A dataset provided by the European Space Agency

Name 011243
Title EPIC Observations of the X-ray and Radio Source LS I +61d303 - GT 0236+610
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112430101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112430102
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112430103
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112430201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112430301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112430401

DOI https://doi.org/10.5270/esa-x0svyad
Author Dr Martin Turner
Description GT- GT0236+610 is an X-ray-radio- (and possibly gamma-ray) source with unique properties, associated to the Be star LSI+61 303 and characterized by strong non thermal outbursts occurring with a periodicity of 26.5 days. The proposed observation with 4 snapshots at different orbital phases will allow to discriminate between the two alternative models of shock emission and supercritical accretion. NOTE FOR THE PLANNING: 4 pointings of 5 ksec each are required, in order to cover different phases of the 26.5 day orbit. The choice in the time constraints form (repeat every 3 orbits) is just a possibility: such a tight constraint on the spacing is not required, as far as different phases are sampled.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2002-02-05T01:44:18Z/2002-09-16T04:11:28Z
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 2003-10-10T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2003-10-10T00:00:00Z, 011243, 17.56_20190403_1200. https://doi.org/10.5270/esa-x0svyad