Size: 2566
Comment: 1st try of modif by KFS
|
Size: 1919
Comment:
|
Deletions are marked like this. | Additions are marked like this. |
Line 10: | Line 10: |
== Picture Gallery & scientific results == ''(empty)'' |
|
Line 14: | Line 11: |
== Short Description == | == Overview, manual, literature == |
Line 18: | Line 15: |
[#beginOfPage Back to top] | |
Line 20: | Line 16: |
== Documentation == | * [http://www.iram.es/IRAMES/otherDocuments/manuals/HERA_manual_v20.pdf HERA manual, version 2.0] by Schuster et al. 2006 |
Line 22: | Line 18: |
[http://www.iram.es/IRAMES/otherDocuments/manuals/HERA_manual_v19.pdf HERA manual, version 1.9] (pdf file) Technical paper [http://www.iram.es/IRAMES/otherDocuments/manuals/0179hera.pdf "A 230 GHz Heterodyne Receiver Array for the IRAM 30m telescope"] (pdf file) |
* [http://esoads.eso.org/abs/2004A%26A...423.1171S Schuster et al. 2004, A&A, 423, 1171] A 230 GHz Heterodyne Receiver Array for the IRAM 30m telescope ([http://www.iram.es/IRAMES/otherDocuments/manuals/0179hera.pdf local copy]) |
Line 29: | Line 23: |
* ''8.1.2005'': One of the 18 pixels is still blind. Only few frequencies can be tuned automatically. Observers should send observing frequencies to the IRAM Granada receiver group at least three weeks in advance. | |
Line 32: | Line 24: |
* ''1.6.2005'': Tests have shown that the pixels of HERA-2 (second polarisation) have relatively strong variations of noise over the IF band (LSB Tuning). While the consequences are not too dramatic for wide band operation (WILMA) unfortunately the narrow band mode as used mostly with VESPA picks up the end of the IF band with the highest noise. The problem will be further investigated and eventual improvements indicated asap. | * see [http://www.iram.es/IRAMES/mainWiki/TelescopeSystemStatus the Telescope Status page] |
Line 36: | Line 28: |
== Problems and Solutions == ''(empty)'' |
|
Line 42: | Line 29: |
[#beginOfPage Back to top] |
Overview, manual, literature
HERA is a heterodyne receiver array for the IRAM 30m telescope. It consists of two arrays of 3x3 pixels with 24" spacing. The two arrays have orthogonal polarization (V, H) the two polarizations pointing at identical locations on the sky. The instantaneous bandwidth of each pixel is 1 GHz. HERA is equipped with a derotator allowing to follow a source in the sky maintaining the same "footprint". The tunable range is between 215 and 272 GHz. In this range the beamwidth varies between 12" and 9". The beam efficiency is between 0.57 and 0.42.
[http://www.iram.es/IRAMES/otherDocuments/manuals/HERA_manual_v20.pdf HERA manual, version 2.0] by Schuster et al. 2006
[http://esoads.eso.org/abs/2004A%26A...423.1171S Schuster et al. 2004, A&A, 423, 1171] A 230 GHz Heterodyne Receiver Array for the IRAM 30m telescope ([http://www.iram.es/IRAMES/otherDocuments/manuals/0179hera.pdf local copy])
[#beginOfPage Back to top]
Status
see [http://www.iram.es/IRAMES/mainWiki/TelescopeSystemStatus the Telescope Status page]
[#beginOfPage Back to top]
The local contact for HERA is Albrecht Sievers: http://www.iram.es/IRAMES/personal/sievers/sievers.gif