Tomás
Ahumada

Presidential Postdoctoral Fellow at the California Institute of Technology.

Last updated
November 5, 2022

Welcome!

The one in the picture is me! I am Tomás Ahumada, a Chilean astronomer searching for optical counterparts to short gamma-ray bursts and gravitational waves. I am currently a Presidential Postdoctoral Fellow at the California Institute of Technology (Caltech), where I am working with Prof. Mansi Kasliwal studying fast evolving transients. I received my PhD in 2022 from the University of Maryland (UMD), where I conducted my research under the supervision of Dr. Leo Singer from NASA Goddard Space Flight Center (GSFC). There, I used the Zwicky Transient Facility (ZTF) to cover large portions of the sky and maximize the probability to find interesting explosions in the northern nightsky, and I used a variety of telescopes across the electromagnetic spectrum to monitor and characterize the newly discover objects assosciated to our searches.
Prior to that, I obtained my undergraduate degree in 2016 from the P. Universidad Católica de Chile where I majored in Astronomy. While there, I worked with both Prof. Felipe Barrientos and Prof. Karim Pichara on using machine learning algorithms to find quasars in the ATLAS survey.
During the southern hemisphere summer in 2016, I was part of the Cerro Tololo (CTIO) Reaserch Experience for Undergraduates and worked with Dr. Bryan Miller (from Gemini Observatory) on identifying globular clusters of the shell-elliptical galaxy NGC3923. After my graduation I interned at Gemini and further analyzed the morphology of the galaxy.

July 26, 2021

GRB200826A

I led the paper on the shortest gamma-ray burst (GRB) powered by a collapsar published in Nature Astronomy. For this discovery, we triggered the Zwicky Transient Facility on a Fermi short GRB and after detecting the afterglow, it was clear that the characteristics of this burst were non-typical for a short GRB. We were granted Director's Discretionary Time at the Gemini telescope and we discovered a rising source that could only be explained by a underlying supernova. Image: NASA

January 10, 2021

GRADMAP Winter workshop

I got to mentor two fantastic undergraduates during the winter of 2021. Along with Lenin Nolasco (CUNY, NY) and Maria Clara Heringer (UFRJ, Brasil), we worked on supernova light-curve modeling and covered the basics of Python.

September 14, 2020

S200105ae and S200115j

We followed-up the neutron star - black hole mergers detected during the third observing run of LIGO/Virgo. Shreya anand and Michael Coughlin were the corresponding authors of this work. Image: Francois Foucart, University of New Hampshire