Just got around to doing a Spyder3 calibration using HCFR @2200 hours on my Panny TC-P58S1. I was out of the country for the first 20 months of ownership (bought it in Japan), and did not have access to my colorimeter.
Custom, Warm, Tint 0, Black Level "Light", Contrast setting of "80", Brightness "74", Color "36", Tint "0"
Contrast set at 34.7 ftL for a IRE100 windown using the colorimeter (set midway between 30 - 40ftL; which was a contrast in the video menu of "80"), and brightness setting equal to 0.65% of that ftL reading for a IRE10 window, about 0.224 ftL, is what I got at brightness of "74".
"Color" in the video menu was initially set at full red window giving "Y" value equal to 21% of a full white 100IRE, which ended up being Color of "36" in the video menu.
R-Cut 7F
G-Cut 80
B-Cut 7D
R-Drv D8
G-Drv E0
B-Drv 93
IRE-0 ftL: 0.004
Sorry I don't have the stock values (hence offsets), as that piece of paper I originally logged them on is now gone after the international move.
Grey scale is spot-on with deltaE values between 1-2 from 20IRE to 90IRE at D6500K.
I used "windowed" greyscale patterns: 80IRE to set the color-Drv levels first, and 20IRE to set the color-Cut levels in the HCFR "live" mode, to minimize delta and track at 6500K, with some back-n-forth to really nail it.
I must say the picture is good now vs. just using other people's offset numbers from the forum, like I did 20 months ago. Goes to show that each panel is a bit different, and it really takes a colorimeter to get each unique TV to it's best potential.
I've usually set the final color level using the "Steaming Rat" method (CLICK HERE)...it targets realistic skin tones to set color levels...usually color (for my taste) runs about 32-34 (vice the colorimeter calculated value of 36)
I'll try to post the HCFR file from my laptop, or post any further tweaks. I have an i1, too, which I might use to verify the Spyder3 settings, which I'll do next week. [EDIT: See post below, #7863]
Calibration disk used: HD709 (avsforum disk) through 1080p HDMI Playstation3 with optimized settings in the video menu.
Cheers,
Doc
Curt Palme: Calibration for Dummies
Custom, Warm, Tint 0, Black Level "Light", Contrast setting of "80", Brightness "74", Color "36", Tint "0"
Contrast set at 34.7 ftL for a IRE100 windown using the colorimeter (set midway between 30 - 40ftL; which was a contrast in the video menu of "80"), and brightness setting equal to 0.65% of that ftL reading for a IRE10 window, about 0.224 ftL, is what I got at brightness of "74".
"Color" in the video menu was initially set at full red window giving "Y" value equal to 21% of a full white 100IRE, which ended up being Color of "36" in the video menu.
R-Cut 7F
G-Cut 80
B-Cut 7D
R-Drv D8
G-Drv E0
B-Drv 93
IRE-0 ftL: 0.004
Sorry I don't have the stock values (hence offsets), as that piece of paper I originally logged them on is now gone after the international move.

Grey scale is spot-on with deltaE values between 1-2 from 20IRE to 90IRE at D6500K.
I used "windowed" greyscale patterns: 80IRE to set the color-Drv levels first, and 20IRE to set the color-Cut levels in the HCFR "live" mode, to minimize delta and track at 6500K, with some back-n-forth to really nail it.
I must say the picture is good now vs. just using other people's offset numbers from the forum, like I did 20 months ago. Goes to show that each panel is a bit different, and it really takes a colorimeter to get each unique TV to it's best potential.
I've usually set the final color level using the "Steaming Rat" method (CLICK HERE)...it targets realistic skin tones to set color levels...usually color (for my taste) runs about 32-34 (vice the colorimeter calculated value of 36)
I'll try to post the HCFR file from my laptop, or post any further tweaks. I have an i1, too, which I might use to verify the Spyder3 settings, which I'll do next week. [EDIT: See post below, #7863]
Calibration disk used: HD709 (avsforum disk) through 1080p HDMI Playstation3 with optimized settings in the video menu.
Cheers,
Doc
Curt Palme: Calibration for Dummies

















