| Proposal ID | 050598 |
| Title | XMM-Newton and MAGIC simultaneous observations of the gamma-ray binary LSI+61303 |
| Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0505980801 |
| DOI | https://doi.org/10.5270/esa-y5696js |
| Principal Investigator, PI | Prof Josep Maria Paredes |
| Abstract | LS I +61 303 is a high mass X-ray binary that has been recently detected as avariable TeV source by MAGIC. We propose to conduct, for the first time,simultaneous X-ray and TeV observations, complemented with a radio monitoring,during several consecutive days centered around the orbital phase where themaximum TeV activity takes place. These observations will allow us to followinter-day spectral variability at X-ray and TeV energies. They will provide abetter sampled evolution of the X-ray flux and photon index around the phaseswhere X-ray outbursts are detected. They will also allow to verify the higherflux - harder spectrum correlation and the apparent non-existence of spectrallines. All this will be crucial to constrain physical properties of the emitter. |
| Publications |
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| Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
| Temporal Coverage | 2007-09-04T01:48:30Z/2007-09-11T05:29:20Z |
| 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 | 2008-11-14T00:00:00Z |
| Last Update | 2025-01-27 |
| Keywords | "orbital phase", "mass xray binary", "xmm newton", "tev energies", "constrain physical properties", "XMM-Newton", "spectral variability", "sampled evolution", "xray flux", "photon index", "xray outburst", "XMM", "variable tev source", "spectral lines" |
| Publisher And Registrant | European Space Agency |
| Credit Guidelines | European Space Agency, Prof Josep Maria Paredes, 2008, 'XMM-Newton and MAGIC simultaneous observations of the gamma-ray binary LSI+61303', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-y5696js |