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RE: Re:[APML] orion mosaic
That's an interesting point, Philip. The problem I see is that the spectral response of film and silicon is simply different than that of the eye. With film you can't really do anything. However, since silicon is silicon is silicon (the detecting material for CCD and CMOS focal plane arrays), you can in theory design a spectral filter for use with the detector which will match the spectral response of the eye. Then you will truly have what the eye would see if it was much more sensitive. I believe such filters are available today.
Cheers,
Jason
-----Original Message-----
From: astro-photo-bounces@seds.org
[mailto:astro-photo-bounces@seds.org]On Behalf Of Philip Perkins
Sent: Thursday, March 31, 2005 4:10 PM
To: Discussion of Film Astrophotography
Subject: Re: Re:[APML] orion mosaic
Rob and Wei-Hao,
I agree this is a wonderful wide field composition. I think there is a lot
to be said for recording objects in the night sky as the human eye might
see them if it were thousands of times more sensitive. For this purpose it
seems to me that recording an unfiltered image on natural daylight film is
very acceptable. In this context use of an Ha filter is probably somewhat
artificial - after all the human eye does not have an Ha filter stuck in
front of it.
The use of an Ha filter is the latest in a long line of CCD imaging
fashions. Remember that a few years ago an image had to be deconvolved to
virtual oblivion before it was considered processed properly. Nowadays
little or no deconvolution is the norm. The next vogue was intense star
colours. After this came galaxy images pock-marked with intense Ha regions
that look like a severe case of acne. We all know that galaxies would
never look like this naturally if we could be a few million light years
closer. Now an Ha filter has to be used if nebulous regions are to be
considered recorded properly. This will surely be replaced by some new
vogue in the future. Possibly new filtering techniques - I see that OIII
filters are starting to be used more and more.
These are all admirable methods in trying to achieve something different
from static celestial objects where, unlike terrestrial objects, the
lighting and aspect can never change. But, broadening the mind a little, I
think there is actually a wide spectrum of other techniques that can show
different aspects of the night sky. Although tried and trusted, the purity
of an unfiltered image on natural daylight film has a certain appeal for
me, of which this image is a classic example. The Ha regions seem to be
very well recorded - besides, Ha is only one aspect - there is a lot else
going on in this image which notch-filtering of Ha wouldn't help, including
the Witch Head nebula.
--Philip
At 06:03 31/03/2005 -0500, you wrote:
>Hi Wei-Hao,
>A beautiful rendition of this region. I like the stars and in particular the
>nice compact starfield in the upper left....I haven't seent this before.
>One comment though is the weakness of the h-alpha emission even from
>a dark sky like yours. Really only narrowband h-alpha imaging can bring
>the faint emission out.
>Rob Gendler
>email: robgendler@att.net
>Web Site: http://www.robgendlerastropics.com
Philip Perkins
<ppastro2@astrocruise.com>
Wiltshire UK & Luberon France
www.astrocruise.com
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