collaborators

8 papers

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 +18

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.EP2026

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

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.GA2025

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…