Zobrazeno 1 - 10
of 4 099
pro vyhledávání: '"FIS/05 ASTRONOMIA E ASTROFISICA"'
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
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
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
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
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
Autor:
A Marino, A Anitra, S M Mazzola, T Di Salvo, A Sanna, P Bult, S Guillot, G Mancuso, M Ng, A Riggio, A C Albayati, D Altamirano, Z Arzoumanian, L Burderi, C Cabras, D Chakrabarty, N Deiosso, K C Gendreau, R Iaria, A Manca, T E Strohmayer
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2022, 515, pp.3838-3852. ⟨10.1093/mnras/stac2038⟩
Monthly Notices of the Royal Astronomical Society, 2022, 515, pp.3838-3852. ⟨10.1093/mnras/stac2038⟩
The neutron star low-mass X-ray binary SWIFT J1749.4–2807 is the only known eclipsing accreting millisecond X-ray pulsar. In this manuscript, we perform a spectral characterization of the system throughout its 2021, 2-week-long outburst, analysing
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 515:1676-1689
We present the results of a cluster search in the gamma-ray sky images of the Large Magellanic Cloud (LMC) region by means of the Minimum Spanning Tree (MST) and DBSCAN algorithms, at energies higher than 6 and 10 GeV, using 12 years of Fermi-LAT dat