A dataset provided by the European Space Agency

Name: Spectral and temporal evolution of 1ES 1959+650 using MAGIC and XMM
Published: 2020-08-12T22:00:00Z

Proposal ID	085098
Title	Spectral and temporal evolution of 1ES 1959+650 using MAGIC and XMM
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0850980101
DOI	https://doi.org/10.5270/esa-gcxhgxu
Principal Investigator, PI	Dr Daniela Dorner
Abstract	After a low state since 2002, bright outbursts in 2016 were surrounded byintermediate activity (2015-2018). Past observations have revealed a peak-shifttowards higher energies hinting an EHBL-like nature, fast intranight andlongterm variability as well as complex correlation patterns between wavebands.These features challenge a simple one-zone synchrotron self-Compton model. Werequest MAGIC observations coordinated with simultaneous multi- wavelengthobservations spanning a wide energy range, to understand the evolution of thebroadband spectrum, compare different flux states, characterize variabilitypatterns, study inter-band correlations and investigate the potential of thesource as astrophysical neutrino emitter.
Publications	An XMM-Newton catalogue of BL Lacs \|de la Calle P\\u00e9rez, I., \\u00c1lvarez Crespo, N., et al. \| A&A \| 655-48 \| 2021 \| 2021A&A...655A..48D \| http://ui.adsabs.harvard.edu/#abs/2021A&A...655A..48D Study of X-Ray Intraday Variability of HBL Blazars Based on Observations Obtained with XMM-Newton \|Devanand, P. U., Gupta, Alok C., et al. \| ApJ \| 939-80 \| 2022 \| 2022ApJ...939...80D \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...939...80D X-Ray Studies of Blazar 1ES 1959+650 Using Swift and XMM-Newton Satellite \|Wani, Kiran, Gaur, Haritma, \| ApJ \| 951-94 \| 2023 \| 2023ApJ...951...94W \| http://ui.adsabs.harvard.edu/#abs/2023ApJ...951...94W
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2019-07-05T20:21:39Z/2019-07-06T08:34:59Z
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	2020-08-12T22:00:00Z
Keywords	"energies hinting", "wide energy range", "temporal evolution", "XMM", "multi wavelength", "bright outburst", "variability patterns", "inter band correlations", "broadband spectrum", "complex correlation patterns", "longterm variability", "peak shift towards", "astrophysical neutrino emitter", "1es 1959", "fast intranight"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Daniela Dorner, 2020, 'Spectral and temporal evolution of 1ES 1959+650 using MAGIC and XMM', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-gcxhgxu