Input frequency range
10.7 GHz ~ 11.7 GHz
Output frequency range
950 MHz ~ 1950 MHz
Low band LO frequency
9.75 GHz
High band input frequency range
11.7 GHz ~ 12.75 GHz
High band output frequency range
1100 MHz ~ 2150 MHz
High band LO frequency
10.6 GHz
Noise figure
0.2 dB typ. (0.7 dB max.)
LO frequency accuracy @ 25° C
±1.0 MHz
LO temperature drift
±3.0 MHz
LO phase noise @ 10 kHz
-90 dBc / Hz
Conversion gain
52 dB ~ 65 dB
Gain ripple (over 26 MHz bandwidth)
±0.75 dB
Gain variation (over full band)
±4 dB max.
Image rejection
40 dB min.
1 dB compression point (@ output)
0.0 dBm min.
Cross polarization isolation
22 dB min.
Control signal Ca (V)
11.0 V ~ 14.0 V
Control signal Cb (H)
16.0 V ~ 20.0 V
Control signal Cc (band switching)
22 kHz, ±4 kHz
DiSEqC A input
The integrated LNB / Das Integrierte LNB
DiSEqC B input
The external LNB / Das Externe LNB
Output VSWR
2.5 : 1 max.
Output VSWR (LNB2)
2.5 : 1 max.
Input VSWR
2.5 : 1 max.
Input VSWR (LNB2)
2.5 : 1 max.
In band spurious level
-60 dBm max.
Current consumption
120 mA max. (11 VDC ~ 20 VDC)
Operating temperature
-30 ° C ~ + 60 ° C
Output impedance
75 Ω (F-type)
Output impedance (LNB2)
75 Ω (F-type)
Output connector type
F-Type (female)
Weight
134 g
With its embedded DiSEqC switch this LNB will enable the connection of an additional single LNB without the need to add an additional external switch. It is suitable for users owning a dish larger or smaller than 80cm or wanting to receive two satellites which are not supported with one of our existing Monoblock LNBs . As it was specifically designed for the European DTH markets, this LNB provides optimized reception capabilities. It is ready for High Definition transmissions and provides excellent Noise Figure performance. Designed to meet the most strict specifications and manufactured to the highest industry quality standards , this LNB is an ideal solution for the satellite broadcast reception across Europe.
Low Phase Noise, DVB-S2 (HDTV) compliant
Low Noise Figure (0.2 dB)
Low Power Consumption
Very High Cross Polarization Isolation
Very High Frequency Stability
