Niklas Wadefalk
Visar 74 publikationer
Optimization of InGaAs Channel for Cryogenic InP HEMT Low-Noise Amplifiers
A 100-µW 4-6 GHz Cryogenic InP HEMT LNA Achieving an Average Noise Temperature of 2.6 K
Influence of Spacer Thickness on the Noise Performance in InP HEMTs for Cryogenic LNAs
On the relation between rf noise and subthreshold swing in InP HEMTs for cryogenic LNAs
A 300-mu W Cryogenic HEMT LNA for Quantum Computing
III-V HEMTs for cryogenic low noise amplifiers
A 300-µW Cryogenic HEMT LNA for Quantum Computing
Low Power Cryogenic Rad-hard LNAs for Space
Low noise 874 GHz receivers for the international submillimetre airborne radiometer (ISMAR)
0.3-14 and 16-28 GHz Wide-Bandwidth Cryogenic MMIC Low-Noise Amplifiers
Cryogenic W-band LNA for ALMA band 2+3 with average noise temperature of 24 K
Cryogenic LNAs for SKA band 2 to 5
Dependence of noise temperature on physical temperature for cryogenic low-noise amplifiers
Two-Finger InP HEMT Design for Stable Cryogenic Operation of Ultra-Low-Noise Ka- and Q-Band LNAs
Two-finger InP HEMT design for stable cryogenic operation of ultra-low-noise Ka-band LNAs
Cryogenic Low Noise Amplifiers in an InP HEMT MMIC Process
Cryogenic low-noise InP HEMTs: A source-drain distance study
10 K Room Temperature LNA for SKA Band 1
Ultra Low Noise 600/1200 GHz and 874 GHz GaAs Schottky Receivers for SWI and ISMAR
Phonon black-body radiation limit for heat dissipation in electronics
SWI 1200/600 GHz highly integrated receiver front-ends
Reliability Assessment of Mixers, Multipliers and Low Noise Amplifiers for Space Applications
Low noise GaAs Schottky TMIC and InP HEMT MMIC based Receivers for the ISMAR and SWI Instruments
Cryogenic noise performance of InGAAs/InAlAs HEMTs grown on InP and GaAs substrate
An InP MMIC process optimized for low noise at Cryo
Cryogenic Broadband Ultra-Low-Noise MMIC LNAs for Radio Astronomy Applications
Characterization and Modeling of Cryogenic Ultralow-Noise InP HEMTs
Cryogenic Performance of Low-Noise InP HEMTs: a Monte Carlo Study
Cryogenic Ultra-Low Noise Amplification - InP PHEMT vs. GaAs MHEMT
Influence of gate-channel distance in low-noise InP HEMTs
Cryogenic 0.5-13 GHz low noise amplifier with 3 K mid-band noise temperature
Ultralow-Power Cryogenic InP HEMT With Minimum Noise Temperature of 1 K at 6 GHz
Cryogenic InAs/AlSb HEMT Wideband Low-Noise IF Amplifier for Ultra-Low-Power Applications
Cryogenic Operation of InAs/AlSb HEMT Hybrid LNAs
Multifunction low noise millimeterwave MMICs for remote sensing
A Broadband, Low Noise, Integrated 340 GHz Schottky Diode Receiver
InAs/AlSb HEMTs for cryogenic LNAs at ultra-low power dissipation
Cryogenic 2-13 GHz Eleven feed for reflector antennas in future wideband radio telescopes
Single-Chip 220-GHz Active Heterodyne Receiver and Transmitter MMICs With On-Chip Integrated Antenna
Integrated front-ends up to 200 GHz
Passivation of InGaAs/InAlAs/InP HEMTs using Al2O3 atomic layer deposition
MMIC-Based Components for MM-Wave Instrumentation
A low noise integrated 0.3-16 GHz differential amplifier for balanced ultra wideband antennas
Design of cryogenic 2-14 GHz Eleven feed for reflector antennas for future radio telescopes
Ultra-Wideband Chip Attenuator for Precise Noise Measurements at Cryogenic Temperatures
Cryogenic 2-14GHz low noise receiver for radio astronomy using Eleven feed
An experimental 210 GHz radar system for 3D stand-off detection
A 210 GHz radar system for 3D stand-off detection
MMIC-based receivers for mm-wave radiometry
Design and realization of a linearly polarized Eleven feed for 1-10 GHz
On the status of Low Noise Millimeterwave MMIC Receivers
Developing a cooled 2-14 GHz Eleven feed for SKA and VLBI 2010
InAs/AlSb HEMTs characterised at cryogenic temperatures
Development of a coolable 2-14 GHz Eleven feed for future radio telescopes for SKA and VLBI 2010
Integrated receivers up to 220 GHz utilizing GaAs-mHEMT technology
Metamorphic HEMT technology for low-noise applications
DC characteristics of InAs/AlSb HEMTs at cryogenic temperatures
Electrical Design of a Cooled 2-14 GHz Eleven Feed for SKA and VLBI 2010
A G-band (140 – 220 GHz) Microstrip MMIC Mixer operating in both Resistive and Drain-Pumped Mode
A 220 GHz Single-Chip Receiver MMIC with Integrated Antenna
Report on Developing Decade Bandwidth Eleven Feeds for Radio Telescopes such as SKA and VLBI 2010
A 220 GHz (G-band) Microstrip MMIC Single-Ended Resistive Mixer
Cryogenic X-Band Low Noise Amplifiers
Noise optimization of InP HEMTs
Cryogenic 2--4 GHz ultra low noise amplifier
The Odin satellite - I. Radiometer design and test
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