Persistent Accreting Neutron Stars in the INTEGRAL Galactic Plane Survey

Details Persistent Accreting Neutron Stars in the INTEGRAL Galactic Plane Survey Persistent Accreting Neutron Stars in the INTEGRAL Galactic Plane Survey

Nov 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002xrb..confe..50w&link_type=abstract

X-ray Binaries in the Chandra and XMM-Newton Era (with an emphasis on Targets of Opportunity), Abstracts of the conference held

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New Observatories

Scientific paper

The INTEGRAL Galactic Plane Survey consists of weekly scans of the galactic plane, during which a large number of different objects will be observed. Our collaboration is responsible for the processing of the data from the ~25 persistent accreting neutron stars. Our plan is to provide the community with basic data (spectral shape, flux, pulse period,...) from the INTEGRAL observations shortly after the data have been taken. Furthermore, simultaneous observations with other instruments are planned. All of these observations will be supplemented with information on the past source behavior, building on a database of earlier observations and fundamental parameters of these sources. I will report on the status of these efforts and will present information about the sensitivity of the plane survey for the class of persistent accreting neutron stars.

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