Status: Bibliographieeintrag
Standort: ---
Exemplare:
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| Online-Ressource |
Verfasst von: | Pace, Francesco [VerfasserIn]  |
| Maturi, Matteo [VerfasserIn]  |
| Bartelmann, Matthias [VerfasserIn]  |
Titel: | Statistical properties of SZ and X-ray cluster detections |
Verf.angabe: | Francesco Pace, Matteo Maturi, Matthias Bartelmann, Nico Cappelluti, Klaus Dolag, Massimo Meneghetti, Lauro Moscardini |
E-Jahr: | 2017 |
Jahr: | August 21, 2017 |
Umfang: | 13 S. |
Fussnoten: | Gesehen am 25.09.2017 |
Titel Quelle: | Enthalten in: De.arxiv.org |
Ort Quelle: | [S.l.] : Arxiv.org, 1991 |
Jahr Quelle: | 2017 |
Band/Heft Quelle: | (2017) Artikel-Nummer 0802.1200, 13 Seiten |
Abstract: | Aims. We calibrate the number density, completeness, reliability and the lower mass limit of galaxy-cluster detections through their thermal SZ signal, and compare them to X-ray cluster detections. Methods. We simulate maps of the thermal SZ effect and the X-ray emission from light cones constructed in a large, hydrodynamical, cosmological simulation volume, including realistic noise contributions. The maps are convolved with linear, optimised, single- and multi-band filters to identify local peaks and their signal-to-noise ratios. The resulting peak catalogues are then compared to the halo population in the simulation volume to identify true and spurious detections. Results. Multi-band filtering improves the statistics of SZ cluster detections considerably compared to single-band filtering. Observations with the characteristics of ACT detect clusters with masses M>6-9e13 M_o/h, quite independent of redshift, reach 50% completeness at ~1e14 M_o/h and 100% completeness at ~2e14 M_o/h. Samples are contaminated by only a few per cent spurious detections. This is broadly comparable to X-ray cluster detections with XMM-Newton with 100 ks exposure time in the soft band, except that the mass limit for X-ray detections increases much more steeply with redshift than for SZ detections. A comparison of true and filtered signals in the SZ and X-ray maps confirms that the filters introduce at most a negligible bias. |
URL: | Bitte beachten Sie: Dies ist ein Bibliographieeintrag. Ein Volltextzugriff für Mitglieder der Universität besteht hier nur, falls für die entsprechende Zeitschrift/den entsprechenden Sammelband ein Abonnement besteht oder es sich um einen OpenAccess-Titel handelt.
kostenfrei: Volltext: http://arxiv.org/abs/0802.1200 |
Datenträger: | Online-Ressource |
Sprache: | eng |
Sach-SW: | Astrophysics |
K10plus-PPN: | 156377352X |
Verknüpfungen: | → Sammelwerk |
Statistical properties of SZ and X-ray cluster detections / Pace, Francesco [VerfasserIn]; August 21, 2017 (Online-Ressource)
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