dc.contributor.author |
Jordi, C |
en |
dc.contributor.author |
Hog, E |
en |
dc.contributor.author |
Brown, A |
en |
dc.contributor.author |
Lindegren, L |
en |
dc.contributor.author |
Bailer-Jones, C |
en |
dc.contributor.author |
Carrasco, J |
en |
dc.contributor.author |
Knude, J |
en |
dc.contributor.author |
Straizys, V |
en |
dc.contributor.author |
Bruijne, J |
en |
dc.contributor.author |
Claeskens, J |
en |
dc.contributor.author |
Drimmel, R |
en |
dc.contributor.author |
Figueras, F |
en |
dc.contributor.author |
Grenon, M |
en |
dc.contributor.author |
Kolka, I |
en |
dc.contributor.author |
Perryman, M |
en |
dc.contributor.author |
Tautvaisiene, G |
en |
dc.contributor.author |
Willemsen, P |
en |
dc.contributor.author |
Brid, A |
en |
dc.contributor.author |
Evans, D |
en |
dc.contributor.author |
Fabricius, C |
en |
dc.contributor.author |
Fiorucci, M |
en |
dc.contributor.author |
Heiter, U |
en |
dc.contributor.author |
Kaempf, T |
en |
dc.contributor.author |
Kazlauskas, A |
en |
dc.contributor.author |
Torra, J |
en |
dc.contributor.author |
Vallenari, A |
en |
dc.contributor.author |
Korakitis, R |
en |
dc.contributor.author |
Malkov, O |
en |
dc.contributor.author |
Smette, A |
en |
dc.contributor.author |
Zdanavicius, K |
en |
dc.date.accessioned |
2014-03-01T01:54:22Z |
|
dc.date.available |
2014-03-01T01:54:22Z |
|
dc.date.issued |
2005 |
en |
dc.identifier.uri |
https://dspace.lib.ntua.gr/xmlui/handle/123456789/27348 |
|
dc.subject |
Chemical Composition |
en |
dc.subject |
Fundamental Parameters Techniques |
en |
dc.subject |
Space Vehicles |
en |
dc.subject |
Structure Formation |
en |
dc.subject |
Ultraviolet |
en |
dc.subject |
Far Red |
en |
dc.subject |
hertzsprung russell |
en |
dc.title |
The design and performance of the Gaia photometric system |
en |
heal.type |
journalArticle |
en |
heal.identifier.primary |
10.1111/j.1365-2966.2005.09944.x |
en |
heal.identifier.secondary |
http://dx.doi.org/10.1111/j.1365-2966.2005.09944.x |
en |
heal.publicationDate |
2005 |
en |
heal.abstract |
The European Gaia astrometry mission is due for launch in 2011. Gaia willrely on the proven principles of ESA's Hipparcos mission to create an all-skysurvey of about one billion stars throughout our Galaxy and beyond, byobserving all objects down to 20th magnitude. Through its massive measurementof stellar distances, motions and multi-colour photometry it will providefundamental |
en |
heal.journalName |
Monthly Notices of The Royal Astronomical Society |
en |
dc.identifier.doi |
10.1111/j.1365-2966.2005.09944.x |
en |