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[vsnet-chat 6018] Re: [AAVSO-DIS] Re: v1413 Aql - Ready for Eclipse




On Sun, 16 Feb 2003, Brian Skiff wrote:

> (which he admits to).  This page contains Roger's threshold vs detection-
> probability table from the 1994 S&T article.  The 50 percent detection
> limit for 10cm (4-inches) aperture is indeed 13.7, as Mike quoted.

Its good to see that my figure came quite close to theirs. I started from
the flux of Vega (gives mag 0 star of B-V=0 is 3.68e-20 ergs/cm^2/s/hz)
and derived the quantum count from it (assuming peak visual at 510nm and
BW of 250nm)

> Party some years ago.  Both the latter indicate reasonable limits of V=8.2
> or so for typical eyes (Nash says his vision is not particularly sharp).

Well, I really have doubts about these tests. Personally, I cant seem to
do much better than about 6.8 from Mauna Kea, and I think my sensitivity
is pretty good even though my acuity is about 20/30, which is probably the
limiting factor. But, I can estimate down to about 16.3 with my 37cm under
ideal conditions, since I can then focus precisely, which is right at my
50% threshold as I calculated, so I feel pretty good about this. Most
observers I personally met are about that same level. It seems to me some
kind of bias is going on in selecting particularly sensitive individuals
for these tests, or they are not being 100% honest?

> instead physio- and psychological factors weigh heavily.  Basically, the
> experienced old observers with 4-5mm pupils see just as faint as younger
> folks with 7-8mm pupils.  And of course telescopically pupil size doesn't

This seems odd. One of the key factors in naked eye, and it is in
the formula I used to derive it as well, is the aperture of the eye. The
difference between 4.5mm and 7.5mm is 1.1 magnitudes. But there may be
some compensatory effect going on with the older eyes, that is as the
pupil size decreases slowly, the retina develops a lower throshold of
signal detection? Dont know if anyone has studied this in detail.

Mike Linnolt



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