There are several likely pulsars in EGRET error boxes which have been detectedin X-rays and are probably associated with known TeV sources. Here we proposeXMM-Newton studies of three of them: GeV J1825-1310 (the Eel), the Rabbit, andGeV J1907+0557, with the primary goal of detecting pulsations using the PN insmall window mode. They are also within X-ray pulsar wind nebulae, and the MOSimagers will be useful in studying the large scale structure of the nebulae.
Characterizing X-Ray Properties of the Gamma-Ray Pulsar PSR J1418-6058 in the Rabbit Pulsar Wind Nebula |Kim, Minjun, An, Hongjun, | ApJ | 892-5 | 2020 | 2020ApJ...892....5K | http://ui.adsabs.harvard.edu/#abs/2020ApJ...892....5K
The INTEGRAL view of the pulsating hard X-ray sky: from accreting and transitional millisecond pulsars to rotation-powered pulsars and magnetars |Papitto, A., Falanga, M., et al. | NewAR | 91-101544 | 2020 | 2020NewAR..9101544P | http://ui.adsabs.harvard.edu/#abs/2020NewAR..9101544P
A Broadband X-Ray Study of the Rabbit Pulsar Wind Nebula Powered by PSR J1418-6058 |Park, Jaegeun, Kim, Chanho, et al. | ApJ | 945-66 | 2023 | 2023ApJ...945...66P | http://ui.adsabs.harvard.edu/#abs/2023ApJ...945...66P
Robust constraints on feebly interacting particles using XMM-Newton |Luque, Pedro De la Torre, Balaji, Shyam, | PhRvD | 109-L101305 | 2024 | 2024PhRvD.109j1305L | http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L
Multimessenger search for electrophilic feebly interacting particles from supernovae |Luque, Pedro De la Torre, Balaji, Shyam, | PhRvD | 109-103028 | 2024 | 2024PhRvD.109j3028L | http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L
Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints |De la Torre Luque, Pedro, Balaji, Shyam, | ApJ | 968-46 | 2024 | 2024ApJ...968...46D | http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D
Instrument
EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage
2009-02-21T14:13:00Z/2009-02-23T03:39:40Z
Version
PPS_NOT_AVAILABLE
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.
European Space Agency, Dr Mallory Roberts, 2010, 'Pulse Searches of Probable GeV Pulsars Associated with TeV Sources', PPS_NOT_AVAILABLE, European Space Agency, https://doi.org/10.5270/esa-n7vyfuo
