activity
20062026
most citedThe Seventh Data Release of the Sloan Digital Sky Survey

5.4k citations · 5.6k across the 7 of their papers we have counts for

collaborators

9 papers

astro-ph.GA2026

The origin of UV emission in extremely low-mass satellite galaxies: Insights from Leo T

S Amrutha, Mousumi Das, Daniel Vaz +1

Leo T, a Milky Way (MW) satellite, is the lowest-mass gas-rich galaxy known to show recent star formation, making it an excellent laboratory for investigating star formation in the…

astro-ph.GA2026

Are High-EW LAEs good analogs for the earliest galaxies? A study on the ionizing conditions and gas properties of LAEs at $2\lesssim z\lesssim7

Lena Pless, Themiya Nanayakkara, Karl Glazebrook +3

Lyman- emitters (LAEs) are frequently proposed as analogs of the low-mass, metal-poor galaxies thought to dominate cosmic reionization. In particular, galaxies with large Ly…

astro-ph.GA2023★ 9 cited

The MUSE-Faint survey. IV. Dissecting Leo T, a gas-rich relic with recent star formation

Daniel Vaz, Jarle Brinchmann, Sebastiaan L. Zoutendijk +6

Leo T () is both the faintest and the least massive galaxy known to contain neutral gas and to display signs of recent star formation. We analyse photometry and stellar…

astro-ph.GA2021★ 18 cited

The Tully-Fisher relation in dense groups at in the MAGIC survey

Valentina Abril-Melgarejo, Benoît Epinat, Wilfried Mercier +11

Galaxies in dense environments are subject to interactions and mechanisms which directly affect their evolution by lowering their gas fractions and reducing their star-forming capa…

astro-ph.GA2017★ 35 cited

The MUSE Hubble Ultra Deep Field Survey: III. Testing photometric redshifts to 30th magnitude

J. Brinchmann, H. Inami, R. Bacon +14

We tested the performance of photometric redshifts for galaxies in the Hubble Ultra Deep field down to 30th magnitude. We compared photometric redshift estimates from three spectra…

astro-ph.GA2017★ 106 cited

The MUSE-Wide Survey: A first catalogue of 831 emission line galaxies

E. C. Herenz, T. Urrutia, L. Wisotzki +11

We present a first instalment of the MUSE-Wide survey, covering an area of 22.2 arcmin (corresponding to 20% of the final survey) in the CANDELS/Deep area of the Chandra…

astro-ph.GA2015★ 106 cited

A young star-forming galaxy at z = 3.5 with an extended Ly\, halo seen with MUSE

Vera Patrício, Johan Richard, Anne Verhamme +12

Spatially resolved studies of high redshift galaxies, an essential insight into galaxy formation processes, have been mostly limited to stacking or unusually bright objects. We pre…

astro-ph2008★ 5.4k cited

The Seventh Data Release of the Sloan Digital Sky Survey

K. Abazajian

This paper describes the Seventh Data Release of the Sloan Digital Sky Survey (SDSS), marking the completion of the original goals of the SDSS and the end of the phase known as SDS…

astro-ph2006

NIR Follow-Up of the VVDS 02hr Field

S. Temporin, A. Iovino, H. J. McCracken +46

We present a new K-band survey covering 623 arcmin in the VVDS 0226-0430 deep field down to a limiting magnitude K 20.5. We use the spectroscopic sample ex…