Share Email Print
cover

Proceedings Paper

1.4-THz receiver for APEX and for GREAT on SOFIA
Author(s): Gundolf Schmidt; Frank Bielau; Urs U. Graf; C. E. Honingh; Karl Jacobs; Katharina Rettenbacher; Jurgen Stutzki; Martina C. Wiedner
Format Member Price Non-Member Price
PDF $14.40 $18.00
cover GOOD NEWS! Your organization subscribes to the SPIE Digital Library. You may be able to download this paper for free. Check Access

Paper Abstract

We are developing a 1.4 THz receiver to explore the far infrared universe, such as probing high mass star forming regions using, e.g., the high J transitions of CO, investigating the warm interstellar medium in N+ or probing cold and dense stellar cores in H2D+. Due to the poor atmospheric transmission at these frequencies we are planning to use this modular receiver on high altitude ground based observatories, for example the Atacama Pathfinder EXperiment (APEX), and as an additional channel for the German Receiver for Astronomy at Terahertz Frequencies (GREAT) on the Stratospheric Observatory For Infrared Astronomy (SOFIA) located on an airplane. To allow successful astronomical observations under poor atmosphere transmission a low receiver noise temperature and a high receiver stability are mandatory. To achieve a low receiver temperature the main effort is directed to develop phonon-cooled NbTiN HEB mixers. For optimum coupling with the telescope beam and easier alignment we are focussing on waveguide mixers. A phase locked Gunn (114-135 GHz) and three multipliers will be used as the Local Oscillator (LO) of 1370-1500 GHz. A liquid He Dewar will be used for operation on SOFIA and a closed-cycle system with a pulse-tube cooler on APEX. Initially, we are aiming for 1 GHz IF bandwidth (214 kms-1 at 1.4 THz) sufficient for galactic observations. First tests and astronomical observations with a similar but lower frequency HEB at 800 GHz have yielded encouraging results.

Paper Details

Date Published: 8 October 2004
PDF: 10 pages
Proc. SPIE 5498, Millimeter and Submillimeter Detectors for Astronomy II, (8 October 2004); doi: 10.1117/12.550334
Show Author Affiliations
Gundolf Schmidt, Univ. zu Koln (Germany)
Frank Bielau, Univ. zu Koln (Germany)
Urs U. Graf, Univ. zu Koln (Germany)
C. E. Honingh, Univ. zu Koln (Germany)
Karl Jacobs, Univ. zu Koln (Germany)
Katharina Rettenbacher, Univ. zu Koln (Germany)
Jurgen Stutzki, Univ. zu Koln (Germany)
Martina C. Wiedner, Univ. zu Koln (Germany)


Published in SPIE Proceedings Vol. 5498:
Millimeter and Submillimeter Detectors for Astronomy II
Jonas Zmuidzinas; Wayne S. Holland; Stafford Withington, Editor(s)

© SPIE. Terms of Use
Back to Top