A dataset provided by the European Space Agency

Name: X-Raying Hot DOGS
Published: 2017-01-20T23:00:00Z
License: https://creativecommons.org/licenses/by-nc/3.0/igo

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 (~10e14 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 z~2.5. 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 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	2015-04-15T08:32:43Z/2016-01-05T00:40:06Z
Version	21.51_20241115_1113
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
Last Update	2026-07-09
Keywords	"exploratory ao12", "spectacular luminosities", "z hyper luminous", "rare population", "additional targets", "xray emitting source", "hot dog", "sky survey", "program aimed", "nuclear region", "huge luminosity", "massive elliptical galaxy", "xray spectrum", "xray properties", "10e14 lsun sources", "luminous qso nucleus"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Enrico Piconcelli, 2017, 'X-Raying Hot DOGS', 21.51_20241115_1113, European Space Agency, https://doi.org/10.5270/esa-9bscyaf
Rights	Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.