A dataset provided by the European Space Agency

Name: Compact Composite AGN-Starbursts: hidden AGN or slow starburst-driven shocks?
Published: 2014-04-12T00:00:00Z

Proposal ID	069354
Title	Compact Composite AGN-Starbursts: hidden AGN or slow starburst-driven shocks?
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693540101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693540201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693540301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693540401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693540501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693540601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693540701
DOI	https://doi.org/10.5270/esa-wgcjzm8
Principal Investigator, PI	Dr Andrew Ptak
Abstract	We propose observations of a sample of IR-selected galaxies dominated by apowerful starburst but where a hidden AGN may enhance the optical emission lineratios. Recent models, however, have shown that objects of composite type couldbe falsely flagged as hosting an AGN in the presence of shocks associated withstarburst superwinds. Radio VLBI observations on the IR-selected sources pointto a lack of AGN, and thus favoring the shock-interpretation for these sources.These observations will increase the current sample with good XMM data and willdetermine whether black holes are accreting and dominating the X-ray emission inthese starbursts. This would aid in determining at what level AGN are present inobjects of composite-type spectra at low redshift.
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 The 2MIG isolated AGNs - I. General and multiwavelength properties of AGNs and host galaxies in the northern sky \|Pulatova N. G. Vavilova I. B. et al. \| MNRAS \| 447-2209 \| 2015 \| 2015MNRAS.447.2209P \| http://ui.adsabs.harvard.edu/#abs/2015MNRAS.447.2209P X-Ray Spectral Properties of the Isolated AGNs: NGC 1050 NGC 2989 ESO 317-038 ESO 438-009 \|Vavilova I. B. Vasylenko A. A. et al. \| OAP \| 28-150 \| 2015 \| 2015OAP....28..150V \| http://ui.adsabs.harvard.edu/#abs/2015OAP....28..150V 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	2012-07-07T08:02:31Z/2013-03-25T08:07:44Z
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	2014-04-12T00:00:00Z
Last Update	2025-01-27
Keywords	"starburst superwinds", "xmm data", "composite type", "falsely flagged", "hidden agn", "level agn", "powerful starburst", "galaxy dominated", "xray emission", "composite type spectra", "XMM", "radio vlbi", "low redshift"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Andrew Ptak, 2014, 'Compact Composite AGN-Starbursts: hidden AGN or slow starburst-driven shocks?', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-wgcjzm8