A dataset provided by the European Space Agency

Name: PG 0804+761: Investigation of a blue outlier outflow
Published: 2011-03-27T00:00:00Z

Proposal ID	060511
Title	PG 0804+761: Investigation of a blue outlier outflow
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0605110101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0605110201
DOI	https://doi.org/10.5270/esa-vtn3kk6
Principal Investigator, PI	Mr Rob Detmers
Abstract	We propose to observe the blue outlier AGN PG 0804+761 for 100,ks with RGS toobtain detailed information on the outflow and further investigate theconnection between blue outliers (blueshifted ion{O},{III} emission) andpowerful outflows. Through this observation we will obtain accurate outflowvelocities and the ionization structure of the outflow, which allows us to testa scenario where the blueshifted emission lines are connected to a high velocityoutflow.
Publications	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 Are X-Ray Emitting Coronae around Supermassive Black Holes Outflowing? \|Liu, Teng, Wang, Jun-Xian, et al. \| ApJ \| 783-106 \| 2014 \| 2014ApJ...783..106L \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...783..106L 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 A hard X-ray view of the soft excess in AGN \|Boissay, Rozenn, Ricci, Claudio, \| A&A \| 588-70 \| 2016 \| 2016A&A...588A..70B \| http://ui.adsabs.harvard.edu/#abs/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 \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...822...21H 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 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 \| http://ui.adsabs.harvard.edu/#abs/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 al. \| A&A \| 611-59 \| 2018 \| 2018A&A...611A..59P \| http://ui.adsabs.harvard.edu/#abs/2018A&A...611A..59P 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 High Density Reflection Spectroscopy - II. The density of the inner black hole accretion disc in AGN \|Jiang, Jiachen, Fabian, Andrew C., et al. \| MNRAS \| 489-3436 \| 2019 \| 2019MNRAS.489.3436J \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.489.3436J The soft X-ray excess: NLS1s versus BLS1s \|Gliozzi, Mario, Williams, James K., \| MNRAS \| 491-532 \| 2020 \| 2020MNRAS.491..532G \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.491..532G Estimating the size of X-ray lamppost coronae in active galactic nuclei \|Ursini, F., Dov\\u010diak, M., et al. \| A&A \| 644-132 \| 2020 \| 2020A&A...644A.132U \| http://ui.adsabs.harvard.edu/#abs/2020A&A...644A.132U On the Observational Difference between the Accretion Disk-Corona Connections among Super- and Sub-Eddington Accreting Active Galactic Nuclei \|Liu, Hezhen, Luo, B., et al. \| ApJ \| 910-103 \| 2021 \| 2021ApJ...910..103L \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...910..103L 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 Supermassive Black Hole Winds in X-rays: SUBWAYS. I. Ultra-fast outflows in quasars beyond the local Universe \|Matzeu, G. A., Brusa, M., et al. \| A&A \| 670-182 \| 2023 \| 2023A&A...670A.182M \| http://ui.adsabs.harvard.edu/#abs/2023A&A...670A.182M 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 Unveiling energy pathways in AGN accretion flows with the warm corona model for the soft excess \|Ballantyne, D. R., Sudhakar, V., et al. \| MNRAS \| 530-1603 \| 2024 \| 2024MNRAS.530.1603B \| http://ui.adsabs.harvard.edu/#abs/2024MNRAS.530.1603B 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	2010-03-10T11:05:02Z/2010-03-12T23:56:10Z
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	2011-03-27T00:00:00Z
Keywords	"blue outlier", "blueshifted emission lines", "outflow velocities", "agn pg 0804", "pg 0804", "powerful outflows", "velocity outflow", "blue outliers blueshifted", "blue outlier outflow", "ionization structure"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Mr Rob Detmers, 2011, 'PG 0804+761: Investigation of a blue outlier outflow', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-vtn3kk6