A dataset provided by the European Space Agency

Name 081121
Title Generic ToO-DDT Proposal for AO16


DOI 10.5270/esa-2vl4012
Description 1) GW170817 27) GW170817 28) Swift J0243.6+6124 29) Swift J0243.6+6124 30) C2016 R2 PANSTARRS 31) C2016 R2 PANSTARRS 32) C2016 R2 PANSTARRS 33) Fermi J1544-0649 34) Swift J1658.2-4242 35) PSR J1946+2052
Publication The Binary Neutron Star Event LIGO-Virgo GW170817 160 Days after Merger: Synchrotron Emission across the Electromagnetic Spectrum . Margutti, R., Alexander, K. D., et all. . ApJ . 856-18 . 2018 . 2018ApJ...856L..18M ,
The evolution of the X-ray afterglow emission of GW 170817- GRB 170817A in XMM-Newton observations . D.Avanzo, P., Campana, S., et all. . A&A . 613-1 . 2018 . 2018A&A...613L...1D ,
An XMM-Newton look at the strongly variable radio-weak BL Lac Fermi J1544-0639 . Ursini, F., Bassani, L., et all. . A&A . 622-116 . 2019 . 2019A&A...622A.116U ,
A long-lived neutron star merger remnant in GW170817: constraints and clues from X-ray observations . Piro, L., Troja, E., et all. . MNRAS . 483-1912 . 2019 . 2019MNRAS.483.1912P ,
Exploring the Interstellar Medium Using an Asymmetric X-Ray Dust Scattering Halo . Jin, Chichuan, Ponti, Gabriele, et all. . ApJ . 875-157 . 2019 . 2019ApJ...875..157J ,
Two Years of Nonthermal Emission from the Binary Neutron Star Merger GW170817: Rapid Fading of the Jet Afterglow and First Constraints on the Kilonova Fastest Ejecta . Hajela, A., Margutti, R., et all. . ApJ . 886-17 . 2019 . 2019ApJ...886L..17H ,
Properties of jet and surrounding material of GW-GRB 170817A . Ziaeepour, Houri, . MNRAS . 490-2822 . 2019 . 2019MNRAS.490.2822Z ,
A year in the life of GW 170817: the rise and fall of a structured jet from a binary neutron st...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2017-12-29T18:19:47Z/2018-03-29T15:23:01Z
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 2019-05-03T22:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2019-05-03T22:00:00Z, 081121, 17.56_20190403_1200. https://doi.org/10.5270/esa-2vl4012