Luis Rodríguez Olmo Stadium / Visitor Center Parking Lot / SETI Institute / HF facility / Cornell campus / Nine towers / Cornell University / Airglow facility / Observatory News / Cornell Theory Center / Ionospheric Interactions facility / Arecibo Observatory / McGill University / Dome Alignment Planned / College of Arts / /
IndustryTerm
and-sideband search techniques / near real-time internet / astrophysical applications / pulsar search data / search data / telephone systems / cable car cable / targeted search covering / systematic search / electricity / search code / gas rich / detected gas / periodicity search / drift-scan search candidates / Deep imaging / /
MusicGroup
MHz / /
Organization
National Science Foundation / Cornell Employee Assembly / VSQ Family Unit / SETI Institute / Cornell University / Cornell Theory Center / Cornell Department of Astronomy / National Aeronautics and Space Administration / McGill University / Montreal / College of Arts and Sciences / National Weather Service / /
Person
Qihou Zhou / Jim Cordes / David Nice (Princeton) / Michael Kramer / Georges Kiriaki Xilouris / Joel Weisberg / Alex Zepka / John Mathews / Craig Tepley / Eva Robles / Rey Vélez / Nathan Carle (Lafayette) / Bob Kerr / Together with Carl Ulbrich / Courtesy Joe Taylor / Carl Ulbrich (Clemson) / Phil Perillat / Tony Acevedo Ionospheric / Georges Daniel / Steve Collins / Joel Weisberg (Carleton) / Diego Janches / Tapasi Ghosh / Monique Petitdidier / Edwin Campos / Daniel R. Altschuler / Mike Sulzer / Andrea Somer / Jonathan Friedman / Maura McLaughlin / Jo Ann Eder / Kiriaki Xilouris / Jill Tarter / Duncan Lorimer / Lymari Castro / Chris Salter / Juan Cabanela / Don Backal / Joe Taylor (Princeton) / Steve Oetting / John Dickey / Jonathan Friedman (Arecibo) / /
Position
electron density model / Major / /
Product
RPG / /
ProvinceOrState
Ohio / Minnesota / Hawaii / Missouri / California / Ontario / /
November 1998, Number 26 A Pulsar named Georges Kiriaki Xilouris and Duncan Lorimer In early June 1998, during our search for pulsars in supernova remnants, we observed the soft γ-ray repeater SGR