A dataset provided by the European Space Agency

Proposal ID 002294
Title X-ray periodicity and the broad iron K line in IRAS18325-5926
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DOI https://doi.org/10.5270/esa-yfnkvrc
Principal Investigator, PI Dr Kazushi Iwasawa
Abstract We propose a 150 ks observation of the bright Seyfert galaxy IRAS18325-5926. The broad iron line and (quasi) periodic X-ray modulation are both importantprobes to the accretion flow very close to a black hole. A 16 h X-rayperiodicity has been found during an ASCA long observation. Our first aimis to investigate the X-ray variability over several periods with a long continuous stare enabled from XMM. The broad iron line in this galaxy peaksaround 7 keV, suggesting a possibility of an ionized disk. We wish to search for a broad, deep iron edge, characteristic of a reflection spectrumof an ionized disk.
Publications
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2001-03-05T10:12:34Z/2001-03-07T01:34:36Z
Version 17.56_20190403_1200
Mission Description The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations. Since Earths atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis.
Creator Contact https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published 2005-01-01T00:00:00Z
Last Update 2025-01-27
Keywords "galaxy pea", "continuous stare enabled", "iras18325 5926", "deep iron edge", "xray periodicity", "xray variability", "x ray periodicity", "broad iron line", "ionized disk", "XMM", "broad iron", "reflection spectrum", "black hole", "accretion flow"
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Kazushi Iwasawa, 2005, 'X-ray periodicity and the broad iron K line in IRAS18325-5926', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-yfnkvrc