High-frequency QPO in black hole binaries

DOI

We present the results of the analysis of a large data base of X-ray observations of 22 galactic black hole transients with the Rossi X-Ray Timing Explorer throughout its operative life for a total exposure time of ~12ms. We excluded persistent systems and the peculiar source GRS 1915+105, as well as the most recently discovered sources. The semi-automatic homogeneous analysis was aimed at the detection of high-frequency (100-1000Hz) quasi-periodic oscillations (QPO), of which several cases were previously reported in the literature.

Cone search capability for table J/MNRAS/426/1701/table1 (Statistics of available data and obtained detections)

Identifier
DOI http://doi.org/10.26093/cds/vizier.74261701
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/MNRAS/426/1701
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/426/1701
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/426/1701
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/MNRAS/426/1701
Provenance
Creator Belloni T.M.; Sanna A.; Mendez M.
Publisher CDS
Publication Year 2013
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Natural Sciences; Physics; Stellar Astronomy