95 citations · 608 across the 16 of their papers we have counts for
16 papers
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 PAU Survey: Classifying low-z SEDs using Machine Learning clustering
A. L. González-Morán, P. Arrabal Haro, C. Muñóz-Tuñón +15
We present an application of unsupervised Machine Learning Clustering to the PAU Survey of galaxy spectral energy distribution (SED) within the COSMOS field. The clustering algorit…
Hubble Space Telescope Observations of Tadpole Galaxies Kiso 3867, SBS0, SBS1, and UM461
Debra Meloy Elmegreen, Bruce G. Elmegreen, John S. Gallagher +8
Tadpole galaxies are metal-poor dwarfs with typically one dominant star-forming region, giving them a head-tail structure when inclined. A metallicity drop in the head suggests tha…
Extremely Metal-Poor Galaxies: The Environment
M. E. Filho, J. Sánchez Almeida, C. Muñoz-Tuñón +3
We have analyzed bibliographical observational data and theoretical predictions, in order to probe the environment in which extremely metal-poor dwarf galaxies (XMPs) reside. We ha…
Extremely Metal-Poor Galaxies: The HI Content
M. E. Filho, B. Winkel, Sánchez Almeida +12
Extremely metal-poor (XMP) galaxies are chemically, and possibly dynamically, primordial objects in the local Universe. Our objective is to characterize the HI content of the XMP g…
The dependence of the Lyman_a luminosity function on Redshift using SHARDS
J. M. Rodriguez-Espinosa, O. Gonzalez-Martin, J. A. Lopez-Aguerri +3
We report in this work on a project aimed at determining Lyα luminosity functions from z=3 to z=6. The project is based on the use of very deep photometry from the SHARDS Survey, i…