A dataset provided by the European Space Agency

Name: XMM and NuSTAR Observations of Local ULIRGs
Published: 2014-11-27T00:00:00Z

Proposal ID	072261
Title	XMM and NuSTAR Observations of Local ULIRGs
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0722610101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0722610201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0722610301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0722610401
DOI	https://doi.org/10.5270/esa-hocbx95
Principal Investigator, PI	Dr Stacy Teng
Abstract	We request a total of 123 ks of EPIC data to observe four local ULIRGs that arePriority A NuSTAR targets. The XMM data will help determine whether the X-rayweak nature of these sources is due to intrinsically weak or highly absorbedAGNs. With NuSTAR, we can reach to unprecedented sensitivities at above 10 keV.Contemporaneous XMM coverage is essential to place constraints on the columndensities and the intrinsic AGN luminosities of these highly absorbed, compositeobjects and to pinpoint the origin of the variability below 10 keV seen in thesesources. Our NuSTAR program will contextualize the AGN contribution to localULIRGs, which will bear on results obtained at other wavelengths on thecosmological significance of ULIRGs to galaxy evolution and black hole growth.
Publications	A NuSTAR Survey of Nearby Ultraluminous Infrared Galaxies \|Teng Stacy H. Rigby Jane R. et al. \| ApJ \| 814-56 \| 2015 \| 2015ApJ...814...56T \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...814...56T 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 Evidence for Relativistic Disk Reflection in the Seyfert 1h Galaxy/ULIRG IRAS 05189-2524 Observed by NuSTAR and XMM-Newton \|Xu Yanjun Balokovic Mislav et al. \| ApJ \| 837-21 \| 2017 \| 2017ApJ...837...21X \| http://ui.adsabs.harvard.edu/#abs/2017ApJ...837...21X AGN spectral states from simultaneous UV and X-ray observations by XMM-Newton \|Svoboda J. Guainazzi M. \| A&A \| 603-127 \| 2017 \| 2017A&A...603A.127S \| http://ui.adsabs.harvard.edu/#abs/2017A&A...603A.127S The NuSTAR Extragalactic Surveys: X-Ray Spectroscopic Analysis of the Bright Hard-band Selected Sample \|Zappacosta L. Comastri A. et al. \| ApJ \| 854-33 \| 2018 \| 2018ApJ...854...33Z \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...854...33Z Diffuse X-Ray-emitting Gas in Major Mergers \|Smith Beverly J. Campbell Kristen et al. \| AJ \| 155-81 \| 2018 \| 2018AJ....155...81S \| http://ui.adsabs.harvard.edu/#abs/2018AJ....155...81S Testing a double AGN hypothesis for Mrk 273 \|Iwasawa K. U V. et al. \| A&A \| 611-71 \| 2018 \| 2018A&A...611A..71I \| http://ui.adsabs.harvard.edu/#abs/2018A&A...611A..71I 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 Kinetic Energy Transfer from X-Ray Ultrafast Outflows to Millimeter/Submillimeter Cold Molecular Outflows in Seyfert Galaxies \|Mizumoto Misaki Izumi Takuma \| ApJ \| 871-156 \| 2019 \| 2019ApJ...871..156M \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...871..156M The Variable and Non-variable X-Ray Absorbers in Compton-thin Type II Active Galactic Nuclei \|Laha Sibasish Markowitz Alex G. et al. \| ApJ \| 897-66 \| 2020 \| 2020ApJ...897...66L \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...897...66L 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 properties of the AGN torus as revealed from a set of unbiased NuSTAR observations \|Zhao X. Marchesi S. et al. \| A&A \| 650-57 \| 2021 \| 2021A&A...650A..57Z \| http://ui.adsabs.harvard.edu/#abs/2021A&A...650A..57Z Fundamental X-ray corona parameters of Swift/BAT AGN \|Hinkle Jason T. Mushotzky Richard \| MNRAS \| 506-4960 \| 2021 \| 2021MNRAS.506.4960H \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.506.4960H 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 Coronal properties of low-accreting AGNs using Swift XMM-Newton and NuSTAR observations \|Jana Arghajit Chatterjee Arka et al. \| MNRAS \| 524-4670 \| 2023 \| 2023MNRAS.524.4670J \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.524.4670J Exploring X-Ray Properties of Low-metallicity Dwarf Galaxies \|Cann Jenna M. Weaver Kimberly A. et al. \| ApJ \| 961-178 \| 2024 \| 2024ApJ...961..178C \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...961..178C 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	2013-08-13T13:20:46Z/2013-11-04T22:17:09Z
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	2014-11-27T00:00:00Z
Last Update	2025-01-27
Keywords	"composite objects", "galaxy evolution", "xmm data", "absorbed agns", "EPIC", "xmm coverage", "nustar targets", "blackhole growth", "cosmological significance", "nustar program", "agn luminosities", "NuSTAR", "epic data", "column densities", "XMM", "local ulirg", "xray weak"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Stacy Teng, 2014, 'XMM and NuSTAR Observations of Local ULIRGs', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-hocbx95