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 Search for Young Stellar Objects within 4XMM-DR13 Using CatBoost and SPE \|Ma Xiangyao Zhang Yanxia et al. \| AJ \| 168-210 \| 2024 \| 2024AJ....168..210M \| http://ui.adsabs.harvard.edu/#abs/2024AJ....168..210M New 511 keV Line Data Provide Strongest sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 973-L6 \| 2024 \| 2024ApJ...973L...6D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...973L...6D
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	2025-08-04
Keywords	"XMM", "xmm newton epic", "XMM-Newton", "agn fraction", "luminous infrared galaxy", "hard xray spectra", "fe line properties", "xmm newton", "snapshot chandra", "EPIC", "nearby lirg population", "kev flux", "nearby lirgs", "heavily obscured agn"
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