Full Gear List Rental
Grip Truck Packages
Click the Downloadable Gear Lists for more detailed info on Kits / Packages
PRICE: $400/day
PRICE: $1300/day
PRICE: $1000/day
*LIGHTS ADDED TO THIS PACKAGE BY REQUEST*
- 1x Litepanels Gemini 2x1 Kit
- 2xVelvet 1x1 Soft Panel
- 1x Aputure 300D Kit
- 4x Crossfade 4ft Quasar Kit
- 1x Fiilex Q8 Travel
- 1x LiteMat 2 S2 Kit
- 2x Quasar QLED 6”
- 1x Quasar QLED 12”
- 1x Litepanels Gemini 2x1 Kit
- 2xVelvet 1x1 Soft Panel
- 1x Aputure 300D Kit
- 4x Crossfade 4ft Quasar Kit
- 1x Fiilex Q8 Travel
- 1x LiteMat 2 S2 Kit
- 2x Quasar QLED 6”
- 1x Quasar QLED 12”
- 1x LiteMat 4 S2 Kit
- 1x Arri M-18
- 2x Quasar Rainbow RGB Tube
- 2x Quasar QLED 6”
- 1x Quasar QLED 12
PRICE: $250/day
PRICE: $500/day
PRICE: $850/day
*LIGHTS ADDED TO THIS PACKAGE BY REQUEST*
- 1ton grip package
- 1x 4x4 Quasar Set w/ Kit
- 2x 1x1 Velvet Soft Kit
- 1x Aputure 300D w/ Litedome
- 1ton grip package
- 1x 2x1Gemini w/ Softbox Kit
- 2x 1x1 Velvet Soft Kit
- 1x 4x4 Quasar set w/ Kit
- 1x Fiilex Q8 Travel
- 1x Litemat S2 /w Softbox Kit
- 3x Q-LED Kit 1x 12" 2x 7"
- 1x Aputure 300D w/ Lightdome
- 1x 750w ETC Leko
*Vans Are driven by certificated LMR Drivers and Crew
**Equipment availability is subject to change and appropriate substitutions are occasionally required
***1.00 per mile mileage comes into effect for any locations 30 Miles out of Chicago
****Expendables paid by Usage, Prices subject to change at any time.
LIGHT MOD RENTS
"Your friendly midwestern lighting guys"
CONTACT: LMR Office @ 773-940-2654
Test Results
Color Rendition
Written by:
Camrin Petramale & Neil Adamson
As discussed in Color: Part 1, there are a number of useful measurements to consider when looking at a fixtures color. Below, we detail how to read two of the graphic measurements.
Also included within the results are each light's Mired number and G/M index number. These numbers give context to the Correction Gels needed to adjust any CCT or G/M shifts from the desired measurements. Refer to the table below for different manufacturer's thresholds on each gel.
Each reading was done with in-house lights which see standard rental house usage. In each test, the newest available fixtures were tested to present as close to an ideal reading as possible. Readings were taken at full intensity with a Sekonic C-800-U at 1 foot from the source in a blacked-out studio. Despite these considerations, it is important to remember that every light will be slightly different and so it is important to run tests on your own when possible.
For additional context, please read Part 1 if you have not already done so.
Gel Name | Rosco MIRED | Rosco Gel # | Lee MIRED | Lee Gel # | CC Number |
|---|---|---|---|---|---|
Full CTO | +167 | 3407 | +159 | 204 | |
1/2 CTO | +81 | 3408 | +109 | 205 | |
1/4 CTO | +42 | 3409 | +64 | 206 | |
1/8 CTO | +20 | 3410 | +26 | 223 | |
1/8 CTB | -12 | 3216 | -18 | 218 | |
1/4 CTB | -30 | 3208 | -35 | 203 | |
1/2 CTB | -68 | 3204 | -78 | 205 | |
Full CTB | -131 | 3202 | -137 | 201 | |
Full Plus Green | 3304 | 244 | 30G | ||
1/2 Plus Green | 3315 | 245 | 15G | ||
1/4 Plus Green | 3316 | 246 | 7.5G | ||
1/8 Plus Green | 3317 | 278 | 3.5G | ||
1/8 Minus Green | 3318 | 279 | 3.5M | ||
1/4 Minus Green | 3314 | 249 | 7.5M | ||
1/2 Minus Green | 3313 | 248 | 15M | ||
Full Minus Green | 3308 | 247 | 30M |
Reading TM-30 Vector Graphs
Areas pulled toward the inside of the reference circle represent deficiencies in accurate color rendering that causes desaturation along the corresponding hues.
Areas pulled toward the inside of the reference circle represent deficiencies in accurate color rendering that causes desaturation along the corresponding hues.
The closer the red circle (the test source) lands along the black circle (reference source), the more accurately the source will render colors in the human vision system
Reading SPDs
Tungsten SPD shape
Daylight SPD shape
Deficient areas may be offset by increases in other wavelengths
While large drops in wavelength densities could indicate poor rendering abilities with these wavelengths, if the spectral response of the camera does not see these areas well, it will not make much impact.
Results
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5600K
3200K
Open-Faced Reflector (Flood)
Open-Faced Reflector (Other)
Open-Faced Reflector (Parabolic)
Lensed Reflector (Fresnel)
Lensed Reflector (Ellipsoidal)
Lensed Reflector (PAR)
Lensed Array
Diffused Source (Bulb)
Diffused Source (Tube)
Diffused Array (Soft Panel)
Array (Tubes)
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Other (Point Source)
Other (Area Source)
Other (Optical Source)
Altman
Aputure
ARRI
Astera
Desisti
Digital Sputnik
ETC
Fiilex
Hive
Intellytech
K5600
Kino Flo
LiteGear
Litepanels
Lowell
LTM
Mole-Richardson
Nanguang
Quasar Science
RagLite
Rosco DMG
Strand
Velvet
ETC
Planckian Deviation
Source Four
50º Lens (ETC)
3200K
Tungsten Halogen
3007
L218 1/8 CTB
0
-----
0.4364
x
0.4038
y
0
⊿uv
TM-30
Rf
100
Rg
100
SSI Tung. or D55
98
CRI -
99.5
TLCI -
100
Spectral Power Distribution
Mole-Richardson
Planckian Deviation
2K "Junior"
Fresnel - Flood
3200K
Tungsten Halogen
3235
-----
0.25M
-----
0.4215
x
0.3988
y
0.0003
⊿uv
TM-30
Rf
100
Rg
100
SSI Tung. or D55
96
CRI -
99.9
TLCI -
100
Spectral Power Distribution
Mole-Richardson
Planckian Deviation
2K "Baby Junior"
Fresnel - Flood
3200K
Tungsten Halogen
3280
-----
0.25M
-----
0.4185
x
0.3974
y
0.0002
⊿uv
TM-30
Rf
100
Rg
100
SSI Tung. or D55
95
CRI -
99.8
TLCI -
100
Spectral Power Distribution
ETC
Planckian Deviation
Source Four
19º Lens (ETC)
3200K
Tungsten Halogen
3007
L218 1/8 CTB
0
-----
0.4364
x
0.4038
y
0
⊿uv
TM-30
Rf
100
Rg
100
SSI Tung. or D55
98
CRI -
99.5
TLCI -
100
Spectral Power Distribution
ETC
Planckian Deviation
Source Four
26º Lens (ETC)
3200K
Tungsten Halogen
3007
L218 1/8 CTB
0
-----
0.4364
x
0.4038
y
0
⊿uv
TM-30
Rf
100
Rg
100
SSI Tung. or D55
98
CRI -
99.5
TLCI -
100
Spectral Power Distribution
Mole-Richardson
Planckian Deviation
1K "Mickey"
Reflector - Flood
3200K
Tungsten Halogen
3048
L218 1/8 CTB
0.25M
-----
0.4342
x
0.4043
y
0.0005
⊿uv
TM-30
Rf
100
Rg
100
SSI Tung. or D55
99
CRI -
99.7
TLCI -
100
Spectral Power Distribution
Mole-Richardson
Planckian Deviation
1K "Baby"
Fresnel - Spot
3200K
Tungsten Halogen
3209
-----
0.25M
-----
0.4229
x
0.399
y
0.0001
⊿uv
TM-30
Rf
100
Rg
100
SSI Tung. or D55
96
CRI -
99.9
TLCI -
100
Spectral Power Distribution
ARRI
Planckian Deviation
650 T
Fresnel - Spot
3200K
Tungsten Halogen
3047
L218 1/8 CTB
0
-----
0.4338
x
0.4034
y
0.0001
⊿uv
TM-30
Rf
100
Rg
100
SSI Tung. or D55
98
CRI -
99.6
TLCI -
100
Spectral Power Distribution
ARRI
Planckian Deviation
650 T
Fresnel - Flood
3200K
Tungsten Halogen
3047
L218 1/8 CTB
0
-----
0.4338
x
0.4034
y
0.0001
⊿uv
TM-30
Rf
100
Rg
100
SSI Tung. or D55
98
CRI -
99.6
TLCI -
100
Spectral Power Distribution
Mole-Richardson
Planckian Deviation
1K "Mickey"
Reflector - Spot
3200K
Tungsten Halogen
3048
L218 1/8 CTB
0.25M
-----
0.4342
x
0.4043
y
0.0005
⊿uv
TM-30
Rf
100
Rg
100
SSI Tung. or D55
99
CRI -
99.7
TLCI -
100
Spectral Power Distribution
Mole-Richardson
Planckian Deviation
1K "Baby"
Fresnel - Flood
3200K
Tungsten Halogen
3209
-----
0.25M
-----
0.4229
x
0.399
y
0.0001
⊿uv
TM-30
Rf
100
Rg
100
SSI Tung. or D55
96
CRI -
99.9
TLCI -
100
Spectral Power Distribution
Mole-Richardson
Planckian Deviation
2K "Baby Junior"
Fresnel - Spot
3200K
Tungsten Halogen
3280
-----
0.25M
-----
0.4185
x
0.3974
y
0.0002
⊿uv
TM-30
Rf
100
Rg
100
SSI Tung. or D55
95
CRI -
99.8
TLCI -
100
Spectral Power Distribution