A dataset provided by the European Space Agency

Name 055454
Title The remarkable X-ray spectrum of the luminous red QSO FTM J0830+3759
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0554540201

DOI 10.5270/esa-anfnj7y
Author Dr Enrico Piconcelli
Description We propose a 50 ks XMM-Newton observation of the X-ray luminous, Type 1 QSO FTM J0830+3785 (z=0.413). We aim at obtaining the first high-quality spectrum of this recently-discovered 2MASS QSO to assess its peculiar X-ray spectral properties. A very short 9 ks Chandra observation has revealed the statistically significant presence of puzzling emission-absorption line-like features at energies which do not correspond to any obvious rest-frame atomic transition. Similar features are observed in the spectra of a handful of intensively-studied Seyferts and attributed to relativistically-moving material surrounding the nuclear X-ray source, but have never been seen in the spectra of members of the poorly-studied, high luminosity (LX >10e45 erg-s) dust-reddened QSO population.
Publication Investigating the Complex X-Ray Spectrum of a Broad-Line 2MASS Red Quasar: XMM-Newton Observation of FTM 0830+3759 . Piconcelli, Enrico, Vignali, Cristian, et all. . ApJ . 710-992 . 2010 . 2010ApJ...710..992P ,
CAIXA: a catalogue of AGN in the XMM-Newton archive. III. Excess variance analysis . Ponti, G., Papadakis, I., et all. . A&A . 542-83 . 2012 . 2012A&A...542A..83P ,
Exospheric solar wind charge exchange as seen by XMM-Newton . Carter, J. A., Semba, S., . AN . 333-313 . 2012 . 2012AN....333..313C ,
The cosmological analysis of X-ray cluster surveys - II. Application of the CR-HR method to the XMM archive . Clerc, N., Sadibekova, T., et all. . MNRAS . 423-3561 . 2012 . 2012MNRAS.423.3561C ,
An XMM-Newton Survey of the Soft X-Ray Background. II. An All-Sky Catalog of Diffuse O VII and O VIII Emission Intensities . Henley, David B., Shelton, Robin L., . ApJS . 202-14 . 2012 . 2012ApJS..202...14H ,
X-ray reverberation around accreting black holes . Uttley, P., Cackett, E. M., et all. . A&ARv . 22-72 . 2014 . 2014A&ARv..22...72U ,
Peering Through the Dust: NuSTAR Observations of Two FIRST-2MASS Red Quasars . LaMassa, Stephanie M., Ricarte, Angelo, et all. . ApJ . 820-70 . 2016 . 2016ApJ...820...70L ,
The Interaction of the Fermi Bubbles with the Milky Way.s Hot Gas Halo . Miller, Matthew J., Bregman, Joel N., . ApJ . 829-9 . 2016 . ...,
SPIDERS: the spectroscopic follow-up of X-ray selected clusters of galaxies in SDSS-IV . Clerc, N., Merloni, A., et all. . MNRAS . 463-4490 . 2016 . 2016MNRAS.463.4490C ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
A new sample of X-ray selected narrow emission-line galaxies. II. Looking for True Seyfert 2 . Pons, E., Watson, M. G., . A&A . 594-72 . 2016 . 2016A&A...594A..72P ,
Dependence of the broad Fe Kalpha line on the physical parameters of AGN . Liu, Zhu, Yuan, Weimin, et all. . MNRAS . 463-684 . 2016 . 2016MNRAS.463..684L ,
X-ray properties of the X-CLASS-redMaPPer galaxy cluster sample: the luminosity-temperature relation . Molham, Mona, Clerc, Nicolas, et all. . MNRAS . 494-161 . 2020 . 2020MNRAS.494..161M ,
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 ,
Multiwavelength classification of X-ray selected galaxy cluster candidates using convolutional neural networks . Kosiba, Matej, Lieu, Maggie, et all. . MNRAS . 496-4141 . 2020 . 2020MNRAS.496.4141K ,
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 2008-11-08T13:23:09Z/2008-11-09T03:48:56Z
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 2009-12-02T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2009-12-02T00:00:00Z, 055454, 17.56_20190403_1200. https://doi.org/10.5270/esa-anfnj7y