A dataset provided by the European Space Agency

Name 074501
Title X-raying the most powerful quasars in the golden epoch of AGN-galaxy evolution
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0745010101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0745010301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0745010401

DOI 10.5270/esa-jzlbgfo
Author Dr Luca Zappacosta
Description We propose to observe four hyper-luminous (L_IR > 10^14 L_sun), dust-reddened, type I quasars at z=2-3, recently discovered in the wide-area UKIDSS and WISE surveys. We will constrain their X-ray luminosity and, through available multiwavelength data, accurately model their SED dinsentangling the disk and corona contribution to such extreme IR luminosities
Publication XMM-Newton publication statistics . Ness, J.-U., Parmar, A. N., et all. . AN . 335-210 . 2014 . 2014AN....335..210N ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
The WISSH quasars project. III. X-ray properties of hyper-luminous quasars . Martocchia, S., Piconcelli, E., et all. . A&A . 608-51 . 2017 . 2017A&A...608A..51M ,
The WISSH quasars project. VII. The impact of extreme radiative field in the accretion disc and X-ray corona interplay . Zappacosta, L., Piconcelli, E., et all. . A&A . 635-5 . 2020 . 2020A&A...635L...5Z ,
X-ray observations of luminous dusty quasars at z > 2 . Lansbury, G. B., Banerji, M., et all. . MNRAS . 495-2652 . 2020 . 2020MNRAS.495.2652L ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2014-11-14T14:25:45Z/2015-02-16T19:58:21Z
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 2016-03-04T23:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2016-03-04T23:00:00Z, 074501, 17.56_20190403_1200. https://doi.org/10.5270/esa-jzlbgfo