activity
20242026
collaborators

5 papers

astro-ph.GA2026

The Metallicity Gradient of Sagittarius Dwarf Spheroidal Galaxy Prior to Infall Constrained by S-PLUS Observations of its Tidal Stream

Felipe Almeida-Fernandes, Guilherme Limberg, Hélio D. Perottoni +16

We study the metallicity distribution along the Sagittarius (Sgr) stream using photometric metallicities from S-PLUS DR4, combined with Gaia DR3 kinematics and APOGEE DR17 spectros…

astro-ph.GA2025

The Universality of Dark Matter Density Profiles for Milky Way Analog Galaxies

Maria Clara Cavalcante-Siviero, K. Menéndez-Delmestre, P. P. B. Beaklini +4

The structure, extent, and mass of the Milky Way's (MW) dark matter (DM) halo are observationally challenging to determine due to our position within the Galaxy. To overcome this l…

astro-ph.GA2025

Identifying a protocluster formation at z 4.5 in the COSMOS field: an extension of Taralay protocluster, traced by Ly-alpha emitters surrounding a submm galaxy

Mariana Rubet, Karín Menéndez-Delmestre, Thiago Signorini Gonçalves +4

We report the discovery of a large-scale structure containing multiple overdensities at in the COSMOS field, with the most prominent one likely infalling towards…

astro-ph.GA2025

The S-PLUS Fornax Project (S+FP): Mapping globular clusters systems within 5 virial radii around NGC 1399

Luis Lomelí-Núñez, A. Cortesi, A. V. Smith Castelli +25

We present the largest sample (13,000 candidates, 3000 of wich are bona-fide candidates) of globular cluster (GCs) candidates reported in the Fornax Cluster so far. The…

astro-ph.GA2024

On the Stellar Disk Vertical Scale Height of Edge-on Galaxies from SG

Notahiana Ranaivoharimina, Toky H. Randriamampandry, Jing Wang +2

Disk galaxies viewed as thin planar structures resulting from the conservation of angular momentum of an initially rotating pre-galactic cloud allow merely a first-order model of g…