A dataset provided by the European Space Agency

Name: X-ray emission of a representative sample of local Luminous Infrared Galaxies
Published: 2011-03-02T00:00:00Z

Proposal ID	060160
Title	X-ray emission of a representative sample of local Luminous Infrared Galaxies
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0601600101
DOI	https://doi.org/10.5270/esa-xy0qhlc
Principal Investigator, PI	Dr Almudena Alonso-Herrero
Abstract	We propose to observe with XMM-Newton 8 Luminous Infrared Galaxies (LIRGs,L_IR=10^11-10^12L_sun) and analyze existing X-ray data for another 7 LIRGs.Previous X-ray studies of local LIRGs are biased towards the most IR-luminousobjects as well as those systems hosting a bright AGN. These 15 local LIRGs arerepresentative of the LIRG class in terms of IR luminosity and nuclear activity.The proposed XMM observations and existing multi-wavelength data will allow tocharacterize the star formation history of these galaxies and relate it to theirX-ray emission. A comprehensive multi-wavelength understanding of the extremeprocesses (star formation and AGN) taking place in local LIRGs is needed toimprove the linkage of X-ray, UV and IR observations of deep cosmological fields.
Publications	The X-ray emission of local luminous infrared galaxies \|Pereira-Santaella M. Alonso-Herrero A. et al. \| A&A \| 535-93 \| 2011 \| 2011A&A...535A..93P \| http://ui.adsabs.harvard.edu/#abs/2011A&A...535A..93P 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 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 A new clean catalogue of extragalactic non-nuclear X-ray sources in nearby galaxies \|Earnshaw H. P. Roberts T. P. et al. \| MNRAS \| 483-5554 \| 2019 \| 2019MNRAS.483.5554E \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.483.5554E 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 impact of precession on the observed population of ULXs \|Khan Norman Middleton Matthew J. et al. \| MNRAS \| 509-2493 \| 2022 \| 2022MNRAS.509.2493K \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.509.2493K The Redshift Evolution of Ultraluminous X-Ray Sources out to z 0.5: Comparison with X-Ray Binary Populations and Contribution to the Cosmic X-Ray Background \|Scott Barrows R. Comerford Julia M. et al. \| ApJ \| 932-27 \| 2022 \| 2022ApJ...932...27S \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...932...27S 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	2010-01-23T16:23:30Z/2010-01-24T04:53:46Z
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	2011-03-02T00:00:00Z
Last Update	2025-01-27
Keywords	"processes star formation", "nuclear activity", "local lirgs", "deep cosmological fields", "comprehensive multi wavelength", "biased towards", "xmm newton", "bright agn", "XMM-Newton", "ir luminous objects", "x ray emission", "agn taking", "xray emission", "star formation history", "XMM", "ir luminosity", "lirg class"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Almudena Alonso-Herrero, 2011, 'X-ray emission of a representative sample of local Luminous Infrared Galaxies', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-xy0qhlc