A dataset provided by the European Space Agency

Name: How Powerful Are Quasar OutflowsquestionMark
Published: 2011-12-22T00:00:00Z

Proposal ID	065133
Title	How Powerful Are Quasar Outflows?
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0651330101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0651330201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0651330301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0651330401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0651330501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0651330601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0651330701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0651330801 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0651330901 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0651331001 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0651331101 ...
DOI	https://doi.org/10.5270/esa-87g5ucw
Principal Investigator, PI	Prof William Brandt
Abstract	X-ray absorption studies of quasar outflows with low-resolution CCD spectroscopycannot reliably determine the outflow kinetic luminosity. We therefore proposean ambitious long-look observation to obtain the first high-quality gratingspectroscopy of a mini-BAL quasar (PG 1114+445). Grating spectroscopy of a smallsample of local Seyfert galaxies has led to highly regarded accuratedeterminations of their wind properties. The proposed extension of gratingspectroscopy to the first mini-BAL quasar level AGN will determine if theoutflow becomes as powerful as required in current AGN feedback scenarios. The375,000 count EPIC spectra from this long-look will enable unprecedentedcomplementary studies of high-energy absorption features and iron K emission.
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 XMM-Newton publication statistics \|Ness, J.-U., Parmar, A. N., et al. \| AN \| 335-210 \| 2014 \| 2014AN....335..210N \| http://ui.adsabs.harvard.edu/#abs/2014AN....335..210N 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 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 Dependence of the broad Fe Kalpha line on the physical parameters of AGN \|Liu, Zhu, Yuan, Weimin, et al. \| MNRAS \| 463-684 \| 2016 \| 2016MNRAS.463..684L \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.463..684L 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 Multiphase quasar-driven outflows in PG 1114+445. I. Entrained ultra-fast outflows \|Serafinelli, Roberto, Tombesi, Francesco, et al. \| A&A \| 627-121 \| 2019 \| 2019A&A...627A.121S \| http://ui.adsabs.harvard.edu/#abs/2019A&A...627A.121S Quasars as standard candles II. The non-linear relation between UV and X-ray emission at high redshifts \|Salvestrini, F., Risaliti, G., et al. \| A&A \| 631-120 \| 2019 \| 2019A&A...631A.120S \| http://ui.adsabs.harvard.edu/#abs/2019A&A...631A.120S 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 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 The EXTraS project: Exploring the X-ray transient and variable sky \|De Luca, A., Salvaterra, R., et al. \| A&A \| 650-167 \| 2021 \| 2021A&A...650A.167D \| http://ui.adsabs.harvard.edu/#abs/2021A&A...650A.167D X-ray obscuration from a variable ionized absorber in PG 1114+445 \|Serafinelli, R., Braito, V., et al. \| A&A \| 654-32 \| 2021 \| 2021A&A...654A..32S \| http://ui.adsabs.harvard.edu/#abs/2021A&A...654A..32S 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 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	2010-05-19T09:48:59Z/2010-12-13T06:33:25Z
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	2011-12-22T00:00:00Z
Keywords	"quasar outflows ?.", "outflow kinetic luminosity", "EPIC", "grating spectroscopy", "local seyfert galaxy", "wind properties", "energy absorption", "xray absorption", "agn feedback scenarios", "quasar outflows", "quality grating spectroscopy"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof William Brandt, 2011, 'How Powerful Are Quasar OutflowsquestionMark', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-87g5ucw