M. Sullivan

University of Oxford

Papers

1

Total Citations

19

H-Index

1

About

M. Sullivan is a leading figure in stellar astrophysics, with a primary focus on the detection and characterization of binary star systems. Their most influential work, "Millions of Multiples: Detecting and Characterizing Close-Separation Binary Systems in Synoptic Sky Surveys" (2013), has garnered 19 citations and introduced a groundbreaking technique for identifying close-separation binaries in wide-field surveys. By leveraging the precision calibration of point-spread functions (PSFs), Sullivan’s method overcomes traditional limitations tied to stellar PSF size, enabling the discovery of elongated objects that reveal hidden companions. This contribution has significantly advanced our understanding of binary star populations, offering a scalable approach for analyzing vast datasets from modern synoptic surveys. Sullivan’s work is pivotal for researchers exploring stellar multiplicity, providing tools that bridge observational constraints and computational precision. Their achievements underscore a commitment to refining detection methodologies, with lasting implications for studies of stellar evolution and galactic structure.

Research Focus

Key Achievements

1
H-Index
1
Papers
19
Total Citations
19
Avg Citations/Paper
🏆 Most Cited Paper
MILLIONS OF MULTIPLES: DETECTING AND CHARACTERIZING CLOSE-SEPARATION BINARY SYSTEMS IN SYNOPTIC SKY SURVEYS
19 citations · 2013
📈 Most Prolific Year: 2013 (1 Papers)
🤝 Key Collaborators: 17
🏛 Institutions: University of Oxford

Top Papers

  1. 1

Key Collaborators

Contact & Links

Available for collaboration
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