Sonntag, 9. März 2014

getting to the Gaia mock Universe

Some notes on practicalities of getting to the A.Robin (?) mock Gaia Universe.

The basic stuff for my purpose is the gums.mw table,
described in http://dc.zah.uni-heidelberg.de/tableinfo/gums.mw

How to get to it:
what works: go to topcoat (download as needed)
and follow instructions in http://voparis-europlanet.obspm.fr/utilities/Tuto_TopCat.pdf

You don't get the file, but you can SQL-type query it.

You get 1.000.000 records easily, but I still have to figure out how
to get the whole file, e.g. as a binary fits.
Markus Demleitner at ARI is the person to talk to; here is what he advises:


Uncheck "synchronuous"; this selects async operation, which lets
you even change your location and IP and retrieve the result later;
also, it gives you, by default, 3600 seconds of query time before
timing out.

magg<17.5 is still a large number of objects and hence a very large
table (I'd expect several 1e8 rows), probably too big for TOPCAT to
keep in memory or to handle directly (though it might be ready
before the 3600 s timeout).  

You could use STILTS to stream things to your disk and select FITS
binary output (see stilts tapquery); but it'd certainly be preferable
if you gave some additional constraints to offload part of your
computation to the server (note that you can also upload your own
object lists).  The server already has indices in place, quite some
memory, etc., so it usually pays to let it do the heavy lifting and
keep the tables you actually deal with of order 1e6 or maybe 1e7
rows.

I am now working on downloading the fits file directly,
and do them with p. in subdir GaiaSims in Apogee.

Freitag, 7. März 2014

Dynamics of K or G dwarfs near the mid-plane

Some thoughts on how to serious is practice about the dynamical modeling
a la Bovy using G and K dwarfs near the galactic mid plane from the SEGUE scans.

1) query all G and K stars with b<30 & spectra in DR10

2) where do we get a/Fe from?

3) get the proper motions both from SDSS and from PS1

4) this is the test-sample on which to compare the two proper motion estimates…

5) do we need to deredden individually?