activity
20002026
most citedCALIFA, the Calar Alto Legacy Integral Field Area survey: I. Survey presentation

1.3k citations · 6.3k across the 97 of their papers we have counts for

collaborators

97 papers

astro-ph.GA2026

J-PLUS: Spectral classification and photometric redshifts for 79 million sources in the fourth data release

A. Hernán-Caballero, H. Vázquez Ramió, C. López-Sanjuan +20

We present spectral classifications and photometric redshifts for 79.2 million sources up to an r-band magnitude of 22 in Data Release 4 of the Javalambre Photometric Local Univers…

astro-ph.SR2026

WEAVE imaging spectroscopy of NGC 6720: an iron bar in the Ring

R. Wesson, J. E. Drew, M. J. Barlow +23

We present spatially resolved spectroscopic observations of the planetary nebula NGC 6720, the Ring Nebula, taken during the science verification phase of WEAVE, a new instrument m…

astro-ph.GA2025

Fossil group origins XIV: The radial orbits of A267

S. Zarattini, A. Biviano, I. Bartalucci +3

Fossil groups (FGs) are groups or clusters of galaxies with a single, massive, central galaxy and with a clear lack of L* galaxies. The physical reason for their large magnitude ga…

astro-ph.GA2025★ 1 cited

The Tremaine-Weinberg method at high redshifts

Mahmood Roshan, Asiyeh Habibi, J. Alfonso L. Aguerri +11

This paper examines the reliability of the Tremaine-Weinberg (TW) method in measuring the pattern speed of barred galaxies at high redshifts. Measuring pattern speeds at high redsh…

astro-ph.GA2024★ 6 cited

The redshift evolution of galactic bar pattern speed in TNG50

Asiyeh Habibi, Mahmood Roshan, Mohammad Hosseinirad +4

In this paper, the redshift evolution of the galactic bar properties, like the bar length, pattern speed, and bar fraction, has been investigated for simulated galaxies at stellar…

astro-ph.GA2024★ 6 cited

Are early-type galaxies quenched by present-day environment? A study of dwarfs in the Fornax Cluster

Romero-Gómez, J., Reynier F. Peletier +2

Galaxies undergo processes throughout their lifetimes that ultimately lead to the expulsion of the gas and the cessation of the star-forming activity. This phenomenon commonly know…