23:01 | guesst | in theory you can do flat field correction in the fpga
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23:02 | Bertl | that's not really the problem, and I think, for now, it can be done in the post processing (which wasn't done with this image)
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23:05 | guesst | i think the image got quite a lot of post to oversaturate the colors.. fpn should be fixed first :)
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23:12 | danH | joined the channel | |
23:13 | Bertl | welcome danH!
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23:14 | Bertl | guesst: agreed, btw, in the image you referred to with sebastian, I see a similar horizontal and vertical pattern in the almost black background as we see with the CMV12k
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23:14 | Bertl | did you address this issue yet and if, how did you address it?
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23:15 | danH | changed nick to: danhanes
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23:15 | danhanes | Hello Bertl - Thanks for the welcome. I would like to join the development party - hw, sw, optics - how can I help ?
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23:16 | Bertl | sounds good, there is quite a lot to do, where do you see your specialities?
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23:17 | danhanes | Well, my IRC is a bit rusty :) But I have a good bit of C background (embedded), HW - logic, analog, smps. And optics.
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23:18 | se6astian | left the channel | |
23:18 | Bertl | okay, did you take a good look at what we did so far? hardware and software wise?
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23:19 | guesst | Bertl: there is just noise from inadequate lighting
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23:19 | danhanes | Yes, I have read all of the IRC logs - really a great way to get a sense of the development trajectory so far. I've looked at some of the VHDL
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23:20 | Bertl | guesst: I clearly see 'fabric like' noise, i.e. row and column specific noise which isn't directly related to the lighting (I hope :)
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23:20 | Bertl | danhanes: okay, so you're comfortable with FPGA development as well?
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23:21 | danhanes | I would not say that I am comfortable, at least not at your level. I did a fair bit with some Altera parts a few years ago.
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23:21 | danhanes | I would like to get into the Apertus code, but I don't want to hold anything up.
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23:22 | Bertl | it is a steep learning curve in any case, but IMHO that's part of the fun :)
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23:23 | guesst | Bertl: there is one horizontal line i know of (it is not a production piece, just a sample) - and the noise you see is dynamic.. comparing several frames
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23:23 | Bertl | danhanes: so, on the harware side, there is not much left for the axiom alpha (the prototype), i.e. we are fairly complete there
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23:23 | danhanes | Indeed, I am working on understanding what you have. It will be a few weeks before I can contribute, I suspect.
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23:24 | Bertl | guesst: do you mind if I mark the issues I'm seeing and upload that somewhere?
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23:24 | guesst | do it
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23:24 | Bertl | because I'm curious where those artefacts come from, as we see them as well
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23:28 | Bertl | danhanes: that leaves the software part, for alpha at least, and there I guess the main part is FPGA after all, but we also have written and still need a bunch of helper tools to make it work properly
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23:29 | danhanes | probably best for me to start with some tools that are not on the critical path. I am sure there will be plenty to do on the FPGA side once I come up to speed.
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23:30 | Bertl | if you are interested in the FPGA part, I'd suggest to install vivado 2013.4 and check out this branch: https://github.com/apertus-open-source-cinema/alpha-software/tree/checker/cmv_des
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23:30 | danhanes | Yes, I was going to ask if you were using the ISE or had switched entirely to Vivado.
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23:30 | Bertl | it contains the (almost) up to date (I'll commit the pending changes soon) recent code to capture images
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23:31 | Bertl | do you have access to a zedboard or anything using a zynq?
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23:31 | danhanes | Not yet. Looks like a zynq is in the near future.
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23:32 | danhanes | I seem to remember a discussion on the '30 vs the '20 xilinx parts. Are you going to switch, and does the (affordable) vivado suppor it ??
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23:34 | Bertl | yes, we are making sure that the WebPack (i.e. the 'free' as in beer) version of vivado will cover the parts we are using
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23:34 | danhanes | great!
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23:34 | Bertl | we are looking at the 7030 and the newest addition the 7015
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23:35 | Bertl | because they both support 4 high speed serial tranceivers
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23:35 | Bertl | i.e. a little more than 6Gbit per channel
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23:36 | danhanes | Haven't looked at the 7015 - i'll check it out. 6G per channel is impressive. 6G SDI ?
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23:39 | Bertl | yes, that's the idea, but supports different protocols as well
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23:39 | guesst | where you would connect a 6G SDI ? :) there is barely 3G capable equipment
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23:39 | Bertl | ah, there is quite a number of recorders out there for dual 3G SDI and such
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23:40 | guesst | yes, if we forget the price :)
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23:42 | Bertl | it seems, you can get equippment for 2-4k USD already
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23:42 | Bertl | which is not so much if you want to record 4k at higher frame rates
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23:43 | guesst | which one?
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23:56 | Bertl | for example the Odyssey7 starts at 1300 USD
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23:57 | Bertl | granted, it wont do 6G SDI at that price :)
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23:59 | guesst | it hardly does 4k at that price :)
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00:00 | Bertl | sure, but the 7Q for example costs about 1k more and does quite well
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00:00 | Bertl | not saying those are the only ones, just as example
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00:01 | Bertl | I'm sure sebastian can give you a few more examples when he gets back
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01:05 | Bertl | danhanes: so, in general, if something is unclear, please ask, I might not always answering immediately but I'll make sure to get back to you
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01:06 | Bertl | for specific tasks on our todo list, there is a wiki page, and if you are interested in helping with the fpga part, contact me personally for small subprojects/tasks
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01:09 | danhanes | Thanks Bertl - I'm downloading Vivado now - slooooow. I look forward to getting to the point that I can help. I'll try to minimize the questions.
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01:10 | Bertl | yeah I always suggest, spend a few minutes on an issue/question and see if you can figure it out, if not, just ask, often it can be easily explained and saves a lot of time searching for a solution
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01:11 | Bertl | this is especially true for FPGA related stuff, I've spent a lot of time already figuring out trivial things, no need to repeat that without good reason
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01:12 | danhanes | Right. You guys have done a very impressive amount of work in a really short time. I'm impressed.
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01:12 | danhanes | Seems the Zedboards are in short supply - 3 weeks.
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01:13 | Bertl | also check out the microzed and maybe alternative zynq based boards
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01:13 | Bertl | I don't think that it really matter much, unless you plan to build/buy a sensor frontend as well
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01:14 | danhanes | I would hope to add a sensor at some point - but maybe best to get going with a microzed for now.
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01:14 | Bertl | for example the zybo looks quite interesting
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01:14 | danhanes | I'll have a look
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01:14 | Bertl | not sure what documentation is provided though, as it isn't open as the zedboard
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01:15 | Bertl | (but I guess they will provide a schematic at least, haven't checked yet though)
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01:15 | danhanes | I suspect I will need a little hand holding getting the platform up at first. I seems that is always the hardest part of any development - getting the tools working.
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01:15 | Bertl | an it features a HDMI interface, which is missing on the microzed
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01:16 | danhanes | HDMI seems critical
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01:16 | Bertl | in my experience it was kind of painless actually
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01:16 | danhanes | That's encouraging
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01:16 | Bertl | I downloaded the full version, installed it on my linux box (in a changeroot) and that's it for the tools
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01:17 | Bertl | the hardware driver is a little more tricky (for jtag) to get working first, but that is documented on the wiki (now)
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01:17 | danhanes | Good - maybe I will be up an running soon. What distro are you using ?
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01:18 | Bertl | mageia, but folks reported ubuntu and fedora as working as well
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01:18 | Bertl | you might also be interested in building one or two of the PMOD debug modules we designed
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01:19 | Bertl | they are quite useful in my experience, and they should for example work just fine on the zybo
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01:19 | danhanes | I use Ubuntu virtualized on my Mac. I may need to dust off the dedicated Linux box sitting in the corner.
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01:19 | Bertl | it might be a good idea, not sure, maybe the tools work on OSX as well
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01:19 | danhanes | I saw some material on the pmod boards. Simple LED arrays really helpful at times.
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01:20 | Bertl | yes, I've used them in countless cases to debug/visualize/check stuff
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01:20 | Bertl | I also got one of those OLS boards to check some things at higher speeds
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01:21 | danhanes | OLS ?
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01:21 | Bertl | http://dangerousprototypes.com/open-logic-sniffer/
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01:21 | Bertl | they are cheap and not very powerfull, but easy to handle and they work just fine for simple stuff
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01:21 | danhanes | Cool. More toys.
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01:22 | danhanes | Haven't seen that site before
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01:22 | danhanes | Good stuff there
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01:23 | Bertl | btw, the PMOD boards are available via OSHpark (the PCBs, you still have to solder on the parts)
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01:24 | danhanes | I was going to ask. I saw a reference to OSHpark in the logs. Do they have the files on hand - I can just order ?
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01:26 | Bertl | yes, you can directly order a pack of three (or multiples) for a really good price
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01:26 | Bertl | the link should be on the wiki, sec
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01:26 | danhanes | 0603 LEDs ?
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01:27 | Bertl | http://vserver.13thfloor.at/Stuff/AXIOM/pmod_debug.{brd,sch,png}
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01:28 | danhanes | Thanks
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01:28 | Bertl | the schematic and board files are eagle
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01:28 | Bertl | http://vserver.13thfloor.at/Stuff/AXIOM/pmod_assembled_top_600dpi.png
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01:28 | Bertl | http://oshpark.com/shared_projects/OhXV1RwT
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01:29 | danhanes | Good stuff. I'll start setting up a dev environment.
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01:32 | danhanes | I've been thinking about getting Eagle. I use Altium at work, but I don't want to blur the work / play line. Using a very old Mac based program now, but time to switch. Any thoughts on KiCad
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01:32 | Bertl | yes, KiCad looks like it is getting somewhere
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01:32 | danhanes | Good to hear. I may try to install it.
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01:33 | Bertl | I would have used it, but I've been already working with eagle for quite a while now, so it was my first choice to get things done quickly
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01:34 | Bertl | for small projects both are quite fine, for larger things it becomes a little tricky
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01:34 | danhanes | Probably best to use something you are familiar with. If I remember Eagle is only $US 200 or so for the non-pro version. Is that what you are using and is it adequate? 120mm x 100mm boards ?
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01:34 | Bertl | the version I've been using for those is the free version
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01:34 | danhanes | Better yet.
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01:34 | Bertl | i.e. you can simply download, install and use it
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01:35 | Bertl | but yes, the simple commercial version is quite cheap, you can get one for less than 100 EUR IIRC
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01:35 | Bertl | (nothing compared to the altium prices :)
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01:36 | danhanes | Altium is nice, but overrated.
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01:36 | Bertl | I'm hoping that kicad will get there soon, now that cern has shown some interest
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01:36 | danhanes | Wasn't aware of CERN involvement. That would be a big plus.
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01:37 | Bertl | http://cernandsociety.web.cern.ch/technology/kicad-development
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01:37 | Bertl | http://www.ohwr.org/projects/cern-kicad/wiki
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01:38 | danhanes | You are a fount of knowledge ....
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01:39 | Bertl | you're welcome! :)
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01:45 | danhanes | Ahh - Vivado just finished downloading. Time to bail. Its early here (21:40). I think you are in Europe - do you sleep ?
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01:46 | Bertl | yes, I sleep occasionally, but I'm not in sync with the local timezone
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01:47 | Bertl | have a good night then
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01:48 | danhanes | Just as well, I suppose. Thank you for the introduction to the project. I look forward to working with you - hope I can help.
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01:48 | Bertl | looking forward as well, cya
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01:57 | danhanes | left the channel | |
03:41 | jucar | joined the channel | |
05:22 | jucar | left the channel | |
05:31 | troy_s | Greets all.
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05:31 | Bertl | hey troy_s! how's going?
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05:31 | troy_s | Bertl: Finally finished for Xmas break.
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05:33 | Bertl | \o/
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05:34 | troy_s | Bertl: How goes Operation Struggle?
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05:34 | Bertl | quite well actually, I've revised the LVDS part, and should be done with that in the next days
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05:35 | troy_s | Bertl: Any luck in sorting out the noise patterns?
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05:35 | troy_s | Voltage or otherwise?
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05:36 | Bertl | well, we see three different 'noise' patterns at the moment
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05:36 | troy_s | Bertl: Hrm. I have seen the columns...
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05:36 | Bertl | a very prominent row and column noise pattern and a 'dark' noise pattern
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05:37 | Bertl | the row pattern will probably be easy to fix with the black columns, unless cmosis screwed up big time
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05:37 | jucar | joined the channel | |
05:37 | Bertl | the column pattern I'm not sure, but we will be able to address/compensate that at least in post processing
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05:38 | troy_s | Flat field and dark frame applied?
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05:38 | Bertl | the 'row noise' is mostly caused by bad design on the cmosis side, there are known fixes (i.e. so that you do not need to compensate them)
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05:38 | Bertl | but unfortunately they disclosed the fixes after we designed the alpha prototype frontend
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05:39 | troy_s | Meaning?
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05:39 | Bertl | so we probably won't be able to apply them on this prototype
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05:39 | Bertl | according to cmosis, the sensors internal voltage reference is insufficient
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05:39 | troy_s | Awesome
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05:40 | Bertl | an external reference can be applied, compensating for most of the row noise
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05:40 | troy_s | Sounds like it might be worth looking at a new vendor...
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05:40 | Bertl | (note: there are two kinds of row noises)
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05:40 | troy_s | I certainly hope they will compensate in some capacity for the existing flawed sensors.
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05:41 | Bertl | I don't think they will change the sensor as it can be worked around in external hardware
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05:41 | Bertl | and to be honest, I prefer a sensor with a problem and known workaround over a sensor with a problem and no known work around :)
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05:41 | troy_s | Is there a method to fake this fix in the prototype imaging pipe?
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05:42 | Bertl | I think we can compensate for 99% of the 'noise' in post processing
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05:42 | Bertl | note that we haven't done any post processing in this regard yet, but most of the noise is either systematic or static
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05:43 | troy_s | I am wondering though, if it is too late for the prototype, if you can fake the exact process. Otherwise it is going to be hit and miss in the post pipe.
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05:43 | Bertl | so I'm confident we will get 'clean' pictures soon
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05:43 | Bertl | what currently worries me most is the third 'noise' style
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05:44 | troy_s | Which is?
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05:45 | Bertl | https://wiki.apertus.org/images/0/0f/Plot4ch.svg
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05:46 | Bertl | this is with different exposure times (just a simple histogram)
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05:46 | Bertl | and what worries me is that the noise doesn't seem to be gaussian
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05:46 | troy_s | Bertl: Which hump scare you? The middle?
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05:46 | Bertl | if you look at the 10s exposure
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05:46 | Bertl | you see that there are actually two maxima
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05:47 | Bertl | I first presumed that they might be because of differences in the colors
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05:47 | Bertl | but looking at the samples separated by color in a closeup:
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05:47 | Bertl | https://wiki.apertus.org/images/a/a7/Plot4ch-big.svg
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05:48 | Bertl | shows that it is some kind of sensel effect
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05:49 | troy_s | Very distinctive camel hump.
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05:49 | Bertl | we haven't done any analysis what happens if we remove the 'hot' pixels yet
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05:49 | troy_s | I am not certain what I am looking at however.
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05:49 | Bertl | maybe they cause the effect
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05:49 | troy_s | What image are you using for the analysis?
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05:49 | Bertl | I would expect an almost gaussian distribution on a 'dark frame' as was used for this
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05:50 | troy_s | So this is from a lens capped darkframe?
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05:50 | Bertl | and I definitely wouldn't expect it to show values aroun half the brightness after 10s dark exposure
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05:50 | Bertl | *around
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05:50 | Bertl | so, IMHO there is some stray light involved
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05:51 | troy_s | Out of interest, what do your evaluations show on Canon and Nikon images?
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05:51 | troy_s | And do the results compare on the perfect sensor versus the imperfect?
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05:51 | Bertl | I don't have access to unprocessed images from those, do you?
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05:51 | troy_s | I can get some raws.
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05:52 | Bertl | that would be great!
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05:52 | troy_s | But it would require at least a dcraw pass.
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05:52 | troy_s | Maybe dump a 16 bit tiff in linear.
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05:52 | Bertl | yeah, I know, they aren't really raw at all :)
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05:53 | troy_s | Bertl: Dark room with lens cap? Can you eradicate the light question?
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05:53 | Bertl | yes, the issue is a little trickier than that but we are working on a solution
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05:53 | Bertl | most of the stray light is caused by the LEDs on the zedboard
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05:53 | troy_s | I mean who knows... it could even be some sort of interference.
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05:53 | Bertl | I already figured out how to disable all but one, so we will have some tests on that soon
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05:54 | Bertl | I suspect a gap between sensor and lens mount or between lens mount and bajonet ring
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05:54 | troy_s | Actually
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05:55 | troy_s | Thinking on it
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05:55 | troy_s | That noise pattern should be perfectly linearized according to exposure
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05:56 | troy_s | So in theory, if it is errant light, it will hold according to exposure.
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05:56 | Bertl | hmm, no, I don't think so
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05:56 | Bertl | the distribution gets broader
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05:56 | troy_s | What do you mean by broader?
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05:56 | Bertl | i.e. the average width will be wider (statistically/gaussian)
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05:56 | Bertl | sec
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05:56 | troy_s | That is Greek damn you!
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05:57 | Bertl | give me a second to explain it, it's not that complicated
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05:57 | Bertl | http://vserver.13thfloor.at/Stuff/AXIOM/RAW/hist.svg
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05:57 | Bertl | you remember this one, yes?
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05:58 | Bertl | I did that way back to see how much external light affects the sensor
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05:58 | troy_s | No
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05:58 | troy_s | Oh yes.
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05:58 | Bertl | what you see there is an almost gaussian distribution (the shape of the curve)
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05:59 | Bertl | i.e. that is a mathematical function which is the result of statistical distribution as it happens for example with thermal noise
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05:59 | Bertl | just look at the shape
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06:00 | Bertl | now what you already see in this simple test is, that as the top of the 'bell shape' moves to the right, it also gets slightly smaller
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06:00 | Bertl | and if you look closely, the bottom of the bell also gets wider
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06:01 | Bertl | this is a property of statistical distribution
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06:01 | Bertl | i.e. it is expected and can be calculated
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06:01 | troy_s | All I want to know is whether that cat is alive or dead.
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06:01 | Bertl | same happens with longer exposure times
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06:02 | Bertl | i.e. the bell shape gets wider and less prominent
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06:02 | troy_s | Right. So the shape of the humps bother you?
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06:03 | Bertl | yes, the shape and the fact that they are around 1500-2000, because that is already half the range, i.e. 50% gray
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06:03 | Bertl | the total range in the plot is 0-4095
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06:03 | Bertl | (or at least it should be, not 100% sure actually, sebastian did the evaluation)
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06:03 | troy_s | So right smack dab in the middle of the sensel's receptive range is a camel?
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06:04 | Bertl | its more in the distribution
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06:04 | Bertl | i.e. it looks like there are a number of more sensitive pixels
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06:05 | Bertl | like 40% of all pixels are like 25% more sensitive than the other 60%
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06:05 | Bertl | and not up to 25% but exactly 25% ... and that sounds a little weird
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06:05 | troy_s | And is this a per channel eval?
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06:05 | troy_s | As in bad filter
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06:05 | troy_s | ?
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06:06 | Bertl | yes, the rgb lines in the big plot are per channel
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06:06 | troy_s | Because when I look at that graph, the channels match perfectly.
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06:06 | Bertl | which is a good thing, yes
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06:07 | troy_s | Except that for some reason the voltage goes batshit in that middle exposure range?
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06:07 | troy_s | Have you ruled out infrared or other contamination from some source?
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06:08 | Bertl | the optic has an IR/UV cutoff, but that won't help with stray IR of course
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06:08 | Bertl | UV isn't such a problem with the sensor if you look at the spectral response
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06:09 | troy_s | Or temperature?
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06:09 | Bertl | temperature is actually quite nice since we have the boxed alpha with fan
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06:09 | Bertl | we keep about 4-5 degree above room temperature
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06:09 | Bertl | but we will do some more tests in this regard as well
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06:10 | troy_s | What is your guess and have you done a distribution analysis?
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06:10 | Bertl | no analysis yet and I have no clue except for stray light on the unusual dark frame results
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06:11 | Bertl | but my current focus is on getting the image capture solid, which as I said should be done in the next few days
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06:11 | troy_s | The odd shape certainly seems to hint that it might be something... but the curves match too damn perfectly.
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06:12 | troy_s | If it were errant light I wouldn't expect perfectly achromatic patterns.
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06:12 | Bertl | yes, well, it seems to be a sensel property or some strange effect in the readout
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06:12 | Bertl | in the IR range, the filters are basically all the same
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06:12 | troy_s | Would be illuminating to reduce that hump into a visual distribution if possible.
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06:12 | Bertl | so between 800nm and 1100nm you get almost the same response regardless of the channel
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06:13 | troy_s | A two dimensional distribution.
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06:13 | troy_s | Right... so it could be IR from an LED perhaps?
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06:13 | Bertl | for example
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06:14 | Bertl | that's why I'm disabling all leds (all but one faint green led) in the next version (from the zedboard)
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06:14 | troy_s | Can't you take a soldering nib to the green one?
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06:15 | Bertl | hehe, yeah wouldn't be a problem, but it would require to a) get the boxed alpha prototype back to me and b) mutilation of an otherwise perfectly fine zedboard :)
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06:16 | Bertl | and I think we can handle that one, the green ones are not really IR active
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06:16 | Bertl | and as I said, it is quite dimm and far away from the lens mount
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06:16 | Bertl | and if we need to, we can simply tape it over with a black tape
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06:17 | troy_s | Well fascinating.
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06:17 | troy_s | I hope se6 manages to get a heavily exposed IT8
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06:17 | troy_s | I suspect the images he has posted will be underexposed... that said I have yet to check them.
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06:18 | troy_s | And I suspect the current state of noise will mangle any matrix anyways.
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06:18 | Bertl | yes, please keep up the input regarding exposure/saturation/etc
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06:18 | Bertl | I guess if you tell him what to do, he should be able to get nice images
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06:19 | troy_s | The nature of color dictates that yellow greens etc live much higher in the luminance compared to blues and reds
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06:19 | Bertl | he has a colormeter available IIRC and some light sources
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06:19 | troy_s | So for a matrix to get a decent handle on the transform, the reds / blues need to be amped up quite high to red sufficiently.
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06:20 | troy_s | Yes. It cracked me up when he said he wouldn't trust the meter.
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06:20 | troy_s | Yet he appears to trust the kinos.
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06:20 | troy_s | Which are well known to be a shitbag of random.
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06:20 | Bertl | hehe, yeah, well, the meter was calibrated a bunch of years ago and never checked again, as fas as I know
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06:21 | troy_s | They shift color temps as they warm (about an hour) and they can skew all along the magenta / green axis.
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06:21 | Bertl | so there might be truth in both
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06:21 | troy_s | The tungsten light is about the smoothest distribution we can expect.
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06:21 | troy_s | So perhaps he can pop a bracketed set using a decent tungsten that has been metered.
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06:22 | troy_s | The Kinos just add more variables into our nightmare.
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06:22 | troy_s | Anyways... that Goren article is very solid.
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06:23 | troy_s | Once we have a matrix or LUT, I can sculpt an OCIO package for testing in any OCIO compatible app.
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06:24 | Bertl | great! so please talk to sebastian (either via email or here on IRC, he should be awake/around soon) and let him know what the best approach would be
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06:25 | Bertl | I think it might also be good to use some daylight (or what's left of it at this time of the year :)
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06:25 | troy_s | Right now, the best thing is to get a big brainer like you to eliminate the errant noise issues
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06:25 | troy_s | Yes.
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06:25 | Bertl | I've seen that in my scene* images
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06:25 | Bertl | even really low daylight gives very pleasing results
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06:25 | troy_s | But noise is a huge issue. Then I would suspect getting a decent interpolation. Or perhaps just use some sensel skipping and use a ‘pure’ set of sensels.
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06:26 | troy_s | The thing we want to get to are a smooth spectro (nigh on impossible with synthetic light emitters)
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06:26 | Bertl | yeah, don't worry, I'm confident we'll get that sorted, and for the calibration, the noise shouldn't matter at all
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06:26 | troy_s | and rid ourselves of the synthetic distributons (noise, interp, etc.)
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06:27 | Bertl | that's why I was so fond of daylight (suddenly :)
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06:27 | Bertl | but tungsten has a really smooth spectrum indeed
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06:27 | troy_s | We can always gaussian the patches a smidge if need be to normalize the metered regions.
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06:27 | troy_s | Tungsten and daylight are hard to beat.
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06:28 | Bertl | btw, I was wondering, from the color PoV, is there any point in using (somewhat) pure sources of color?
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06:29 | troy_s | And frankly a decent matrix or LUT for 5500 and 3200 covers about 99.5% of shooter needs to start.
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06:29 | troy_s | Bertl: Pure?
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06:29 | Bertl | I'm asking because it would be fairly trivial to get a whole bunch of LEDs with very narrow emission bands
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06:29 | troy_s | Oh... that might be interesting to experiment with. It is a little like audio though.
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06:29 | Bertl | and it would also be trivial to shine them on/through white paper
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06:30 | troy_s | We want a perfectly straight line similar to what tungsten or the sun offers. If we use many ‘humps’ of light, where the crossovers land can mangle your evals.
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06:31 | troy_s | The secret is the IT8. So that is where our reference of ‘color’ is.
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06:31 | troy_s | It is all somewhat arbitrary as color is really synthetic; a psychophysical phenomenon as the color nerds call it.
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06:32 | troy_s | Ok.
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06:32 | troy_s | Must install another kitchen strip of lights. Joy.
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06:33 | troy_s | Fascinating chat Bertl. Thanks. Very illuminating. Keep me abreast of your noise work and research.
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06:33 | Bertl | will do, have fun and thanks in advance!
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06:34 | troy_s | Chat soon!
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07:59 | Bertl | off to bed now ... have a good one everyone!
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08:19 | se6astian | good morning
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09:13 | philippej | Hi everyone !
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09:17 | se6astian | hello!
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10:15 | philippej | how to setup a test lab for cheap : http://www.imatest.com/docs/lab/#lighting
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10:15 | philippej | I'd say that using tungsteen is the best way to avoid trouble
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10:16 | philippej | as we know the way it makes light, burning a filament, a bit like sunlight, and provides the most efficient color rendition of articfical lighting. Even if kino tubes are rated 90% color rendition index, it's nowhere near the 99% we get with tungsteen. Imho
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10:25 | se6astian | interesting link, thanks
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10:26 | philippej | Bertl, will you able to provide the external vref on the current prototype's hardware?
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13:39 | FergusL | HI here
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13:40 | FergusL | wow, I'm sure that huge Bertl VS troy_s backlog will be full of good information, reading now
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13:57 | se6astian | the apertus° history now also accessible in a new language: https://www.apertus.org/zh-hans/%E9%A1%B9%E7%9B%AE%E5%8E%86%E7%A8%8B :D
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14:04 | FergusL | very interesting chat last night
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14:05 | FergusL | quite greek to me though
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15:11 | Bertl | morning everyone!
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15:16 | se6astian | hello!
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15:46 | philippej | heya
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15:46 | Bertl | whoa, full house today :)
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15:47 | Bertl | and yes, I agree, tungsten or daylight is probably our best option for the IT8 chart atm
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21:40 | se6astian | good night!
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