A dataset provided by the European Space Agency

Name: Deep observations of NGC 4472:a special ULX comma point sources comma and diffuse emission
Published: 2017-01-20T23:00:00Z

Proposal ID	076163
Title	Deep observations of NGC 4472:a special ULX, point sources, and diffuse emission
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0761630101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0761630201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0761630301
DOI	https://doi.org/10.5270/esa-q0duo42
Principal Investigator, PI	Dr Thomas Maccarone
Abstract	We propose deep observations of the Virgo Cluster galaxy NGC 4472. Our primaryaim is to understand the variability of the likely ultracompact black hole X-raybinary in one of its globular clusters. Characterizing this object s variabilitywill place important constraints on whether beaming can explain the highluminosities of ULXs. Also, NGC 4472 is the brightest galaxy in the LocalUniverse, making it ideal for studies of compact binary populations, and as agiant galaxy falling into a large cluster, it presents rich opportunities forstudies of diffuse emission. The OM data will be used for searches for classicalnovae and U-band studies of the galaxy s globular clusters.
Publications	X-Ray Variability from the Ultraluminous Black Hole Candidate X-Ray Binary in the Globular Cluster RZ 2109 \|Dage, Kristen C., Zepf, Stephen E., et al. \| ApJ \| 862-108 \| 2018 \| 2018ApJ...862..108D \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...862..108D Extended X-Ray Study of M49: The Frontier of the Virgo Cluster \|Su, Y., Kraft, R. P., et al. \| AJ \| 158-6 \| 2019 \| 2019AJ....158....6S \| http://ui.adsabs.harvard.edu/#abs/2019AJ....158....6S Peculiar Outbursts of an Ultra-luminous Source: Likely Signs of an Aperiodic Disk-wind \|Stiele, H., Kong, A. K. H., \| ApJ \| 877-115 \| 2019 \| 2019ApJ...877..115S \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...877..115S Slow decline and rise of the broad O III emission line in globular cluster black hole candidate RZ2109 \|Dage, Kristen C., Zepf, Stephen E., et al. \| MNRAS \| 489-4783 \| 2019 \| 2019MNRAS.489.4783D \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.489.4783D The Metal Content of the Hot Atmospheres of Galaxy Groups \|Gastaldello, Fabio, Simionescu, Aurora, et al. \| Univ \| 7-208 \| 2021 \| 2021Univ....7..208G \| http://ui.adsabs.harvard.edu/#abs/2021Univ....7..208G 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 An XMM-Newton Early-type Galaxy Atlas \|Islam, Nazma, Kim, Dong-Woo, et al. \| ApJS \| 256-22 \| 2021 \| 2021ApJS..256...22I \| http://ui.adsabs.harvard.edu/#abs/2021ApJS..256...22I Recurrent X-ray flares of the black hole candidate in the globular cluster RZ 2109 in NGC 4472 \|Tiengo, A., Esposito, P., et al. \| A&A \| 661-68 \| 2022 \| 2022A&A...661A..68T \| http://ui.adsabs.harvard.edu/#abs/2022A&A...661A..68T Variability in a low-mass active galactic nucleus: oscillation or eruption? \|Webbe, Robbie, Young, A. J., \| MNRAS \| 518-3428 \| 2023 \| 2023MNRAS.518.3428W \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.518.3428W Dynamical Response of Solar Wind Charge Exchange Soft X-Ray Emission in Earth.s Magnetosphere to the Solar Wind Proton Flux \|Zhang, Yingjie, Sun, Tianran, et al. \| ApJ \| 948-69 \| 2023 \| 2023ApJ...948...69Z \| http://ui.adsabs.harvard.edu/#abs/2023ApJ...948...69Z Searching for quasi-periodic eruptions using machine learning \|Webbe, Robbie, Young, A. J., \| RASTI \| 2-238 \| 2023 \| 2023RASTI...2..238W \| http://ui.adsabs.harvard.edu/#abs/2023RASTI...2..238W An extreme ultra-compact X-ray binary in a globular cluster: multiwavelength observations of RZ 2109 explored in a triple system framework \|Dage, Kristen C., Bahramian, Arash, et al. \| MNRAS \| 529-1347 \| 2024 \| 2024MNRAS.529.1347D \| http://ui.adsabs.harvard.edu/#abs/2024MNRAS.529.1347D 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	2016-01-05T08:25:28Z/2016-01-10T16:38:16Z
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	2017-01-20T23:00:00Z
Keywords	"compact binary populations", "brightest galaxy", "special ulx", "local universe", "NGC 4472", "om data", "globular clusters", "classical novae", "giant galaxy", "ngc 4472", "diffuse emission"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Thomas Maccarone, 2017, 'Deep observations of NGC 4472:a special ULX comma point sources comma and diffuse emission', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-q0duo42