A dataset provided by the European Space Agency

Name: The extreme X-ray spectrum and iron line of PG 2112+059
Published: 2008-11-28T00:00:00Z

Proposal ID	050050
Title	The extreme X-ray spectrum and iron line of PG 2112+059
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0500500601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0500500701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0500500801 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0500500901
DOI	https://doi.org/10.5270/esa-zi8aao2
Principal Investigator, PI	Dr Norbert Schartel
Abstract	The 70ks XMM-Newton observation of the X-ray weak quasars PG 2112+059 in lowstate shows an X-ray spectrum with characteristics not reported so far for anyother AGN. The quasar not only shows an extremely strong relativistic broad ironline, the whole spectrum can be understood as relativistically blurredreflection from a rotating inner disk around a supermassive Kerr black hole,whereas the usual power-law continuum is completely suppressed. We propose tomonitor PG 2112+059 with two 70ks observations separated by half a year and, ifthe low state is detected, to study the detailed properties of the broad ironline with a (triggered) 220ks observations.
Publications	A long hard look at the minimum state of PG 2112+059 with XMM-Newton \|Schartel, N., Rodriguez-Pascual, P. M., et al. \| A&A \| 512-75 \| 2010 \| 2010A&A...512A..75S \| http://ui.adsabs.harvard.edu/#abs/2010A&A...512A..75S Identifying XMM-Newton observations affected by solar wind charge exchange - Part II \|Carter, J. A., Sembay, S., \| A&A \| 527-115 \| 2011 \| 2011A&A...527A.115C \| http://ui.adsabs.harvard.edu/#abs/2011A&A...527A.115C The XMM Cluster Survey: optical analysis methodology and the first data release \|Mehrtens, Nicola, Romer, A. Kathy, et al. \| MNRAS \| 423-1024 \| 2012 \| 2012MNRAS.423.1024M \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.1024M An All-Sky Atlas of Radio/X-ray Associations \|Flesch, E., \| PASA \| 27-283 \| 2010 \| 2010PASA...27..283F \| http://ui.adsabs.harvard.edu/#abs/2010PASA...27..283F The XMM Cluster Survey: X-ray analysis methodology \|Lloyd-Davies, E. J., Romer, A. Kathy, et al. \| MNRAS \| 418-14 \| 2011 \| 2011MNRAS.418...14L \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.418...14L Exospheric solar wind charge exchange as seen by XMM-Newton \|Carter, J. A., Semba, S., \| AN \| 333-313 \| 2012 \| 2012AN....333..313C \| http://ui.adsabs.harvard.edu/#abs/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 al. \| MNRAS \| 423-3561 \| 2012 \| 2012MNRAS.423.3561C \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.3561C Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog \|Lin, Dacheng, Webb, Natalie A., \| ApJ \| 756-27 \| 2012 \| 2012ApJ...756...27L \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...756...27L 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 \| http://ui.adsabs.harvard.edu/#abs/2012ApJS..202...14H The Long-term X-Ray Variability of Broad Absorption Line Quasars \|Saez, C., Brandt, W. N., et al. \| ApJ \| 759-42 \| 2012 \| 2012ApJ...759...42S \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...759...42S Properties of the integrated spectrum of serendipitous 2XMM catalog sources \|Chaudhary, P., Brusa, M., et al. \| A&A \| 518-58 \| 2010 \| 2010A&A...518A..58C \| http://ui.adsabs.harvard.edu/#abs/2010A&A...518A..58C Rest-frame stacking of 2XMM catalog sources. Properties of the Fe Kalpha line \|Chaudhary, P., Brusa, M., et al. \| A&A \| 537-6 \| 2012 \| 2012A&A...537A...6C \| http://ui.adsabs.harvard.edu/#abs/2012A&A...537A...6C Automatic Classification of Time-variable X-Ray Sources \|Lo, Kitty K., Farrell, Sean, et al. \| ApJ \| 786-20 \| 2014 \| 2014ApJ...786...20L \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...786...20L The diversity of quasars unified by accretion and orientation \|Shen, Yue, Ho, Luis C., \| Natur \| 513-210 \| 2014 \| 2014Natur.513..210S \| http://ui.adsabs.harvard.edu/#abs/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 \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y Sunyaev-Zel.dovich effect or not? Detecting the main foreground effect of most galaxy clusters \|Xiao, Weike, Chen, Chen, et al. \| MNRAS \| 432-41 \| 2013 \| 2013MNRAS.432L..41X \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.432L..41X Unveiling the X-ray/UV properties of disk winds in active galactic nuclei using broad and mini-broad absorption line quasars \|Giustini, M., \| AN \| 337-459 \| 2016 \| 2016AN....337..459G \| http://ui.adsabs.harvard.edu/#abs/2016AN....337..459G 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 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 \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...829....9M SPIDERS: the spectroscopic follow-up of X-ray selected clusters of galaxies in SDSS-IV \|Clerc, N., Merloni, A., et al. \| MNRAS \| 463-4490 \| 2016 \| 2016MNRAS.463.4490C \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.463.4490C 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 XMM Cluster Outskirts Project (X-COP): Physical conditions of Abell 2142 up to the virial radius \|Tchernin, C., Eckert, D., et al. \| A&A \| 595-42 \| 2016 \| 2016A&A...595A..42T \| http://ui.adsabs.harvard.edu/#abs/2016A&A...595A..42T Dark matter distribution in X-ray luminous galaxy clusters with Emergent Gravity \|Ettori, S., Ghirardini, V., et al. \| MNRAS \| 470-29 \| 2017 \| 2017MNRAS.470L..29E \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.470L..29E Anisotropy of the galaxy cluster X-ray luminosity-temperature relation \|Migkas, Konstantinos, Reiprich, Thomas H., \| A&A \| 611-50 \| 2018 \| 2018A&A...611A..50M \| http://ui.adsabs.harvard.edu/#abs/2018A&A...611A..50M Reconstruction of the two-dimensional gravitational potential of galaxy clusters from X-ray and Sunyaev-Zel.dovich measurements \|Tchernin, C., Bartelmann, M., et al. \| A&A \| 614-38 \| 2018 \| 2018A&A...614A..38T \| http://ui.adsabs.harvard.edu/#abs/2018A&A...614A..38T The XMM Cluster Survey: Present status and latest results \|Viana, P. T. P., Mehrtens, N., et al. \| AN \| 334-462 \| 2013 \| 2013AN....334..462V \| http://ui.adsabs.harvard.edu/#abs/2013AN....334..462V The Physics of Galaxy Cluster Outskirts \|Walker, Stephen, Simionescu, Aurora, et al. \| SSRv \| 215-7 \| 2019 \| 2019SSRv..215....7W \| http://ui.adsabs.harvard.edu/#abs/2019SSRv..215....7W Testing emergent gravity on galaxy cluster scales \|Tamosiunas, Andrius, Bacon, David, et al. \| JCAP \| 5-53 \| 2019 \| 2019JCAP...05..053T \| http://ui.adsabs.harvard.edu/#abs/2019JCAP...05..053T Chandra Follow-up of the SDSS DR8 Redmapper Catalog Using the MATCha Pipeline \|Hollowood, Devon L., Jeltema, Tesla, et al. \| ApJS \| 244-22 \| 2019 \| 2019ApJS..244...22H \| http://ui.adsabs.harvard.edu/#abs/2019ApJS..244...22H Stellar mass as a galaxy cluster mass proxy: application to the Dark Energy Survey redMaPPer clusters \|Palmese, A., Annis, J., et al. \| MNRAS \| 493-4591 \| 2020 \| 2020MNRAS.493.4591P \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.493.4591P X-ray properties of the X-CLASS-redMaPPer galaxy cluster sample: the luminosity-temperature relation \|Molham, Mona, Clerc, Nicolas, et al. \| MNRAS \| 494-161 \| 2020 \| 2020MNRAS.494..161M \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.494..161M Multiwavelength classification of X-ray selected galaxy cluster candidates using convolutional neural networks \|Kosiba, Matej, Lieu, Maggie, et al. \| MNRAS \| 496-4141 \| 2020 \| 2020MNRAS.496.4141K \| http://ui.adsabs.harvard.edu/#abs/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 al. \| MNRAS \| 497-3976 \| 2020 \| 2020MNRAS.497.3976C \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.497.3976C An X-Ray- and SZ-bright Diffuse Source toward M31: A Local Hot Bridge \|Qu, Zhijie, Huang, Rui, et al. \| ApJ \| 907-14 \| 2021 \| 2021ApJ...907...14Q \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...907...14Q 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 Yet another test of Radial Acceleration Relation for galaxy clusters \|Pradyumna, S., Gupta, Sajal, et al. \| PDU \| 31-100765 \| 2021 \| 2021PDU....3100765P \| http://ui.adsabs.harvard.edu/#abs/2021PDU....3100765P Graviton mass from X-COP galaxy clusters \|Pi\\u00f3rkowska-Kurpas, Aleksandra, Cao, Shuo, \| JHEAp \| 33-37 \| 2022 \| 2022JHEAp..33...37P \| http://ui.adsabs.harvard.edu/#abs/2022JHEAp..33...37P Moffat.s modified gravity tested on X-COP galaxy clusters \|Harikumar, Sreekanth, Biesiada, Marek, \| EPJC \| 82-241 \| 2022 \| 2022EPJC...82..241H \| http://ui.adsabs.harvard.edu/#abs/2022EPJC...82..241H The Solar Cycle Temporal Variation of the Solar Wind Charge Exchange X-Ray Lines \|Qu, Zhijie, Koutroumpa, Dimitra, et al. \| ApJ \| 930-21 \| 2022 \| 2022ApJ...930...21Q \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...930...21Q The gravitational field of X-COP galaxy clusters \|Eckert, D., Ettori, S., et al. \| A&A \| 662-123 \| 2022 \| 2022A&A...662A.123E \| http://ui.adsabs.harvard.edu/#abs/2022A&A...662A.123E A test of galaxy cluster fundamental plane for the X-COP sample \|Pradyumna, S., Desai, Shantanu, \| JCAP \| 1-58 \| 2022 \| 2022JCAP...01..058P \| http://ui.adsabs.harvard.edu/#abs/2022JCAP...01..058P A disturbing FABLE of mergers, feedback, turbulence, and mass biases in simulated galaxy clusters \|Bennett, Jake S., Sijacki, Debora, \| MNRAS \| 514-313 \| 2022 \| 2022MNRAS.514..313B \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.514..313B Constraints on dark matter self-interaction from the internal density profiles of X-COP galaxy clusters \|Eckert, D., Ettori, S., et al. \| A&A \| 666-41 \| 2022 \| 2022A&A...666A..41E \| http://ui.adsabs.harvard.edu/#abs/2022A&A...666A..41E Investigating the turbulent hot gas in X-COP galaxy clusters \|Dupourqu\\u00e9, S., Clerc, N., et al. \| A&A \| 673-91 \| 2023 \| 2023A&A...673A..91D \| http://ui.adsabs.harvard.edu/#abs/2023A&A...673A..91D Testing generalized scalar-tensor theories of gravity with clusters of galaxies \|Haridasu, Balakrishna S., Karmakar, Purnendu, et al. \| PhRvD \| 107-124059 \| 2023 \| 2023PhRvD.107l4059H \| http://ui.adsabs.harvard.edu/#abs/2023PhRvD.107l4059H 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 From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources \|Rodriguez, Antonio C., \| PASP \| 136-054201 \| 2024 \| 2024PASP..136e4201R \| http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R 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	2007-05-03T21:45:24Z/2007-11-06T00:17:52Z
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	2008-11-28T00:00:00Z
Keywords	"XMM", "pg 2112", "xray spectrum", "iron line", "triggered 220", "broad iron line", "completely suppressed", "XMM-Newton", "rotating inner disk", "xmm newton", "relativistically blurred reflection"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Norbert Schartel, 2008, 'The extreme X-ray spectrum and iron line of PG 2112+059', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-zi8aao2