TY - JOUR
T1 - CAVITY
T2 - Calar Alto Void Integral-field Treasury surveY: I. First public data release
AU - García-Benito, Rubén
AU - Jiménez, Andoni
AU - Sánchez-Menguiano, Laura
AU - Ruiz-Lara, Tomás
AU - Duarte Puertas, Salvador
AU - Domínguez-Gómez, Jesús
AU - Bidaran, Bahar
AU - Torres-Ríos, Gloria
AU - Argudo-Fernández, María
AU - Espada, Daniel
AU - Pérez, Isabel
AU - Verley, Simon
AU - Conrado, Ana M.
AU - Florido, Estrella
AU - Rodríguez, Mónica I.
AU - Zurita, Almudena
AU - Alcázar-Laynez, Manuel
AU - De Daniloff, Simon B.
AU - Lisenfeld, Ute
AU - Van De Weygaert, Rien
AU - Courtois, Hélène M.
AU - Falcón-Barroso, Jesús
AU - Ferré-Mateu, Anna
AU - Galbany, Lluís
AU - González Delgado, Rosa M.
AU - Del Moral-Castro, Ignacio
AU - Peletier, Reynier F.
AU - Román, Javier
AU - Sánchez, Sebastián F.
AU - Sánchez-Alarcón, Pablo M.
AU - Sánchez-Blázquez, Patricia
AU - Villalba-González, Pedro
AU - Azzaro, Marco
AU - Blazek, Martín
AU - Fernández, Alba
AU - Gallego, Julia
AU - Góngora, Samuel
AU - Guijarro, Ana
AU - De Guindos, Enrique
AU - Hermelo, Israel
AU - Hernández, Ricardo
AU - De Juan, Enrique
AU - Vico Linares, José Ignacio
N1 - Publisher Copyright:
© The Authors 2024.
PY - 2024/11
Y1 - 2024/11
N2 - 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.
AB - 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.
KW - Galaxies: evolution
KW - Galaxies: general
KW - Surveys
KW - Techniques: imaging spectroscopy
KW - Techniques: spectroscopic
UR - http://www.scopus.com/inward/record.url?scp=85209250156&partnerID=8YFLogxK
U2 - 10.1051/0004-6361/202451400
DO - 10.1051/0004-6361/202451400
M3 - Article
AN - SCOPUS:85209250156
SN - 0004-6361
VL - 691
JO - Astronomy & Astrophysics
JF - Astronomy & Astrophysics
M1 - A161
ER -