Zobrazeno 1 - 10
of 4 546
pro vyhledávání: '"Astrofisica"'
[pt] Conforme entramos na era de precisão da astronomia multimensageira, novas janelas se abrem para compreendermos melhor o Universo, desde a escala quântica até a escala cósmica. Em particular, o estudo de fenômenos astrofísicos de altas ener
Autor:
Guillermo Arreaga Garcia
Publikováno v:
Epistemus, Vol 16, Iss 33 (2022)
En el presente trabajo se exponen los resultados de un proyecto de simulación numérica diseñado para estudiar el proceso de formación de la nube interestelar conocida como "the Brick". Dicha nube está localizada cerca del centro de la Vía Láct
Externí odkaz:
https://doaj.org/article/eab213fe696b4cf1ab00e77b67aa7c14
Autor:
L Barrufet, P A Oesch, R Bouwens, H Inami, L Sommovigo, H Algera, E da Cunha, M Aravena, P Dayal, A Ferrara, Y Fudamoto, V Gonzalez, L Graziani, A P S Hygate, I de Looze, T Nanayakkara, A Pallottini, R Schneider, M Stefanon, M Topping, P van der Werf
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 522(3):3926-3934
We present the first observational infrared luminosity function (IRLF) measurement in the Epoch of Reionization (EoR) based on a ultraviolet (UV)-selected galaxy sample with the Atacama Large Millimeter Array (ALMA) spectroscopic observations. Our an
Autor:
Dimitra Pierroutsakou, Alfonso Boiano, Ciro Boiano, Marco La Commara, Giovanni La Rana, Marco Mazzocco, Concetta Parascandolo, Cosimo Signorini, Francesca Soramel, Emanuele Strano
Publikováno v:
Nucleus, Vol 0, Iss 63, Pp 53-57 (2019)
The low-energy light radioactive ion beam in-flight facility EXOTIC and the associated experimental set-up,operational at Legnaro National Laboratories of the National Institute of Nuclear Physics (LNL-INFN, Italy) and designed for nuclear physics an
Externí odkaz:
https://doaj.org/article/c69ae7e1bf92406e959cd7a8a101576a
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 522:3986-3991
The earliest JWST observations have revealed an unexpected abundance of super-early (z > 10), massive ($M_*\, \approx 10^9 {\rm M}_{\odot }$ ) galaxies at the bright-end (MUV ≈ −21) of the ultraviolet luminosity function (UV LF). We present a min
Possible evidence for a large-scale enhancement in the Lyman-α forest power spectrum at redshiftz≥ 4
Autor:
Margherita Molaro, Vid Iršič, James S Bolton, Maggie Lieu, Laura C Keating, Ewald Puchwein, Martin G Haehnelt, Matteo Viel
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 521:1489-1501
Inhomogeneous reionization enhances the 1D Ly α forest power spectrum on large scales at redshifts z ≥ 4. This is due to coherent fluctuations in the ionized hydrogen fraction that arise from large-scale variations in the post-reionization gas tem
Autor:
Rebecca L Davies, E Ryan-Weber, V D’Odorico, S E I Bosman, R A Meyer, G D Becker, G Cupani, L C Keating, M Bischetti, F B Davies, A-C Eilers, E P Farina, M G Haehnelt, A Pallottini, Y Zhu
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 521:314-331
Intervening CIV absorbers are key tracers of metal-enriched gas in galaxy halos over cosmic time. Previous studies suggest that the CIV cosmic mass density ($\Omega_{\rm CIV}$) decreases slowly over 1.5 $\lesssim z\lesssim$ 5 before declining rapidly
Autor:
A. Limonta, M. Zannoni, G. Coppi, G. Conenna, F. Boussaha, A. Tartari, M. Gervasi, F. Nati, A. Passerini, P. de Bernardis, A. Coppolecchia, G. D’Alessandro, S. Masi, A. Paiella, M. Bersanelli, C. Franceschet, E. Manzan, A. Mennella
Publikováno v:
Journal of Low Temperature Physics. 209:631-639
With this contribution we show the readout electronics for kinetic inductance detectors (KIDs) that we are developing based on commercial IQ transceivers from National Instruments and using a Virtex 5 class FPGA. It will be the readout electronics of
Publikováno v:
Monthly Notices of the Royal Astronomical Society: Letters. 520:L16-L20
Recent attempts to detect [OIII] 88$μ$m emission from super-early ($z>10$) galaxy candidates observed by JWST have been unsuccessful. By using zoom-in simulations, we show that these galaxies are faint, and mostly fall below the local metal-poor $\r
Autor:
Ewald Puchwein, James S Bolton, Laura C Keating, Margherita Molaro, Prakash Gaikwad, Girish Kulkarni, Martin G Haehnelt, Vid Iršič, Tomáš Šoltinský, Matteo Viel, Dominique Aubert, George D Becker, Avery Meiksin
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 519:6162-6183
We present the Sherwood-Relics simulations, a new suite of large cosmological hydrodynamical simulations aimed at modelling the intergalactic medium (IGM) during and after the cosmic reionization of hydrogen. The suite consists of over 200 simulation