2006MNRAS.365..165S

Query : 2006MNRAS.365..165S

2006MNRAS.365..165S - Mon. Not. R. Astron. Soc., 365, 165-170 (2006/January-1)

Efficient analysis in planet transit surveys.

SCHWARZENBERG-CZERNY A. and BEAULIEU J.-P.

Abstract (from CDS):

With the growing number of projects dedicated to the search for extrasolar planets via transits, there is a need to develop fast, automatic, robust methods with a statistical background in order to carry out the analysis efficiently. We propose a modified analysis of variance (AoV) test particularly suitable for the detection of planetary transits in stellar light curves. We show how labour savings of a factor of over 10 could be achieved by the careful organization of computations. Based on solid analytical statistical formulations, we discuss the performance of our and other methods for different signal-to-noise ratios and numbers of observations.

Abstract Copyright: 2005 The Authors. Journal compilation © 2005 RAS

Journal keyword(s): methods: data analysis - methods: statistical - techniques: photometric - sur-veys - stars: oscillations - planetary systems

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 HD 209458b Pl 22 03 10.7727465312 +18 53 03.549393384           ~ 2037 1

Query : 2006MNRAS.365..165S

Basic data :
HD 209458b -- Extra-solar Planet
Other object types: otypes_help 		Pl? (), Pl (2000ApJ), * (HD)
ICRS coord. (ep=J2000) : 		22 03 10.7727465312 +18 53 03.549393384 (Optical) [ 0.0213 0.0227 90 ] A 2020yCat.1350....0G
FK4 coord. (ep=B1950 eq=1950) : 		22 00 48.0717927453 +18 38 32.219124290 [ 0.0213 0.0227 90 ]
Gal coord. (ep=J2000) : 		076.7533281569711 -28.5269056004135 [ 0.0213 0.0227 90 ]
Proper motions mas/yr : 		29.766 -17.976 [0.028 0.025 90] A 2020yCat.1350....0G
Parallaxes (mas): 		20.7694 [0.0266] A 2020yCat.1350....0G
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HD 209458b NAME Osiris

References (2037 between 1850 and 2026) (Total 2037)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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