A dataset provided by the European Space Agency

Name: NGC 1194: X-RAY REPROCESSING IN A LOCAL COMPTON THICK MASER AGN
Published: 2021-02-10T23:00:00Z

Proposal ID	085220
Title	NGC 1194: X-RAY REPROCESSING IN A LOCAL COMPTON THICK MASER AGN
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0852200101
DOI	https://doi.org/10.57780/esa-1al1z7t
Principal Investigator, PI	Dr Tracey Turner
Abstract	NGC 1194 is one of the hardest AGN in the local sky and a rare example ofa nearby Compton-thick Seyfert galaxy. This AGN houses a water maser,providing an intriguing possible origin for the Compton-thick gas. Werequest a joint 60 ks NuSTAR/XMM observation to build a model for thisspectacular AGN. Availability of an accurate black hole mass and maserdisk inclination give a solid framework of scale-size, Eddington ratio andorientation for interpretation of the X-ray data.
Publications	Elucidating the global distribution of reprocessing gas in NGC 1194 \|Turner, T. J., Reeves, J. N., et al. \| MNRAS \| 498-1983 \| 2020 \| 2020MNRAS.498.1983T \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.498.1983T 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 WISDOM Project - XVI. The link between circumnuclear molecular gas reservoirs and active galactic nucleus fuelling \|Elford, Jacob S., Davis, Timothy A., et al. \| MNRAS \| 528-319 \| 2024 \| 2024MNRAS.528..319E \| http://ui.adsabs.harvard.edu/#abs/2024MNRAS.528..319E 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
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2020-01-16T23:28:22Z/2020-01-17T19:05:02Z
Version	18.01_20200110_1700
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	2021-02-10T23:00:00Z
Keywords	"NuSTAR", "eddington ratio", "xray data", "XMM", "spectacular agn", "maser disk inclination", "ngc 1194", "blackhole mass", "water maser", "NGC 1194", "hardest agn", "xray reprocessing", "scale size", "local sky", "solid framework", "rare example", "compton thick gas", "agn houses"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Tracey Turner, 2021, 'NGC 1194: X-RAY REPROCESSING IN A LOCAL COMPTON THICK MASER AGN', 18.01_20200110_1700, European Space Agency, https://doi.org/10.57780/esa-1al1z7t