A dataset provided by the European Space Agency

Proposal ID 082415
Title Neutron stars multi-lambda fast variability: probing disk-jet connection
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DOI https://doi.org/10.5270/esa-ycyn624
Principal Investigator, PI Mr Federico Vincentelli
Abstract Fast optical-infrared photometry applied to black hole X-ray binaries has nowrevealed its great potential and has shown to be one of the best ways to probethe jet in its inner most regions. Nonetheless Neutron Star X-ray binaries,which are clearly dominated by the jet at IR wavelength, have not been studiedyet with such approach. Here we propose to observe the Neutron Star Low MassX-ray binary 4U 1728-34 simultaneously with XMM-Newton and HAWK-I@VLT. We ask toperform 6 (7 ks apiece) pointings to be matched by 6 (1 h apiece) HAWK-I@VLTobservations. These data will allow us to study the disc-jet interaction indifferent accretion regimes and to search for, and investigate the between jetproperties in black holes and neutron stars X-ray binaries.
Publications
Instrument EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2018-09-01T22:53:49Z/2018-10-07T01:56:03Z
Version 19.17_20220121_1250
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 2019-11-05T23:00:00Z
Last Update 2025-08-04
Keywords "XMM", "jet properties", "XMM-Newton", "apiece hawk", "apiece pointings", "disc jet interaction", "xmm newton", "accretion regimes", "ir wavelength", "blackhole xray binary"
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Mr Federico Vincentelli, 2019, 'Neutron stars multi-lambda fast variability: probing disk-jet connection', 19.17_20220121_1250, European Space Agency, https://doi.org/10.5270/esa-ycyn624