activity
20162025
most citedA Magnified Compact Galaxy at Redshift 9.51 with Strong Nebular Emission Lines

98 citations · 299 across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph.GA2025★ 1 cited

Spatially resolved gas-phase metallicity at z~2-3 with JWST/NIRISS

Ayan Acharyya, Peter J. Watson, Benedetta Vulcani +24

Spatially resolved gas-phase metallicity maps are a crucial element in understanding the chemical evolution of galaxies. We present spatially resolved metallicity maps obtained fro…

astro-ph.GA2025

Joint Survey Processing. III. Compact Oddballs in the COSMOS Field -- Little Red Dots and Transients

Yu-Heng Lin, Andreas L. Faisst, Ranga-Ram Chary +7

We present the HST ACS G800L grism spectroscopy observation of the faint active galactic nuclei (AGN) candidates in the COSMOS field at redshift of 6 selected by the point-source m…

astro-ph.GA2025★ 7 cited

The Lyman-alpha and Continuum Origins Survey. I. Survey description and Ly imaging

Alexandra Le Reste, Claudia Scarlata, Matthew Hayes +25

Understanding the mechanisms driving the escape of ionizing or Lyman continuum (LyC) emission from the interstellar medium of galaxies is necessary to constrain the evolution of re…

astro-ph.GA2025

The JWST/PASSAGE Survey: Testing Reionization Histories with JWST's First Unbiased Survey for Lyman alpha Emitters at Redshifts 7.5-9.5

Axel Runnholm, Matthew J. Hayes, Vihang Mehta +25

Lyman (Ly) emission is one of few observable features of galaxies that can trace the neutral hydrogen content in the Universe during the Epoch of Reionization (EoR). To acco…

astro-ph.GA2025

Systematic Bias in Ionizing Radiation Escape Fraction Measurements from Foreground Large-Scale Structures

C. Scarlata, W. Hu, M. J. Hayes +8

We investigate the relationship between the Lyman-alpha (Lya) forest transmission in the intergalactic medium (IGM) and the environmental density of galaxies, focusing on its impli…

astro-ph.GA2023★ 13 cited

On the evolution of the size of Lyman alpha halos across cosmic time: no change in the circumgalactic gas distribution when probed by line emission

Axel Runnholm, Matthew J. Hayes, Yu-Heng Lin +18

Lyman (Ly) is now routinely used as a tool for studying high-redshift galaxies and its resonant nature means it can trace neutral hydrogen around star-forming galaxies. Inte…

astro-ph.GA2023★ 3 cited

An Empirical reionization history model inferred from the low-redshift Lyman continuum survey and the star-forming galaxies at

Yu-Heng Lin, Claudia Scarlata, Hayley Williams +8

We present a new analysis of the rest-frame UV and optical spectra of a sample of three galaxies discovered behind the gravitational lensing cluster RX\,J2129.4+0009. We comb…

astro-ph.GA2023★ 34 cited

The Universe is at Most 88% Neutral at z=10.6

Sean Bruton, Yu-Heng Lin, Claudia Scarlata +1

Recent observations of GN-z11 with JWST have revealed a Ly emission line with an equivalent width of 18 angstroms. At z=10.6, this galaxy is expected to lie in the heart…

astro-ph.GA2022★ 61 cited

Evolution of the Mass-Metallicity Relation from Redshift to the Local Universe

Danial Langeroodi, Jens Hjorth, Wenlei Chen +17

A tight positive correlation between the stellar mass and the gas-phase metallicity of galaxies has been observed at low redshifts. The redshift evolution of this correlation can s…

astro-ph.GA2022★ 5 cited

Low Metallicity Galaxies from the Dark Energy Survey

Yu-Heng Lin, Claudia Scarlata, Vihang Mehta +6

We present a new selection of 358 blue compact dwarf galaxies (BCDs) from 5,000 square degrees in the Dark Energy Survey (DES), and the spectroscopic follow-up of a subsample of 68…

astro-ph.CO2022★ 1 cited

Towards a non-Gaussian Generative Model of large-scale Reionization Maps

Yu-Heng Lin, Sultan Hassan, Bruno Régaldo-Saint Blancard +2

High-dimensional data sets are expected from the next generation of large-scale surveys. These data sets will carry a wealth of information about the early stages of galaxy formati…

astro-ph.GA2022★ 98 cited

A Magnified Compact Galaxy at Redshift 9.51 with Strong Nebular Emission Lines

Hayley Williams, Patrick L. Kelly, Wenlei Chen +21

Ultraviolet light from early galaxies is thought to have ionized gas in the intergalactic medium. However, there are few observational constraints on this epoch because of the fain…

astro-ph.GA2021★ 6 cited

A Peculiar Type~II QSO Identified via Broad-band Detection of Extreme Nebular Line Emission

Yu-Heng Lin, Claudia Scarlata, Matthew Hayes +5

We present S82-20, an unusual redshift 3 object identified in SDSS-Stripe 82 broad-band images. The rest-frame ultraviolet spectrum of S82-20 shows emission lines from hig…

hep-ph2017★ 66 cited

Non-leptonic two-body weak decays of

C. Q. Geng, Y. K. Hsiao, Yu-Heng Lin +1

We study the non-leptonic two-body weak decays of with () representing as the baryon (meson) states. Based on the flavor symmetr…

hep-ph2016★ 4 cited

Roles of scalar mesons in charmless decays

Y. K. Hsiao, Yu-Heng Lin, Yao Yu +1

We first study the charmless two-body decays with the scalar mesons as the final states and predict that ${\cal B}(Λ_b\to Λf_0(980,1500))=(2.9\pm 0.7,12.4\pm 3.8)\times 10^{-…