A dataset provided by the European Space Agency

Name 020063
Title CENTRALLY-CONCENTRATED ENERGY SOURCES IN LINER ULTRALUMINOUS INFRARED GALAXIES
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0200630101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0200630201

DOI 10.5270/esa-rchzfkw
Author Dr MASATOSHI IMANISHI
Description We propose XMM observations of two LINER-type ultraluminous infrared galaxies for which our infrared 3--4 micron slit spectroscopy has revealed the presence of centrally-concentrated energy sources, as is expected for a buried AGN. The main goal is to obtain direct X-ray evidence that the centrally-concentrated energy sources are indeed buried AGNs (strong 2--10 keV X-ray emitter), and not unusually centrally-concentrated starbursts (weak X-ray emitter).
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A Comparison of X-Ray Photon Indices among the Narrow- and Broad-line Seyfert 1 Galaxies . Ojha, Vineet, Chand, Hum, et all. . ApJ . 896-95 . 2020 . 2020ApJ...896...95O ,
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SPIDERS: overview of the X-ray galaxy cluster follow-up and the final spectroscopic data release . Clerc, N., Kirkpatrick, C. C., et all. . MNRAS . 497-3976 . 2020 . 2020MNRAS.497.3976C ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2004-04-13T23:05:58Z/2004-12-21T09:08:05Z
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 2006-07-08T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2006-07-08T00:00:00Z, 020063, 17.56_20190403_1200. https://doi.org/10.5270/esa-rchzfkw