A dataset provided by the European Space Agency

Name 055517
Title Testing strong gravity in the NLS1 PKS 0558-504
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0555170201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0555170301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0555170401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0555170501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0555170601
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0555170701
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0555170801
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0555170901
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0555171001
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0555171101

DOI 10.5270/esa-a2caiek
Author Dr Iossif Papadakis
Description We propose to observe the radio-loud NLS1 galaxy PKS~0558--504 with XMM for five orbits (650 ksec). There has been evidence for QPOs with time scales of 7 ksec and 21 ksec in previous short XMM observations. These time scales are near a frequency ratio of 3:1, a well known result from Galactic Black Hole binaries. The main aims of the proposed XMM observation are to confirm the presence of a QPO like feature at 7 ksec, to search for evidence for the associated 21 ksec modulation, and for the third possible time scale of 14 ks (the one with a 3:2 frequency ratio). Confirmation of the presence of these time scales will provide a unique probe of strong gravity in the vicinity of an AGN black hole.
Publication XMM-Newton long-look observation of the narrow line Seyfert 1 galaxy PKS 0558-504. I. Spectral analysis . Papadakis, I. E., Brinkmann, W., et all. . A&A . 510-65 . 2010 . 2010A&A...510A..65P ,
XMM-Newton long-look observation of the narrow-line Seyfert 1 galaxy PKS 0558-504. II. Timing analysis . Papadakis, I. E., Brinkmann, W., et all. . A&A . 518-28 . 2010 . 2010A&A...518A..28P ,
XMM-Newton and FUSE Tentative Evidence for a WHIM Filament Along the Line of Sight to PKS 0558-504 . Nicastro, F., Krongold, Y., et all. . ApJ . 715-854 . 2010 . 2010ApJ...715..854N ,
A Panchromatic View of PKS 0558-504: An Ideal Laboratory to Study the Disk-Jet Link . Gliozzi, M., Papadakis, I. E., et all. . ApJ . 717-1243 . 2010 . 2010ApJ...717.1243G ,
An All-Sky Atlas of Radio-X-ray Associations . Flesch, E., . PASA . 27-283 . 2010 . 2010PASA...27..283F ,
X-ray variability of 104 active galactic nuclei. XMM-Newton power-spectrum density profiles . Gonzalez-Martin, O., Vaughan, S., . A&A . 544-80 . 2012 . 2012A&A...544A..80G ,
Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog . Lin, Dacheng, Webb, Natalie A., . ApJ . 756-27 . 2012 . 2012ApJ...756...27L ,
A Comparison of Hard X-ray Photon Indices and Iron Kalpha Emission Lines in X-ray Luminous Narrow- and Broad-line Seyfert 1 Galaxies . Zhou, Xin-Lin, Zhang, Shuang-Nan, . ApJ . 713-11 . 2010 . ...,
Automatic Classification of Time-variable X-Ray Sources . Lo, Kitty K., Farrell, Sean, et all. . ApJ . 786-20 . 2014 . 2014ApJ...786...20L ,
Ultrafast outflows in radio-loud active galactic nuclei . Tombesi, F., Tazaki, F., et all. . MNRAS . 443-2154 . 2014 . 2014MNRAS.443.2154T ,
The diversity of quasars unified by accretion and orientation . Shen, Yue, Ho, Luis C., . Natur . 513-210 . 2014 . 2014Natur.513..210S ,
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 ,
A hard X-ray view of the soft excess in AGN . Boissay, Rozenn, Ricci, Claudio, . A&A . 588-70 . 2016 . 2016A&A...588A..70B ,
The Rotation of the Hot Gas around the Milky Way . Hodges-Kluck, Edmund J., Miller, Matthew J., . ApJ . 822-21 . 2016 . 2016ApJ...822...21H ,
A search for X-ray reprocessing echoes in the power spectral density functions of AGN . Emmanoulopoulos, D., Papadakis, I. E., et all. . MNRAS . 461-1642 . 2016 . 2016MNRAS.461.1642E ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
The X-ray continuum time-lags and intrinsic coherence in AGN . Epitropakis, A., Papadakis, I. E., . MNRAS . 468-3568 . 2017 . 2017MNRAS.468.3568E ,
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 ,
The close environments of accreting massive black holes are shaped by radiative feedback . Ricci, Claudio, Trakhtenbrot, Benny, et all. . Natur . 549-488 . 2017 . 2017Natur.549..488R ,
BAT AGN Spectroscopic Survey (BASS) - VI. The GammaX-L-LEdd relation . Trakhtenbrot, Benny, Ricci, Claudio, et all. . MNRAS . 470-800 . 2017 . 2017MNRAS.470..800T ,
BAT AGN Spectroscopic Survey. V. X-Ray Properties of the Swift-BAT 70-month AGN Catalog . Ricci, C., Trakhtenbrot, B., et all. . ApJS . 233-17 . 2017 . 2017ApJS..233...17R ,
The Swift-BAT AGN Spectroscopic Survey. IX. The Clustering Environments of an Unbiased Sample of Local AGNs . Powell, M. C., Cappelluti, N., et all. . ApJ . 858-110 . 2018 . 2018ApJ...858..110P ,
Testing the X-ray reverberation model KYNREFREV in a sample of Seyfert 1 Active Galactic Nuclei . Caballero-Garcia, M. D., Papadakis, I. E., et all. . MNRAS . 480-2650 . 2018 . 2018MNRAS.480.2650C ,
Are narrow-line Seyfert 1 galaxies highly accreting low-MBH AGNs? . Williams, James K., Gliozzi, Mario, . MNRAS . 480-96 . 2018 . 2018MNRAS.480...96W ,
Hot corona properties of Swift-BAT-detected AGNs . Wang, Chan, Yu, Li-Ming, et all. . MNRAS . 487-2463 . 2019 . 2019MNRAS.487.2463W ,
The soft X-ray excess: NLS1s versus BLS1s . Gliozzi, Mario, Williams, James K., . MNRAS . 491-532 . 2020 . 2020MNRAS.491..532G ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2008-09-07T01:13:40Z/2008-09-16T14:46:01Z
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 2009-10-28T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2009-10-28T00:00:00Z, 055517, 17.56_20190403_1200. https://doi.org/10.5270/esa-a2caiek