A dataset provided by the European Space Agency

Name: X-Raying Hot DOGS
Published: 2017-01-20T23:00:00Z

Proposal ID	076102
Title	X-Raying Hot DOGS
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0761020101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0761020201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0761020301
DOI	https://doi.org/10.5270/esa-9bscyaf
Principal Investigator, PI	Dr Enrico Piconcelli
Abstract	Hot dust-obscured galaxies (Hot DOGs) are a very rare population of high-z hyperluminous (virgul10e14 Lsun) sources recently discovered in the WISE all-sky survey.Our exploratory AO12 observation provided the first X-ray spectrum of a Hot DOGand revealed a buried and intrinsically luminous QSO nucleus. We propose tocontinue this program aimed at probing the X-ray properties of these exceptionalAGN by observing three additional targets at zvirgul2.5. Given their spectacularluminosities and redshifts they may represent a rapid, dust-enshrouded phaseleading to the formation of the most massive elliptical galaxies. The proposedobservations are designed to get insight into the properties of the nuclearregion and the X-ray emitting source, responsible of their huge luminosity.
Publications	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 A new multiwavelength census of blazars \|Paggi, A., Bonato, M., et al. \| A&A \| 641-62 \| 2020 \| 2020A&A...641A..62P \| http://ui.adsabs.harvard.edu/#abs/2020A&A...641A..62P 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 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	2015-04-15T08:32:43Z/2016-01-05T00:40:06Z
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	"program aimed", "xray properties", "10e14 lsun sources", "z hyper luminous", "massive elliptical galaxy", "xray spectrum", "nuclear region", "rare population", "exploratory ao12", "additional targets", "hot dog", "spectacular luminosities", "xray emitting source", "luminous qso nucleus", "huge luminosity", "sky survey"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Enrico Piconcelli, 2017, 'X-Raying Hot DOGS', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-9bscyaf