V. Braito
INAF
26 Papers
171 Citations
V. Braito is an academic researcher from INAF. The author has contributed to research in topics: Galaxy & Quasar. The author has an hindex of 14, co-authored 26 publications. Previous affiliations of V. Braito include University of Maryland, Baltimore County.
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Papers
Short term X-ray spectral variability of the quasar PDS 456 observed in a low flux state
G. Matzeu,James Reeves,James Reeves,Emanuele Nardini,V. Braito,V. Braito,M. Costa,Francesco Tombesi,Francesco Tombesi,J. Gofford +9 more
TL;DR: In this paper, the spectral energy distribution of the soft X-ray spectrum of the nearby luminous quasar PDS 456 has been investigated using optical/UV photometry and hard Xray spectra from the later XMM-Newton/NuSTAR campaign.
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Resolving the Soft X-Ray Ultrafast Outflow in PDS 456
James Reeves,James Reeves,V. Braito,V. Braito,George Chartas,Fred Hamann,S. Laha,S. Laha,E. Nardini,E. Nardini +9 more
TL;DR: In this paper, the authors acknowledge support from grant 80NSSC20K0793.0 and partial support from the EU Horizon 2020 Marie Sklodowska-Curie grant agreement no.2017-14-H.
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A new relativistic component of the accretion disk wind in PDS 456
TL;DR: In this paper, the relativistic component of the wind through hard X-ray observations with NuSTAR and XMM-Newton, obtained in March 2017 when the quasar was in a low flux state, was revealed in the iron K band.
A New Relativistic Component of the Accretion Disk Wind in PDS 456
TL;DR: In this article, the relativistic component of the wind through hard X-ray observations with NuSTAR and XMM-Newton, obtained in 2017 March when the quasar was in a low-flux state, was revealed.
Discovery of broad soft x-ray absorption lines from the quasar wind in pds 456
James Reeves,James Reeves,V. Braito,V. Braito,Emanuele Nardini,Ehud Behar,Ehud Behar,P. T. O'Brien,Francesco Tombesi,Francesco Tombesi,Tracey Jane Turner,M. Costa +11 more
TL;DR: In this paper, a high-resolution soft X-ray spectroscopy of the prototype accretion disk wind quasar, PDS 456, is presented, where broad absorption line (BAL) profiles are revealed in the XMM-Newton reflection grating spectrometer spectra.
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