Nope. Redownloaded to be sure, no change at all from what I did have
Nope. Redownloaded to be sure, no change at all from what I did have
You could try the filtering in Gaia Archive with:
WHERE r_est < 100000 AND radius_val > 0 AND phot_g_mean_mag > 8.5 and parallax > 0
Filtering by parallax means nothing lol. All stars have a parallax > 0. Parallax is the angle formed by the apparent shift of the background in relation to the object viewed from two different positions. The distance can then be calculated via trigonometry. No parallax would mean a star located at infinity distance!'phot_g_mag > 8.5' ensures that most Hipparchos stars are excluded and 'parallax > 0' should filter out most stars with incorrect distances!
Weird. I'll take a look into it.Nope. Redownloaded to be sure, no change at all from what I did have
Ok, so yeah, 2M still had wrong RA. Fixed now. Also fixed 800k being wrong fileNope. Redownloaded to be sure, no change at all from what I did have
NO!
Why are some parallaxes less than zero?
Negative parallaxes are caused by errors in the observations. Even if a negative distance has no physical meaning, there are a certain number of stars expected to have negative parallaxes just from an error propagation perspective. The negative parallax tail is a very useful diagnostic on the quality of the astrometric solution. Further details can be found here and here.
Yes my mistake. What I meant was getting the parallax to determine the error in the parallax is not very useful. Instead, there is a parallax_error value that can be fetched from Gaia directly to calculate relative error %.NO!
Quote from the Gaia FAQ:Why are some parallaxes less than zero?
Negative parallaxes are caused by errors in the observations. Even if a negative distance has no physical meaning, there are a certain number of stars expected to have negative parallaxes just from an error propagation perspective. The negative parallax tail is a very useful diagnostic on the quality of the astrometric solution. Further details can be found here and here.
Maybe you should nevertheless follow SpaceEnigneer's advice!
The Gaia catalog is definitely worth it IMHO. It is just not optimized yet, neither is SE for this job. As Space Engineer mentioned in a previous post not even 0990 will be ready for this task. Even Gaia is not completed as all data are not yet processed. In its final form there will be approximately 1 billion stars. SE will need to be adapted to be able to accept such huge catalog(s). Space Engineer is a coding master & magician so I am confident SE will eventually include the Gaia catalog in all of its glory.Is the GAIA add on worth it in your opinion even if the spectral classes and types of stars is randomized? And is it recommended to turn off all procedural stuff?Guys its (probably) not (just) the cpu.. the program runs out of usable RAM. The moment it hits 3+ gigs of RAM usage it quits to desktop. I have a monster CPU and have the same fate.. I tried the 5M database and even when I disable proc+cat. galaxies, proc.stars & proc clusters I can go up to ~10.5 Magnitude (veery slowly) and then desktop.. If the above are enabled I can not even dream of 10 magnitude: ~8-9 and desktop.. (all this @ 5760x1080 resolution as I have 3 TVs..).
I dont mind limiting stars to around Mag 8.5, thats the dimmest the human eye can see anyway under no light pollution.
I dont use a very high resolution on the monitor I run it on, it's 1280x1024. I have all very high settings enabled and a 6 GB video card and 16 GB RAM.
We're going to have to wait until the next gaia release for proper stellar types and classes.Omg thats huge, one billion stars is more massive than any planetarium program I know of.
One question I have is when the data is fully processed will all the spectral types and classes of stars be known? I would hope that was part of the initial collection of data, as thats pretty essential. It's pretty easy to determine stellar class and color using photographic data (B-V) and absolute magnitude and distance.
No, it is not. How would you determine to whuch branch star belogs, if those "branches" are so fuzzy? Only white dwarfs can easily be classified (well, most of them). Red giants have many "luninosity class" branches, which are not visible here. Some stars even changes their class!