Zobrazeno 1 - 10
of 39
pro vyhledávání: '"Gabriele Pezzulli"'
Autor:
Anqi Li, Filippo Fraternali, Antonino Marasco, Scott C Trager, Gabriele Pezzulli, Pavel E Mancera Piña, Marc A W Verheijen
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 520, 147-160. Oxford University Press
We use a dynamical model of galactic fountain to study the neutral extraplanar gas (EPG) in the nearby spiral galaxy NGC 2403. We have modelled the EPG as a combination of material ejected from the disc by stellar feedback (i.e. galactic fountain) an
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 509(4), 4849-4864. Oxford University Press
As the closest $L^{\ast}$ galaxy to our own Milky Way, the Andromeda galaxy (M31) is an ideal laboratory for studies of galaxy evolution. The AMIGA project has recently provided observations of the cool ($T\sim10^4$ K) phase of the circumgalactic med
Autor:
Jorryt Matthee, Sergio Da Graça Santos, Huub Röttgering, Ricardo Amorín, David Sobral, Max Gronke, Matthew Hayes, Joao Calhau, Ana Paulino-Afonso, Gabriele Pezzulli, Rohan P. Naidu, Daniel Schaerer
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 505(1), 1382-1412. Oxford University Press
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2021, 505, pp.1382-1412. ⟨10.1093/mnras/stab1304⟩
Monthly Notices of the Royal Astronomical Society, 505(1), 1382-1412
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2021, 505, pp.1382-1412. ⟨10.1093/mnras/stab1304⟩
Monthly Notices of the Royal Astronomical Society, 505(1), 1382-1412
We present the first results from the X-SHOOTER Lyman-$\alpha$ survey at $z=2$ (XLS-$z2$). XLS-$z2$ is a deep spectroscopic survey of 35 Lyman-$\alpha$ emitters (LAEs) utilising $\approx90$ hours of exposure time with VLT/X-SHOOTER and covers rest-fr
Autor:
Rohan P Naidu, Jorryt Matthee, Pascal A Oesch, Charlie Conroy, David Sobral, Gabriele Pezzulli, Matthew Hayes, Dawn Erb, Ricardo Amorín, Max Gronke, Daniel Schaerer, Sandro Tacchella, Josephine Kerutt, Ana Paulino-Afonso, João Calhau, Mario Llerena, Huub Röttgering
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 510(3), 4582-4607. Oxford University Press
Monthly Notices of the Royal Astronomical Society, 510(3), 4582–4607
Monthly Notices of the Royal Astronomical Society, 510(3), 4582-4607
Monthly Notices of the Royal Astronomical Society, 510(3), 4582–4607
Monthly Notices of the Royal Astronomical Society, 510(3), 4582-4607
The ionizing photon escape fraction [Lyman continuum (LyC) fesc] of star-forming galaxies is the single greatest unknown in the reionization budget. Stochastic sightline effects prohibit the direct separation of LyC leakers from non-leakers at signif
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1caa7fe83ee4df3974e132f6b1e98126
https://research.rug.nl/en/publications/3261bd27-606b-42d3-ae4f-92cb0c976a96
https://research.rug.nl/en/publications/3261bd27-606b-42d3-ae4f-92cb0c976a96
Autor:
Jorryt Matthee, Rohan P Naidu, Gabriele Pezzulli, Max Gronke, David Sobral, Pascal A Oesch, Matthew Hayes, Dawn Erb, Daniel Schaerer, Ricardo Amorín, Sandro Tacchella, Ana Paulino-Afonso, Mario Llerena, João Calhau, Huub Röttgering
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 512(4), 5960-5977. Oxford University Press
Monthly Notices of the Royal Astronomical Society, 512(4), 5960-5977
Monthly Notices of the Royal Astronomical Society, 512(4), 5960-5977
The cosmic ionizing emissivity from star-forming galaxies has long been anchored to UV luminosity functions. Here, we introduce an emissivity framework based on Lyα emitters (LAEs), which naturally hones in on the subset of galaxies responsible for
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::34a1503f93efb7ded08002f7a648f1c9
https://doi.org/10.1093/mnras/stac801
https://doi.org/10.1093/mnras/stac801
Autor:
Simon J. Lilly, Sebastiano Cantalupo, Joop Schaye, Gabriele Pezzulli, Raffaella Anna Marino, Jorryt Matthee, Ruari Mackenzie, Lutz Wisotzki, S. Muzahid
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 502(1), 494-509
Monthly Notices of the Royal Astronomical Society, 502(1), 494-509. Oxford University Press
Monthly Notices of the Royal Astronomical Society, 502(1), 494-509. Oxford University Press
We present the results from a MUSE survey of twelve $z\simeq3.15$ quasars, which were selected to be much fainter (20
Comment: Accepted to MNRAS. 17 pages, 7 figures
Comment: Accepted to MNRAS. 17 pages, 7 figures
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::db5d992b85f1c6ff75e6638189605427
http://hdl.handle.net/1887/3275656
http://hdl.handle.net/1887/3275656
Autor:
Gabriele Pezzulli
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 508(4), 5842-5853. Oxford University Press
Two currently debated problems in galaxy evolution, the fundamentally local or global nature of the main sequence of star formation and the evolution of the mass-size relation of star forming galaxies (SFGs), are shown to be intimately related to eac
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1cc371b7ba54733640d70d09b8d99116
Publikováno v:
Astronomy & Astrophysics, 644
Astronomy & astrophysics, 644:125. EDP Sciences
Astronomy & astrophysics, 644:125. EDP Sciences
In the last decades, much effort has been put into finding the star formation law which could unequivocally link the gas and the star formation rate (SFR) densities measured on sub-kiloparsec scale in star-forming galaxies. The conventional approach
Autor:
Sean D. Johnson, Gabriele Pezzulli, Ruari Mackenzie, J. S. den Brok, Tanya Urrutia, Wolfram Kollatschny, Mirko Krumpe, Sebastiano Cantalupo, Raffaella Anna Marino, Jorryt Matthee
A prediction of the classic active galactic nuclei (AGN) unification model is the presence of ionisation cones with different orientations depending on the AGN type. Confirmations of this model exist for present times, but it is less clear in the ear
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::77ffb060051222ad6dc2d282df87122c
http://arxiv.org/abs/2005.01732
http://arxiv.org/abs/2005.01732
Autor:
Kyle A. Oman, A. Marasco, Lorenzo Posti, Lexi Gault, John J. Salzer, Kameron Reiter, Enrico M. Di Teodoro, Tom Oosterloo, John M. Cannon, Nicholas J. Smith, Katherine L. Rhode, Martha P. Haynes, Elizabeth A. K. Adams, Pavel E. Mancera Piña, L. Leisman, Filippo Fraternali, Gabriele Pezzulli, Cecilia Bacchini
Publikováno v:
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2020, 495 (4), pp.3636-3655. ⟨10.1093/mnras/staa1256⟩
Monthly Notices of the Royal Astronomical Society, 495 (4)
Monthly Notices of the Royal Astronomical Society, 495(4), 3636-3655. Oxford University Press
Monthly notices of the Royal Astronomical Society, 2020, Vol.495(4), pp.3636-3655 [Peer Reviewed Journal]
Monthly Notices of the Royal Astronomical Society
Mon.Not.Roy.Astron.Soc., 2020, 495 (4), pp.3636-3655. ⟨10.1093/mnras/staa1256⟩
Monthly Notices of the Royal Astronomical Society, 495 (4)
Monthly Notices of the Royal Astronomical Society, 495(4), 3636-3655. Oxford University Press
Monthly notices of the Royal Astronomical Society, 2020, Vol.495(4), pp.3636-3655 [Peer Reviewed Journal]
Monthly Notices of the Royal Astronomical Society
We study the gas kinematics of a sample of six isolated gas-rich low surface brightness galaxies, of the class called ultra-diffuse galaxies (UDGs). These galaxies have recently been shown to be outliers from the baryonic Tully–Fisher relation (BTF
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::23451887085a7a5e8d42422b772cfd05