A dataset provided by the European Space Agency

Name: Chasing the Most Powerful Blazars
Published: 2018-08-11T22:00:00Z

Proposal ID	080200
Title	Chasing the Most Powerful Blazars
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0802000101
DOI	https://doi.org/10.5270/esa-3zrr6tl
Principal Investigator, PI	Dr Vaidehi Paliya
Abstract	We request a 20 ksec XMM-Newton observation of a gamma-ray luminous quasar, NVSSJ163547+362930 (z = 3.62). It is one of the five blazars detected by Fermi-LATbeyond z = 3.1 and not present in earlier gamma-ray catalogs. However, thissource has no previous X-ray spectral measurements. The X-ray observations willmeasure the onset of the inverse Compton emission which is expected to be veryhard. This will enables us to accurately determine the associated jet power andthe particle population responsible for the observed emission.
Publications	Blazars at the Cosmic Dawn \|Paliya, Vaidehi S., Ajello, M., et al. \| ApJ \| 897-177 \| 2020 \| 2020ApJ...897..177P \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...897..177P 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 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 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	2017-07-23T10:27:12Z/2017-07-23T16:50:32Z
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	2018-08-11T22:00:00Z
Keywords	"jet power", "fermi lat", "powerful blazar", "inverse compton emission", "XMM", "xray spectral measurements", "nvss j163547", "362930 z", "gamma ray catalogs", "XMM-Newton", "particle population", "xmm newton"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Vaidehi Paliya, 2018, 'Chasing the Most Powerful Blazars', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-3zrr6tl