A 230 GHz heterodyne receiver array for the IRAM 30 m telescope-Reference-Cited by-同舟云学术

A 230 GHz heterodyne receiver array for the IRAM 30 m telescope

Published:2004-08-12 Issue:3 Volume:423 Page:1171-1177
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Schuster K.-F.,Boucher C.,Brunswig W.,Carter M.,Chenu J.-Y.,Foullieux B.,Greve A.,John D.,Lazareff B.,Navarro S.,Perrigouard A.,Pollet J.-L.,Sievers A.,Thum C.,Wiesemeyer H.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361:20034179/pdf

Reference18 articles.

1. A low noise SIS receiver covering the frequency range 215?250 GHz

2. Brüll, M. 2000, Diploma Thesis, Feb., I. Physikalisches Institut der Universität zu Köln

3. Carter, M., Baryshev, A., Hesper, R., et al. 2002, 13th Int. Symp. Space Terahertz Techn. Proc., Cambridge, Mass., 515

4. Gallego, J. D. 1995, Tech. Report CAY 1995-3, Centro Astronomico de Yebes

Cited by 83 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Kinetic temperature of massive star-forming molecular clumps measured with formaldehyde;Astronomy & Astrophysics;2024-07

2. Design of a 240 GHz on-chip dual-polarization receiver for SIS mixer arrays;Superconductor Science and Technology;2023-04-13

3. VERTICO V: The environmentally driven evolution of the inner cold gas discs of Virgo cluster galaxies;Publications of the Astronomical Society of Australia;2023

4. Dissecting Nearby Galaxies with piXedfit. II. Spatially Resolved Scaling Relations among Stars, Dust, and Gas;The Astrophysical Journal;2022-08-01

5. Dissecting Nearby Galaxies with piXedfit. I. Spatially Resolved Properties of Stars, Dust, and Gas as Revealed by Panchromatic SED Fitting;The Astrophysical Journal;2022-02-01