A dataset provided by the European Space Agency

Name 015266
Title PG 1448+273: The hottest accretion disk among Active Galactic Nuclei
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0152660101

DOI 10.5270/esa-49lnb0e
Author Mr Toshihiro Kawaguchi
Description The switch from the standard accretion disk to the slim accretion disk has long been a natural, theoretical consequence of high accretion rate. To test this paradigm, small black-hole mass and high accretion objects are desirable. We therefore propose a 20 ksec XMM-Newton observation of a Narrow-Line Seyfert 1 galaxy extremely suitable to this purpose, PG 1448+273, to examine and derive constraints on the slim disk model, through detailed modeling of both spectral and temporal behaviors.
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Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2003-02-08T13:11:03Z/2003-02-08T19:10:32Z
Version 17.56_20190403_1200
Mission Description The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's 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 Earth's 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 2004-03-25T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2004-03-25T00:00:00Z, 015266, 17.56_20190403_1200. https://doi.org/10.5270/esa-49lnb0e