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20132026
most citedHydrogen reionisation ends by : Lyman- optical depth measured by the XQR-30 sample

302 citations · 6.5k across the 129 of their papers we have counts for

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21 papers · 1 filter

astro-ph.GA2022★ 28 cited

[CII] halos in ALPINE galaxies: smoking-gun of galactic outflows?

E. Pizzati, A. Ferrara, A. Pallottini +3

ALMA observations have revealed that many high redshift galaxies are surrounded by extended (10-15 kpc) [CII]-emitting halos which are not predicted by even the most advanced zoom-…

astro-ph.GA2022★ 18 cited

Interpreting ALMA non-detections of JWST super-early galaxies

M. Kohandel, A. Ferrara, A. Pallottini +3

Recent attempts to detect [OIII] 88m emission from super-early () galaxy candidates observed by JWST have been unsuccessful. By using zoom-in simulations, we show that the…

astro-ph.CO2022

CONCERTO: Simulating the CO, [CII], and [CI] line emission of galaxies in a 117 field and the impact of field-to-field variance

A. Gkogkou, M. Béthermin, G. Lagache +29

In the submm regime, spectral line scans and line intensity mapping (LIM) are new promising probes for the cold gas content and star formation rate of galaxies across cosmic time.…

astro-ph.GA2022★ 14 cited

Is the star formation rate in quasars overestimated?

Fabio Di Mascia, Stefano Carniani, Simona Gallerani +4

The large total infrared (TIR) luminosities () observed in quasars are generally converted into high star formation rates ($SFR \gtr…

astro-ph.GA2022★ 6 cited

ALMA Observations for CO Emission from Luminous Lyman-break Galaxies at -

Yoshiaki Ono, Seiji Fujimoto, Yuichi Harikane +14

We present our new Atacama Large Millimeter/submillimeter Array (ALMA) observations targeting CO(6-5) emission from three luminous Lyman break galaxies (LBGs) at $z_{\rm spec} = 6.…

astro-ph.GA2022★ 44 cited

A new look at the infrared properties of z 5 galaxies

L. Sommovigo, A. Ferrara, S. Carniani +6

Recent ALMA large surveys unveiled the presence of significant dust continuum emission in star-forming galaxies at . Unfortunately, such large programs -- i.e. ALPINE ($z\sim…

astro-ph.GA2022★ 231 cited

On the stunning abundance of super-early, massive galaxies revealed by JWST

A. Ferrara, A. Pallottini, P. Dayal

The earliest JWST observations have revealed an unexpected abundance of super-early (), massive () galaxies at the bright-end ($M_{\rm UV}\approx -…

astro-ph.GA2022★ 22 cited

The black hole and host galaxy growth in an isolated QSO observed with ALMA

R. Tripodi, C. Feruglio, F. Fiore +11

The outstanding mass growth of supermassive black holes (SMBHs) at the Reionisation Epoch and how it is related to the concurrent growth of their host galaxies, poses challenges to…

astro-ph.GA2022★ 40 cited

The ALMA REBELS Survey: The Cosmic HI Gas Mass Density in Galaxies at

K. E. Heintz, P. A. Oesch, M. Aravena +12

The neutral atomic gas content of individual galaxies at large cosmological distances has until recently been difficult to measure due to the weakness of the hyperfine HI 21-cm tra…

astro-ph.GA2022

The ALMA REBELS Survey: Average [CII] sizes of Star-Forming Galaxies from to

Y. Fudamoto, R. Smit, R. A. A. Bowler +36

We present the average [CII] emission line sizes of UV-bright star-forming galaxies at . Our results are derived from a stacking analysis of [CII] $158\,\rm{…

astro-ph.CO2022★ 91 cited

Long Dark Gaps in the Ly Forest at : Evidence of Ultra Late Reionization from XQR-30 Spectra

Yongda Zhu, George D. Becker, Sarah E. I. Bosman +22

We present a new investigation of the intergalactic medium (IGM) near reionization using dark gaps in the Lyman- (Ly) forest. With its lower optical depth, Ly offers a pot…

astro-ph.GA2022★ 60 cited

Dynamical characterization of galaxies up to

F. Rizzo, M. Kohandel, A. Pallottini +4

The characterization of the dynamical state of galaxies up to z~7 is crucial for constraining the mechanisms driving the mass assembly in the early Universe. However, it is unclear…

astro-ph.GA2022★ 56 cited

CONCERTO: High-fidelity simulation of millimeter line emissions of galaxies and [CII] intensity mapping

M. Bethermin, A. Gkogkou, M. Van Cuyck +27

The intensity mapping of the [CII] 158um line redshifted to the sub-mm window is a promising probe of the z>4 star formation and its spatial distribution into the large-scale struc…

astro-ph.GA2022★ 93 cited

The ALMA REBELS Survey: Specific Star-Formation Rates in the Reionization Era

Michael W. Topping, Daniel P. Stark, Ryan Endsley +21

We present specific star-formation rates for 40 UV-bright galaxies at observed as part of the Reionization Era Bright Emission Line Survey (REBELS) ALMA large program. T…

astro-ph.GA2022★ 126 cited

The ALMA REBELS Survey: Dust Continuum Detections at z > 6.5

Hanae Inami, Hiddo S. B. Algera, Sander Schouws +25

We report 18 dust continuum detections () at and out of 49 ultraviolet(UV)-bright galaxies ( mag) at , observed…

astro-ph.GA2022

The 21-cm signal from the Cosmic Dawn: metallicity dependence of high mass X-ray binaries

Harman Deep Kaur, Yuxiang Qin, Andrei Mesinger +3

X-rays from High-Mass X-ray Binaries (HMXBs) are likely the main source of heating of the intergalactic medium (IGM) during Cosmic Dawn (CD), before the completion of reionization.…

astro-ph.GA2022★ 124 cited

The ALMA REBELS Survey: the dust content of Lyman Break Galaxies

P. Dayal, A. Ferrara, L. Sommovigo +22

We include a fully coupled treatment of metal and dust enrichment into the Delphi semi-analytic model of galaxy formation to explain the dust content of 13 Lyman Break Galaxies (LB…

astro-ph.GA2022★ 104 cited

The ALMA REBELS Survey. Epoch of Reionization giants: properties of dusty galaxies at

A. Ferrara, L. Sommovigo, P. Dayal +27

We analyse FIR dust continuum measurements for 14 galaxies () in the ALMA REBELS LP to derive their physical properties. Our model uses three input data: (a) the UV spe…

astro-ph.GA2022★ 131 cited

The REBELS ALMA Survey: cosmic dust temperature evolution out to z 7

L. Sommovigo, A. Ferrara, A. Pallottini +27

ALMA observations have revealed the presence of dust in the first generations of galaxies in the Universe. However, the dust temperature remains mostly unconstrained due to t…

astro-ph.GA2022★ 51 cited

The ALMA REBELS Survey: Efficient Ly Transmission of UV-Bright z7 Galaxies from Large Velocity Offsets and Broad Line Widths

Ryan Endsley, Daniel P. Stark, Rychard J. Bouwens +19

Recent work has shown that UV-luminous reionization-era galaxies often exhibit strong Lyman-alpha emission despite being situated at redshifts where the IGM is thought to be substa…

astro-ph.GA2022★ 99 cited

A survey of high- galaxies: SERRA simulations

A. Pallottini, A. Ferrara, S. Gallerani +10

We introduce SERRA, a suite of zoom-in high-resolution () cosmological simulations including non-equilibrium chemistry and on-the-fly radiative transfer. The outpu…