A dataset provided by the European Space Agency

Name: A unique TeV source in Monoceros
Published: 2008-10-26T00:00:00Z
License: https://creativecommons.org/licenses/by-nc/3.0/igo

Proposal ID	050520
Title	A unique TeV source in Monoceros
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0505200101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0505200201
DOI	https://doi.org/10.5270/esa-vhk8p9b
Principal Investigator, PI	Dr Jim Hinton
Abstract	A new source of very-high-energy (> 100 GeV) gamma-rays has recently beendiscovered in the interaction region between the Rosette Nebula and theMonoceros Loop SNR (confidential information). This source is unique in both itslocation (in spatial coincidence with a molecular cloud and the limb of an SNR)and its point-like nature. The gamma-ray source is coincident with a weak ROSATX-ray source, but the sensitivity of XMM-Newton is required to identify thenature of this unusual high-energy object.
Publications	The XMM Cluster Survey: optical analysis methodology and the first data release \|Mehrtens Nicola Romer A. Kathy et al. \| MNRAS \| 423-1024 \| 2012 \| 2012MNRAS.423.1024M \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.1024M HESS J0632+057: A New Gamma-Ray Binary? \|Hinton J. A. Skilton J. L. et al. \| ApJ \| 690-101 \| 2009 \| 2009ApJ...690L.101H \| http://ui.adsabs.harvard.edu/#abs/2009ApJ...690L.101H The TeV Binary HESS J0632+057 in the Low and High X-Ray State \|Rea Nanda Torres Diego F. \| ApJ \| 737-12 \| 2011 \| 2011ApJ...737L..12R \| http://ui.adsabs.harvard.edu/#abs/2011ApJ...737L..12R The XMM Cluster Survey: X-ray analysis methodology \|Lloyd-Davies E. J. Romer A. Kathy et al. \| MNRAS \| 418-14 \| 2011 \| 2011MNRAS.418...14L \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.418...14L Exospheric solar wind charge exchange as seen by XMM-Newton \|Carter J. A. Semba S. \| AN \| 333-313 \| 2012 \| 2012AN....333..313C \| http://ui.adsabs.harvard.edu/#abs/2012AN....333..313C An XMM-Newton Survey of the Soft X-Ray Background. II. An All-Sky Catalog of Diffuse O VII and O VIII Emission Intensities \|Henley David B. Shelton Robin L. \| ApJS \| 202-14 \| 2012 \| 2012ApJS..202...14H \| http://ui.adsabs.harvard.edu/#abs/2012ApJS..202...14H 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 A New TeV Binary: The Discovery of an Orbital Period in HESS J0632+057 \|Bongiorno S. D. Falcone A. D. et al. \| ApJ \| 737-11 \| 2011 \| 2011ApJ...737L..11B \| http://ui.adsabs.harvard.edu/#abs/2011ApJ...737L..11B Sunyaev-Zeldovich effect or not? Detecting the main foreground effect of most galaxy clusters \|Xiao Weike Chen Chen et al. \| MNRAS \| 432-41 \| 2013 \| 2013MNRAS.432L..41X \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.432L..41X The Interaction of the Fermi Bubbles with the Milky Ways Hot Gas Halo \|Miller Matthew J. Bregman Joel N. \| ApJ \| 829-9 \| 2016 \| 2016ApJ...829....9M \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...829....9M 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 Anisotropy of the galaxy cluster X-ray luminosity-temperature relation \|Migkas Konstantinos Reiprich Thomas H. \| A&A \| 611-50 \| 2018 \| 2018A&A...611A..50M \| http://ui.adsabs.harvard.edu/#abs/2018A&A...611A..50M The XMM Cluster Survey: Present status and latest results \|Viana P. T. P. Mehrtens N. et al. \| AN \| 334-462 \| 2013 \| 2013AN....334..462V \| http://ui.adsabs.harvard.edu/#abs/2013AN....334..462V Orbital solution leading to an acceptable interpretation for the enigmatic gamma-ray binary HESS J0632+057 \|Moritani Yuki Kawano Takafumi et al. \| PASJ \| 70-61 \| 2018 \| 2018PASJ...70...61M \| http://ui.adsabs.harvard.edu/#abs/2018PASJ...70...61M Testing emergent gravity on galaxy cluster scales \|Tamosiunas Andrius Bacon David et al. \| JCAP \| 5-53 \| 2019 \| 2019JCAP...05..053T \| http://ui.adsabs.harvard.edu/#abs/2019JCAP...05..053T Chandra Follow-up of the SDSS DR8 Redmapper Catalog Using the MATCha Pipeline \|Hollowood Devon L. Jeltema Tesla et al. \| ApJS \| 244-22 \| 2019 \| 2019ApJS..244...22H \| http://ui.adsabs.harvard.edu/#abs/2019ApJS..244...22H Decade-long X-ray observations of HESS J0632+057 \|Malyshev Denys Chernyakova Maria et al. \| AN \| 340-465 \| 2019 \| 2019AN....340..465M \| http://ui.adsabs.harvard.edu/#abs/2019AN....340..465M Stellar mass as a galaxy cluster mass proxy: application to the Dark Energy Survey redMaPPer clusters \|Palmese A. Annis J. et al. \| MNRAS \| 493-4591 \| 2020 \| 2020MNRAS.493.4591P \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.493.4591P An X-Ray- and SZ-bright Diffuse Source toward M31: A Local Hot Bridge \|Qu Zhijie Huang Rui et al. \| ApJ \| 907-14 \| 2021 \| 2021ApJ...907...14Q \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...907...14Q 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 Observation of the Gamma-Ray Binary HESS J0632+057 with the H.E.S.S. MAGIC and VERITAS Telescopes \|Adams C. B. Benbow W. et al. \| ApJ \| 923-241 \| 2021 \| 2021ApJ...923..241A \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...923..241A The Solar Cycle Temporal Variation of the Solar Wind Charge Exchange X-Ray Lines \|Qu Zhijie Koutroumpa Dimitra et al. \| ApJ \| 930-21 \| 2022 \| 2022ApJ...930...21Q \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...930...21Q 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 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	2007-09-17T00:21:54Z/2007-09-17T15:28:54Z
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	2008-10-26T00:00:00Z
Last Update	2026-06-19
Keywords	"spatial coincidence", "gev gamma rays", "rosette nebula", "XMM", "xmm newton", "molecular cloud", "energy object", "supernova remnant", "tev source", "XMM-Newton", "interaction region", "gamma ray source", "ROSAT"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Jim Hinton, 2008, 'A unique TeV source in Monoceros', 21.51_20241115_1113, European Space Agency, https://doi.org/10.5270/esa-vhk8p9b
Rights	Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.