A dataset provided by the European Space Agency

Name: Searching for Nearby ULXs in HST Imaged Galaxies
Published: 2014-05-16T22:00:00Z

Proposal ID	072191
Title	Searching for Nearby ULXs in HST Imaged Galaxies
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0721910101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0721910201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0721910301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0721910401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0721910501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0721910601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0721910701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0721910801 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0721910901 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0721911001 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0721911101 ...
DOI	https://doi.org/10.5270/esa-n98u0k9
Principal Investigator, PI	Prof Philip Kaaret
Abstract	We propose to survey 11 nearby galaxies with XMM to search for new ultraluminousX-ray sources (ULXs). Most ULXs are associated with star formation and arelikely stellar mass black holes in super-Eddington accretion states or withmildly beamed emission. Some of the strongest intermediate mass black hole(IMBH) candidates are found in galaxies with low star formation rates (SFRs).Our survey will sample late-type galaxies with low SFRs that lack deep X-raydata but are covered by archival Hubble Space Telescope observations enabling usto identify optical counterparts and study the surrounding environments.
Publications	Searching for X-ray sources in nearby late-type galaxies with low-star formation rates \|Chatterjee K. Kaaret P. et al. \| MNRAS \| 456-2966 \| 2016 \| 2016MNRAS.456.2966C \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.456.2966C 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 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 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	2013-08-08T08:32:42Z/2014-01-26T13:11:55Z
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	2014-05-16T22:00:00Z
Last Update	2025-01-27
Keywords	"hst imaged galaxy", "low sfrs", "star formation", "optical counterparts", "stellar mass blackhole", "super eddington accretion", "XMM", "mildly beamed emission", "nearby galaxy", "deep xray data", "nearby ulxs", "HST"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof Philip Kaaret, 2014, 'Searching for Nearby ULXs in HST Imaged Galaxies', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-n98u0k9