Svea Hernández

Space Telescope Science Institute — United States

Physics and Astronomy · Physical Sciences

18h-index959citations105works5.82yr avg
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Research Topics

Stellar, planetary, and galactic studies(46), Astrophysics and Star Formation Studies(35), Astronomy and Astrophysical Research(32), Galaxies: Formation, Evolution, Phenomena(26), Gamma-ray bursts and supernovae(15)

Publications105 total

CLASSY XIII. Cutting through the Clouds - Comparing Indirect Tracers of Ionizing Photon Escape
arXiv (Cornell University)·2025Open Access
The Interstellar Medium in I Zw 18 Seen with JWST/MIRI. II. Warm Molecular Hydrogen and Warm Dust
The Astrophysical Journal·2025· 1 citedOpen Access
CLASSY XII: nitrogen enrichment shaped by gas density and feedback
Monthly Notices of the Royal Astronomical Society·2025· 5 citedOpen Access
The Interstellar Medium in I Zw 18 Seen with JWST/MIRI. I. Highly Ionized Gas
The Astrophysical Journal·2025· 2 citedOpen Access
The Interstellar Medium in I Zw 18 Seen with JWST/MIRI. III. Spatially Resolved Three Ionization State Oxygen Abundance
The Astrophysical Journal·2025· 6 citedOpen Access
The Interstellar Medium in I Zw 18 seen with JWST/MIRI: II. Warm Molecular Hydrogen and Warm Dust
arXiv (Cornell University)·2025Open Access
CLUES. III. Do User Choices Impact the Results of SED Fitting? Tests of “Off-the-shelf” Stellar Population and Dust Extinction Models in the CLUES Sample
The Astrophysical Journal·2025· 1 citedOpen Access
The Interstellar Medium in I Zw 18 seen with JWST/MIRI: III. Spatially Resolved Three Ionization State Oxygen Abundance
arXiv (Cornell University)·2025Open Access
CLASSY XII: Nitrogen Enrichment Shaped by Gas Density and Feedback
arXiv (Cornell University)·2025Open Access
A JWST/MIRI View of the Interstellar Medium in M83. I. Resolved Molecular Hydrogen Properties, Star Formation, and Feedback
The Astrophysical Journal·2025· 3 citedOpen Access
CLUES III: Do User Choices Impact The Results of SED Fitting? Tests of 'Off-The-Shelf' Stellar Population and Dust Extinction Models in the CLUES Sample
arXiv (Cornell University)·2025Open Access
Exploring the Mysterious High-ionization Source Powering [Ne<scp> v</scp>] in High-<i>z</i> Analog SBS0335-052 E with JWST/MIRI
The Astrophysical Journal·2025· 3 citedOpen Access
The UV Legacy Library of Young Stars as Essential Standards (ULLYSES) Large Director’s Discretionary Program with Hubble. I. Goals, Design, and Initial Results
The Astrophysical Journal·2025· 14 citedOpen Access
JWST/MIRI Detection of [Ne v] and [Ne <scp>vi</scp>] in M83: Evidence for the Long Sought-after Active Galactic Nucleus?
The Astrophysical Journal·2025· 7 citedOpen Access
High-quality photoplethysmography signals using a new non-contact method
2025
JWST/MIRI detection of [Ne V] and [Ne VI] in M83: Evidence for the long sought-after AGN?
arXiv (Cornell University)·2025Open Access
A JWST/MIRI View of the ISM in M83: I. Resolved Molecular Hydrogen Properties, Star Formation, and Feedback
arXiv (Cornell University)·2024Open Access
Mapping Multiphase Metals in Star-forming Galaxies: A Spatially Resolved UV+Optical Study of NGC 5253
The Astrophysical Journal·2024· 1 citedOpen Access
JWST NIRSpec Spectroscopy of the Triply Lensed z = 10.17 Galaxy MACS0647–JD
The Astrophysical Journal·2024· 63 citedOpen Access
The exploratory phase for Lifetime Position 7 in the Cosmic Origins Spectrograph FUV channel
2024
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Frequent Co-authors

Bethan L. James(26), Alessandra Aloisi(22), Matilde Mingozzi(17), Matthew Hayes(16), Claus Leitherer(15), Nimisha Kumari(13), L. J. Smith(13), John Chisholm(12), Aida Wofford(12), Angela Adamo(11), Danielle A. Berg(10), Crystal L. Martin(10), R. Amorín(9), S. Charlot(9), Evan D. Skillman(9), Xinfeng Xu(9), Daniela Calzetti(9), Karla Z. Arellano-Córdova(8), Themiya Nanayakkara(8), Andrew J. Fox(8)