CAVITY: Calar Alto Void Integral-field Treasury surveY

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 regions of the cosmic web, located in the Local Universe. This paper describes the first public data release (DR1) of CAVITY, comprising science-grade optical data cubes for the initial 100 out of a total of ~300 galaxies in the Local Universe (0.005 < z < 0.050). These data were acquired using the integral-field spectrograph PMAS/PPak mounted on the 3.5m telescope at the Calar Alto observatory. The DR1 galaxy sample encompasses diverse characteristics in the color-magnitude space, morphological type, stellar mass, and gas ionisation conditions, providing a rich resource for addressing key questions in galaxy evolution through spatially resolved spectroscopy. The galaxies in this study were observed with the low-resolution V500 set-up, spanning the wavelength range 3745-7500 Å, with a spectral resolution of 6.0 Å (FWHM). Here, we describe the data reduction and characteristics and data structure of the CAVITY datasets essential for their scientific utilisation, highlighting such concerns as vignetting effects, as well as the identification of bad pixels and management of spatially correlated noise. We also provide instructions for accessing the CAVITY datasets and associated ancillary data through the project’s dedicated database.

Authors

Publication Details

Journal
Astronomy and Astrophysics
Published
2024-10-09
DOI
https://doi.org/10.1051/0004-6361/202451400
Citations
4
Primary Topic
Galaxies: Formation, Evolution, Phenomena
Type
article
Field-Weighted Citation Impact
1.33
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article

CAVITY: Calar Alto Void Integral-field Treasury surveY

Alba Fernández, M. Błażek, L. Sánchez-Menguiano, P. M. Sánchez-Alarcón et al.
4 citations
Astronomy and Astrophysics
Galaxies: Formation, Evolution, Phenomena
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article

CAVITY: Calar Alto Void Integral-field Treasury surveY

Alba Fernández, M. Błażek, L. Sánchez-Menguiano, P. M. Sánchez-Alarcón, L. Galbany, Ignacio del Moral-Castro, S. Góngora, A. Conrado, A. Guijarro, J. Falcón‐Barroso, Isabel Pérez, M. Rodríguez, R. F. Peletier, Jesús Domínguez-Gómez, Javier Román, E. de Guindos, E. Florido, S. Verley, M. Argudo–Fernández, D. Espada, P. Sánchez–Blázquez, S. Duarte Puertas, M. Azzaro, Bahar Bidaran, R. García-Benito, I. Hermelo, E. de Juan, José Ignacio Linares, Anna Ferré-Mateu, A. Zurita, R. M. González Delgado, U. Lisenfeld, Julia Gallego, Rien van de Weygaert, T. Ruiz-Lara, S. F. Sánchez, H. M. Courtois, Manuel Alcázar-Laynez, P. Villalba-González, G. Torres-Ríos, Simon B. De Daniloff, Andoni Jiménez, Ricardo Robledo Hernández
article en
4 citations

Abstract

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 regions of the cosmic web, located in the Local Universe. This paper describes the first public data release (DR1) of CAVITY, comprising science-grade optical data cubes for the initial 100 out of a total of ~300 galaxies in the Local Universe (0.005 < z < 0.050). These data were acquired using the integral-field spectrograph PMAS/PPak mounted on the 3.5m telescope at the Calar Alto observatory. The DR1 galaxy sample encompasses diverse characteristics in the color-magnitude space, morphological type, stellar mass, and gas ionisation conditions, providing a rich resource for addressing key questions in galaxy evolution through spatially resolved spectroscopy. The galaxies in this study were observed with the low-resolution V500 set-up, spanning the wavelength range 3745-7500 Å, with a spectral resolution of 6.0 Å (FWHM). Here, we describe the data reduction and characteristics and data structure of the CAVITY datasets essential for their scientific utilisation, highlighting such concerns as vignetting effects, as well as the identification of bad pixels and management of spatially correlated noise. We also provide instructions for accessing the CAVITY datasets and associated ancillary data through the project’s dedicated database.

Astronomy and AstrophysicsVol. 691
Openalex Percentile: Top 19%
Galaxies: Formation, Evolution, Phenomena
1.33
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