A dataset provided by the European Space Agency

Name: H 0557-385 and the evolution of ionised outflows in Seyfert galaxies
Published: 2007-12-05T00:00:00Z

Proposal ID	040426
Title	H 0557-385 and the evolution of ionised outflows in Seyfert galaxies
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0404260101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0404260201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0404260301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0404260401
DOI	https://doi.org/10.5270/esa-masn2lt
Principal Investigator, PI	Dr Alexander Blustin
Abstract	We propose to perform a 130 ks observation of the Seyfert 1 galaxy H 0557-385,to obtain a high quality RGS spectrum of its very high column density ionisedoutflow (warm absorber). We will compare the properties of this outflow withthose of closer, less luminous Seyferts to investigate how the outflowcharacteristics depend on luminosity. Since Seyfert warm absorbers are just aghostly reminder of the much deeper, faster outflows in Broad Absorption Linequasars (BALQSOs), we will investigate whether this extreme object pointstowards the existence of an intermediate class of ionised outflow withproperties somewhere between those of nearby Seyferts and luminous BALQSOs. Thiswill provide an insight into how AGN outflows have evolved as the AGN population has dimmed with cosmic time.
Publications	The Swift Burst Alert Telescope Detected Seyfert 1 Galaxies: X-Ray Broadband Properties and Warm Absorbers \|Winter, Lisa M., Veilleux, Sylvain, et al. \| ApJ \| 745-107 \| 2012 \| 2012ApJ...745..107W \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...745..107W 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 Evidence for ultra-fast outflows in radio-quiet AGNs. I. Detection and statistical incidence of Fe K-shell absorption lines \|Tombesi, F., Cappi, M., et al. \| A&A \| 521-57 \| 2010 \| 2010A&A...521A..57T \| http://ui.adsabs.harvard.edu/#abs/2010A&A...521A..57T X-ray Outflows in the Swift Burst Alert Detected Seyfert 1s \|Winter, Lisa M., \| ApJ \| 725-126 \| 2010 \| 2010ApJ...725L.126W \| http://ui.adsabs.harvard.edu/#abs/2010ApJ...725L.126W 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 Fe Kalpha line profile in AGNs: average shape and redshift dependence \|Mao, Wei-Ming, Hu, Chen, et al. \| RAA \| 10-905 \| 2010 \| 2010RAA....10..905M \| http://ui.adsabs.harvard.edu/#abs/2010RAA....10..905M Obscuring clouds playing hide-and-seek in the active nucleus H0557-385 \|Longinotti, A. L., Bianchi, S., et al. \| MNRAS \| 394-1 \| 2009 \| 2009MNRAS.394L...1L \| http://ui.adsabs.harvard.edu/#abs/2009MNRAS.394L...1L 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 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 Swift Follow-up Observations of Candidate Gravitational-wave Transient Events \|Evans, P. A., Fridriksson, J. K., et al. \| ApJS \| 203-28 \| 2012 \| 2012ApJS..203...28E \| http://ui.adsabs.harvard.edu/#abs/2012ApJS..203...28E A systematic cross-search for radio/infrared counterparts of XMM- Newton sources \|Combi, J. A., Albacete Colombo, J. F., et al. \| Ap&SS \| 331-53 \| 2011 \| 2011Ap&SS.331...53C \| http://ui.adsabs.harvard.edu/#abs/2011Ap&SS.331...53C 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 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 Absorption at the dust sublimation radius and the dichotomy between X-ray and optical classification in the Seyfert galaxy H0557-385 \|Coffey, D., Longinotti, A. L., et al. \| MNRAS \| 443-1788 \| 2014 \| 2014MNRAS.443.1788C \| http://ui.adsabs.harvard.edu/#abs/2014MNRAS.443.1788C 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 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 Multiwavelength search for counterparts of supersoft X-ray sources in M31 \|Chiosi, E., Orio, M., et al. \| MNRAS \| 443-1821 \| 2014 \| 2014MNRAS.443.1821C \| http://ui.adsabs.harvard.edu/#abs/2014MNRAS.443.1821C 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 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 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 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 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 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 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 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 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 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 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 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	2006-08-11T07:08:01Z/2006-11-04T11:06:32Z
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	2007-12-05T00:00:00Z
Keywords	"luminous seyferts", "quality rgs spectrum", "cosmic time", "agn population", "nearby seyferts", "seyfert warm absorbers", "ionised outflows", "0557 385", "seyfert galaxy", "ionised outflow", "luminous balqsos", "intermediate class", "faster outflows", "agn outflows", "outflow characteristics depend", "ghostly reminder"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Alexander Blustin, 2007, 'H 0557-385 and the evolution of ionised outflows in Seyfert galaxies', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-masn2lt