FEATURES

• High CRI>95 up to 98 light quality utilizing or
• 8.6W nominal power consumption
• 280mm×20mm×2.0mm Zhaga compliant linear PCB
• Comes with Wago connectors for solderless daisy chain connection
• Constant current variant available on request

• OVERVIEW

• SPECIFICATIONS

• ACCESSORIES

• INSTALLATION

• APPLICATIONS

• YUJILEDSCRI 98 LED linear module comes in a Zhaga standard footprint and provides a convenient PCB solution for high CRI LED applications. It is designed according to the Zhaga standard and is compatible with various common luminaires. It does not require additional heat sink and can be daisy-chained simply with the provided Wago connectors without soldering. Providing 98 Ra, this versatile LED module can be used in a variety of applications demanding high color quality and performance.

• Power	8.6W
  Dimensions	280mm*20mm*2.0mm
  Light Source	21*or
  CCT & Luminous Flux	2700K	480lm-545lm
  	3200K	520lm-630lm
  	5000K	545lm-630lm
  	5600K	560lm-650lm
  	6500K	610lm-700lm
  CRI (Ra)	98 (typical)
  R9	90 (typical)
  Viewing Angle	120°
  Forward Voltage	DC 24V
  Forward Current	360mA
  On-Board Terminals
  Packaging	10pcs/pack
  Warranty	3 years

• Power Supply	. * Make sure to select 24V to ensure compatibility with this product.
  Connector	10pcsconnectors are included in the packaging. Double-ended board-to-board connectors for YUJILEDS MCPCB Modules allow for quick and effective linear connectivity.

• • High-end architectural lighting
  • Horticulture lighting
  • Photographic/broadcast lighting
  • Human-centric lighting
  • Photoelectric device and relevant research

30-DAY RETURE POLICY

YUJILEDS High CRI LED Webstore provides a 30-dayfor all our orders. You could return any product you purchase to us for a full refund or an exchange within 30 days of receiving your product.

We know you'll love YUJILEDS products as much as we do. But if for any reason, you're not completely satisfied with our product or service, just return your order within 30 days and we'll issue a full refund. See.

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