most citedObservational biases on rotation curves from IFU data at cosmic noon

2 citations · 3 across the 5 of their papers we have counts for

collaborators

5 papers

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★ 2 cited

Observational biases on rotation curves from IFU data at cosmic noon

Amanda E. de Araujo-Carvalho, Thiago S. Gonçalves, Davor Krajnović +2

Through studying rotation curves, which depict how the velocity of the stars and gas changes with distance from the center of the galaxy, it has been confirmed that dark matter dom…

astro-ph.GA2025★ 1 cited

Bar properties as a function of wavelength in TNG50: analysis of mock images

Gustavo F. Gonçalves, Rubens E. G. Machado, Karín Menéndez-Delmestre +1

Recent studies used TNG50 galaxies to study bar formation, evolution, and properties like length, strength, and pattern speed. In simulations, these are typically derived from part…

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

The S-PLUS Fornax Project (S+FP): A first 12-band glimpse of the Fornax galaxy cluster

A. V. Smith Castelli, A. Cortesi, R. F. Haack +40

The Fornax galaxy cluster is the richest nearby (D ~ 20 Mpc) galaxy association in the southern sky. As such, it provides a wealth of oportunities to elucidate on the processes whe…