activity
19992024
most citedQuasar-Lyman Forest Cross-Correlation from BOSS DR11 : Baryon Acoustic Oscillations

572 citations · 1.1k across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.CO2024★ 23 cited

Analytical and EZmock covariance validation for the DESI 2024 results

Daniel Forero-Sánchez, Michael Rashkovetskyi, Otávio Alves +44

The estimation of uncertainties in cosmological parameters is an important challenge in Large-Scale-Structure (LSS) analyses. For standard analyses such as Baryon Acoustic Oscillat…

astro-ph.GA2022★ 150 cited

Overview of the DESI Milky Way Survey

Andrew P. Cooper, Sergey E. Koposov, Carlos Allende Prieto +62

We describe the Milky Way Survey (MWS) that will be undertaken with the Dark Energy Spectroscopic Instrument (DESI) on the Mayall 4m telescope at the Kitt Peak National Observatory…

astro-ph.CO2013★ 572 cited

Quasar-Lyman Forest Cross-Correlation from BOSS DR11 : Baryon Acoustic Oscillations

Andreu Font-Ribera, David Kirkby, Nicolas Busca +40

We measure the large-scale cross-correlation of quasars with the Lyman alpha forest absorption, using over 164,000 quasars from Data Release 11 of the SDSS-III Baryon Oscillation S…

astro-ph2004★ 31 cited

EROS 2 photometry of probable R Coronae Borealis stars in the Small Magellanic Cloud

P. Tisserand, J. B. Marquette, J. P. Beaulieu +1

EROS 2 (Experience de Recherche d'Objets Sombres) conducted a survey of the SMC between July 1996 and February 2003 in two EROS broad-band colours, V_E and R_E. The photometric dat…

astro-ph2002★ 24 cited

EROS 2 proper motion survey: Constraints on the halo white dwarfs

B. Goldman, C. Afonso, Ch. Alard +9

We are conducting a 377-square-degree proper motion survey in the ~V and I bands in order to determine the cool white dwarf contribution to the Galactic dark matter. Using the 250…

astro-ph2001★ 208 cited

The ANTARES Optical Module

The ANTARES Collaboration

The ANTARES collaboration is building a deep sea neutrino telescope in the Mediterranean Sea. This detector will cover a sensitive area of typically 0.1 km-squared and will be equi…