XPANEL FLAT panels
Ultra-thin panels in 12 catalogue sizes and 24 to 90 W. Suspended on cable or rod, or surface mounted against the ceiling.
- 24 – 90 W
- Power range
- 5
- Models
- 12
- Catalogue sizes
- 27
- Codes in the series
The models
5 groups, all in view. The catalogue lists no recessed version of this series.
In view
In view: on the slab or hung on wire, with the body as part of the space.
27 codes| Model | Dimensions | Optic | Power | Codes |
|---|---|---|---|---|
| SP27 | 300 – 1500180 mm | Opal | 24 – 48 W | 5 |
| XP1826 UGR < 19 | 450 – 1200 mm | Microprismatic | 30 – 80 W | 4 |
| XP2017-C Dual emission | 450 – 900 mm | Not declared | 30 – 90 W | 6 |
| XP2017-R Dual emission | 450 – 900 mm | Not declared | 30 – 90 W | 6 |
| XP2017-S Dual emission | 450 – 900 mm | Not declared | 30 – 90 W | 6 |
The XP2017 is the same panel in three mountings —cable, rod and surface— which is why it appears three times in the catalogue under different codes.
Optics and distribution
What sits in front of the LED. The diffuser is declared in position 10 of the code and drives both output and glare control. The catalogue declares no aperture for these diffusers, so no beam is drawn.
- No aperture in catalogue Microprismatic Workstations · UGR < 19 4 codes PM
- No aperture in catalogue Opal Diffuse light, even surface 5 codes P
Colour of the light
27 of the 27 codes in the series declare a colour temperature in the catalogue.
- 3000 K Warm
- 4000 K Neutral
- 5000 K Cool neutral
- 6000 K Cool
- Tunable White (Color Changing) Tunable on site
Dimming
Most of the series is quoted in ON-OFF, DALI and 0-10 V. It is defined at order time: the driver is fitted at the factory and cannot be swapped on site.
- ON/OFF
- No dimming. The base method on every code.
- DALI
- Addressable per luminaire, scenes and sensors.
- 0-10 V / 1-10 V
- Analogue, with separate control wiring.
- Color Changing
- Colour temperature shift, on 18 codes in the series.
Technical specifications
Values for the complete series, taken from the catalogue. For a specific code, the datasheet gives the exact figure.
Photometry
| Efficacy | 100 · 100-130 · 110lm/W lm/W (±5%) |
|---|---|
| Colour temperature | |
| |
| Colour rendering | Ra > 82 · Ra > 90 |
| Glare | UGR < 19 with microprismatic · 4 codes |
Electrical
| Power | 24 – 90 W |
|---|---|
| Input voltage | 220 – 240 V · 50/60 Hz |
| LED chip | Everlight · Everlight 2835 |
| Driver | NON-Flicking/LOW THD/HIGH PF / Color Changing · ON-OFF / 1-10V / DALI / Color Changing · ON-OFF (AGT) / DALI / 0-10V / Color Changing |
Construction
| Body | Aluminium |
|---|---|
| Sizes | 12 catalogue sizes |
| Diffusers and optics | Microprismatic · Opal |
| Finishes | |
Colour is indicative on screen. To specify, ask for the physical sample. | |
| Emission | Direct, or dual up/down emission · 9 codes |
Installation and life
| Warranty | 5 years |
|---|---|
| Ingress protection | IP20 |
One code, one exact product
Every attribute that defines a variant, in a fixed order of 15 positions. No ambiguity in quotes, purchase orders or specifications.
- CMX 01
- XP 02
- C 03
- X 04
- 450 05
- T5 06
- 220240 07
- 9 08
- 30 09
- X 10
- SFC 11
- X 12
- DU 13
- B 14
- 45 15
See the full map of the code
- 01 CMX Brand Cromatix
- 02 XP Series XPanel
- 03 C Model C
- 04 X Profile Not applicable
- 05 450 Size 450 mm
- 06 T5 Chip Everlight 2835
- 07 220240 Voltage 220-240 V
- 08 9 CRI Ra ≥ 90
- 09 30 CCT 3000 K
- 10 X Diffuser Not applicable
- 11 SFC Mounting Surface
- 12 X Control Not at this level
- 13 DU Variant Dual emission
- 14 B Finish Black
- 15 45 Power 45 W
X means the position does not apply or there is no data: the code always keeps its 15 positions so it stays machine-parseable. Colour temperature is the first two digits of the Kelvin value, and power carries no leading zeros.
Representative configurations
Real catalogue codes, chosen to cover the range of the series: three lengths of the profile with most codes, plus dual emission, the lens and the emergency kit. Flux is power times efficacy from the catalogue itself; where efficacy is a range it is left blank.
| MODEL_CODE | Model | Dimensions | Power | Flux | Efficacy | CRI |
|---|---|---|---|---|---|---|
| CMX-XP-C-X-450-T5-220240-9-30-X-SFC-X-X-B-30 | XP2017-C | D450 × H17 mm | DIRECT:30W | 3.300 lm | 110lm/W | > 90 |
| CMX-XP-C-X-600-T5-220240-9-30-X-SFC-X-X-B-40 | XP2017-C | D600 × H17 mm | DIRECT:40W | 4.400 lm | 110lm/W | > 90 |
| CMX-XP-C-X-900-T5-220240-9-30-X-SFC-X-X-B-60 | XP2017-C | D900 × H17 mm | DIRECT:60W | 6.600 lm | 110lm/W | > 90 |
| CMX-XP-X-X-450-T-220240-8-30-PM-SWR-X-X-W-30 | XP1826 | D450 × H26 mm | 30W(Down) | 3.000 lm | 100lm/W | > 82 |
| CMX-XP-C-X-450-T5-220240-9-30-X-SFC-X-DU-B-45 | XP2017-C | D450 × H17 mm | DIRECT:30W / INDIRECT:15W | 4.950 lm | 110lm/W | > 90 |
| CMX-XP-X-27-300-T5-220240-8-30-P-SFC-X-X-W-24 | SP27 | 300 × 300 × 27 mm | 24W | — | 100-130lm/W | > 82 |
Photometry and documentation
Photometry is a measurement, not a description: an IES or LDT file corresponds to one physical configuration and changes with length, optic, diffuser and colour temperature.
That is why we do not publish a single series-wide file. Tell us which configuration you are evaluating and we will send the right one, together with the datasheet for that code.
XPANEL FLAT in project
Frequently asked questions
How is it different from XPanel Slim?
Flat is the low-profile panel used as a piece, alone or clustered. Slim is the rectangular line meant to connect into runs. Both share the XP prefix in the code.
Is it suitable for screen-based offices?
With the microprismatic diffuser, yes: 4 of the 27 codes declare UGR < 19. The opal ones give more output but carry no UGR figure.
Is there a version that also lights the ceiling?
Yes. 9 of the 27 codes are dual emission, with output up and down.
How do I get the photometry for a Dialux calculation?
Write to us with the complete MODEL_CODE and we will send the matching IES or LDT file.
Tell us about the project
If the requirement is already defined, the length and colour temperature are enough to reach a concrete proposal. If you are still exploring, we start from what the light has to resolve.