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20112026
most citedCALIFA, the Calar Alto Legacy Integral Field Area survey: I. Survey presentation

1.3k citations · 4.5k across the 25 of their papers we have counts for

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12 papers · 1 filter

astro-ph.GA2020

The Future of IMF studies with the ELT and MICADO I: The local Universe as a resolved IMF laboratory

Kieran Leschinski, João Alves

Aims. In this work we aim to estimate the lowest stellar mass that MICADO at the ELT will be able to reliably detect given a stellar density and distance. We also show that instrum…

astro-ph.GA2017★ 117 cited

Fibers in the NGC1333 proto-cluster

A. Hacar, M. Tafalla, J. Alves

Are the initial conditions for clustered star formation the same as for non-clustered star formation? To investigate the initial gas properties in young proto-clusters we carried o…

astro-ph.GA2016★ 30 cited

Aperture effects on the oxygen abundance determinations from CALIFA data

J. Iglesias-Páramo, J. M. Vílchez, F. F. Rosales-Ortega +23

This paper aims at providing aperture corrections for emission lines in a sample of spiral galaxies from the Calar Alto Legacy Integral Field Area Survey (CALIFA) database. In part…

astro-ph.GA2016★ 272 cited

CALIFA, the Calar Alto Legacy Integral Field Area survey: IV. Third Public data release

S. F. Sánchez, R. García-Benito, S. Zibetti +60

This paper describes the Third Public Data Release (DR3) of the Calar Alto Legacy Integral Field Area (CALIFA) survey. Science-grade quality data for 667 galaxies are made public,…

astro-ph.GA2016★ 189 cited

Star formation along the Hubble sequence: Radial structure of the star formation of CALIFA galaxies

R. M. González Delgado, R. Cid Fernandes, E. Pérez +21

The aim of this paper is to characterize the radial structure of the star formation rate (SFR) in galaxies in the nearby Universe as represented by the CALIFA survey. The sample un…

astro-ph.GA2015★ 101 cited

The Musca cloud: A 6 pc-long velocity-coherent, sonic filament

A. Hacar, J. Kainulainen, M. Tafalla +2

Filaments play a central role in the molecular clouds' evolution, but their internal dynamical properties remain poorly characterized. To further explore the physical state of thes…