activity
20172022
most citedSDSS-IV MaNGA: Effects of Morphology in the global and local Star Formation Main Sequences

106 citations · 252 across the 11 of their papers we have counts for

collaborators

24 papers

astro-ph.GA202253 cited

SDSS IV MaNGA: Visual Morphological and Statistical Characterization of the DR15 sample

J. A. Vázquez-Mata, H. M. Hernández-Toledo, V. Avila-Reese +6

We present a detailed visual morphological classification for the 4614 MaNGA galaxies in SDSS Data Release 15, using image mosaics generated from a combination of r-band (SDSS and…

astro-ph.CO20223 cited

Galaxy Correlation Function and Local Density from Photometric Redshifts Using the Stochastic Order Redshift Technique (SORT)

James Kakos, Joel R. Primack, Aldo Rodriguez-Puebla +3

The stochastic order redshift technique (SORT) is a simple, efficient, and robust method to improve cosmological redshift measurements. The method relies upon having a small ($\sim…

astro-ph.GA202118 cited

The galaxy HI-(sub)halo connection and the HI spatial clustering of local galaxies

A. R. Calette, Aldo Rodríguez-Puebla, Vladimir Avila-Reese +1

We extend the local stellar galaxy-(sub)halo connection to the atomic hydrogen (HI) component by seeding semi-empirically galaxies into a large N-body dark matter (DM) simulation.…

astro-ph.GA20217 cited

The HI and stellar mass bivariate distribution of centrals and satellites for all, late- and early-type local galaxies

A. R. Calette, Vladimir Avila-Reese, Aldo Rodríguez-Puebla +2

We characterize the conditional distributions of the HI gas-to-stellar mass ratio, , given the stellar mass, , of local galaxies from $M_{\a…

astro-ph.GA202117 cited

The evolution of compact massive quiescent and starforming galaxies derived from the and relations

L. Zanisi, F. Shankar, H. Fu +12

The mean size ( effective radius ) of Massive Galaxies (MGs, ) is observed to increase steadily with cosmic time. It is still unclear whether th…

astro-ph.GA2020

The star-forming main sequence and the contribution of dust-obscured star formation since from the FUV+IR luminosity functions

Aldo Rodriguez-Puebla, Vladimir Avila-Reese, Mariana Cano-Diaz +5

An analytical approach is proposed to study the evolution of the star-forming galaxy (SFG) main sequence (MS) and the fraction of dust-obscured SF up to . Far-ultraviolet (…