
Specification Minimum Typical Maximum
Input Return Loss
at 250MHz……………………………. 11dB
at 950MHz……………………………. 20dB
at 1450MHz…………………………... 20dB
at 2150MHz…………………………... 11dB
Output Return Loss
at 250MHz……………………………. 15dB
at 950MHz……………………………. 18dB
at 1450MHz…………………………... 20dB
at 2150MHz…………………………... 11dB
1dB Input Gain Compression Point5
at 250MHz…………………………….. -3dBm
at 950MHz…………………………….. -3dBm
at 1450MHz…………………………… -3dBm
at 2150MHz………..………………….. -5dBm
Input Signal Power for 3rd Order Intermod Rejection Ratio of 40dB6
at 250MHz…………………………….. -7dBm
at 950MHz…………………………….. -10dBm
at 1450MHz…………………………… -12dBm
at 2150MHz………..………………….. -15dBm
DC Supply Voltage ………………………………. 12VDC
DC Supply Current………………………………... 650mA
For Indoor Use Only. The HD4PNBFG20B is supplied with an external 12VDC power supply.
Operating temperature of the HD4PNBFG20B is –40 C to +85 C. The mechanical dimensions are
6.4”W 4.4”L 1.5”H
(Specifications subject to change without notice.)
Notes:
1. Absolute Maximum Power is the total power that arrives at the amplifier input from 250MHz to 2150MHz. Satellite power
meters typically read the power level of a single transponder at a time. If all transponders are active from 250MHz to
2150MHz and the power of all transponders are equal, then total available input power across the 250MHz to 2150MHz
bandwidth is approximated by taking the satellite power meter reading at 1450MHz and adding 20dB. Make sure not to
exceed -20dBm as measured with a satellite power meter at 1450MHz.
2. The –75dBm level assumes that the overall system noise figure is not too high such that the carrier-to-noise ratio of the
satellite signal has not been degraded such that signal recovery is not possible. Signal levels lower than –75dBm can be
recovered with properly designed systems having over-all low system noise figures. Low noise figure systems are
achieved by avoiding the addition of too many attenuators or too much loss in front of an amplifier block. It is always
better to add loss after an amplifier to minimize system noise figure as long as the signal at the amplifier input does not
over-drive that amplifier.
3. Assumes maximum power levels as measured with a satellite power meter and all transponder signals active from
250MHz to 2150MHz. (See note 1) A frequency response loss slope of 6dB is assumed, i.e. transponder power measured
at 250MHz with a satellite power meter is 6dB higher than power measured at 2150MHz due to cable loss versus
frequency characteristics. If transponder power levels are equal, limit the maximum power to –20dBm at all frequencies.
An easy method to determine if the amplifier is being over-driven is to connect a satellite power meter to the output of the
amplifier and check C/N, BER, and IRD performance. If acceptable transponder power levels are measured but low C/N
values, high BER values, and low IRD levels are measured, reduce the input level into the amplifier until good C/N, BER,
and IRD results are measured.
4. Channel-to-Channel Isolation is measured referenced to the output of each amplifier. Channel-to-Channel Isolation has a
typical value of 35dB at 2150MHz.
5. Measured using a single CW signal. No transponder signals present.
6. Measured using two CW signals with 1MHz spacing. No transponder signals present.
Copyright © 2010 HDTV Labs, All Rights Reserved. HD4PNBFG20B Manual Version: Rev. 1.1