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20092026
most citedLight Curves of the Neutron Star Merger GW170817/SSS17a: Implications for R-Process Nucleosynthesis

839 citations · 6.8k across the 82 of their papers we have counts for

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Showing 2023Show all

8 papers · 1 filter

astro-ph.IM2023

Boost recall in QSO selection from highly imbalanced photometric datasets

Giorgio Calderone, Francesco Guarneri, Matteo Porru +9

Context. The identification of bright QSOs is of great importance to probe the intergalactic medium and address open questions in cosmology. Several approaches have been adopted to…

astro-ph.GA2023★ 1 cited

Crossing the Rubicon of Reionization with z~5 QSOs

A. Grazian, K. Boutsia, E. Giallongo +12

One of the key open questions in Cosmology is the nature of the sources that completed the cosmological hydrogen Reionization at z~5.2. High-z primeval galaxies have been long cons…

astro-ph.HE2023

Swift/UVOT discovery of Swift J221951-484240: a UV luminous ambiguous nuclear transient

S. R. Oates, N. P. M. Kuin, M. Nicholl +57

We report the discovery of Swift J221951-484240 (hereafter: J221951), a luminous slow-evolving blue transient that was detected by the Neil Gehrels Swift Observatory Ultra-violet/O…

astro-ph.GA2023★ 2 cited

Searching for Intragroup Light in Deep U-band Imaging of the COSMOS Field

Tyler McCabe, Caleb Redshaw, Lillian Otteson +24

We present the results of deep, ground based U-band imaging with the Large Binocular Telescope of the Cosmic Evolution Survey (COSMOS) field as part of the near-UV imaging program,…

astro-ph.CO2023★ 24 cited

Spectroscopy of QUBRICS quasar candidates: 1672 new redshifts and a Golden Sample for the Sandage Test of the Redshift Drift

Stefano Cristiani, Matteo Porru, Francesco Guarneri +10

The QUBRICS (QUasars as BRIght beacons for Cosmology in the Southern hemisphere) survey aims at constructing a sample of the brightest quasars with z>~2.5, observable with faciliti…

astro-ph.GA2023★ 37 cited

Ionized gas kinematics and chemical abundances of low-mass star-forming galaxies at

M. Llerena, R. Amorín, L. Pentericci +6

We selected 35 low-mass SFGs (7.9<log(M/M)<10.3) from deep spectroscopic surveys based on their CIII]1908 emission. We used follow-up NIR observations to examine thei…