activity
20232026
most citedExploring the nature of dark matter with the extreme galaxy AGC 114905

28 citations · 54 across the 15 of their papers we have counts for

collaborators

16 papers

astro-ph.GA2026

LIGHTS. Limitations of Far-Infrared Tracers for Galactic Cirrus Mitigation in the Era of Ultra-Deep Imaging

Ouldouz Kaboud, Ignacio Trujillo, Ignacio Ruiz Cejudo +18

Current and forthcoming deep optical imaging surveys are reaching surface brightness levels fainter than 30 mag/arcsec, where Galactic cirrus emission becomes a significant con…

astro-ph.GA2026

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy

Carlos Marrero-de la Rosa, Ignacio Trujillo, Ignacio Ruiz Cejudo +12

The maximum physical extent that galaxies can reach is poorly understood. In this regard, IC 1101, one of the most extended and massive galaxies known, provides a valuable opportun…

astro-ph.GA2026

Witnessing the rapid growth of disk galaxies over cosmic time using JWST and HST

Samane Raji, Mireia Montes, Ignacio Trujillo +3

Measuring galaxy sizes is fundamental to understanding how galaxies grow and evolve. Traditional methods to measure sizes either trace the concentration of light (i.e., effective r…

astro-ph.GA2026

JWST spectra are consistent with the edge-on star-forming galaxy scenario for the "runaway supermassive black hole"

Jorge Sanchez Almeida, Ignacio Trujillo, Sebastian F. Sanchez +1

The linear structure reported by van Dokkum et al. (2023) has been proposed as either a massive stellar wake produced by a runaway supermassive black hole (SMBH) or a bulgeless edg…

astro-ph.GA2025★ 7 cited

LIGHTS. A robust technique to identify galaxy edges

Giulia Golini, Ignacio Trujillo, Dennis Zaritsky +19

The LIGHTS survey is imaging galaxies at a depth and spatial resolution comparable to what the Legacy Survey of Space and Time (LSST) will produce in 10 years (i.e., 31 mag/a…

astro-ph.EP2025

A targeted, parallax-based search for Planet Nine

Hector Socas-Navarro, Ignacio Trujillo

The hypothesized Planet Nine is thought to reside in the distant outer solar system, potentially explaining various anomalies in the orbits of extreme trans-Neptunian objects (ETNO…

astro-ph.GA2025★ 3 cited

UV LIGHTS. New tools for revealing the low surface brightness regime in the ultraviolet

Ignacio Ruiz Cejudo, Ignacio Trujillo, Giulia Golini +16

Ultra-deep optical surveys have reached unprecedented depths, facilitating the study of faint galactic structures. However, the ultraviolet bands, crucial for stellar population st…

astro-ph.GA2025★ 1 cited

Constraining the shape of dark matter haloes using only starlight. I. A new technique and its application to the galaxy Nube

Jorge Sanchez Almeida, Ignacio Trujillo, Mireia Montes +1

We present a new technique to constrain the gravitational potential of a galaxy from the observed stellar mass surface density alone under a number of assumptions. It uses the clas…

astro-ph.GA2024★ 2 cited

LIGHTS. The extended point spread functions of the LIGHTS survey at the LBT

Nafise Sedighi, Zahra Sharbaf, Ignacio Trujillo +13

With the arrival of the next generation of ultra-deep optical imaging surveys reaching 30 mag/arcsec (3; 10"10"), the removal of scattered light due to th…

astro-ph.GA2024

The stellar distribution in ultra-faint dwarf galaxies suggests deviations from the collision-less cold dark matter paradigm

Jorge Sanchez Almeida, Ignacio Trujillo, Angel R. Plastino

Unraveling the nature of dark matter (DM) stands as a primary objective in modern physics. Here we present evidence suggesting deviations from the collisionless Cold DM (CDM) parad…

astro-ph.GA2024★ 4 cited

Application of the Eddington inversion method to constrain the dark matter halo of galaxies using only observed surface brightness profiles

Jorge Sanchez Almeida, Angel R. Plastino, Ignacio Trujillo

*** Context: The halos of low-mass galaxies may allow us to constrain the nature of dark matter (DM), but the kinematic measurements to diagnose the required properties are technic…

astro-ph.GA2024★ 1 cited

LIGHTS. Survey Overview and a Search for Low Surface Brightness Satellite Galaxies

Dennis Zaritsky, Giulia Golini, Richard Donnerstein +12

We present an overview of the LIGHTS (LBT Imaging of Galactic Halos and Tidal Structures) survey, which currently includes 25 nearby galaxies that are on average 1 mag faint…

astro-ph.GA2024

Deep HST imaging favors the bulgeless edge-on galaxy explanation for the hypothetical stellar wake created by a runaway supermassive black hole

Mireia Montes, Jorge Sánchez Almeida, Ignacio Trujillo

A long linear structure recently discovered could be the stellar wake produced by the passage of a runaway supermassive black hole (SMBH) or, alternatively, a bulgeless edge-on gal…

astro-ph.GA2024★ 28 cited

Exploring the nature of dark matter with the extreme galaxy AGC 114905

Pavel E. Mancera Piña, Giulia Golini, Ignacio Trujillo +1

AGC 114905 is a dwarf gas-rich ultra-diffuse galaxy seemingly in tension with the cold dark matter (CDM) model. Specifically, the galaxy appears to have an extremely low-density ha…

astro-ph.GA2023

Can cuspy dark matter dominated halos hold cored stellar mass distributions?

Jorge Sanchez Almeida, Angel R. Plastino, Ignacio Trujillo

According to the current concordance cosmological model, the dark matter (DM) particles are collision-less and produce self-gravitating structures with a central cusp which, genera…

astro-ph.GA2023★ 8 cited

Super-massive black hole wake or bulgeless edge-on galaxy?

Jorge Sanchez Almeida, Mireia Montes, Ignacio Trujillo

van Dokkum et al. (2023) reported the serendipitous discovery of a thin linear object interpreted as the trail of star-forming regions left behind by a runaway supermassive black h…