activity
20082026
most citedThe CARMENES search for exoplanets around M dwarfs: High-resolution optical and near-infrared spectroscopy of 324 survey stars

253 citations · 1.1k across the 25 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

6 papers · 1 filter

astro-ph.GA2024

CAVITY: Calar Alto Void Integral-field Treasury surveY. I. First public data release

Rubén García-Benito, Andoni Jiménez, Laura Sánchez-Menguiano +40

The Calar Alto Void Integral-field Treasury surveY (CAVITY) is a legacy project aimed at characterising the population of galaxies inhabiting voids, which are the most under-dense…

astro-ph.GA2024★ 19 cited

CAVITY, Calar Alto Void Integral-field Treasury surveY and project extension

I. Pérez, S. Verley, L. Sánchez-Menguiano +58

We have learnt in the last decades that the majority of galaxies belong to high density regions interconnected in a sponge-like fashion. This large-scale structure is characterised…

astro-ph.GA2020★ 12 cited

Gas and dust cooling along the major axis of M33 (HerM33es) -- Herschel/PACS [CII] and [OI] observations

Carsten Kramer, Thomas Nikola, Sibylle Anderl +17

M33 is a gas rich spiral galaxy of the Local Group. We investigate the relationship between the two major gas cooling lines and the total infrared (TIR) dust continuum. We mapped t…

astro-ph.GA2016★ 20 cited

Dust Properties in HII Regions in M33

M. Relano, R. Kennicutt, U. Lisenfeld +11

The conversion of the IR emission into star formation rate can be strongly dependent on the physical properties of the dust, which are affected by the environmental conditions wher…

astro-ph.GA2016★ 27 cited

Millimeter and Submillimeter Excess Emission in M33 revealed by Planck and LABOCA

I. Hermelo, M. Relaño, U. Lisenfeld +6

Previous studies have shown the existence of an excess of emission at submillimeter (submm) and millimeter (mm) wavelengths in the spectral energy distribution (SED) of many low-me…

astro-ph.GA2014★ 28 cited

The Heating of Mid-Infrared Dust in the Nearby Galaxy M33: A Testbed for Tracing Galaxy Evolution

M. Calapa, D. Calzetti, B. T. Draine +10

Because the 8 μm polycyclic aromatic hydrocarbon (PAH) emission has been found to correlate with other well-known star formation tracers, it has widely been used as a star formatio…