A dataset provided by the European Space Agency

Name 050644
Title Understanding the extreme soft X-ray excess in RE 1034+396
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0506440101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0506440201

DOI 10.5270/esa-p41ngxn
Author Prof Martin Ward
Description We propose a 90ks XMM--Newton observation of the Narrow Line Seyfert 1 galaxy RE 1034+396. This has the strongest soft X-ray excess ever seen in an active galaxy (AGN). It also has extremely low absorption in the line-of-sight, so has excellent FUSE-EUVE-HST data to delineate the lower energy extent of the soft X-ray excess and especially how this connects onto the accretion disc emission. RE1034+396 thus represents the extreme of the NLS1 population, and the best hope for constraining the nature of the soft excess.
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An All-Sky Atlas of Radio-X-ray Associations . Flesch, E., . PASA . 27-283 . 2010 . 2010PASA...27..283F ,
A periodicity of ~1hour in X-ray emission from the active galaxy RE J1034+396 . Gierlinski, Marek, Middleton, Matthew, et all. . Natur . 455-369 . 2008 . 2008Natur.455..369G ,
RE J1034+396: the origin of the soft X-ray excess and quasi-periodic oscillation . Middleton, Matthew, Done, Chris, et all. . MNRAS . 394-250 . 2009 . 2009MNRAS.394..250M ,
Searching for the trigger of the active galactic nucleus quasi-periodic oscillation: 8 years of RE J1034+396 . Middleton, Matthew, Uttley, Phil, . MNRAS . 417-250 . 2011 . 2011MNRAS.417..250M ,
A Bayesian test for periodic signals in red noise . Vaughan, S., . MNRAS . 402-307 . 2010 . 2010MNRAS.402..307...,
X-ray reverberation close to the black hole in RE J1034+396 . Zoghbi, A., Fabian, A. C., . MNRAS . 418-2642 . 2011 . 2011MNRAS.418.2642Z ,
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An Archival Chandra and XMM-Newton Survey of Type 2 Quasars . Jia, Jianjun, Ptak, Andrew, et all. . ApJ . 777-27 . 2013 . 2013ApJ...777...27J ,
Tracking the Evolution of Quasi-periodic Oscillation in RE J1034+396 Using the Hilbert-Huang Transform . Hu, Chin-Ping, Chou, Yi, et all. . ApJ . 788-31 . 2014 . 2014ApJ...788...31H ,
Delving Into X-ray Obscuration of Type 2 AGN, Near and Far . LaMassa, Stephanie M., Yaqoob, Tahir, et all. . ApJ . 787-61 . 2014 . 2014ApJ...787...61L ,
The diversity of quasars unified by accretion and orientation . Shen, Yue, Ho, Luis C., . Natur . 513-210 . 2014 . 2014Natur.513..210S ,
Detection of a QPO in five XMM-Newton observations of RE J1034+396 . Alston, W. N., Markeviciute, J., et all. . MNRAS . 445-16 . 2014 . 2014MNRAS.445L..16A ,
Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift . Yershov, V. N., . Ap&SS . 354-97 . 2014 . 2014Ap&SS.354...97Y ,
Revealing the X-ray variability of AGN with principal component analysis . Parker, M. L., Fabian, A. C., et all. . MNRAS . 447-72 . 2015 . 2015MNRAS.447...72P ,
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Obscuration-dependent Evolution of Active Galactic Nuclei . Buchner, Johannes, Georgakakis, Antonis, et all. . ApJ . 802-89 . 2015 . 2015ApJ...802...89B ,
X-ray reverberation around accreting black holes . Uttley, P., Cackett, E. M., et all. . A&ARv . 22-72 . 2014 . 2014A&ARv..22...72U ,
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Quasi periodic oscillations in active galactic nuclei . Alston, W., Fabian, A., et all. . AN . 337-417 . 2016 . 2016AN....337..417A ,
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The Interaction of the Fermi Bubbles with the Milky Way.s Hot Gas Halo . Miller, Matthew J., Bregman, Joel N., . ApJ . 829-9 . 2016 . 2016ApJ...829....9M ,
The mass of the black hole in RE J1034+396 . Czerny, B., You, B., et all. . A&A . 594-102 . 2016 . 2016A&A...594A.102C ,
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 ,
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The X-ray Binary analogy to the first AGN QPO . Middleton, M., Done, C., . AIPC . 1248-325 . 2010 . 2010AIPC.1248..325M ,
The model constraints from the observed trends for the quasi-periodic oscillation in RE J1034+396 . Czerny, B., Lachowicz, P., et all. . A&A . 524-26 . 2010 . 2010A&A...524A..26C ,
AGN spectral states from simultaneous UV and X-ray observations by XMM-Newton . Svoboda, J., Guainazzi, M., . A&A . 603-127 . 2017 . 2017A&A...603A.127S ,
Testing warm Comptonization models for the origin of the soft X-ray excess in AGNs . Petrucci, P.-O., Ursini, F., et all. . A&A . 611-59 . 2018 . 2018A&A...611A..59P ,
Long-term X-ray variability characteristics of the narrow-line Seyfert 1 galaxy RE J1034+396 . Chaudhury, K., Chitnis, V. R., et all. . MNRAS . 478-4830 . 2018 . 2018MNRAS.478.4830C ,
The soft X-ray excess: NLS1s versus BLS1s . Gliozzi, Mario, Williams, James K., . MNRAS . 491-532 . 2020 . 2020MNRAS.491..532G ,
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 ,
Reobserving the NLS1 galaxy RE J1034+396 - I. The long-term, recurrent X-ray QPO with a high significance . Jin, Chichuan, Done, Chris, . MNRAS . 495-3538 . 2020 . 2020MNRAS.495.3538J ,
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 ,
Re-observing the NLS1 galaxy RE J1034+396 - II. New insights on the soft X-ray excess, QPO, and the analogy with GRS 1915+105 . Jin, Chichuan, Done, Chris, . MNRAS . 500-2475 . 2021 . 2021MNRAS.500.2475J ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2007-05-31T19:47:14Z/2007-06-01T22:40:00Z
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 2008-06-25T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2008-06-25T00:00:00Z, 050644, 17.56_20190403_1200. https://doi.org/10.5270/esa-p41ngxn