![]() |
|
|
Thread Tools | Display Modes |
#1
|
|||
|
|||
![]()
well done. I found your technical notes very good.
Jerry Robin Leadbeater wrote: Hi, I am not a regular contributor to this group but I posted this on uk.sci.astronomy yesterday and it was felt it warranted a wider audience, so here goes! I have been attempting to record the optical pulses from the pulsar in M1 using a strobe technique and my home built CCD camera. It has been tough extracting it from the noise but I am fairly convinced I have managed it. I have done a bit of searching and I cannot find any record on the web at least of this having been done on an amateur basis before, but I expect to be proved wrong ;-) It is certainly an interesting and challenging project though! You can see images of the Pulsar 'on' and 'off ' at my site here http://www.leadbeaterhome.fsnet.co.u...o_image_33.htm and there is a link from there to pages which explain the technique and go into the results in more detail Clear Skies, Robin www.leadbeaterhome.fsnet.co.uk/astro.htm |
#2
|
|||
|
|||
![]()
Nice job, Robin. I wonder if a BW TV camera would be able
to pick this up on a 16" telescope... Eric. You can see images of the Pulsar 'on' and 'off ' at my site here http://www.leadbeaterhome.fsnet.co.u...o_image_33.htm |
#3
|
|||
|
|||
![]()
In article , matt
wrote: it seems like the ideal equipment would be a long exposure camera with an electronic or electronically controlled separate shutter . Modulate the shutter with a 30Hz PWM signal over a long exposure , then change PWM phase 180deg (maintain the 30Hz timebase coherence) and do another exposure . That's what these people are doing, using an electronicly-controlled motor driving a disk with a slot in it. (Something like an LCD electronic shutter would be too slow. A micromirror array could probably respond fast enough, but is a lot more complicated to put together.) One way to do this more efficiently, doing all phases in one exposure, would be to jitter the camera at the right frequency. Maybe spinning a thin slanted piece of glass so that the image moves on the film plane in a small circle. Maybe an off-center weight on the shaft of a motor attached to the camera, using the flexibility of the telescope. -- David M. Palmer (formerly @clark.net, @ematic.com) |
#4
|
|||
|
|||
![]() "Eric" wrote in message ... Nice job, Robin. I wonder if a BW TV camera would be able to pick this up on a 16" telescope... Eric. Hi Eric, You would still need some sort of strobe technique as the frame rate would not be fast enough to catch the 30/sec double pulse. I suspect it would not be sensitive enough either. I have a very sensitive camera and it needs a few seconds exposure to catch the mag 16 pulsar. To catch it in a 1/60sec frame I estimate would have needed at least 100x more light ie an 80 inch scope. I would not mind having a try though if you know where I can borrow one ;-) Robin -- ---------------------------------------------------------------- Robin Leadbeater N54.75 W3.24 www.leadbeaterhome.fsnet.co.uk/astro.htm ---------------------------------------------------------------- |
#5
|
|||
|
|||
![]() "David M. Palmer" wrote in message ... One way to do this more efficiently, doing all phases in one exposure, would be to jitter the camera at the right frequency. Maybe spinning a thin slanted piece of glass so that the image moves on the film plane in a small circle. Maybe an off-center weight on the shaft of a motor attached to the camera, using the flexibility of the telescope. Hi David, ISTR someone suggesting I try that, (not you was it?) but there are a lot of other structures at similar brightness close to the pulsar in the crab so I suspect it might disappear into the background once everything gets shaken about. Also I think you would need to be super accurate with your speed to avoid smearing. By taking shorter exposures and stacking to increase signal to noise, you can tolerate small drifts in frequency. Should work for an isolated object though. It is certainly a very elegant idea Clear Skies Robin -- ---------------------------------------------------------------- Robin Leadbeater N54.75 W3.24 www.leadbeaterhome.fsnet.co.uk/astro.htm ---------------------------------------------------------------- |
#6
|
|||
|
|||
![]()
The strobe wheel technique was used at Lick Observatory to produce the first
pictures showing the pulsar pulsing and thus also confirming which star it was in the field. However the first, days earlier, identification of that star was done at Kitt Peak National Observatory by using a small pinhole aperture to isolate the star at the focus of the 84-inch telescope. The detection of the pulses for that was by a photomultiplier with its output being signal averaged synchronous with the pulsar repetition rate. This same technique was used with a 36-inch telescope for the very first detection of the optical pulses from the Crab pulsar by Steward Obs. of the Univ. of Arizona.. Don "William C. Keel" wrote: In sci.astro.amateur Robin Leadbeater wrote: "Eric" wrote in message ... Nice job, Robin. I wonder if a BW TV camera would be able to pick this up on a 16" telescope... Eric. Hi Eric, You would still need some sort of strobe technique as the frame rate would not be fast enough to catch the 30/sec double pulse. I suspect it would not be sensitive enough either. I have a very sensitive camera and it needs a few seconds exposure to catch the mag 16 pulsar. To catch it in a 1/60sec frame I estimate would have needed at least 100x more light ie an 80 inch scope. I would not mind having a try though if you know where I can borrow one ;-) This may be a case for the long-forgotten art of the mechanical strobe disk, eliminating the need for rapid readout or 100% efficiency. That's how the pulsar was first identified with a particularly optical object, using an intensified TV camera. Getting the timing and phasing right are left as exercises for folks who (unlike me) know how to do it. Bill Keel |
#7
|
|||
|
|||
![]() "William C. Keel" wrote in message ... This may be a case for the long-forgotten art of the mechanical strobe disk, eliminating the need for rapid readout or 100% efficiency. That's how the pulsar was first identified with a particularly optical object, using an intensified TV camera. Getting the timing and phasing right are left as exercises for folks who (unlike me) know how to do it. Bill Keel Hi Bill, Yep, that's the way I did it. See http://www.leadbeaterhome.fsnet.co.u...etection_1.htm Robin |
#8
|
|||
|
|||
![]() "Eric" wrote in message ... Robin Leadbeater wrote: "Eric" wrote in message ... Nice job, Robin. I wonder if a BW TV camera would be able to pick this up on a 16" telescope... Eric. Hi Eric, You would still need some sort of strobe technique as the frame rate would not be fast enough to catch the 30/sec double pulse. I suspect it would not be sensitive enough either. I have a very sensitive camera and it needs a few seconds exposure to catch the mag 16 pulsar. To catch it in a 1/60sec frame I estimate would have needed at least 100x more light ie an 80 inch scope. I would not mind having a try though if you know where I can borrow one ;-) I'm just writing things down quickly - 29.804 Hz and 30.0 Hz gives a 0.196 Hz beat frequency. This is about 5.113 s. At 30 fps, that's 153ish frames. If I average 9 frames at a time, I get 17 frames per beat period. 9 frames at 30 fps is about 1/3 s exposure. I know we can get the central star in the ring with a 1s exposure, so if I gather frames for 30ish seconds, I might be able to pull it out of the noise. Have I missed anything really terrible ? Eric. Hi Eric, If Pat's figure (up thread) of 40 photons in a 3.9m scope is right you are going to be down to less than 1 photon per video frame in a 16inch so it could be tough to pull it out of the noise. But the big problem is that your video shutter is open for 1/30 sec for each frame so there will be only a few frames without the main pulse in them. (2 in 300 I think, even if the pulse is very sharp) Another complication is the pulsar actually produces a smaller intermediate pulse. (ie a pulse every 1/60 sec, alternately large and small) which will degrade the on/off difference further. Can you see the (mag15?) ring central star in a stack of 1/30sec video frames? If so you will know you are at least in the right sensitivity ballpark. Robin |
Thread Tools | |
Display Modes | |
|
|
![]() |
||||
Thread | Thread Starter | Forum | Replies | Last Post |
First-Known Double Pulsar Opens Up New Astrophysics (Forwarded) | Andrew Yee | Astronomy Misc | 6 | January 19th 04 11:49 PM |
Outer Space/NASA Pictures | . | Space Station | 0 | September 8th 03 04:03 PM |
Outer Space Pictures | . | Space Station | 0 | September 8th 03 03:51 PM |
Whats in the sky today | tmc@anospammingcarrari.org | Amateur Astronomy | 3 | July 14th 03 04:24 AM |
Einstein's Gravitational Waves May Set Speed Limit For Pulsar Spin | Ron Baalke | Astronomy Misc | 1 | July 3rd 03 08:49 AM |