activity
20022025
most citedCALIFA, the Calar Alto Legacy Integral Field Area survey: I. Survey presentation

1.3k citations · 12.3k across the 113 of their papers we have counts for

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Showing 2014 · astro-ph.GAShow all

9 papers · 2 filters

astro-ph.GA2014

The CALIFA survey: Status Report

S. F. Sánchez, J. M. Vílchez, C. J. Walcher +5

We present here a brief summary of the status of the on-going CALIFA survey with an em- phasis on the results that have been recently published. In particular, we make a summary of…

astro-ph.GA2014★ 257 cited

CALIFA: a diameter-selected sample for an integral field spectroscopy galaxy survey

C. J. Walcher, L. Wisotzki, S. Bekeraité +48

We describe and discuss the selection procedure and statistical properties of the galaxy sample used by the Calar Alto Legacy Integral Field Area Survey (CALIFA), a public legacy s…

astro-ph.GA2014★ 144 cited

Insights on the stellar mass-metallicity relation from the CALIFA survey

R. M. González Delgado, R. Cid Fernandes, R. García-Benito +27

We use spatially and temporally resolved maps of stellar population properties of 300 galaxies from the CALIFA integral field survey to investigate how the stellar metallicity (Z*)…

astro-ph.GA2014★ 506 cited

The SAMI Galaxy Survey: instrument specification and target selection

J. J. Bryant, M. S. Owers, A. S. G. Robotham +54

The SAMI Galaxy Survey will observe 3400 galaxies with the Sydney-AAO Multi-object Integral-field spectrograph (SAMI) on the Anglo-Australian Telescope (AAT) in a 3-year survey whi…

astro-ph.GA2014★ 159 cited

The SAMI Galaxy Survey: Early Data Release

J. T. Allen, S. M. Croom, I. S. Konstantopoulos +45

We present the Early Data Release of the Sydney-AAO Multi-object Integral field spectrograph (SAMI) Galaxy Survey. The SAMI Galaxy Survey is an ongoing integral field spectroscopic…

astro-ph.GA2014★ 207 cited

Stellar Population gradients in galaxy discs from the CALIFA survey

P. Sanchez-Blazquez, F. Rosales-Ortega, J. Mendez-Abreu +27

While studies of gas-phase metallicity gradients in disc galaxies are common, very little has been done in the acquisition of stellar abundance gradients in the same regions. We pr…