Zobrazeno 1 - 10
of 44
pro vyhledávání: '"James W. Trayford"'
Autor:
Antonios Katsianis, Peter Camps, Mattia Vaccari, Bert Vandenbroucke, Tom Theuns, James W. Trayford, Maarten Baes, Lucia Marchetti, Ana Trčka
Publikováno v:
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Monthly Notices of the Royal Astronomical Society, 494(2), 2912-2924
Monthly Notices of the Royal Astronomical Society, 494(2), 2912-2924
We present infrared luminosity functions and dust mass functions for the EAGLE cosmological simulation, based on synthetic multi-wavelength observations generated with the SKIRT radiative transfer code. In the local Universe, we reproduce the observe
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::52e1d0824a2e7e1195f29e03676efa48
https://doi.org/10.1093/mnras/staa990
https://doi.org/10.1093/mnras/staa990
Autor:
James W. Trayford, Chris Power, Ruby J. Wright, Luke J. M. Davies, O. Ivy Wong, Claudia del P. Lagos
Publikováno v:
Monthly Notices of the RAS (0035-8711)
Monthly Notices of the RAS (0035-8711), 487(3), 3740-3758
Monthly Notices of the RAS (0035-8711), 487(3), 3740-3758
We use the \eagle\ simulations to study the connection between the quenching timescale, $\tau_{\rm Q}$, and the physical mechanisms that transform star-forming galaxies into passive galaxies. By quantifying $\tau_{\rm Q}$ in two complementary ways -
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::33556497e6354ece18e1ef23d45559b9
https://doi.org/10.1093/mnras/stz1410
https://doi.org/10.1093/mnras/stz1410
Autor:
Joop Schaye, James W. Trayford
Publikováno v:
Monthly Notices of the RAS (0035-8711), 485(4), 5715-5732
We explore scaling relations between the physical properties of spatially resolved regions within the galaxies that emerge in the Evolution and Assembly of GaLaxies and their Environments (EAGLE) hydrodynamical, cosmological simulations. Using 1 kpc-
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::717dfc6016c4aacdb56be012059a2c12
https://doi.org/10.1093/mnras/stz757
https://doi.org/10.1093/mnras/stz757
Autor:
A. Nersesian, Tom Theuns, Peter Camps, Ana Trčka, Wouter Dobbels, Maarten Baes, James W. Trayford
Publikováno v:
Monthly Notices of the RAS (0035-8711), 484(3), 4069-4082
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Monthly notices of the Royal Astronomical Society, 2019, Vol.484(3), pp.4069-4082 [Peer Reviewed Journal]
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Monthly notices of the Royal Astronomical Society, 2019, Vol.484(3), pp.4069-4082 [Peer Reviewed Journal]
The cosmic spectral energy distribution (CSED) is the total emissivity as a function of wavelength of galaxies in a given cosmic volume. We compare the observed CSED from the UV to the submm to that computed from the EAGLE cosmological hydrodynamical
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b2a8acd51d08f4c36fa75ef2963aff6a
https://doi.org/10.1093/mnras/stz302
https://doi.org/10.1093/mnras/stz302
Autor:
Francesco D'Eugenio, Claudia del P. Lagos, C. Derkenne, J. T. Mendel, David Fisher, Chiaki Kobayashi, R. Bassett, Aaron S. G. Robotham, A. Poci, J. van de Sande, A. Khalid, Sarah M. Sweet, Scott M. Croom, A. J. Battisti, Sabine Bellstedt, E. Gjergo, Anshu Gupta, K. E. Harborne, Luke J. M. Davies, Sam P. Vaughan, Emily Wisnioski, Philip Taylor, Edward N. Taylor, L. Zanisi, Kim-Vy Tran, Sukyoung K. Yi, P. Sharda, Jonathan Bland-Hawthorn, Yingjie Peng, Tania M. Barone, James W. Trayford, Felix Schulze, Richard M. McDermid, Simon P. Driver, Sree Oh, Matthew Colless, Anna Ferré-Mateu, F. Collacchioni, Tiantian Yuan, Caroline Foster, Donghyeon J. Khim, E. J. Johnston, Rhea-Silvia Remus
We present an overview of the Middle Ages Galaxy Properties with Integral Field Spectroscopy (MAGPI) survey, a Large Program on ESO/VLT. MAGPI is designed to study the physical drivers of galaxy transformation at a lookback time of 3-4 Gyr, during wh
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::20706abe5bcef82659fa0b0da76ce633
http://arxiv.org/abs/2011.13567
http://arxiv.org/abs/2011.13567
Publikováno v:
Monthly Notices of the RAS (0035-8711), 491(3), 3937-3951
Monthly Notices of the RAS (0035-8711)
Trayford, J W, Lagos, C D P, Robotham, A S G & Obreschkow, D 2020, ' Fade to grey : systematic variation of galaxy attenuation curves with galaxy properties in the EAGLE simulations ', Monthly Notices of the Royal Astronomical Society, vol. 491, no. 3, pp. 3937-3951 . https://doi.org/10.1093/mnras/stz3234
Monthly Notices of the RAS (0035-8711)
Trayford, J W, Lagos, C D P, Robotham, A S G & Obreschkow, D 2020, ' Fade to grey : systematic variation of galaxy attenuation curves with galaxy properties in the EAGLE simulations ', Monthly Notices of the Royal Astronomical Society, vol. 491, no. 3, pp. 3937-3951 . https://doi.org/10.1093/mnras/stz3234
We present a simple model for galaxy attenuation by fitting skirt radiative transfer calculations for ∼10 000 eagle galaxies at redshifts z = 2 − 0. Our model adapts the two-component screen model of Charlot & Fall, parametrizing the optical dept
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b1709a911e3ea02022c81e131cc9a40e
https://ui.adsabs.harvard.edu/abs/2019MNRAS.tmp.2823T
https://ui.adsabs.harvard.edu/abs/2019MNRAS.tmp.2823T
Autor:
Matías Bravo, Chris Power, Aaron S. G. Robotham, Claudia del P. Lagos, Danail Obreschkow, Rodrigo Tobar, Simon P. Driver, Luke J. M. Davies, Pascal J. Elahi, James W. Trayford, Sabine Bellstedt
Publikováno v:
Lagos, C D P, Robotham, A S G, Trayford, J W, Tobar, R, Bravo, M, Bellstedt, S, Davies, L J M, Driver, S P, Elahi, P J, Obreschkow, D & Power, C 2019, ' From the far-ultraviolet to the far-infrared – galaxy emission at 0≤z≤10 in theSHARKsemi-analytic model ', Monthly Notices of the Royal Astronomical Society, vol. 489, no. 3, pp. 4196-4216 . https://doi.org/10.1093/mnras/stz2427
Monthly Notices of the RAS (0035-8711), 489(3), 4196-4216
Monthly Notices of the RAS (0035-8711), 489(3), 4196-4216
We combine the Shark semi-analytic model of galaxy formation with the ProSpect software tool for spectral energy distribution (SED) generation to study the multi-wavelength emission of galaxies from the far-ultraviolet (FUV) to the far-infrared (FIR)
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d641050d84fdb8c50ebf1ed7d0a7324d
https://hdl.handle.net/1887/84655
https://hdl.handle.net/1887/84655
Autor:
Tom Theuns, Peter Camps, Joop Schaye, Ana Trčka, Guillermo A. Blanc, James W. Trayford, Antonios Katsianis, Valentino Gonzalez, Marko Stalevski, Maarten Baes, Xianzhong Zheng, Luke J. M. Davies, Claudia del P. Lagos
Publikováno v:
The astrophysical journal, 2019, Vol.879(1), pp.11 [Peer Reviewed Journal]
ASTROPHYSICAL JOURNAL
Astrophysical Journal (0004-637X), 879(1), 11
ASTROPHYSICAL JOURNAL
Astrophysical Journal (0004-637X), 879(1), 11
The scatter (${\rm\sigma_{\text{sSFR}}}$) of the specific star formation rates (sSFRs) of galaxies is a measure of the diversity in their star formation histories (SFHs) at a given mass. In this paper we employ the EAGLE simulations to study the depe
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b3019bcc99d2782efe178486ce12d6af
https://doi.org/10.3847/1538-4357/ab1f8d
https://doi.org/10.3847/1538-4357/ab1f8d
Autor:
Tom Theuns, Joop Schaye, James W. Trayford, Ian Smail, Richard G. Bower, Peter Camps, Stuart McAlpine, Robert A. Crain, Maarten Baes, A. M. Swinbank
Publikováno v:
Monthly Notices of the RAS (0035-8711), 488(2), 2440-2454
Monthly Notices of the RAS (0035-8711)
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Monthly notices of the Royal Astronomical Society, 2019, Vol.488(2), pp.2440-2454 [Peer Reviewed Journal]
Monthly Notices of the RAS (0035-8711)
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Monthly notices of the Royal Astronomical Society, 2019, Vol.488(2), pp.2440-2454 [Peer Reviewed Journal]
We exploit EAGLE, a cosmological hydrodynamical simulation, to reproduce the selection of the observed sub-millimeter (submm) galaxy population by selecting the model galaxies at $z \geq 1$ with mock submm fluxes $S_{850} \geq 1$ mJy. There is a reas
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::950b132ddcf4b4a46665eb0de8863ac6
https://doi.org/10.1093/mnras/stz1692
https://doi.org/10.1093/mnras/stz1692
Autor:
Joop Schaye, Richard G. Bower, Vivienne Wild, James W. Trayford, Stuart McAlpine, Robert A. Crain, M. M. Pawlik, Matthieu Schaller
Publikováno v:
Nature Astronomy, 3, 440-446
About 35 years ago a class of galaxies with unusually strong Balmer absorption lines and weak emission lines was discovered in distant galaxy clusters. These objects, alternatively referred to as post-starburst, E+A or k+a galaxies, are now known to
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::dc621704e8e6ed4cf6857b71e1e93f1a
http://hdl.handle.net/10138/308516
http://hdl.handle.net/10138/308516