This paper presents an ultra-wideband Phased Array Feed (PAF) based on novel flat bend crossed dipole fed by 50Ohm coaxial line. The PAF is dual-polarized and made from all-metal to minimize Ohmic losses and simplify cryogenic integration. It is optimized for 1-2 GHz band and can be good PAF candidate for the Five hundred meter Aperture Spherical Telescope (FAST) and Qi Tai Telescope (QTT) as well as other radio telescopes
Radio astronomy is becoming increasingly demanding in bandwidth. This thesis presents a new type of ...
In traditional antenna design, metal components are not placed in the central part of the antenna as...
Ultrawideband (UWB) phased antenna arrays are critical to the success of future multi-functional com...
This paper presents a novel Phased Array Feed (PAF) element based on flat bend crossed dipole fed by...
In this article, two new ultra-wideband (UWB) dual-polarized Bowtie antennas are investigated as the...
This paper presents design scenarios of Octave-bandwidth Phase Array Feed (PAF) based on a novel wid...
Recently there has been a growing interest in reducing the number of antennas on different platforms...
A novel method to form multiple instantaneous beams on the sky with a reflector antenna is to employ...
A dual polarized Quad-Ridge Flared Horn (QRFH) feed for receiver systems is proposed and presented. ...
In this article, two new ultra‐wideband (UWB) dual‐polarized Bowtie antennas are investigated as the...
One of the many challenges in radio astronomy is the ability to make accurate measure-ments quickly....
The international radio astronomy community is currently pursuing the development of a giant radio t...
Low-noise phased-array feeds are a new way to expand the field of view of radio telescopes at centim...
We describe the design and architecture of PHAROS2, a cryogenically cooled 4-8 GHz Phased Array Feed...
Phased array feed (PAF) receivers used on radio astronomy telescopes offer the promise of increased ...
Radio astronomy is becoming increasingly demanding in bandwidth. This thesis presents a new type of ...
In traditional antenna design, metal components are not placed in the central part of the antenna as...
Ultrawideband (UWB) phased antenna arrays are critical to the success of future multi-functional com...
This paper presents a novel Phased Array Feed (PAF) element based on flat bend crossed dipole fed by...
In this article, two new ultra-wideband (UWB) dual-polarized Bowtie antennas are investigated as the...
This paper presents design scenarios of Octave-bandwidth Phase Array Feed (PAF) based on a novel wid...
Recently there has been a growing interest in reducing the number of antennas on different platforms...
A novel method to form multiple instantaneous beams on the sky with a reflector antenna is to employ...
A dual polarized Quad-Ridge Flared Horn (QRFH) feed for receiver systems is proposed and presented. ...
In this article, two new ultra‐wideband (UWB) dual‐polarized Bowtie antennas are investigated as the...
One of the many challenges in radio astronomy is the ability to make accurate measure-ments quickly....
The international radio astronomy community is currently pursuing the development of a giant radio t...
Low-noise phased-array feeds are a new way to expand the field of view of radio telescopes at centim...
We describe the design and architecture of PHAROS2, a cryogenically cooled 4-8 GHz Phased Array Feed...
Phased array feed (PAF) receivers used on radio astronomy telescopes offer the promise of increased ...
Radio astronomy is becoming increasingly demanding in bandwidth. This thesis presents a new type of ...
In traditional antenna design, metal components are not placed in the central part of the antenna as...
Ultrawideband (UWB) phased antenna arrays are critical to the success of future multi-functional com...