray AGN clustering ? | |
| dc.type | info:eu-repo/semantics/article | |
| dc.type | info:eu-repo/semantics/acceptedVersion | |
| dc.audience | students | |
| dc.audience | researchers | |
| dc.audience | generalPublic | |
