activity
20062023
most citedThe Data Processing Pipeline for the MUSE Instrument

361 citations · 914 across the 23 of their papers we have counts for

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Showing astro-ph.GAShow all

5 papers · 1 filter

astro-ph.GA2018★ 3 cited

Dissecting the Core of the Tarantula Nebula with MUSE

Paul A Crowther, Norberto Castro, Chris Evans +3

We provide an overview of Science Verification MUSE observations of NGC 2070, the central region of the Tarantula Nebula in the Large Magellanic Cloud. Integral-field spectroscopy…

astro-ph.GA2015★ 88 cited

A MUSE map of the central Orion Nebula (M 42)

Peter M. Weilbacher, Ana Monreal-Ibero, Wolfram Kollatschny +15

We present a new integral-field spectroscopic dataset of the central part of the Orion Nebula (M 42), observed with the MUSE instrument at the ESO VLT. We reduced the data with the…

astro-ph.GA2015★ 11 cited

Towards DIB mapping in galaxies beyond 100 Mpc. A radial profile of the 5780.5 diffuse interstellar band in AM 1353-272 B

Ana Monreal-Ibero, Peter M. Weilbacher, Martin Wendt +5

Diffuse Interstellar Bands (DIBs) are non-stellar weak absorption features of unknown origin found in the spectra of stars viewed through one or several clouds of Interstellar Medi…

astro-ph.GA2012★ 29 cited

The central density of R136 in 30 Doradus

Fernando J. Selman, Jorge Melnick

The central density rho_0 of a stellar cluster is an important physical parameter for determining its evolutionary and dynamical state. How much mass segregation there is, or wheth…

astro-ph.GA2009★ 151 cited

The massive star initial mass function of the Arches cluster

Pablo Espinoza, Fernando J. Selman, Jorge Melnick

The massive Arches cluster near the Galactic center should be an ideal laboratory for investigating massive star formation under extreme conditions. But it comes at a high price: t…