Version 2.1 A & C of the Celestia extended stars databas
Posted: 09.05.2003, 17:24
Hello !
I have generated a new extended stars database for Celestia that should no more enter in conflict with Sun's neighborhood.
You can download them for the moment at :
http://perso.wanadoo.fr/celestia.stars/
V2.1 A : 1 016 385 stars (16.6 Mb)
V2.1 C : 2 072 873 stars (32.7 Mb)
Imprecision on data that comes from the Tycho catalogs and the current limits of the interpolation procedure are more noticeable for Sun’s neighborhood. To avoid any conflict with well known nearby stars, no Tycho stars have been added in this new release below 25 pc. Tycho stars with known parallaxes have been put farther when it has been established that error on their parallaxes could lead to stars with distances greater than 25 pc.
I will now work on the systematic integration of non-Hipparcos stars that come from the Gliese catalog. The goal is of course is to get an accurate representation of our neighborhood within 25 pc.
Let me know if you find other inconsistancies that could be corrected.
Best regards
Pascal
I have generated a new extended stars database for Celestia that should no more enter in conflict with Sun's neighborhood.
You can download them for the moment at :
http://perso.wanadoo.fr/celestia.stars/
V2.1 A : 1 016 385 stars (16.6 Mb)
V2.1 C : 2 072 873 stars (32.7 Mb)
Imprecision on data that comes from the Tycho catalogs and the current limits of the interpolation procedure are more noticeable for Sun’s neighborhood. To avoid any conflict with well known nearby stars, no Tycho stars have been added in this new release below 25 pc. Tycho stars with known parallaxes have been put farther when it has been established that error on their parallaxes could lead to stars with distances greater than 25 pc.
I will now work on the systematic integration of non-Hipparcos stars that come from the Gliese catalog. The goal is of course is to get an accurate representation of our neighborhood within 25 pc.
Let me know if you find other inconsistancies that could be corrected.
Best regards
Pascal