Light curve of OGLE-2005-BLG-390

Data obtained by PLANET/RoboNet, OGLE, and MOA on the microlensing event OGLE-2005-BLG-390 together with a model light curve, showing the planetary deviation on its falling part, lasting about a day. Also shown are best-fitting models with a single lens and a binary source (long-dashed) and a single-source-single-lens light curve (short-dashed). Each point represents the brightness in a single image and the data are colour-coded in order to indicate the telescope : Danish 1.54m at ESO La Silla (Chile), Perth 0.6m (Bickley, Western Australia), Canopus 1.0m (Hobart, Tasmania, Australia), Faulkes North 2.0m (Haleakela, Hawaii, USA), OGLE 1.3m (Las Campanas, Chile), and MOA 1.8m at Mt John Observatory (New Zealand). The regular cycle of colours shows how observing is taken over by the next telescope in turn as the night ends at each site. An enlargement of the planetary deviation is shown as inset in the top right.

Credit:

ESO

Over de afbeelding

Id:eso0603b
Type:Kaart
Publicatiedatum:25 januari 2006
Gerelateerde berichten:eso0603
Grootte:2212 x 1304 px

Over het object

Naam:OGLE-2005-BLG-390Lb
Type:Milky Way : Star : Circumstellar Material : Planetary System
Afstand:20000 lichtjaren
Categorie:Exoplanets
Stars

Image Formats

Grote JPEG
354,0 KB