Zobrazeno 1 - 10
of 45
pro vyhledávání: '"J N Reeves"'
Autor:
J. N. Reeves, V. Braito, A. Luminari, D. Porquet, M. Laurenti, G. Matzeu, A. Lobban, S. Hagen
Publikováno v:
The Astrophysical Journal, Vol 974, Iss 1, p 58 (2024)
PG 1448+273 is a luminous, nearby ( z = 0.0645), narrow-line Seyfert 1 galaxy, which likely accretes close to the Eddington limit. Previous X-ray observations of PG 1448+273 with XMM-Newton in 2017 and NuSTAR in 2022 revealed the presence of an ultra
Externí odkaz:
https://doaj.org/article/7995d10d59e34018b3b354c71ba64668
Publikováno v:
The Astrophysical Journal, Vol 952, Iss 1, p 52 (2023)
PG 1448+273 is a luminous, nearby ( z = 0.0645), narrow-line Seyfert 1 galaxy, which likely accretes close to the Eddington limit. XMM-Newton observations of PG 1448+273 in 2017 revealed the presence of an ultrafast outflow, as seen through its blues
Externí odkaz:
https://doaj.org/article/d7217375c5a44689a36d078bec82ac7e
Autor:
G A Matzeu, M Lieu, M T Costa, J N Reeves, V Braito, M Dadina, E Nardini, P G Boorman, M L Parker, S A Sim, D Barret, E Kammoun, R Middei, M Giustini, M Brusa, J Pérez Cabrera, S Marchesi
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2022, 515, pp.6172-6190. ⟨10.1093/mnras/stac2155⟩
Monthly Notices of the Royal Astronomical Society, 2022, 515, pp.6172-6190. ⟨10.1093/mnras/stac2155⟩
We present a new X-Ray Accretion Disk-wind Emulator (\textsc{xrade}) based on the 2.5D Monte Carlo radiative transfer code which provides a physically-motivated, self-consistent treatment of both absorption and emission from a disk-wind by computing
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4f069c8bcd01da113e3649eb3994c20a
http://arxiv.org/abs/2207.13731
http://arxiv.org/abs/2207.13731
Autor:
A. M. Joyce, Michael Parker, J. N. Reeves, Z. Igo, W. N. Alston, L. Härer, G. A. Matzeu, Andrew Lobban, Felix Fürst
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 500:4506-4513
We present an improved model for excess variance spectra describing ultrafast outflows and successfully apply it to the luminous ($L_{\rm bol}\sim 10^{47}\mathrm{erg}\, \mathrm{s}^{-1}$) low-redshift (z = 0.184) quasar Pico del Dias Survey (PDS) 456.
Autor:
V. Braito, J. N. Reeves, G. Matzeu, P. Severgnini, L. Ballo, C. Cicone, R. Della Ceca, M. Giustini, M. Sirressi
Past X-ray observations of the nearby Seyfert 2 MCG-03-58-007 revealed the presence of a powerful and highly variable disk wind, where two possible phases outflowing with $v_{\rm out1}/c\sim -0.07$ and $v_{\rm out2}/c\sim -0.2$ were observed. Multi-e
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f9ff814d4fbf66ac5297130690af8471
http://arxiv.org/abs/2111.04559
http://arxiv.org/abs/2111.04559
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2021, 654, pp.A89. ⟨10.1051/0004-6361/202141577⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 654, pp.A89. ⟨10.1051/0004-6361/202141577⟩
Astronomy and Astrophysics-A&A, 2021, 654, pp.A89. ⟨10.1051/0004-6361/202141577⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 654, pp.A89. ⟨10.1051/0004-6361/202141577⟩
(Abridged) Soft and hard X-ray excesses, compared to the continuum power-law shape between ~2-10 keV, are common features observed in the spectra of active galactic nuclei (AGN) and are associated with the accretion disc-corona system around the supe
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ae8ee4ddad7f13ec4dd23ed635b839c5
https://hal.science/hal-03386492v2/file/aa41577-21.pdf
https://hal.science/hal-03386492v2/file/aa41577-21.pdf
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2021, 649, pp.L3. ⟨10.1051/0004-6361/202140953⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 649, pp.L3. ⟨10.1051/0004-6361/202140953⟩
Astronomy and Astrophysics-A&A, 2021, 649, pp.L3. ⟨10.1051/0004-6361/202140953⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 649, pp.L3. ⟨10.1051/0004-6361/202140953⟩
Six XMM-Newton observations of the bright narrow line Seyfert 1, Mrk 110, from 2004-2020, are presented. The analysis of the grating spectra from the Reflection Grating Spectrometer (RGS) reveals a broad component of the He-like Oxygen (OVII) line, w
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::38a4d145cbc6633674e6cb24f0330287
http://hdl.handle.net/20.500.12386/32283
http://hdl.handle.net/20.500.12386/32283
Autor:
Sylvain Veilleux, S. Laha, J. N. Reeves, Randall K. Smith, Matteo Guainazzi, Gerard A. Kriss, Christopher S. Reynolds, Daniel Proga
Publikováno v:
Nature Astronomy
Outflows from active galactic nuclei (AGN) are one of the fundamental mechanisms by which the central supermassive black hole interacts with its host galaxy. Detected in $\ge 50\%$ of nearby AGN, these outflows have been found to carry kinetic energy
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::122a04ab9ac56e73aabc5316c65771a9
http://arxiv.org/abs/2012.06945
http://arxiv.org/abs/2012.06945
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2020, 500 (2), pp.1974-1991. ⟨10.1093/mnras/staa3377⟩
Monthly Notices of the Royal Astronomical Society, 2020, 500 (2), pp.1974-1991. ⟨10.1093/mnras/staa3377⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2020, 500 (2), pp.1974-1991. ⟨10.1093/mnras/staa3377⟩
Monthly Notices of the Royal Astronomical Society, 2020, 500 (2), pp.1974-1991. ⟨10.1093/mnras/staa3377⟩
New Swift monitoring observations of the variable, radio-quiet quasar, PDS 456, are presented. A bright X-ray flare was captured in September 2018, the flux increasing by a factor of 4 and with a doubling time-scale of 2 days. From the light crossing
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::915654a5948be825b751814e64003291
http://arxiv.org/abs/2010.14295
http://arxiv.org/abs/2010.14295
A joint XMM-Newton and NuSTAR observation was conducted for the bright, local Seyfert 1.9 galaxy, NGC 1194. The hard spectral form of this AGN was modeled using the toroidal reprocessor MYTORUS. The decoupled model form provides a good description of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6465faad0f5f519e65f7315730321923
http://arxiv.org/abs/2007.04366
http://arxiv.org/abs/2007.04366