activity
20122026
most citedThe Galaxy-Halo Connection Over The Last 13.3 Gyrs

245 citations · 2.2k across the 55 of their papers we have counts for

collaborators

55 papers

astro-ph.GA2026

Tracing luminous infrared galaxy populations through cluster evolution in a cosmological mock redshift survey

Norma Araceli Nava-Moreno, Alfredo Montaña, Itziar Aretxaga +2

We present GARDENS-Wide, a new 100 square degree mock redshift survey of the dusty star-forming galaxy population based on the MultiDark-Planck 2 dark-matter halo simulation. The m…

astro-ph.GA2026

Asymmetries in spatially unresolved 21-cm emission line profiles of isolated galaxies

Aditya Manuwal, H. M. Hernández-Toledo, J. A. Vázquez-Mata +4

The origin of asymmetry in the of galaxies remains an elusive problem, largely due to the difficulties associated with distinguishing between its se…

astro-ph.GA2026

Empirical estimates of how massive galaxies can be in ΛCDM

Miguel Enríquez-Vargas, Aldo Rodríguez-Puebla, Aditya Manuwal +3

Using Extreme Value Statistics applied to the observed galaxy stellar mass and the UV luminosity functions, we empirically estimate masses and luminosities of the most extreme gala…

astro-ph.GA2025

Visual morphological classification of the full MaNGA DR17 sample: a general characterization

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

We present the MaNGA Visual Morphology (MVM) catalogue, featuring a visual morphological classification of 10,059 galaxies in the final MaNGA sample. By combining SDSS and DESI Leg…

astro-ph.GA2025

Pressure Regulated Formation of Molecular Clouds and Stars: The case of the Milky Way

José Franco, Aldo Rodríguez-Puebla, Javier Ballesteros-Paredes +1

We present a steady-state analytical model for pressure-regulated formation of molecular clouds (MC) and stars (SF) in gaseous galactic disks and apply it to the Milky Way (MW). MC…

astro-ph.GA2025

The MaNGA Dwarf Galaxy Sample (MaNDala): stellar profiles and gradients characterization

M. Cano-DÍaz, A. Rodríguez-Puebla, A. C. Robleto-Orús +8

We derived radial profiles and inner/outer gradients of various stellar population (SP) properties for 124 bright dwarf galaxies, , from th…

astro-ph.GA2025

On matching galaxy number densities to reconstruct galaxy evolutionary tracks

Aldo Rodriguez-Puebla, Vladimir Avila-Reese, Joel R. Primack +1

The cumulative number density matching approach equates number densities between adjacent redshifts to derive empirical galaxy evolution tracks from the observed galaxy stellar mas…

astro-ph.GA2025★ 4 cited

Shedding light on the star formation rate-halo accretion rate connection and halo quenching mechanism via DECODE, the Discrete statistical sEmi-empiriCal mODEl

Hao Fu, Lumen Boco, Francesco Shankar +9

Aims: The relative roles of the physical mechanisms involved in quenching galaxy star formation are still unclear. We tackle this fundamental problem with our cosmological semi-emp…

astro-ph.GA2024★ 1 cited

The Co-Evolution Between Galaxies and Dark Matter Halos

Aldo Rodriguez-Puebla

The current cosmological paradigm asserts that dark matter halos provide the gravitational scaffolding for galaxy formation through a combination of hierarchical structure formatio…

astro-ph.GA2024

Non-Monotonic Relations of Galaxy Star Formation, Radius, and Structure at Fixed Stellar Mass

Jimena Stephenson, Aldo Rodriguez-Puebla, S. M. Faber +9

We investigate the relation between galaxy structure and star formation rate (SFR) in a sample of central galaxies with and axial ratios .…

astro-ph.GA2024★ 2 cited

A mock redshift catalogue of the dusty star-forming galaxy population with intrinsic clustering and lensing for deep millimetre surveys

Norma Araceli Nava-Moreno, Alfredo Montaña, Itziar Aretxaga +3

We present a new cosmologically motivated mock redshift survey of the Dusty Star-Forming Galaxy population. Our mock survey is based on the Bolshoi-Planck dark-matter halo simulati…

astro-ph.GA2024★ 6 cited

Star-forming and Quiescent Central Galaxies Cluster Similarly: Implications for the Galaxy-Halo Connection

James Kakos, Aldo Rodriguez-Puebla, Joel R. Primack +4

We measure the clustering of low-redshift SDSS galaxies as a function of stellar mass () and specific star formation rate (sSFR) and compare the result…

astro-ph.GA2023★ 14 cited

The evolution of radial gradients of MaNGA quiescent elliptical galaxies: inside-out quenching or outer mass growth?

V. Avila-Reese, H. Ibarra-Medel, I. Lacerna +5

Using spatially-resolved fossil record analysis on a large sample of 'red and dead' elliptical galaxies (classical ellipticals, CLEs) from the MaNGA/SDSS-IV DR15 survey, we reconst…

astro-ph.GA2023★ 43 cited

The growth of brightest cluster galaxies in the TNG300 simulation:dissecting the contributions from mergers and in situ star formation

Daniel Montenegro-Taborda, Vicente Rodriguez-Gomez, Annalisa Pillepich +4

We investigate the formation of brightest cluster galaxies (BCGs) in the TNG300 cosmological simulation of the IllustrisTNG project. Our cluster sample consists of 700 haloes with…

astro-ph.GA2022★ 12 cited

SDSS-IV MaNGA: The MaNGA Dwarf Galaxy Sample

M. Cano-Díaz, H. M. Hernández-Toledo, A. Rodríguez-Puebla +10

We present the MaNGA Dwarf galaxy, MaNDala, Value-Added-Catalog, VAC, from the final release of the Sloan Digital Sky Survey-IV program. MaNDala consists of 136 randomly selected b…

astro-ph.GA2022★ 141 cited

SDSS-IV MaNGA: pyPipe3D analysis release for 10,000 galaxies

S. F. Sánchez, J. K. Barrera-Ballesteros, E. Lacerda +12

We present here the analysis performed using the pyPipe3D pipeline for the final MaNGA dataset included in the SDSS seventeenth data-release. This dataset comprises more than 10,00…

astro-ph.GA2022★ 53 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.CO2022★ 3 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.GA2022★ 5 cited

The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar and APOGEE-2 Data

Abdurro'uf, Katherine Accetta, Conny Aerts +337

This paper documents the seventeenth data release (DR17) from the Sloan Digital Sky Surveys; the fifth and final release from the fourth phase (SDSS-IV). DR17 contains the complete…

astro-ph.GA2021★ 11 cited

The differences between mass- and light-derived structural parameters over time for MaNGA Elliptical galaxies

H. Ibarra-Medel, V. Avila-Reese, I. Lacerna +4

We apply stellar population synthesis analysis to obtain spatially-resolved archaeological inferences for a large sample of "red and dead" Elliptical galaxies (Classical Elliptical…

astro-ph.GA2021★ 18 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.GA2021★ 7 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.GA2021★ 17 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★ 9 cited

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 (…