The [O iii]+H β equivalent width distribution at z ≃ 7: implications for the contribution of galaxies to reionization

R Endsley, DP Stark, J Chevallard… - Monthly Notices of the …, 2021 - academic.oup.com
We quantify the distribution of [O iii]+ H β line strengths at z≃ 7 using a sample of 20 bright
(≲–21) galaxies. We select these systems over wide-area fields (2.3 deg2 total) using a new …

Strong Lyman-α emission in an overdense region at z = 6.8: a very large (R ∼ 3 physical Mpc) ionized bubble in COSMOS?

R Endsley, DP Stark - Monthly Notices of the Royal Astronomical …, 2022 - academic.oup.com
Our understanding of reionization has advanced considerably over the past decade, with
several results now demonstrating that the intergalactic medium transitioned from …

MMT spectroscopy of Lyman-alpha at z ≃ 7: evidence for accelerated reionization around massive galaxies

R Endsley, DP Stark, S Charlot… - Monthly Notices of …, 2021 - academic.oup.com
Reionization-era galaxies tend to exhibit weak Ly α emission, likely reflecting attenuation
from an increasingly neutral IGM. Recent observations have begun to reveal exceptions to …

Galaxy clusters around radio-loud active galactic nuclei at 1.3< z< 3.2 as seen by spitzer

D Wylezalek, A Galametz, D Stern… - The Astrophysical …, 2013 - iopscience.iop.org
We report the first results from the Clusters Around Radio-Loud AGN program, a Cycle 7 and
8 Spitzer Space Telescope snapshot program to investigate the environments of a large …

A geometrically supported z∼ 10 candidate multiply imaged by the Hubble Frontier Fields cluster A2744

A Zitrin, W Zheng, T Broadhurst… - The Astrophysical …, 2014 - iopscience.iop.org
The deflection angles of lensed sources increase with their distance behind a given lens.
We utilize this geometric effect to corroborate the z phot≃ 9.8 photometric redshift estimate of …

Breakdown of Kennicutt–Schmidt law at giant molecular cloud scales in M33

S Onodera, N Kuno, T Tosaki, K Kohno… - The Astrophysical …, 2010 - iopscience.iop.org
We have mapped the northern area (30'× 20') of a Local Group spiral galaxy M33 in 12 CO
(J= 1–0) line with the 45 m telescope at the Nobeyama Radio Observatory. Along with Hα …

Identifying the SN 2022acko progenitor with JWST

SD Van Dyk, KA Bostroem, WK Zheng… - Monthly Notices of …, 2023 - academic.oup.com
We report on analysis using the JWST to identify a candidate progenitor star of the Type II-
plateau (II-P) supernova SN 2022acko in the nearby, barred spiral galaxy NGC 1300. To our …

THE VLA-COSMOS PERSPECTIVE ON THE INFRARED–RADIO RELATION. I. NEW CONSTRAINTS ON SELECTION BIASES AND THE NON-EVOLUTION OF THE …

MT Sargent, E Schinnerer, E Murphy… - The Astrophysical …, 2010 - iopscience.iop.org
ABSTRACT VLA 1.4 GHz (σ∼ 0.012 mJy) and MIPS 24 and 70 μm (σ∼ 0.02 and 1.7 mJy,
respectively) observations covering the 2 deg 2 COSMOS field are combined with an …

The Xmm cluster survey: active galactic nuclei and starburst galaxies in xmmxcs J2215. 9− 1738 at z= 1.46

M Hilton, E Lloyd-Davies, SA Stanford… - The Astrophysical …, 2010 - iopscience.iop.org
We use Chandra X-ray and Spitzer infrared (IR) observations to explore the active galactic
nucleus (AGN) and starburst populations of XMMXCS J2215. 9− 1738 at z= 1.46, one of the …

Environmental impacts on molecular gas in protocluster galaxies at z ∼ 2

K Tadaki, T Kodama, M Hayashi… - Publications of the …, 2019 - academic.oup.com
We present the results from ALMA CO (3–2) observations of 66 Hα-selected galaxies in
three protoclusters around radio galaxies: PKS 1138− 262 (= 2.16), USS 1558− 003 …