activity
20112026
most citedOn the Stellar Populations of Galaxies at z=9-11: The Growth of Metals and Stellar Mass at Early Times

212 citations · 3.2k across the 77 of their papers we have counts for

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Showing 2018Show all

6 papers · 1 filter

astro-ph.SR2018★ 56 cited

Supernova dust yields: the role of metallicity, rotation, and fallback

S. Marassi, R. Schneider, M. Limongi +3

Supernovae (SNe) are considered to have a major role in dust enrichment of high redshift galaxies and, due to the short lifetimes of interstellar grains, in dust replenishment of l…

astro-ph.GA2018★ 13 cited

The infrared-luminous progenitors of high-z quasars

Michele Ginolfi, Raffaella Schneider, Rosa Valiante +4

Here we explore the infrared (IR) properties of the progenitors of high-z quasar host galaxies. Adopting the cosmological, data constrained semi-analytic model GAMETE/QSOdust, we s…

astro-ph.GA2018★ 25 cited

Radiative transfer of ionizing radiation through gas and dust: stellar source case

Martin Glatzle, Benedetta Ciardi, Luca Graziani

We present a new dust extension to the Monte Carlo radiative transfer code crash, which enables it to simulate the propagation of ionizing radiation through mixtures of gas and dus…

astro-ph.CO2018★ 23 cited

X-ray ionization of the intergalactic medium by quasars

Luca Graziani, B. Ciardi, M. Glatzle

We investigate the impact of quasars on the ionization of the surrounding intergalactic medium (IGM) with the radiative transfer code \texttt{CRASH4}, now accounting for X-rays and…

astro-ph.CO2018★ 64 cited

The Epoch of IGM heating by early sources of X-rays

Marius Berge Eide, Luca Graziani, Benedetta Ciardi +3

Observations of the 21 cm line from neutral hydrogen indicate that an Epoch of Heating (EoH) might have preceded the later Epoch of Reionization (EoR). Here we study the effects on…

astro-ph.GA2018★ 47 cited

Chasing the observational signatures of seed black holes at z > 7: candidate observability

Rosa Valiante, Raffaella Schneider, Luca Zappacosta +3

Observing the light emitted by the first accreting black holes (BHs) would dramatically improve our understanding of the formation of quasars at z > 6, possibly unveiling the natur…