The Faint Sky Variability Survey - I. Goals and data reduction process

Monthly Notices of the Royal Astronomical Society

Volumn 339, Issue 2, 2003, Pages 427-434

  Groot, P J ^a,b,c   Vreeswijk, P M ^c   Huber, M E ^d,e   Everett, M E ^d   Howell, S B ^d   Nelemans, G ^c,f   Van Paradijs, J ^c,g   Van Den Heuvel, E P J ^c   Augusteijn, T ^h,i   Kuulkers, E ^j   Rutten, R G M ^h   Storm, J ^k  

^a RADBOUD UNIVERSITY NIJMEGEN   (Netherlands)

^b HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^c UNIVERSITY OF AMSTERDAM   (Netherlands)

^d PLANETARY SCIENCE INSTITUTE   (United States)

^e UNIVERSITY OF WYOMING   (United States)

^f UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^g UNIVERSITY OF ALABAMA IN HUNTSVILLE   (United States)

^h ISAAC NEWTON GROUP OF TELESCOPES   (Spain)

ⁱ NORDIC OPTICAL TELESCOPE   (Spain)

^j EUROPEAN SPACE AGENCY   (Netherlands)

^k ASTROPHYSIKALISCHES INSTITUT POTSDAM   (Germany)

more..

Author keywords

Galaxy: stellar content; Methods: data analysis; Stars: variables: other; Surveys; Techniques: photometric

Indexed keywords

DATA REDUCTION; PHOTOMETRY; STARS;

GALACTIC LATITUDE; GALAXY:STELLAR CONTENT; METHODS. DATA ANALYSIS; PHOTOMETRIC PRECISION; PHOTOMETRICS; REDUCTION PROCESS; STAR: VARIABLE: OTHER; STARS: VARIABLES; TECHNIQUES: PHOTOMETRIC; TIME-SCALES;

SURVEYS;

EID: 10744228372     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2003.06182.x     Document Type: Review

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