activity
19942026
most citedThe most metal-poor galaxies

371 citations · 4.7k across the 108 of their papers we have counts for

collaborators

108 papers

astro-ph.GA2026

Supernovae Ia ejecta velocities and host galaxy environments: the role of survey-selection effects

L. V. Barkhudaryan, A. A. Hakobyan, M. H. Gevorgyan +6

The origin of the near-maximum-light Si II 6355 velocity diversity among supernovae Ia (SNe Ia) remains uncertain. Previous studies have suggested that high-velocity (HV) and no…

astro-ph.GA2025★ 1 cited

Calcium versus silicon ejecta velocities and decline rates in supernovae Ia: The role of high-velocity features

A. A. Hakobyan, M. H. Gevorgyan, A. G. Karapetyan +4

Photospheric and high-velocity features (PVFs and HVFs) of Si II 6355 and Ca II IR3 lines in supernova Ia (SN Ia) spectra provide insights into ejecta structure, energetics, and…

astro-ph.GA2024★ 3 cited

The Lyman Alpha Reference Sample. XVI. Global 21cm HI properties of Lyman- emitting galaxies

A. Le Reste, M. J. Hayes, J. M. Cannon +9

The Lyman- (Lya) line of hydrogen is a well-known tracer of galaxies at high-z. However, the connection between Lya observables and galaxy properties has not fully been establis…

astro-ph.GA2024

Haro 11: The Spatially Resolved Lyman Continuum Sources

Lena Komarova, M. S. Oey, Svea Hernandez +13

As the nearest confirmed Lyman continuum (LyC) emitter, Haro 11 is an exceptional laboratory for studying LyC escape processes crucial to cosmic reionization. Our new HST/COS G130M…

astro-ph.GA2023★ 9 cited

The Lyman Reference Sample XIV: Lyman imaging of 45 low redshift star-forming galaxies and inferences on global emission

Jens Melinder, Göran Östlin, Matthew Hayes +18

We present Ly imaging of 45 low redshift star-forming galaxies observed with the Hubble Space Telescope. The galaxies have been selected to have moderate to high star formation…

astro-ph.GA2022

The Lyman Alpha Reference Sample XIII: High-Angular Resolution 21cm HI observations of Ly emitting galaxies

A. Le Reste, M. Hayes, J. M. Cannon +8

The Ly emission line is one of the main observables of galaxies at high redshift, but its output depends strongly on the neutral gas distribution and kinematics around the star-…