Hi John,

Thank you .

I have understand this effect of the photo emulsion.

Regards,

Oleg

> > UNA 0525-42438046
> > Visual Magnitude: 0.10
> > Blue Magnitude: 0.10
> > ...
> > Mean J2000 RA: 20h26m53.043s DE:-37°24'11.55"
> 
> I get the same type of results here.  Note that all of these examples happen 
> to be very near relatively bright stars, so the Palomar sky survey plates are 
> saturated.  The deeper catalogs are all based on those plates, so there are 
> errors in these regions.  You can use the DSS online overlay (these are the 
> Palomar images) to see what I mean- just one huge white ball about an 
> arcminute wide, so when these plates were processed (by machines) to find the 
> stars in the USNO catalogs, the fainter stars in these regions aren't really 
> detected at all- these are just spurious detections.  
> 
> Apparently there's a glitch in CdC that doesn't read the "magnitude 99" 
> correctly.  But this works right if you use USNO-B.
> 
> But note using B that there are also many mag 99 stars in a cross pattern 
> just outside the big white ball- this is the diffraction spikes, incorrectly 
> detected as stars!
>  
> -John
> 
>  
> > UNA 0525-42045984
> > Visual Magnitude: 0.10
> > Blue Magnitude: 0.10
> > ...
> > Mean J2000 RA: 20h07m44.780s DE:-31°45'07.78"
> > 
> > -Oleg :)

More catalogues for CdC on http://astroclub.biz/ru/?page_id=3

With best regards,
Oleg Maliy
Zaporozhye Astronomical Club "Altair"   http://astroclub.biz/ru/

Zaporozhye (47N48, 35E10)
Ukraine

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