48 citations · 95 across the 10 of their papers we have counts for
11 papers
More fundamental than the fundamental metallicity relation: The effect of the stellar metallicity on the gas-phase mass-metallicity and gravitational potential-metallicity relations
Laura Sánchez-Menguiano, Sebastián F. Sánchez, Jorge Sánchez Almeida +1
Context. One of the most fundamental scaling relations in galaxies is observed between metallicity and stellar mass -- the mass-metallicity relation (MZR) -- although recently a st…
HII regions and diffuse ionized gas in the AMUSING++ Compilation: I. Catalogue presentation
A. Z. Lugo-Aranda, S. F. Sánchez, J. K. Barrera-Ballesteros +4
We present a catalog of 52,000 extragalactic HII regions and their spectroscopic properties obtained using Integral Field Spectroscopy (IFS) from MUSE observations. The sampl…
The EDGE-CALIFA Survey: An Extragalactic Database for Galaxy Evolution Studies
Tony Wong, Yixian Cao, Yufeng Luo +22
The EDGE-CALIFA survey provides spatially resolved optical integral field unit (IFU) and CO spectroscopy for 125 galaxies selected from the CALIFA Data Release 3 sample. The Extrag…
Unveiling a hidden bar-like structure in NGC1087: kinematic and photometric evidence using MUSE/VLT, ALMA and JWST
Carlos López-Cobá, Lihwai Lin, Sebastián F. Sánchez
We report a faint non-axisymmetric structure in NGC\,1087 through the use of JWST Near Infrared Camera { (NIRCam)}, with an associated kinematic counterpart observed as an oval dis…
Stellar mass is not the best predictor of galaxy metallicity. The gravitational potential-metallicity relation
Laura Sánchez-Menguiano, Jorge Sánchez Almeida, Sebastián F. Sánchez +1
Interpreting the scaling relations followed by galaxies is a fundamental tool for assessing how well we understand galaxy formation and evolution. Several scaling relations involvi…
The WHaD diagram: Classifying the ionizing source with one single emission line
S. F. Sánchez, A. Z. Lugo-Aranda, J. Sánchez Almeida +4
The usual approach to classify the ionizing source using optical spectroscopy is based on the use of diagnostic diagrams that compares the relative strength of pairs of collisition…
Bidimensional Exploration of the warm-Temperature Ionised gaS (BETIS) I. Showcase sample and first results
R. González-Díaz, F. F. Rosales-Ortega, L. Galbany +6
We present the Bidimensional Exploration of the warm-Temperature Ionised gaS (BETIS) project, designed for the spatial and spectral study of the diffuse ionised gas (DIG) in a sele…
Recovering lost light: discovery of supernova remnants with integral field spectroscopy
Héctor Martínez-Rodríguez, Lluís Galbany, Carles Badenes +8
We present results from a systematic search for broad ( 400 \kms) \ha\ emission in Integral Field Spectroscopy data cubes of 1200 nearby galaxies obtained with PMAS and…
EDGE-CALIFA survey: Self-regulation of Star formation at kpc scales
J. K. Barrera-Ballesteros, S. F. Sánchez, T. Heckman +11
We present the relation between the star formation rate surface density, , and the hydrostatic mid-plane pressure, P, for 4260 star-forming regions of kpc si…
2D-Galactic chemical evolution: the role of the spiral density wave
Mercedes Mollá, Sheillah Wekesa, Oscar Cavichia +6
We present a 2-dimensional chemical evolution code applied to a Milky Way type galaxy, incorporating the role of spiral arms in shaping azimuthal abundance variations, and confront…
The SELGIFS data challenge: generating synthetic observations of CALIFA galaxies from hydrodynamical simulations
Giovanni Guidi, Javier Casado, Yago Ascasibar +6
In this work we present a set of synthetic observations that mimic the properties of the Integral Field Spectroscopy (IFS) survey CALIFA, generated using radiative transfer techniq…