A dataset provided by the European Space Agency

Name: ToO Observations of New Galactic Gamma-ray Transients Discovered with Fermi
Published: 2011-02-23T00:00:00Z

Proposal ID	065241
Title	ToO Observations of New Galactic Gamma-ray Transients Discovered with Fermi
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0652410201
DOI	https://doi.org/10.5270/esa-lnx82o4
Principal Investigator, PI	Dr Dirk Pandel
Abstract	During the first year of operation, the Fermi gamma-ray observatory has detectedtwo new transient GeV sources in the Galactic plane. The nature of theseGalactic gamma-ray transients is currently not known. We propose XMM-Newton ToOobservations of new transients discovered with the Fermi LAT in the Galacticplane. The XMM-Newton observations will enable us to more accurately localizethe transients, identify counterparts at other wavelengths, determine theirX-ray to gamma-ray flux ratio, measure their X-ray spectrum, and characterizetheir variability and decay time scale. This proposal is part of amultiwavelength program that includes observations at radio and TeV energies.
Publications	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 Peak of spectral energy distribution plays an important role in intra-day variability of blazars? \|Gupta, Alok C., Kalita, Nibedita, et al. \| MNRAS \| 462-1508 \| 2016 \| 2016MNRAS.462.1508G \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.462.1508G 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 Signature of inverse Compton emission from blazars \|Gaur, Haritma, Mohan, Prashanth, et al. \| MNRAS \| 473-3638 \| 2018 \| 2018MNRAS.473.3638G \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.473.3638G 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 Study of Intra-Day Flux Distributions of Blazars Using XMM-Newton Satellite \|Wani, Kiran, Gaur, Haritma, \| Univ \| 8-578 \| 2022 \| 2022Univ....8..578W \| http://ui.adsabs.harvard.edu/#abs/2022Univ....8..578W 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	2010-02-09T21:47:25Z/2010-02-10T01:39:21Z
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	2011-02-23T00:00:00Z
Keywords	"multiwavelength program", "fermi lat", "decay time scale", "XMM", "xray spectrum", "transient gev sources", "galactic plane", "tev energies", "XMM-Newton", "xmm newton"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Dirk Pandel, 2011, 'ToO Observations of New Galactic Gamma-ray Transients Discovered with Fermi', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-lnx82o4