Keysight (Agilent) E5505A CALIBRATION and Keysight (Agilent) E5505A REPAIR
 
A calibration by Custom-Cal is performed by engineers with extensive OEM experience. We have the expertise and the necessary standards to perform the Keysight (Agilent) E5505A Calibration, onsite calibration may be available. We specialize in quick turnaround times and we can handle expedited deliveries upon request.

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   Keysight (Agilent) E5505A   Description / Specification:   Spec Sheet 
Keysight (Agilent) E5505A 26.5 GHz Phase Noise Measurement Solution

The Keysight Technologies E5505A 26.5 GHz phase noise measurement solution offers the most flexible set of measurements on one-port VCOs, DROs, crystal oscillators and synthesizers. Two-port devices, including amplifiers and converters, plus CW, pulsed and spurious signals can also be measured. The E5505A measurements include absolute and residual phase noises, AM noise, and low-level spurious signals. The stand-alone instrument architecture easily configures for various measurement techniques, including the PLL/reference source technique, residual and FM discriminator methods. It includes a baseband test set: N5500A-7011 Standard configuration, 50 kHz to 1.6 GHz, 0 to 23 dBm; N5500A-001 High power, 0 to 30 dBm, high frequency input, 1.2 to 26.5 GHz, and AM noise or N5500A-201 High frequency input, 1.2 to 26.5 GHz, 0 to 23 dBm. A low noise microwave downconverter: E5505A-100 Downconverter not included; N5502A Low noise 18 GHz microwave downconverter or N5507A Low noise 26.5 GHz microwave downconverter. A baseband swept analyzer: E5505A-110 Spectrum analyzer not included; N9030A PXA high-performance signal analyzer (3 Hz to 3.6/8.4/13.6/26.5/43/44/50 GHz); N9020A MXA mid-performance signal analyzer (10 Hz to 3.6/8.4/13.6/26.5 GHz); N9010A EXA economy signal analyzer (10 Hz to 3.6/7.0/13.6/26.5/32/44 GHz); N9000A CXA low-cost signal analyzer (9 kHz to 3/7.5 GHz); E4411B ESA-L (9 kHz to 1.5 GHz) spectrum analyzer; E4402B ESA-E (100 Hz to 3 GHz) spectrum analyzer or E444xA PSA Series (3 Hz to 6.7/13.2/26.5/42.98/44/50 GHz) spectrum analyzer. Operating characteristics. Offset frequency range: 0.01 Hz to 2 MHz. System noise response: –180 dBc/Hz typically (>10 kHz offsets). System spurious response: < –120 dBc typically. Phase detector input power: (<1.6 GHz carrier frequency), R input = 0 to +23 dBm, L input = +15 to +23 dBm. Downconverter input range: 1 GHz to 18 GHz, 1.5 GHz to 26.5 GHz. External noise input port: 0.01 Hz to 100 MHz. Measurement accuracy: ±2 dB (< 1.0 MHz offsets), ±4 dB (< 100 MHz offsets).



 

Standard Calibration $1,265.00 *
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*This is a Web introductory price for one calibration of the Keysight (Agilent) E5505A. Price does not in most cases include measurement performance data. Pricing does include NIST traceable calibration and issue of a calibration certificate and calibration label. Pricing may vary slightly due to volume and location of laboratory supporting calibration. Volume pricing may apply. On-site fees may apply depending on logistics, location and volume of work to be completed during the visit.


Related RF Terms and Definitions. For a complete list go to our  Terms and Definitions Page.

Averaging
Averaging is a mathematical process to reduce the variation in a measurement by summing the data points from multiple measurements and dividing by the number of points summed.

Jitter
Jitter in technical terms is the deviation in or displacement of some aspect of the pulses in a high-frequency digital signal. Jitter is the time variation of a periodic signal in electronics and telecommunications, often in relation to a reference clock source. Jitter may be observed in characteristics such as the frequency of successive pulses, the signal amplitude, or phase of periodic signals. Jitter is a significant, and usually undesired, factor in the design of almost all communications links (e.g., USB, PCI-e, SATA, OC-48). In clock recovery applications it is called timing jitter.

Pulse Power
Pulse Power, the energy transfer rate is averaged over the pulse width. Pulse width is considered to be the time between the 50 percent risetime/falltime amplitude points. Pulse power averages out any aberrations in the pulse envelope such as overshoot or ringing.

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