A dataset provided by the European Space Agency

Name: The first X-ray view of Ton 28
Published: 2018-08-07T22:00:00Z

Proposal ID	080456
Title	The first X-ray view of Ton 28
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0804560101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0804560201
DOI	https://doi.org/10.5270/esa-jnjcj8f
Principal Investigator, PI	Dr Elisabeta Lusso
Abstract	Ton 28 is a very luminous (Lbol=3e46 erg/s), low redshift (z=0.329), radio-quietquasar, widely studied in the literature for its peculiar optical spectralproperties. Ton 28 exhibits strong, blueshifted absorption and emissionfeatures, interpreted with the release of a large-scale outflowing material.Although Ton 28 has a clear ROSAT detection, it has been completely overlookedfrom X-ray observatories. Our main aim is to obtain a high quality spectrum ofTon 28, as it is one of the brightest AGN that still lacks an X-ray observation.Since the launch of a powerful wind is only seen in highly bright objects, Ton28 also represents the most promising target to possess an ultra fast outflow.
Publications	Towards an informed quest for accretion disc winds in quasars: the intriguing case of Ton 28 \|Nardini, E., Lusso, E., \| MNRAS \| 482-134 \| 2019 \| 2019MNRAS.482L.134N \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.482L.134N On the Observational Difference between the Accretion Disk-Corona Connections among Super- and Sub-Eddington Accreting Active Galactic Nuclei \|Liu, Hezhen, Luo, B., et al. \| ApJ \| 910-103 \| 2021 \| 2021ApJ...910..103L \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...910..103L 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 A Systematic Study of the Short-term X-Ray Variability of Seyfert Galaxies. I. Diversity of the X-Ray rms Spectra \|Hu, Jingwei, Jin, Chichuan, et al. \| ApJ \| 936-105 \| 2022 \| 2022ApJ...936..105H \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...936..105H 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 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	2017-05-14T05:24:33Z/2017-05-16T12:11:20Z
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	2018-08-07T22:00:00Z
Keywords	"ultra fast outflow", "blueshifted absorption", "promising target", "quality spectrum", "scale outflowing material", "rosat detection", "luminous lbol", "bright objects", "xray observatories", "optical spectral properties", "brightest agn", "3e46 erg", "radio quiet quasar", "ROSAT", "powerful wind", "low redshift z", "completely overlooked"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Elisabeta Lusso, 2018, 'The first X-ray view of Ton 28', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-jnjcj8f