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Veselina Kalinova

Researcher at Max Planck Society

Publications -  28
Citations -  2632

Veselina Kalinova is an academic researcher from Max Planck Society. The author has contributed to research in topics: Galaxy & Galaxy formation and evolution. The author has an hindex of 16, co-authored 26 publications receiving 2177 citations. Previous affiliations of Veselina Kalinova include University of Alberta.

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CALIFA, the Calar Alto Legacy Integral Field Area survey : I. Survey presentation

Sebastián F. Sánchez, +84 more
TL;DR: The Calar Alto Legacy Integral Field Area (CALIFA) survey as discussed by the authors was designed to provide a first step in this direction by obtaining spatially resolved spectroscopic information of a diameter selected sample of similar to 600 galaxies in the Local Universe.
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CALIFA : a diameter-selected sample for an integral field spectroscopy galaxy survey

C. J. Walcher, +60 more
TL;DR: In this paper, the authors describe the selection procedure and statistical properties of the galaxy sample used by the Calar Alto Legacy Integral Field Area (CALIFA) survey, a public legacy survey of 600 galaxies using integral field spectroscopy.
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The CALIFA survey across the Hubble sequence: Spatially resolved stellar population properties in galaxies

TL;DR: In this article, the authors apply the fossil record method based on spectral synthesis techniques to recover the following physical properties for each spatial resolution element in the target galaxies: the stellar mass surface density (μ_*), stellar extinction (A_V), lightweighted and mass-weighted ages (L, M), and mass weighted metallicity (M).
Journal ArticleDOI

CALIFA, the Calar Alto Legacy Integral Field Area survey: I. Survey presentation

Sebastián F. Sánchez, +84 more
TL;DR: The Calar Alto Legacy Integral Field Area (CALIFA) survey as mentioned in this paper was designed to provide a first step in this direction, obtaining spatially resolved spectroscopic information of a diameter selected sample of galaxies in the Local Universe (0.005 < z < 0.03).