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G. C. Sloan

University of North Carolina at Chapel Hill · US
Area of research
Astronomy and Astrophysics · Instrumentation
Research interest
Research interests include Stellar, planetary, and galactic studies, Astrophysics and Star Formation Studies, Astronomy and Astrophysical Research, and Astro and Planetary Science.
h-index
48
citations
7,753
works
243
NIH funding
primary concept
email

Recent publications

Discovery of SiC and Iron Dust around AGB Stars in the Very Metal-poor Sextans a Dwarf Galaxy with JWST: Implications for Dust Production at High Redshift
The Astrophysical Journal 2025cited by 2position: middledoi
The Mid-infrared Instrument for JWST and Its In-flight Performance
Publications of the Astronomical Society of the Pacific 2023cited by 288position: middledoi
JWST MIRI/MRS in-flight absolute flux calibration and tailored fringe correction for unresolved sources
Astronomy and Astrophysics 2023cited by 48position: middledoi
Spectroscopic Time Series Performance of the Mid-infrared Instrument on the JWST
Publications of the Astronomical Society of the Pacific 2023cited by 45position: middledoi
JWST MIRI Flight Performance: Detector Effects and Data Reduction Algorithms
Publications of the Astronomical Society of the Pacific 2023cited by 40position: lastdoi
Observations of the planetary nebula SMP LMC 058 with the JWST MIRI medium resolution spectrometer
Monthly Notices of the Royal Astronomical Society 2023cited by 27position: middledoi
The James Webb Space Telescope Absolute Flux Calibration. I. Program Design and Calibrator Stars
arXiv (Cornell University) 2022cited by 100position: middledoi
EU Del: exploring the onset of pulsation-driven winds in giant stars
Monthly Notices of the Royal Astronomical Society 2016cited by 13position: middledoi
AN INFRARED CENSUS OF DUST IN NEARBY GALAXIES WITH<i>SPITZER</i>(DUSTiNGS). II. DISCOVERY OF METAL-POOR DUSTY AGB STARS
The Astrophysical Journal 2015cited by 75position: middledoi
Spitzer Space Telescope spectra of post-AGB stars in the Large Magellanic Cloud – polycyclic aromatic hydrocarbons at low metallicities
Monthly Notices of the Royal Astronomical Society 2014cited by 90position: middledoi
THE DUST BUDGET OF THE SMALL MAGELLANIC CLOUD: ARE ASYMPTOTIC GIANT BRANCH STARS THE PRIMARY DUST SOURCE AT LOW METALLICITY?
The Astrophysical Journal 2012cited by 148position: lastdoi

Grants

No grants ingested yet.

Frequent collaborators

Á. Labiano · California Institute of Technology4 papers (2023–2023) · 4 papers (2012–2023)Ori D. Fox · University of California, Berkeley4 papers (2023–2023) · 3 papers (2023–2023)Michael Mueller · Organisation de Coopération et de Développement Economiques3 papers (2023–2023)Omnarayani Nayak · Goddard Space Flight Center3 papers (2023–2023)Ioannis Argyriou · KU Leuven3 papers (2023–2023)Iain McDonald · University of Manchester3 papers (2012–2016) · 3 papers (2023–2023)David R. Law · Wenzhou Medical University3 papers (2023–2023)A. Noriega‐Crespo · California Institute of Technology3 papers (2023–2023)Danny Gasman · KU Leuven3 papers (2023–2023)Martha L. Boyer · University of Maryland, College Park3 papers (2012–2022)G. H. Rieke · University of Arizona3 papers (2022–2023)Patrick Kavanagh · University of Tübingen2 papers (2023–2023)M. Meixner · University of Notre Dame2 papers (2012–2015)P. Guillard · California Institute of Technology2 papers (2023–2023)Pamela Klaassen · McMaster University2 papers (2023–2023)Kirsten L. Larson · California Institute of Technology2 papers (2023–2023)Michael E. Ressler · California Institute of Technology2 papers (2023–2023)