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Re: [APML] 2 new images
Hi Jerry,
I would say, Centuria 800 is simply a grainy and perhaps high-speed
version of Centuria 400. Both have low reciprocity failure under
low intensity. Both are sharp. It was confirmed that Centuria 400
has very good red (H-Alpha, in particular) and blue sensitivity.
Ron Pearson posted a comet picture by Centuria 400 on Astromart.
>From that picture, it seems that Centuria 400 is sensitive to green
light as well.
I only used E200 one or two times. So I cannot comment too much
about Centuria vs E200. Judging from other people's pictures by
E200, Centuria 400/800 seems to have better RGB balance over
E200. E200 is too red. Centuria seems more grainy than E200.
This month, I used Centuria 800 and E200 on the same target and
with the same telescope setup. After I scan and process the
images, I should be able to make better comparison of these two.
I have a larger picture of IC2177:
http://www.ifa.hawaii.edu/~wang/gallery/picutres/I2177-large.jpg
Although the images is a stacked of threee shots and is heavily
smoothed in PhotoShop, you can see the noise (grains) of Centuria
800.
About measuring stellar diameters, I do this on the scanned images.
For example, my scanner is a 1600 dpi one. 1600 dpi means that
each pixel is 25.4mm/1600 = 16 micron. So if a star has diameter
of 3 pixels, its physical diameter is ~50 micron.
Cheers,
Wei-Hao
______________________________________________________________________
Wei-Hao Wang :)
Institute for Astronomy at University of Hawaii
Address: Phone: 808-956-9867
2680 Woodlawn Drive Personal Website:
Honolulu, HI 96822 http://www.ifa.hawaii.edu/~wang
______________________________________________________________________
On Thu, 26 Feb 2004, Jerry Lodriguss wrote:
>
> Hi Wei-Hao,
>
> These are some very nice shots. The Centuria 800 looks great, at least at
> web resolution. The color sensitivity is great too. Do you find the
> Centuria 400 to be pretty much the same? How would you compare it to E200?
>
> How did you measure the star diameters?
>
> Jerry
>
>
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