Sander, 
You ask a very good question. 
I've closely read Bill Gray's summary about the GSC-ACT at 
[ http://www.projectpluto.com/gsc_act.htm ]. The answer to your 
question depends on what you want to use the GSC-ACT for? Reading the 
thread of your post tonight hasn't offered me any insight about 
that?  My primary use for CDC is making charts for AAVSO visual 
variable star estimates. 

Since around 1994-95  the AAVSO has used GSC astrometric positions to 
create a star field (print black star dots on a sheet of paper)for 
their charts. Although the GSC  is  considered to be inadequate for 
photometric magitude data  and the AAVSO mostly uses it only on 
preliminary charts for a nova or supernova and GSC magitude estimates 
can be later revised using adequate photometery.

Sander from reading your post you find the Tycho-2 Catalog to be 
indequate in astrometry and you'd like to see as many stars on your 
screen has your C11 telescope shows.

You have only 2 options for a "CDC cat folder ready" catalogue and 
thats the quote, "obsolete" GSC-ACT 1.14GB. or the "dense" USNO A2.0 
which is exactly 6,315,439,692 bytes and +500,000,000 stars and 11 
CDs of star catalog. (I don't feel the current state of art USNO-
B1.0  which is 80GB with 100 CDs of stars catalog is an option for 
most CDC users.)

Let me quote a tiny portion of Bill Gray's "GSC-ACT files and 
information" URL:

"The purpose of the GSC-ACT project is to recalibrate the Hubble 
Guide Star Catalog (GSC), version 1.1, using the ACT (Astrographic 
Catalog/Tycho) data from the US Naval Observatory."  . . .  "I expect 
the main use of GSC-ACT will be in asteroid astrometry. And for this 
purpose, the answer to the question of "How much of an improvement is 
GSC-ACT over GSC 1.x?" is: "It cuts down errors a lot." . . .  "What 
about photometry?" . . . "First, there is a lack of suitable data. 
The Tycho dataset provides excellent photometry for stars down to 
about magnitude 11, and it is true that this could be used to 
recalibrate bright stars. But it would not necessarily help much at 
fainter magnitudes (i.e., for about 90% of GSC.) (But this objection 
may vanish. It does appear that Brian Skiff's LONEOS.PHOT photometric 
database could extend the range of "decent" photometry quite 
nicely.)  . . .  Second, it's not clear that the photometry could be 
improved very much. The raw magnitude data coming in from GSC 1.1 is 
sufficiently "random" that recalibration might not result in much of 
a benefit.  And thirdly, Dave Monet has recalibrated the A1.0 dataset 
(both photometrically and astrometrically), using ACT. This resulted 
in a much better photometric dataset than GSC-ACT could hope to be.


Sander, is that as clear as "MUD"?  
Personally, I feel Bill Gray knows what he is talking about on the 
topic of star catalogues. This is because any optical telescope has a 
certain degree of image field curvature and when the image forms on a 
flat CCD chip or photographic plate it distorts a tiny bit.  When all 
the image data of a whole sky survey is combined to create a star 
catalog all those many optically distortioned plates joined together 
creates two kinds of "errors".  First - the stars in the center of 
the field are in better focus the those towards the edge, this makes 
errors in star magitudes (photometric errors).  Second - the 
positions of the stars in the center of the field are more accurate 
that those towards the edge this makes star positions distorted 
(astrometric errors).  Brian Skiff's LONEOS.PHOT photometric database 
seems to be some sort of "software voo-doo" to focus those somewhat 
out of focus stars at the edge of a CCD or photo plate and reduce 
magitude errors. 

To offer a reply to your question: 
I would recommend the GSC-ACT for 2 reasons. First- I think you'll 
learn to deal with an astrometric error of .3 arcseconds (.3") on a 
computer screen, just set the CDC (HST GSC original fits) field at 
min 0 & max 1. Second-The magitude errors (for example:  Star 
GSC4766. 1330   - Magnitude: 14.39+/-0.40).
This star's magitude could be as bright as 13.99 or as faint as 14.79 
and I kinda doubt something like that is going to give you or very 
many amateur astronomers any heartburn!

Best Wishes,
Danny

Mudcreek Observarory
Parker County Texas
Latitude:    +32 deg 34 min 11 sec - north
Longitude : -97 deg 46 min 43 sec - west

=====================================================================
--- In [email protected], Sander Pool <[EMAIL PROTECTED]> 
wrote:
>
> 
> Yes, I saw that catalog but it doesn't appear to be available for 
> download anywhere. Some sites hold information files and code but 
no 
> data. If you know of a location please let me know.
> 
> I requested a CD set.
> 
>     Sander
> 
> starryeyeguy wrote:
> >
> > UCAC-2 covers the south pole to about +30 dec from 8th to 16th
> > magnitude. There is a supplement for the brighter stars derived 
from
> > Tycho-2. The complete catalog should be available next year.
> >
> > Cheers,
> >
> > Geoff Chester
> >
> > --- In [email protected] 
> > <mailto:skychart-discussion%40yahoogroups.com>, Sander Pool 
<sander@>
> > wrote:
> > >
> > >
> > > I'm seeing more stars in my C11 than the Tycho-2 catalog 
contains.
> > There
> > > is the GSC-ACT catalog but its homepage on projectpluto says 
it's
> > > obsolete. USNO is nice but huge and I don't need mag-20 (I 
wish :).
> > > UCAC-2 sounds promising and contains the range of stars I care
> > about. If
> > > I'm reading http://ad.usno.navy.mil/ucac/ 
> > <http://ad.usno.navy.mil/ucac/> correctly it's mostly geared
> > > towards the Southern hemisphere though, right?
> > >
> > > So, which catalog do you recommend for dim stars in CdC?
> > >
> > > Thanks,
> > >
> > > Sander
> > >
> >
> >
>






 
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