A dataset provided by the European Space Agency

Name: Doubling the number of existing good quality spectra of obscured AGN
Published: 2010-01-24T00:00:00Z

Proposal ID	055417
Title	Doubling the number of existing good quality spectra of obscured AGN
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0554170101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0554170201
DOI	https://doi.org/10.5270/esa-1rah3sz
Principal Investigator, PI	Dr Matteo Guainazzi
Abstract	This program aims at observing all known obscured AGN (5 objects) for whichhigh-quality RGS spectra can be measured within a reasonable allocation time(less than 2.5 XMM-Newton orbits). The proposed observations would double thenumber of objects, where diagnostics of the physical conditions in thecircumnuclear gas (density, ionization state, metallicity) is possible. Thisgoal can be achieved with a total time allocation of 965 ks.
Publications	Understanding Dual Active Galactic Nucleus Activation in the nearby Universe \|Koss Michael Mushotzky Richard et al. \| ApJ \| 746-22 \| 2012 \| 2012ApJ...746L..22K \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...746L..22K Uncovering Obscured Active Galactic Nuclei in Homogeneously Selected Samples of Seyfert 2 Galaxies \|LaMassa Stephanie M. Heckman T. M. et al. \| ApJ \| 729-52 \| 2011 \| 2011ApJ...729...52L \| http://ui.adsabs.harvard.edu/#abs/2011ApJ...729...52L A Stochastic Model for the Luminosity Fluctuations of Accreting Black Holes \|Kelly Brandon C. Sobolewska Malgorzata \| ApJ \| 730-52 \| 2011 \| 2011ApJ...730...52K \| http://ui.adsabs.harvard.edu/#abs/2011ApJ...730...52K Final verdict from XMM-Newton: the X-ray obscured Seyfert galaxy NGC 5506 has a broad Fe Kalpha line \|Guainazzi M. Bianchi S. et al. \| MNRAS \| 406-2013 \| 2010 \| 2010MNRAS.406.2013G \| http://ui.adsabs.harvard.edu/#abs/2010MNRAS.406.2013G On the driver of relativistic effect strength in Seyfert galaxies \|Guainazzi M. Bianchi S. et al. \| A&A \| 531-131 \| 2011 \| 2011A&A...531A.131G \| http://ui.adsabs.harvard.edu/#abs/2011A&A...531A.131G 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 \| http://ui.adsabs.harvard.edu/#abs/2012A&A...544A..80G Disentangling AGN and Star Formation in Soft X-Rays \|LaMassa Stephanie M. Heckman T. M. \| ApJ \| 758-82 \| 2012 \| 2012ApJ...758...82L \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...758...82L 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 \| 2010ApJ...713L..11Z \| http://ui.adsabs.harvard.edu/#abs/2010ApJ...713L..11Z Insight into Active Galactic Nucleus and Host Galaxy Co-evolution from Hard X-Ray Emission \|Wang J. Zhou X. L. \| ApJ \| 768-176 \| 2013 \| 2013ApJ...768..176W \| http://ui.adsabs.harvard.edu/#abs/2013ApJ...768..176W Search for X-ray occultations in active galactic nuclei \|Torricelli-Ciamponi G. Pietrini P. et al. \| MNRAS \| 442-2116 \| 2014 \| 2014MNRAS.442.2116T \| http://ui.adsabs.harvard.edu/#abs/2014MNRAS.442.2116T 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 The Link between the Hidden Broad Line Region and the Accretion Rate in Seyfert 2 Galaxies \|Marinucci Andrea Bianchi Stefano et al. \| ApJ \| 748-130 \| 2012 \| 2012ApJ...748..130M \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...748..130M Non-detection of X-ray emission from sterile neutrinos in stacked galaxy spectra \|Anderson Michael E. Churazov Eugene \| MNRAS \| 452-3905 \| 2015 \| 2015MNRAS.452.3905A \| http://ui.adsabs.harvard.edu/#abs/2015MNRAS.452.3905A X-ray spectral parameters for a sample of 95 active galactic nuclei \|Vasylenko A. A. Zhdanov V. I. \| Ap&SS \| 360-71 \| 2015 \| 2015Ap&SS.360...71V \| http://ui.adsabs.harvard.edu/#abs/2015Ap&SS.360...71V A comprehensive analysis of the hard X-ray spectra of bright Seyfert galaxies \|Lubinski P. Beckmann V. et al. \| MNRAS \| 458-2454 \| 2016 \| 2016MNRAS.458.2454L \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.458.2454L Fe-K Line Time Variability and Ni Abundance of Distant Reflectors in Seyfert Galaxies \|Fukazawa Yasushi Furui Shunya et al. \| ApJ \| 821-15 \| 2016 \| 2016ApJ...821...15F \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...821...15F Ensemble X-ray variability of active galactic nuclei. II. Excess variance and updated structure function \|Vagnetti F. Middei R. et al. \| A&A \| 593-55 \| 2016 \| 2016A&A...593A..55V \| http://ui.adsabs.harvard.edu/#abs/2016A&A...593A..55V 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 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 \| http://ui.adsabs.harvard.edu/#abs/2016A&A...594A..72P The close environments of accreting massive black holes are shaped by radiative feedback \|Ricci Claudio Trakhtenbrot Benny et al. \| Natur \| 549-488 \| 2017 \| 2017Natur.549..488R \| http://ui.adsabs.harvard.edu/#abs/2017Natur.549..488R BAT AGN Spectroscopic Survey (BASS) - VI. The GammaX-L/LEdd relation \|Trakhtenbrot Benny Ricci Claudio et al. \| MNRAS \| 470-800 \| 2017 \| 2017MNRAS.470..800T \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.470..800T BAT AGN Spectroscopic Survey. V. X-Ray Properties of the Swift/BAT 70-month AGN Catalog \|Ricci C. Trakhtenbrot B. et al. \| ApJS \| 233-17 \| 2017 \| 2017ApJS..233...17R \| http://ui.adsabs.harvard.edu/#abs/2017ApJS..233...17R Multi-epoch analysis of the X-ray spectrum of the active galactic nucleus in NGC 5506 \|Sun Shangyu Guainazzi Matteo et al. \| MNRAS \| 478-1900 \| 2018 \| 2018MNRAS.478.1900S \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.478.1900S The Swift/BAT AGN Spectroscopic Survey. IX. The Clustering Environments of an Unbiased Sample of Local AGNs \|Powell M. C. Cappelluti N. et al. \| ApJ \| 858-110 \| 2018 \| 2018ApJ...858..110P \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...858..110P Are narrow-line Seyfert 1 galaxies highly accreting low-MBH AGNs? \|Williams James K. Gliozzi Mario \| MNRAS \| 480-96 \| 2018 \| 2018MNRAS.480...96W \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.480...96W A Study of X-Ray Emission of Galaxies Hosting Molecular Outflows (MOX Sample) \|Laha Sibasish Guainazzi Matteo et al. \| ApJ \| 868-10 \| 2018 \| 2018ApJ...868...10L \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...868...10L X-ray occultations in active galactic nuclei: distribution in size of orbiting clouds and total mass content in the cloud ensemble \|Pietrini P. Torricelli-Ciamponi G. \| A&A \| 628-26 \| 2019 \| 2019A&A...628A..26P \| http://ui.adsabs.harvard.edu/#abs/2019A&A...628A..26P Hot corona properties of Swift/BAT-detected AGNs \|Wang Chan Yu Li-Ming et al. \| MNRAS \| 487-2463 \| 2019 \| 2019MNRAS.487.2463W \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.487.2463W Testing the Lamp-post and Wind Reverberation Models with XMM-Newton Observations of NGC 5506 \|Zoghbi Abderahmen Kalli Sihem et al. \| ApJ \| 893-97 \| 2020 \| 2020ApJ...893...97Z \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...893...97Z 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 Local Active Galactic Nuclei with Large Broad-Hu03b1 Variability Reside in Red Galaxies \|Liu Wen-Juan Lira Paulina et al. \| ApJ \| 915-63 \| 2021 \| 2021ApJ...915...63L \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...915...63L Are Compton-thin AGNs Globally Compton Thin? \|Tzanavaris P. Yaqoob T. et al. \| ApJ \| 922-85 \| 2021 \| 2021ApJ...922...85T \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...922...85T A Systematic Study of the Short-term X-Ray Variability of Seyfert Galaxies. I. Diversity of the X-Ray rms Spectra \|Hu Jingwei Jin Chichuan et al. \| ApJ \| 936-105 \| 2022 \| 2022ApJ...936..105H \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...936..105H The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII O VIII and Fe L-shell Transitions \|Pan Zeyang Qu Zhijie et al. \| ApJS \| 271-62 \| 2024 \| 2024ApJS..271...62P \| http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P 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	2008-07-27T07:20:37Z/2009-01-03T20:14:25Z
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	2010-01-24T00:00:00Z
Keywords	"total time allocation", "reasonable allocation time", "xmm newton orbits", "quality spectra", "XMM", "program aims", "circumnuclear gas density", "obscured agn", "XMM-Newton", "physical conditions", "quality rgs spectra"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Matteo Guainazzi, 2010, 'Doubling the number of existing good quality spectra of obscured AGN', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-1rah3sz