Astronomy and Astrophysics – Astronomy
Scientific paper
Jul 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006spie.6275e..16c&link_type=abstract
Millimeter and Submillimeter Detectors and Instrumentation for Astronomy III. Edited by Zmuidzinas, Jonas; Holland, Wayne S.; W
Astronomy and Astrophysics
Astronomy
1
Scientific paper
A 16 pixel heterodyne receiver for 2.5 THz has been developed based on NbN superconducting hot-electron bolometer (HEB) mixers. The receiver uses a quasioptical RF coupling approach where HEB mixers are integrated into double dipole antennas on 1.5μm thick Si3N4/SiO2 membranes. Spherical mirrors (one per pixel) and backshort distance from the antenna have been used to design the output mixer beam profile. The camera design allows all 16 pixel IF readout in parallel. The gain bandwidth of the HEB mixers on Si3N4/SiO2 membranes was found to be 0.7÷0.9 GHz, which is much smaller than for similar devices on silicon. Application of buffer layers and use of alternative types of membranes (e.g. silicon-on-insulator) is under investigation.
Baubert Jean
Cherednichenko Sergey
Dauplay Frederic
Delorme Yan
Drakinskiy Vladimir
No associations
LandOfFree
2.5 THz multipixel heterodyne receiver based on NbN HEB mixers does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with 2.5 THz multipixel heterodyne receiver based on NbN HEB mixers, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and 2.5 THz multipixel heterodyne receiver based on NbN HEB mixers will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1893653