A dataset provided by the European Space Agency

Name: Ultralong GRBs: a nearby laboratory for PopIII openPar-likeclosePar star explosions
Published: 2018-08-02T22:00:00Z

Proposal ID	076345
Title	Ultralong GRBs: a nearby laboratory for PopIII (-like) star explosions
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0763450301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0763450401
DOI	https://doi.org/10.5270/esa-vafgfdz
Principal Investigator, PI	Dr Luigi Piro
Abstract	Swift observations of gamma-ray bursts recently highlighted the existence ofrare high-energy transients, characterized by extremely long durations (fromhours to days). The origin of these enigmatic events, dubbed ultralong GRBs,remains uncertain with the prime model being the collapse of a low-metallicityBlue Supergiant star. In this scenario ultralong GRBs could represent the localanalogues of pop III GRBs, thus providing a nearby laboratory to investigateprimordial star explosions. Here we propose a ToO program to observe a newlydiscovered ultralong GRB. The requested X-ray observations will be complementedby an extensive follow-up campaign through our on-going radio, optical, and IRprograms.
Publications	Classification of 4XMM-DR9 sources by machine learning \|Zhang, Yanxia, Zhao, Yongheng, \| MNRAS \| 503-5263 \| 2021 \| 2021MNRAS.503.5263Z \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z X\\u2011HESS: A large sample of highly accreting serendipitous AGN under the XMM\\u2011Newton microscope \|Laurenti, M., Tombesi, F., et al. \| AN \| 344-20230053 \| 2023 \| 2023AN....34430053L \| http://ui.adsabs.harvard.edu/#abs/2023AN....34430053L From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources \|Rodriguez, Antonio C., \| PASP \| 136-054201 \| 2024 \| 2024PASP..136e4201R \| http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R 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	2017-07-18T17:44:27Z/2017-07-20T09:03:45Z
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.
Creator Contact	https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published	2018-08-02T22:00:00Z
Keywords	"primordial star explosions", "nearby laboratory", "ultralong grbs", "local analogues", "ultralong grb", "gamma ray bursts", "dubbed ultralong grbs", "prime model", "enigmatic events", "requested xray", "star explosions", "energy transients", "ir programs", "scenario ultralong grbs", "pop iii grbs"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Luigi Piro, 2018, 'Ultralong GRBs: a nearby laboratory for PopIII openPar-likeclosePar star explosions', PPS_NOT_AVAILABLE, European Space Agency, https://doi.org/10.5270/esa-vafgfdz