| Name | 020355 |
| Title | FLUX VARIABILITY IN (ANOMALOUS) X-RAY PULSARS |
| URL | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0203550201 |
| DOI | https://doi.org/10.5270/esa-sncllbc |
| Author | European Space Agency |
| Description | We propose to observe the anomalous X-ray pulsars (AXPs) 1E 1048.1-5937, 1E 2259+586 and 1RXS J1708-4009 five times each using EPIC over the course of AO3. Our goal is to measure the pulsed fluxes and spectral parameters at multiple epochs with a single imaging instrument, in order to settle, once and for all, the controversial issue of whether AXPS are flux-variable sources. Determining if there is flux variability in AXPs, and whether it is correlated with spectral parameters, pulsed fraction, spin-down rate, and/or bursting activity is central to physically understanding this exotic class of neutron stars, and to constraining the magnetar model. |
| Publication | No observations found associated with the current proposal |
| Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
| Temporal Coverage | 2004-02-11T16:27:34Z/2005-07-29T00:42:42Z |
| 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 | 2006-08-20T00:00:00Z |
| Publisher And Registrant | European Space Agency |
| Credit Guidelines | European Space Agency, 2006, Flux Variability In Openparanomalousclosepar X-Ray Pulsars, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-sncllbc |