A dataset provided by the European Space Agency

Name: Hard X-ray spectra of nearby LIRGs from GOALS
Published: 2013-05-12T00:00:00Z

Proposal ID	067030
Title	Hard X-ray spectra of nearby LIRGs from GOALS
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0670300101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0670300301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0670300401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0670300601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0670300701
DOI	https://doi.org/10.5270/esa-i0z3skw
Principal Investigator, PI	Dr Kazushi Iwasawa
Abstract	We propose XMM-Newton EPIC observations of six luminous infrared galaxies,selected from the GOALS sample. The targets are selected based on the 2-7 keVflux measured with snapshot Chandra observations, aiming to study their hardX-ray spectra and Fe line properties with XMM-Newton. This proposed follow- upobservations are essential to determine the AGN fraction in the nearby LIRGpopulation by minimizing the bias against heavily obscured AGN which generallyhave faint hard X-ray emission and a large throughput of XMM-Newton is requiredto examine its nature.
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 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 Study of X-Ray Emission of Galaxies Hosting Molecular Outflows (MOX Sample) \|Laha Sibasish Guainazzi Matteo et al. \| ApJ \| 868-10 \| 2018 \| 2018ApJ...868...10L \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...868...10L A Comparison of X-Ray Photon Indices among the Narrow- and Broad-line Seyfert 1 Galaxies \|Ojha Vineet Chand Hum et al. \| ApJ \| 896-95 \| 2020 \| 2020ApJ...896...95O \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...896...95O 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 A hard X-ray view of luminous and ultra-luminous infrared galaxies in GOALS - I. AGN obscuration along the merger sequence \|Ricci C. Privon G. C. et al. \| MNRAS \| 506-5935 \| 2021 \| 2021MNRAS.506.5935R \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.506.5935R Comprehensive Broadband X-Ray and Multiwavelength Study of Active Galactic Nuclei in 57 Local Luminous and Ultraluminous Infrared Galaxies Observed with NuSTAR and/or Swift/BAT \|Yamada Satoshi Ueda Yoshihiro et al. \| ApJS \| 257-61 \| 2021 \| 2021ApJS..257...61Y \| http://ui.adsabs.harvard.edu/#abs/2021ApJS..257...61Y Low-frequency Radio Continuum Imaging and SED Modeling of 11 LIRGs: Radio-only and FUV to Radio Bands \|Dey Subhrata Goyal Arti et al. \| ApJ \| 938-152 \| 2022 \| 2022ApJ...938..152D \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...938..152D 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 The origin of the X-ray emission from the non-starburst gas-rich luminous infrared galaxies Arp 302 \|Jiang Jiachen Baker William et al. \| MNRAS \| 528-1223 \| 2024 \| 2024MNRAS.528.1223J \| http://ui.adsabs.harvard.edu/#abs/2024MNRAS.528.1223J 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	2012-01-16T13:18:23Z/2012-04-23T15:25:13Z
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	2013-05-12T00:00:00Z
Last Update	2025-01-27
Keywords	"EPIC", "agn fraction", "luminous infrared galaxy", "hard xray spectra", "nearby lirg population", "heavily obscured agn", "xmm newton epic", "xmm newton", "XMM-Newton", "kev flux", "nearby lirgs", "XMM", "snapshot chandra", "fe line properties"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Kazushi Iwasawa, 2013, 'Hard X-ray spectra of nearby LIRGs from GOALS', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-i0z3skw