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Messages 1124 - 1153 of 1656   Oldest  |  < Older  |  Newer >  |  Newest
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1124
Seen some impressive spectrae in the files and photos section. How large a scope is needed to produce informative spectra of 3rd or 4th mag stars? How about...
Jim Ferreira
oldfrankland
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Jun 8, 2008
1:45 am
1125
Hi Jim, ... 4th mag stars? Well it depends on your camera and somewhat on the dispersion you use (How far you mount the grating from the CCD) but with low...
staranalyser
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Jun 8, 2008
1:44 pm
1126
Hi Jim, it's nice to see you evolving your interest into spectroscopy. It seems to be the "natural" evolution after doing pretty picture astronomy. I think you...
ssb73q
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Jun 8, 2008
7:39 pm
1127
Hi Richard Actually, the interest in spectroscopy is an expansion of my off and on work in photoelectric photometry; eruptive variables. As for the 'pretty...
Jim Ferreira
oldfrankland
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Jun 9, 2008
7:08 pm
1128
Most informative, Robin. Thanks. How does seeing conditions; specifically turbulance, affect resolution of spectral lines? Cheers, Jim Livermore CA ... or ......
Jim Ferreira
oldfrankland
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Jun 9, 2008
7:13 pm
1129
... Hi Jim, With a slitless setup (The simplest configuration) the resolution is dependent on the size of the star image, so seeing (and guiding if you are...
staranalyser
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Jun 10, 2008
12:23 am
1130
Hi Jim, what you can see for a given exposure with an Ha filter is typical of the Ha brightness in a spectrum. That should give you some idea of what the...
ssb73q
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Jun 10, 2008
6:13 pm
1131
Hi Richard, I will be most interested in hearing about your experiments with the PIN diode. I too have experimented with them, but have found the amplifier...
Jeff Hopkins
hposoft
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Jun 10, 2008
6:26 pm
1132
Hi Jeff, thanks for the information. I had considered using a photomultiplier, but was concerned with the high voltages, magnetic field effects, and risk of...
ssb73q
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Jun 10, 2008
6:53 pm
1133
Hi Jeff, BTW, I'm waiting for a avalanche PIN with wide spectral response to appear on eBay. Regards, Richard ... eBay ... doing ... <<snip>>...
ssb73q
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Jun 10, 2008
7:00 pm
1134
... some ... Hi Richard, That depends very much on the distribution of light across the spectrum. To take an extreme example, Wolf Rayet stars have ...
staranalyser
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Jun 10, 2008
10:59 pm
1135
... Well it is definitely OT since we have now even moved away from spectroscopy ;-) I would suggest continuing off list or moving the subject to a more ...
staranalyser
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Jun 10, 2008
11:13 pm
1136
Hi Robin, ok, back to SA spectroscopy, but another harebrain thought? I wonder if it would make any sense to use high transmission RGB filters to increase the...
ssb73q
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Jun 11, 2008
3:39 pm
1137
No, it won't. Why should it ? They just block light in and out of band that could be used for increasing the SNR of the spectra. The only usefull applications...
Wolfgang Renz
aavso_rwg
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Jun 11, 2008
6:22 pm
1138
Hi Richard, Wolfgang, It is rare for me to disagree with Wolfgang ;-) but in fact pre filtering does have a potential advantage with slitless spectroscopy in a...
staranalyser
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Jun 11, 2008
11:20 pm
1139
Hi Robin I thought about light pollution too. But using a filter helps then just if the filter excludes all the major local light pollution emission lines. But...
Wolfgang Renz
aavso_rwg
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Jun 12, 2008
12:42 am
1140
Hi Robin, thanks for the reply and information. That was my sense for maximizing seeing deep by increasing the S/N and using a more sensitive mono camera than...
ssb73q
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Jun 12, 2008
3:06 am
1141
Hi Richard, One limitation of imaging RGB filters would be that they do not have sharp cut offs so the sensitivity is dropping away from the centre wavelength....
staranalyser
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Jun 12, 2008
11:33 am
1142
Hi Robin, as a extension of the increased S/N result by narrowing the bandpass, is there any useful astro LRS spectrometry application to see dimmer object's...
ssb73q
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Jun 12, 2008
12:02 pm
1143
Hi Robin, BTW, I forgot to add in my last post that interference type RGB filters do have sharp cutoff, see: http://panther-observatory.com/Baader_LRGB.htm ...
ssb73q
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Jun 12, 2008
12:08 pm
1144
... Hi Wolfgang, I have added a copy to my folder in the files section http://tech.groups.yahoo.com/group/staranalyser/files/User_Folders/robi ...
staranalyser
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Jun 12, 2008
1:56 pm
1145
Hi Robin, well, you made it home safely as I can see. You got an efficiency curve for the SA in the files section. Could you let me know how you actually did...
dieterkuespert
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Jun 14, 2008
2:20 pm
1146
Hi Dieter, Yes we had a great time meeting everyone at the spectroscopy conference in Heidelberg and later, touring that area of the country. I had to dig into...
staranalyser
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Jun 15, 2008
11:47 am
1147
Hi Robin Thx for showing us your work. Have you thought about using an other long pass filter that starts at a shorter wavelength ? e.g. the 495 or the 570 nm...
Wolfgang Renz
aavso_rwg
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Jun 15, 2008
3:18 pm
1148
Hi Wolfgang, ... at ... filters ? ... red stars ... The choice of cut off was largely based on Brian's advice. ...
staranalyser
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Jun 15, 2008
6:30 pm
1149
Hi Wolfgang, "why should it?" Let me walk you though the issue. Let's assume that a certain sky condition limits the maximum exposure time for a given object...
ssb73q
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Jun 15, 2008
6:43 pm
1150
Hi Robin, I think that trying a light pollution filter like the Baader UHC-S for PNs may have merit? They would pass all the useful emission lines while...
ssb73q
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Jun 15, 2008
7:18 pm
1151
Hi Richard, It has a rather strange response curve in the 600-900nm range of interest for this application though. http://www.baader- ...
staranalyser
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Jun 15, 2008
8:36 pm
1152
Hi Robin, I agree, I wasn't thinking beyond ~700nm. All the LPRs I have spectrophotometer tested have erratic behavior beyond ~700nm. However, in the visible,...
ssb73q
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Jun 15, 2008
9:15 pm
1153
Hi Robin Thx for your instructive explainations. ... With HPS dominated LP one longer than ~ 620 nm (even ~ 650 nm if one wants get rid of nearly all of it,...
Wolfgang Renz
aavso_rwg
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Jun 16, 2008
5:14 pm
Messages 1124 - 1153 of 1656   Oldest  |  < Older  |  Newer >  |  Newest
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