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Ryley Hill

Dalhousie University · CA
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Area of research
Instrumentation · Astronomy and Astrophysics
Research interest
Research interests include Physics, Astrophysics, Galaxy, Astronomy, Redshift, and Core (optical fiber).
h-index
citations
464
works
12
NIH funding
primary concept
email

Recent publications

Brightest Cluster Galaxy Formation in the z = 4.3 Protocluster SPT 2349-56: Discovery of a Radio-loud Active Galactic Nucleus
The Astrophysical Journal 2024cited by 17position: middledoi
Spatial variations in aromatic hydrocarbon emission in a dust-rich galaxy
Nature 2023cited by 64position: middledoi
The Rest-frame Submillimeter Spectrum of High-redshift, Dusty, Star-forming Galaxies from the SPT-SZ Survey
The Astrophysical Journal 2023cited by 16position: middledoi
High resolution spectral imaging of CO(7–6), [CI](2–1), and continuum of three high-<i>z</i> lensed dusty star-forming galaxies using ALMA
Astronomy and Astrophysics 2022cited by 17position: middledoi
Multiphase ISM in the z = 5.7 Hyperluminous Starburst SPT 0346–52
The Astrophysical Journal 2022cited by 13position: middledoi
Molecular Line Observations in Two Dusty Star-forming Galaxies at z = 6.9
The Astrophysical Journal 2021cited by 36position: middledoi
Overdensities of submillimetre-bright sources around candidate protocluster cores selected from the South Pole Telescope survey
Monthly Notices of the Royal Astronomical Society 2021cited by 33position: middledoi
Optical and near-infrared observations of the SPT2349-56 proto-cluster core at <i>z</i> = 4.3
Monthly Notices of the Royal Astronomical Society 2021cited by 28position: middledoi
Rapid build-up of the stellar content in the protocluster core SPT2349−56 at z = 4.3
Monthly Notices of the Royal Astronomical Society 2021cited by 28position: firstdoi
The Complete Redshift Distribution of Dusty Star-forming Galaxies from the SPT-SZ Survey
The Astrophysical Journal 2020cited by 118position: middledoi
Megaparsec-scale structure around the protocluster core SPT2349–56 at <i>z</i> = 4.3
Monthly Notices of the Royal Astronomical Society 2020cited by 74position: firstdoi
Using ALMA to resolve the nature of the early star-forming large-scale structure PLCK G073.4−57.5
HAL (Le Centre pour la Communication Scientifique Directe) 2019cited by 20position: middle

Grants

No grants ingested yet.

Frequent collaborators

Justin Spilker · University of Arizona9 papers (2020–2023) · 9 papers (2020–2023)S. C. Chapman · Herzberg Institute of Astrophysics9 papers (2020–2023)C. Reuter · New York University9 papers (2020–2023)Daniel P. Marrone · California Institute of Technology9 papers (2020–2023)Christopher C. Hayward · California Institute of Technology9 papers (2020–2023)J. D. Vieira · University of Illinois Urbana-Champaign9 papers (2020–2023)Sreevani Jarugula · University of Illinois Urbana-Champaign8 papers (2020–2023)A. Weiß · University of Illinois Urbana-Champaign8 papers (2020–2023)Kedar A. Phadke · University of Illinois Urbana-Champaign8 papers (2020–2023)M. Béthermin · University of Illinois Urbana-Champaign6 papers (2020–2022)Matthew A. Malkan · University of California, Los Angeles6 papers (2020–2023)Anthony H. Gonzalez · University of Florida6 papers (2020–2023)Yashar Hezaveh · McGill University6 papers (2020–2022) · 6 papers (2020–2023)M. Archipley · University of Chicago6 papers (2020–2023)Chenxing Dong · University of Florida6 papers (2020–2022)Desika Narayanan · University of Copenhagen5 papers (2020–2022)Katrina C. Litke · University of Arizona5 papers (2020–2022)K. M. Rotermund · Lawrence Berkeley National Laboratory5 papers (2020–2021)
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