A dataset provided by the European Space Agency

Name: INTEGRAL Spectra of X-ray Bright Compton-Thin Seyfert 2s
Published: 2014-01-23T00:00:00Z

Proposal ID	070118
Title	INTEGRAL Spectra of X-ray Bright Compton-Thin Seyfert 2s
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0701180101
DOI	https://doi.org/10.5270/esa-kouy6o3
Principal Investigator, PI	Dr Alex Markowitz
Abstract	We propose to use INTEGRAL to obtain high quality broadband hard X-ray spectraof two Compton-thin Seyfert 2s with insui??cient hard X-ray coverage to date:our primary object, Mkn 348, and a secondary target, the NELG NGC 526a. Bothtargets are X-ray bright, and have archival, long-term averaged RXTE-PCAspectra, as well as XMM-Newton and Suzaku spectra. Our proposed observationswith INTEGRAL IBIS/ISGRI and JEM-X, combined with the lower energy archivalspectra, will allow us to deconvolve broadband spectral components, constrainCompton rei??ection, and search for high-energy continuum cutoi??s. We alsorequest simultaneous XMM-Newton observations to aid in normalizing thelow-energy spectrum.
Publications	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 \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y Chandra and XMM-Newton Observations of H2O Maser Galaxy Mrk 348 \|Wang J. Zhang J. S. \| JApA \| 35-545 \| 2014 \| 2014JApA...35..545W \| http://ui.adsabs.harvard.edu/#abs/2014JApA...35..545W X-ray spectral variability of Seyfert 2 galaxies \|Hernandez-Garcia L. Masegosa J. et al. \| A&A \| 579-90 \| 2015 \| 2015A&A...579A..90H \| http://ui.adsabs.harvard.edu/#abs/2015A&A...579A..90H Unveiling the Physics of Low-luminosity AGNs through X-Ray Variability: LINER versus Seyfert 2 \|Hernandez-Garcia L. Masegosa J. et al. \| ApJ \| 824-7 \| 2016 \| 2016ApJ...824....7H \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...824....7H The Million Optical - Radio/X-ray Associations (MORX) Catalogue \|Flesch Eric W. \| PASA \| 33-52 \| 2016 \| 2016PASA...33...52F \| http://ui.adsabs.harvard.edu/#abs/2016PASA...33...52F The Variable and Non-variable X-Ray Absorbers in Compton-thin Type II Active Galactic Nuclei \|Laha Sibasish Markowitz Alex G. et al. \| ApJ \| 897-66 \| 2020 \| 2020ApJ...897...66L \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...897...66L Classification of 4XMM-DR9 sources by machine learning \|Zhang Yanxia Zhao Yongheng \| MNRAS \| 503-5263 \| 2021 \| 2021MNRAS.503.5263Z \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z Robust constraints on feebly interacting particles using XMM-Newton \|Luque Pedro De la Torre Balaji Shyam \| PhRvD \| 109-L101305 \| 2024 \| 2024PhRvD.109j1305L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L Multimessenger search for electrophilic feebly interacting particles from supernovae \|Luque Pedro De la Torre Balaji Shyam \| PhRvD \| 109-103028 \| 2024 \| 2024PhRvD.109j3028L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 968-46 \| 2024 \| 2024ApJ...968...46D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2013-01-04T10:34:07Z/2013-01-04T14:12:42Z
Version	17.56_20190403_1200
Mission Description	The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs 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 Earths 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	2014-01-23T00:00:00Z
Last Update	2025-01-27
Keywords	"Mkn 348", "integral spectra", "jem x", "xmm newton", "nelg ngc 526a", "XMM-Newton", "xray bright", "mkn 348", "integral ibis", "constrain compton rei", "XMM", "primary object", "low energy spectrum", "secondary target", "suzaku spectra", "NGC 526"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Alex Markowitz, 2014, 'INTEGRAL Spectra of X-ray Bright Compton-Thin Seyfert 2s', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-kouy6o3