-
2 strongly lensed galaxies MUSE & ALMA datacubes
We compare the molecular and ionized gas kinematics of two strongly lensed galaxies at z~1 that lie on the main sequence at this redshift, based on observations from ALMA and... -
OTELO survey catalog
The evolution of galaxies through cosmic time is studied observationally by means of extragalactic surveys. The usefulness of these surveys is greatly improved by increasing the... -
Close pairs of galaxies in MUSE Deep Fields
Using the ILLUSTRIS cosmological simulation project, we investigate the relation between the separation of galaxies in a pair, both in velocity and projected spatial separation... -
HRS galaxies Halpha kinematic survey
We present new 2D high resolution Fabry-Perot spectroscopic observations of 152 star-forming galaxies which are part of the Herschel Reference Survey (HRS), a complete K-band... -
Cosmic Horseshoe (J1148+1930) Ha and OIII spectra
We present a detailed analysis of the inner mass structure of the Cosmic Horseshoe (J1148+1930) strong gravitational lens system observed with the Hubble Space Telescope (HST)... -
SPT-S J041839-4751.8 APEX spectra
We present a study of six far-infrared fine structure lines in the z=4.225 lensed dusty star-forming galaxy SPT 0418-47 (SPT-S J041839-4751.8) to probe the physical conditions... -
Stellar populations of quiescent galaxies
Our aim is to determine the distribution of stellar population parameters (extinction, age, metallicity, and star formation rates) of quiescent galaxies within the rest-frame... -
Tucana dSph CMD and star formation history
We report a new star formation history for the Tucana dwarf spheroidal galaxy, obtained from a new look at a deep HST/ACS colour-magnitude diagram. We combined information from... -
B2 0258+35 VLA and VLBI HI absorption spectra
Low-luminosity radio-loud active galactic nuclei (AGN) are of importance in studies concerning feedback from radio AGN since a dominant fraction of AGN belong to this class. We... -
Supernova ASASSN-14jb light curves and spectra
We present optical photometry and spectroscopy of the Type II supernova ASASSN-14jb, together with very large telescope (VLT) multi unit spectroscopic explorer (MUSE) integral... -
NGC1326A, 1425 and 4548 supergiants VI mags
Studies on the massive star population in galaxies beyond the Local Group are the key to understand the link between their numbers and modes of star formation in different... -
Radiative contribution from stripped stars
Stars stripped of their envelopes from interaction with a binary companion emit a significant fraction of their radiation as ionizing photons. They are potentially important... -
Mapping the stellar age of the Milky Way
The bulge represents the best compromise between old and massive Galactic component, and as such its study is a valuable opportunity to understand how the bulk of the Milky Way... -
CO spectra of 55 LIRGs and ULIRGs
We present IRAM-30m Telescope ^12^CO and ^13^CO observations of a sample of 55 luminous and ultraluminous infrared galaxies (LIRGs and ULIRGs) in the local universe. This sample... -
Star cluster formation in a tidal debris
The formation of globular clusters remains an open debate. Dwarf starburst galaxies are efficient at forming young massive clusters with similar masses as globular clusters and... -
SPT0346-52 CO and H2O ALMA images
We present and study spatially resolved imaging obtained with the Atacama Large Millimeter/submillimeter Array (ALMA) of multiple ^12^CO(J=6-5, 8-7 and 9-8) and two... -
[ESS2003] Q2343-BX610 reduced PdBI spectra
We have used the Plateau De Bure Interferometer to observe multiple CO and neutral carbon transitions in a z=2.2 main sequence disk galaxy, BX610. Our observation of CO(7-6),... -
Statistical HATLAS Lensed Objects Selec.
The statistical analysis of large sample of strong lensing events can be a powerful tool to extract astrophysical or cosmological valuable information. Their selection using... -
Cosmology from galaxy lensing and clustering
The combination of Galaxy-Galaxy Lensing (GGL) and Redshift Space Distortion of galaxy clustering (RSD) is a privileged technique to test General Relativity predictions, and... -
GAS II. UV luminosity functions & InfraRed eXcess
Dust is a crucial component of the interstellar medium of galaxies. The presence of dust strongly affects the light produced by stars within a galaxy. As these photons are our...