A dataset provided by the European Space Agency

Name: Understanding X-ray Emission from AGN in Low Surface Brightness Galaxies
Published: 2017-03-09T23:00:00Z

Proposal ID	076330
Title	Understanding X-ray Emission from AGN in Low Surface Brightness Galaxies
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0763300101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0763300201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0763300301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0763300501
DOI	https://doi.org/10.5270/esa-7glpowx
Principal Investigator, PI	Dr Harsha Raichur
Abstract	We propose for XMM-Newton observations of 6 nearby, bulge dominated giant lowsurface brightness (GLSB) galaxies. They have diffuse stellar disks and massiveHI disks but are overall poor in star formation. They are possibly the most darkmatter dominated spirals in our nearby universe and yet a significant fractionof them have prominent bulges that host AGN activity. Optical studies indicatethat their AGN black hole masses are low compared to their galaxy masses and liebelow the M-sigma correlation. Not much is known about the AGN activity andbulge evolution in these galaxies, especially in the X-ray domain. Our proposedXMM-Newton observations will be used to detect and characterize the X-rayproperties of these systems.
Publications	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 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	2015-10-27T14:28:55Z/2016-02-18T11:19:10Z
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	2017-03-09T23:00:00Z
Keywords	"agn blackhole masses", "xray properties", "star formation", "XMM", "prominent bulges", "massive hi dis", "galaxy masses", "xray domain", "agn activity", "nearby universe", "XMM-Newton", "xray emission", "bulge evolution", "diffuse stellar dis", "sigma correlation", "xmm newton"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Harsha Raichur, 2017, 'Understanding X-ray Emission from AGN in Low Surface Brightness Galaxies', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-7glpowx