Dr. Vicente Estrada-Carpenter

Beus Prize Postdoctoral Fellow

Arizona State University, Tempe, AZ

My main areas of interest are galaxy evolution, galaxy assembly, stellar populations, spatially resolved stellar populations, and spectral analysis.

Grism Data

I work with JWST/NIRISS grism data, mainly from the CANUCS survey.

Forward Modelling

To deal with the systematics of grism data I use a forward modeling technique.

Stellar Populations

I derive metallicities, ages, and other stellar population parameters.

Formation Histories

I constrain (non-parametric) star-formation histories for massive quiescent and star-forming galaxies.

Curriculum Vitae

Labors of Lab

Science

Science

Estrada-Carpenter et al. 2019

CLEAR. I. Ages and Metallicities of Quiescent Galaxies at 1.0 < z < 1.8 Derived from Deep Hubble Space Telescope Grism Data

Using a forward modeling technique, we fit the stellar populations of a sample of 31 massive quiescent galaxies in the CLEAR survey, in a redshift range of 1 < z < 1.8. Our measurements indicate that massive quiescent galaxies in this redshift range have ~ solar stellar metallicities. Thus, there is no evolution in the stellar metallicity - mass relation, up to a redshift of z ~ 1.8. We also show that many of these galaxies had formed ~70% of their stellar mass by z ~ 2-3.

Estrada-Carpenter et al. 2020

CLEAR II: Evidence for Early Formation of the Most Compact Quiescent Galaxies at High Redshift

Combining photometric, G102 grism, and G141 grism data, we constrain the stellar populations and derive "non-parametric" star-formation histories for a sample of 97 massive quiescent galaxies in the CLEAR survey, in a redshift range of 0.8 < z < 2.5. By comparing formation redshifts (where the galaxy formed half its mass) to stellar surface mass densities within 1 kiloparsec we see that the most compact galaxies are biased to form early (z>2.5), while less compact galaxies show a wide range of formation redshifts. Our results favor a scenario where compact galaxies formed rapidly at high redshift, then go through subsequent evolution through minor mergers.

Outreach

I enjoy speaking with the public and have given several talks at Astronomy on Tap BCS.

I work with undergraduate students at Texas A&M. These research projects include creating an interactive website for the CLEAR collaboration, color gradients of quiescent galaxies, H-alpha maps of interacting galaxies, simulated JWST NIRCAM Paschen-alpha map for CEERS.

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Contact

Contact

Address

School of Earth and Space Exploration
ISTB4 497
Arizona State University, Tempe, AZ, 85287

Email

vestrad9@asu.edu