I now have a Canon 1000D bought off EBay which I aim to modify and use purely for astrophotography. Before I modify and bugger it up I'm going to perform some basic tests - read noise/bias/darks etc. as I think it would be useful for those considering using one if these for the same purpose.
All noise reduction turned off etc, etc...
Notes frame sizes and download times:
EOS1000D: 3906 x 2602 pixels, CR2 file size 8,578kb, download time approx 2s
EOS450D : 4290 x 2856 pixel, CR2 file size 11,317kb, download time approx 3s
Both cameras set to ISO 800
Bias frames:
20 x 1/4000s taken at 1 intervals
Taking the 10th frame from each camera, just straight conversion in MaximDL with no scaling.
EOS450D
Red Green Blue
Maximum: 2076 901 1370
Minimum : 0 518 0
Average : 1307 696 1061
Std Dev : 26.0 8.2 21.0
EOS1000D
Red Green Blue
Maximum: 418 222 361
Minimum : 0 125 0
Average : 326 174 264
Std Dev : 7.0 2.3 5.6
These are figures for the whole frame and whilst they don't tell us that much I can already see that the standard deviation of the noise on the 1000D is significantly lower. This may change when I do the dark frames over the weekend.
Next installment tomorrow will be read noise.
Robert
Very interesting Robert.
Robert,
Those figures are in ADUs. To make a meaningful comparison they both need to be measured in electrons. But you'll end up doing this anyway to calculate the read noise.
http://forum.orpington-astronomy.org.uk/index.php?topic=3473
Mark
Updated the original post with ISO.
Thanks for the feedback.
Interesting. Thanks Robert. The 1000D is one of the cameras I have been considering.
No hope for me then, I have a 450D
:!
It's purely a comparison Carole, I'm not sure which camera will work out better.
Strange the 1000 is reviewed as a detuned 450 or a tuned 400, sensor (mp) being the same as 400 but less than 450.
The sensors are the same physical size so the the 1000 has larger pixels than the 450 ?
That would suggest that bigger is better (in this case)
EOS 1000D pixels are 5.68 micron = 32.3 square microns
EOS 450D pixels are 5.15 micron = 26.5 square microns
You would think a small but significant difference however a lot is down to the sensor design. For example the 550D is supposed to be much better at low light than the 450D despite having tiny 4.17 micron pixels.
I read somewhere something along the lines of the lenses (?) being smaller allowing the pixels to be stacked closer on certain sensors. If that's the case then there would be less dead space and more area assigned to actually catching photons - I think
*Edit*
Where I read it -
http://www.dpreview.com/reviews/canoneos550d/ (http://www.dpreview.com/reviews/canoneos550d/)
(http://a.img-dpreview.com/reviews/canoneos550d/images/whatsnew/ML-001.jpg)
I'm afraid some of this technical stuff is beyond me. When you've finished Robert would you mind posting your results in non technical terms as well please.
Thanks
Carole
Well, I've finally got around to doing some measurements and am not getting the results I expected.
Firstly the saturation point of each of the colour channels is at a different ADU level:
R G B
450D 19014 10120 15429
1000D 4452 2370 3614
Remember the 450D has 14bit A-D converter whereas the 1000D has 12bit and because of that you would need to multiply the 1000D figures by 4 to give a 16bit equivalence.
This was measured using a very simple procedure.
1) Take a flat field image long enough to saturate each colour across the ccd (10s in this case)
2) Import to MaximDL and subtract the master bias (10 frames)
3) Convert to colour using the conversion routine for the camera model.
4) Measure the average pixel value in ADU's.
Because of this I thought it would be worthwhile calculating the gain and full well depth of each colour and these are the results. Intrigueingly the channels seem to be quite different when I would have expected them to be the same. There seem to be two possible explanations for this:
1) There are different gains for each channel.
2) I've made a mistake !
Working out the figures assuming I've done everything correctly:
Gain
===
450D
-----
Channel S Sigma Noise Variance Gain (e/ADU) Full well ADU's Well depth (e)
R 2603 76.45 54.06 2922.88 0.89 19014 16933
G 2358 42.48 30.04 902.42 2.61 10120 26443
B 3259 68.31 48.31 2333.63 1.40 15429 21547
1000D
------
Channel S Sigma Noise Variance Gain (e/ADU) Full well ADU's Well depth (e)
R 874 19.05 13.47 181.51 4.82 4452 21438
G 768 10.56 7.47 55.73 13.78 2370 32660
B 1058 17.16 12.13 147.24 7.19 3614 25968
The full well depth is just calculated by multiplying the gain by the saturation values above. The Gain is the number of electrons that represent one ADU (Analogue to Digital Unit).
All measurements made at ISO 200 in each camera.
On the face of it the 1000D has a higher well depth than the 450D but each ADU represents more electrons so there is less resolution in the signal.
Thoughts anyone ?
Next Step - Read noise.
Robert
Robert,
The gain for each channel should be the same and the well depths (in electrons) should be similar (though not identical because of the bias).
I think that colour balance scaling is being applied at some stage in your processing and this is upseting your calculations. An RGB colour balance multipliers of (1.9, 1.0, 1.5) are broadly correct for a "sunny day" colour balance. This is what you appear to be seeing with the RGB ratios in your saturated frames.
Mark
Thanks Mark
I was mulling that over when I wrote the message last night but then thought that the RAW's would not be affected by colour balance. I wonder whether MaximDL is applying some correction even though I made sure the scaling factors were 100% (ie. no change). This behaviour could explain a few things.
Will do some more digging...
Robert
I'm away at the end of the week so spent this evening removing the IR cut filter from the 1000D. It's now much more sensitive to IR. I still have all the figures from before the mod so will continue the calculations when I get the chance.
Robert
Well done!
Did you find it a complicated process?
Mark
You have done well there, Robert!
It quite easy thanks to the excellent Gary Honis video on youtube. I specifically bought a screwdriver that was an exact fit for the screws and that made taking it apart a breeze 8) The most tricky part was keeping the front glass clean. I managed to get a couple of flecks of dust on it and the act of wiping those off induced some static charge on the glass which then acted like a magnet to more dust on the other side, took me 20 mins to get the glass clear again ! In all the process took under 2 hours, not as quick as the video but not too bad either. I also managed to keep the IR filter in one piece. I could probably do it again in about 40 mins or less (for a filter removal) now I know what I'm doing. The most worrying part of the whole process was powering it back on afterwards... heart in mouth... but it worked thankfully!
Robert
I'm impressed Robert - Just watched the video - You can tell that Gary has done it a few times before... :-( Out of interest what did you replace the filter with?
John
Thanks John, I didn't replace the filter, it was a removal only job. Less glass = less refractions = less reflections.
Robert
P.S. It's good to see you posting again :)
Thks. So does that mean camera is an astro only job or will you still be able to manually focus using lenses..?
Well, it does focus though not so accurately, I guess it depends what you're focusing on. Anything with a depth of field might be ok but in any case manual focus still works.
Robert
Just bought me a 450D, before viewing the video. :o should be interesting. Any tips Robert?
Yep, Make sure you do it in as dust free an environment as possible (a damp rag helps) and ensure the screwdriver is a perfect fit. If you can earth yourself too then the dust won't be as attracted to the parts you want to keep clean. Otherwise be careful not to mix the screws up, I grouped them in the order I took the camera apart which makes life easy when reversing the process.
It's not that difficult but if you get any dust on the glass then it's a real pain.
Robert
Thanks Robert I'll look forward to that :-?