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20032026
most citedAccurate photometric redshifts for the CFHT Legacy Survey calibrated using the VIMOS VLT Deep Survey

1.7k citations · 11.2k across the 166 of their papers we have counts for

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Showing 2024Show all

9 papers · 1 filter

astro-ph.HE2024★ 14 cited

GRB Redshift Estimation using Machine Learning and the Associated Web-App

Aditya Narendra, Maria Dainotti, Milind Sarkar +7

Context. Gamma-ray bursts (GRBs), observed at redshifts as high as 9.4, could serve as valuable probes for investigating the distant Universe. However, this necessitates an increas…

astro-ph.HE2024

GRB Redshift Classifier to Follow-up High-Redshift GRBs Using Supervised Machine Learning

Maria Giovanna Dainotti, Shubham Bhardwaj, Christopher Cook +8

Gamma-ray bursts (GRBs) are intense, short-lived bursts of gamma-ray radiation observed up to a high redshift () due to their luminosities. Thus, they can serve as cosmo…

astro-ph.IM2024★ 2 cited

ANDES, the high resolution spectrograph for the ELT: science goals, project overview and future developments

A. Marconi, M. Abreu, V. Adibekyan +286

The first generation of ELT instruments includes an optical-infrared high-resolution spectrograph, indicated as ELT-HIRES and recently christened ANDES (ArmazoNes high Dispersion E…

astro-ph.GA2024

The quiescent population at : Environmental impact on the mass-size relation

M. Figueira, M. Siudek, A. Pollo +5

How the quiescent galaxies evolve with redshift and the factors that impact their evolution are still debated. It is still unclear what the dominant mechanisms of passive galaxy gr…

astro-ph.CO2024

Halo asymmetry in the modelling of galaxy clustering

Anna Durkalec, Agnieszka Pollo, Ummi Abbas

Conventional studies of galaxy clustering within the framework of halo models typically assume that the density profile of all dark matter haloes can be approximated by the Navarro…

astro-ph.GA2024★ 18 cited

Effects of galaxy environment on merger fraction

W. J. Pearson, D. J. D. Santos, T. Goto +13

Aims. In this work, we intend to examine how environment influences the merger fraction, from the low density field environment to higher density groups and clusters. We also aim t…