We propose a survey of unclassified INTEGRAL sources from the latestINTEGRAL/IBIS catalog. Using several parameter cuts, we have identified asub-sample that must be dominated by Galactic sources such as accretingbinaries, CVs, young pulsars and their nebulae, and magnetars. We aim toidentify their X-ray counterparts, localize their positions (to1..-2..precision), measure X-ray properties, and determine the nature of thesources through multiwavelength classification. This will increase thepopulation of classified Galactic sources detected in both hard and soft X-rays.The prudent snap-shot survey approach, supplemented with the multiwavelengthclassification, will shed light on population of Galactic
Publications
Multiwavelength observations of the Galactic X-ray binaries IGR J20155+3827 and Swift J1713.4-4219 |Onori, F., Fiocchi, M., et al. | MNRAS | 503-472 | 2021 | 2021MNRAS.503..472O | http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503..472O
The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII, O VIII, and Fe L-shell Transitions |Pan, Zeyang, Qu, Zhijie, et al. | ApJS | 271-62 | 2024 | 2024ApJS..271...62P | http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P
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
2017-05-01T09:06:05Z/2018-03-22T15:29:53Z
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.
European Space Agency, Prof Oleg Kargaltsev, 2019, 'Snap-shot survey of INTEGRAL sources in the Galactic plane', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-0wri8z8
