H-alpha 30092018, first light asi290mm
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H-alpha 30092018, first light asi290mm
Bought a new camera, the ZWO ASI290mm. ZWO confirmed that the fact that it has a rolling shutter does not affect its capabilities of H-alpha imaging.
+ Compared with the PGR 174, I don't need a 2x barlow to achieve the same image scale.
+ Less weight, now I don't need the 2 degrees wedge and the barlow
+ A lot of light to work with, quite sensitive!
+ imaging without a barlow and a wedge makes everything a bit easier. Less reflections etc.
- FPS is lower than with the PGR.
Seeing was bad today, with an exposure between 3 to 6 ms, I was not able to get any useful avi's. Normal set up, so:
160mm D-Erf - 150 mm f/8 SW - 1,25x Glasspath - Baader 35nm H-alpha - pst etalon - Lunt BF1200.
Took out the blue glass of the Lunt BF1200 and tried again. Wow, that is a whole different ballgame. Exposure of about 0,3 ms (!). If I up the gain, artefacts appear, so it is a bit too fast. Have a ND0.6 filter on the post, but today worked without it. Between 1,0 - 1,5 ms is what I will be aiming at.
Two examples, not the best, but the best I could manage under these circumstances. Interesting camera!
30092018_11h41m_SW150_GP1,25_ASI290mm_ps_gradient by bart moors, on Flickr
30092018_11h45m_SW150_GP1,25_ASI290mm_PS by bart moors, on Flickr
+ Compared with the PGR 174, I don't need a 2x barlow to achieve the same image scale.
+ Less weight, now I don't need the 2 degrees wedge and the barlow
+ A lot of light to work with, quite sensitive!
+ imaging without a barlow and a wedge makes everything a bit easier. Less reflections etc.
- FPS is lower than with the PGR.
Seeing was bad today, with an exposure between 3 to 6 ms, I was not able to get any useful avi's. Normal set up, so:
160mm D-Erf - 150 mm f/8 SW - 1,25x Glasspath - Baader 35nm H-alpha - pst etalon - Lunt BF1200.
Took out the blue glass of the Lunt BF1200 and tried again. Wow, that is a whole different ballgame. Exposure of about 0,3 ms (!). If I up the gain, artefacts appear, so it is a bit too fast. Have a ND0.6 filter on the post, but today worked without it. Between 1,0 - 1,5 ms is what I will be aiming at.
Two examples, not the best, but the best I could manage under these circumstances. Interesting camera!
30092018_11h41m_SW150_GP1,25_ASI290mm_ps_gradient by bart moors, on Flickr
30092018_11h45m_SW150_GP1,25_ASI290mm_PS by bart moors, on Flickr
Last edited by bart1805 on Sun Sep 30, 2018 6:06 pm, edited 1 time in total.
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Re: H-alpha 30092018, first light asi290mm
Great results with beautiful details, Bart ! I was out this morning shooting AR2723 also.... still processing images.
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Re: H-alpha 30092018, first light asi290mm
Thanks Apollo. Hope to be able to make an animation before solar season is over for me.
Next time will also try with the lens piece of the Baader Q-turret barlow in the nosepiece of the ASI. Will result in about f/14. Curious if Newton Rings will appear.
Next time will also try with the lens piece of the Baader Q-turret barlow in the nosepiece of the ASI. Will result in about f/14. Curious if Newton Rings will appear.
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Re: H-alpha 30092018, first light asi290mm
I very much like the soft processing of your first image, Bart. For a first image with the new camera I think it it incredibly good !
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Re: H-alpha 30092018, first light asi290mm
Hi Marty,
Baader D-Erf. It does exactly what it should do.
Bart.
Baader D-Erf. It does exactly what it should do.
Bart.
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Re: H-alpha 30092018, first light asi290mm
Hi, Bart
Congratulations on your new instrument and great first results.
I had some questions about your BF mod and the camera itself.
Is the blue glass on the telescope side of the BF1200? I can tell that the glass on the camera side of the BF1200 the glass is red on my BF1200 but I can't see the glass color on the telescope side or whether it's in an internal location. I want to know because I'm looking for ways of getting faster shutter speeds on my high res setups. I only do imaging with no visual work.
I've had poor luck with 2 of the 3 ZWO cameras I've bought. They suffered from "fixed pattern noise" which shows up sometimes as a pattern of small rectangles like the mesh on a screen door. ZWO's advice was to keep the gamma at 50 (neutral for ASI cameras), a very limiting solution which didn't really work anyway. Have you noticed this problem with your 290? Thanks
Lou (gabrieli)
Congratulations on your new instrument and great first results.
I had some questions about your BF mod and the camera itself.
Is the blue glass on the telescope side of the BF1200? I can tell that the glass on the camera side of the BF1200 the glass is red on my BF1200 but I can't see the glass color on the telescope side or whether it's in an internal location. I want to know because I'm looking for ways of getting faster shutter speeds on my high res setups. I only do imaging with no visual work.
I've had poor luck with 2 of the 3 ZWO cameras I've bought. They suffered from "fixed pattern noise" which shows up sometimes as a pattern of small rectangles like the mesh on a screen door. ZWO's advice was to keep the gamma at 50 (neutral for ASI cameras), a very limiting solution which didn't really work anyway. Have you noticed this problem with your 290? Thanks
Lou (gabrieli)
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Re: H-alpha 30092018, first light asi290mm
Hi Lou,
Thanks!
Here is an interesting thread on the blue glass of the Lunt Blocking filter:
https://www.cloudynights.com/topic/6153 ... y-lunt-bf/
On the camera sideyou are looking at the blocking filter.
I can see that pattern when the exposure is very, very short. 0,3ms is very fast. On the dangerous side I would say. So will try out the ND0.6 filter.
CS! Bart.
Thanks!
Here is an interesting thread on the blue glass of the Lunt Blocking filter:
https://www.cloudynights.com/topic/6153 ... y-lunt-bf/
On the camera sideyou are looking at the blocking filter.
I can see that pattern when the exposure is very, very short. 0,3ms is very fast. On the dangerous side I would say. So will try out the ND0.6 filter.
CS! Bart.
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Re: H-alpha 30092018, first light asi290mm
Lou,
On both the ASI 174MM and the ASI 160MM, I work at zero gamma (=50) with Firecapture. Adjust the ROI to give the best coverage and then adjust the Gain to give a good histogram....seems to work for me....
On both the ASI 174MM and the ASI 160MM, I work at zero gamma (=50) with Firecapture. Adjust the ROI to give the best coverage and then adjust the Gain to give a good histogram....seems to work for me....
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Re: H-alpha 30092018, first light asi290mm
Thanks, should have mentioned that, don't do this if you go visual.
It seemed to be a much bigger reduction than 50%. Will put it on the "check it next time list".
It seemed to be a much bigger reduction than 50%. Will put it on the "check it next time list".
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Re: H-alpha 30092018, first light asi290mm
Using a Baader D-ERF up front and a secondary mini ERF another Baader ERF I think gives more “protection “ than the original blue glass filter element.
"Astronomical Spectroscopy - The Final Frontier" - to boldly go where few amateurs have gone before
https://groups.io/g/astronomicalspectroscopy
http://astronomicalspectroscopy.com
"Astronomical Spectroscopy for Amateurs" and
"Imaging Sunlight - using a digital spectroheliograph" - Springer
https://groups.io/g/astronomicalspectroscopy
http://astronomicalspectroscopy.com
"Astronomical Spectroscopy for Amateurs" and
"Imaging Sunlight - using a digital spectroheliograph" - Springer
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Re: H-alpha 30092018, first light asi290mm
Thanks, SkyBurner
I was very aware of potential eye damage in removing the blue glass.
I only do imaging since in my area good skies are very rare.
I read somewhere that using 3.8 density solar film instead of 5.0 density solar film results in a 4 f stop increase in light passed and that is recommended
for photographic use only. The 50% reduction in Ha quoted above with the blue glass in place suggests much less than that when the blue glass is removed.
My shutter speeds, especially when double stacking, are in the range of 15 to 25 ms and that is often with gain turned up.
So, when I hear that some people are achieving 3 - 5ms, I want to know what they are doing to reach these fast speeds.
I know some rare PST etalons are very bright and give very uniform results by the two I have are not in that category.
Lou
I was very aware of potential eye damage in removing the blue glass.
I only do imaging since in my area good skies are very rare.
I read somewhere that using 3.8 density solar film instead of 5.0 density solar film results in a 4 f stop increase in light passed and that is recommended
for photographic use only. The 50% reduction in Ha quoted above with the blue glass in place suggests much less than that when the blue glass is removed.
My shutter speeds, especially when double stacking, are in the range of 15 to 25 ms and that is often with gain turned up.
So, when I hear that some people are achieving 3 - 5ms, I want to know what they are doing to reach these fast speeds.
I know some rare PST etalons are very bright and give very uniform results by the two I have are not in that category.
Lou
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Re: H-alpha 30092018, first light asi290mm
Good images with the new camera
http://brierleyhillsolar.blogspot.co.uk/
Solar images, a collection of all the most up to date live solar data on the web, imaging & processing tutorials - please take a look!
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Re: H-alpha 30092018, first light asi290mm
Thanks Eric and Marc.
@Lou: your pictures of 15 august were taken with an exposure of 15-25 ms? Gamma at neutral?
3-5 ms for DS H-alpha is something I was never able to do with the PGR camera. Will try it out with the 290MM.
@Lou: your pictures of 15 august were taken with an exposure of 15-25 ms? Gamma at neutral?
3-5 ms for DS H-alpha is something I was never able to do with the PGR camera. Will try it out with the 290MM.
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Re: H-alpha 30092018, first light asi290mm
Nice results Bart
I have the color version
I have the color version
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Re: H-alpha 30092018, first light asi290mm
Fantastic first light, looks a very good camera
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Re: H-alpha 30092018, first light asi290mm
Hi, Bart
The August 15 images were taken at 25 ms (25000µs on the settings for my Blackfly S) with both gamma and gain turned up. I used a Lunt152 + a Quark Chromosphere working at f/25. The scene had bright highlights.
The 3 - 5 ms shutter speeds I was referring to were for single PST high transmission etalons as you seem to be using.
Lou
The August 15 images were taken at 25 ms (25000µs on the settings for my Blackfly S) with both gamma and gain turned up. I used a Lunt152 + a Quark Chromosphere working at f/25. The scene had bright highlights.
The 3 - 5 ms shutter speeds I was referring to were for single PST high transmission etalons as you seem to be using.
Lou
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Re: H-alpha 30092018, first light asi290mm
Hi Lou, how high is the QE of your camera at the H-alpha wavelength? I think it could be way lower than the QE of the 290mm. CS! Bart.
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Re: H-alpha 30092018, first light asi290mm
Hi, Bart
From the FLIR spec sheet on their website the QE for the Blackfly S (5.1 MP) is 76 at 525nm. The QE of your 290 is stated as 80 on the ZWO site but the
wavelength is not specified.
Lou
From the FLIR spec sheet on their website the QE for the Blackfly S (5.1 MP) is 76 at 525nm. The QE of your 290 is stated as 80 on the ZWO site but the
wavelength is not specified.
Lou
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Re: H-alpha 30092018, first light asi290mm
Hi Bart...
Very sharp images with the ASI290...well done
I have used my 290 on a limited basis on the shorter focal length scopes to match the pixel size. It is primarily used on the C14 for planetary imaging...nice resolution with no need for barlows!
Trying to interpret the QE of the CMOS chips is a hassle...they tell us the wavelength with the maximum sensitivity and show the response curve with the most sensitive set as 100% . It is more useful when they tell you the QE of the most sensitive part and you can do the math form there. I always liked the absolute QE data supplied on the CCD's.
Brian
Very sharp images with the ASI290...well done
I have used my 290 on a limited basis on the shorter focal length scopes to match the pixel size. It is primarily used on the C14 for planetary imaging...nice resolution with no need for barlows!
Trying to interpret the QE of the CMOS chips is a hassle...they tell us the wavelength with the maximum sensitivity and show the response curve with the most sensitive set as 100% . It is more useful when they tell you the QE of the most sensitive part and you can do the math form there. I always liked the absolute QE data supplied on the CCD's.
Brian
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Maple Ridge Observatory
Cambray, ON Canada
Photos: https://www.flickr.com/photos/185395281@N08/albums
10'x15 Roll-off Roof Observatory
Takahashi EM400 Mount carrying:
C14 + Lunt 80ED
Deep Sky Work - ASI294MM Pro+EFW 7x36/Canon 60D (Ha mod), ONAG
Planetary Work - SBIG CFW10, ASI462MM
2.2m Diameter Dome
iOptron CEM70G Mount carrying:
Orion EON 130ED, f7 OTA for Day & Night Use
Ha Setup: Lunt LS80PT/LS75FHa/B1200Ha + Home Brew Lunt Double Stack/B1800Ha on the Orion OTA + Daystar Quantum
WL, G-Band & CaK Setup: Lunt Wedge & Lunt B1800CaK, Baader K-Line and Altair 2nm G-Band filter
ASI1600MM, ASI432MM, ASI294MM Pro, ASI174MM, ASI462MM
Maple Ridge Observatory
Cambray, ON Canada
Photos: https://www.flickr.com/photos/185395281@N08/albums
10'x15 Roll-off Roof Observatory
Takahashi EM400 Mount carrying:
C14 + Lunt 80ED
Deep Sky Work - ASI294MM Pro+EFW 7x36/Canon 60D (Ha mod), ONAG
Planetary Work - SBIG CFW10, ASI462MM
2.2m Diameter Dome
iOptron CEM70G Mount carrying:
Orion EON 130ED, f7 OTA for Day & Night Use
Ha Setup: Lunt LS80PT/LS75FHa/B1200Ha + Home Brew Lunt Double Stack/B1800Ha on the Orion OTA + Daystar Quantum
WL, G-Band & CaK Setup: Lunt Wedge & Lunt B1800CaK, Baader K-Line and Altair 2nm G-Band filter
ASI1600MM, ASI432MM, ASI294MM Pro, ASI174MM, ASI462MM