A dataset provided by the European Space Agency

Name 065241
Title ToO Observations of New Galactic Gamma-ray Transients Discovered with Fermi
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0652410201

DOI 10.5270/esa-lnx82o4
Author Dr Dirk Pandel
Description During the first year of operation, the Fermi gamma-ray observatory has detected two new transient GeV sources in the Galactic plane. The nature of these Galactic gamma-ray transients is currently not known. We propose XMM-Newton ToO observations of new transients discovered with the Fermi LAT in the Galactic plane. The XMM-Newton observations will enable us to more accurately localize the transients, identify counterparts at other wavelengths, determine their X-ray to gamma-ray flux ratio, measure their X-ray spectrum, and characterize their variability and decay time scale. This proposal is part of a multiwavelength program that includes observations at radio and TeV energies.
Publication 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 ,
Peak of spectral energy distribution plays an important role in intra-day variability of blazars? . Gupta, Alok C., Kalita, Nibedita, et all. . MNRAS . 462-1508 . 2016 . 2016MNRAS.462.1508G ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
Signature of inverse Compton emission from blazars . Gaur, Haritma, Mohan, Prashanth, et all. . MNRAS . 473-3638 . 2018 . 2018MNRAS.473.3638G ,
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 Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's 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 Earth's 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
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2011-02-23T00:00:00Z, 065241, 17.56_20190403_1200. https://doi.org/10.5270/esa-lnx82o4