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| Subsections | === Summary === |
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| === Summary === === What is new? === === Applications === === Reminders === === Observing time estimates === === Pooled observing === === Service observing === === Remote observing === === Technical Information about the 30m Telescope === ==== HERA ==== ==== The single pixel heterodyne receivers ==== ===== Extended tuning range: 72 - 80 GHz. ===== ===== General point about receiver operations. ===== ===== Polarimeter XPOL ===== ===== MPIfR Bolometer arrays ===== |
Proposals for three types of receivers will be considered for the coming winter semester: 1. the observatory's set of four dual polarization heterodyne receivers centered at wavelengths of 3, 2, 1.3, and 1.1 mm. 2. the 9 pixel dual-polarization heterodyne receiver array, HERA, operating at 1.3 mm wavelength 3. The MAMBO-2 bolometer array with 117 pixels operating at 1.2 mm; the smaller MAMBO-1 array with 37 pixels is kept as a backup. Emphasis will be put on observations at the shorter wavelengths, but 3mm proposals are also encouraged inasmuch as they are suited for medium or low quality weather backup onservations. About 2000 hours of observing time are expected to be available. === What is new? === === Applications === === Reminders === === Observing time estimates === === Pooled observing === === Service observing === === Remote observing === === Technical Information about the 30m Telescope === ==== HERA ==== ==== The single pixel heterodyne receivers ==== ===== Extended tuning range: 72 - 80 GHz. ===== ===== General point about receiver operations. ===== ===== Polarimeter XPOL ===== ===== MPIfR Bolometer arrays ===== ==== The Telescope ==== ===== Beam and Efficiencies ===== ===== Pointing and Focusing ===== ===== Wobbling Secondary ===== ==== Backends ==== |
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* The Telescope o Beam and Efficiencies o Pointing and Focusing o Wobbling Secondary * Backends |
Call for Observing Proposals on the 30m Telescope
Summary
Proposals for three types of receivers will be considered for the coming winter semester:
- the observatory's set of four dual polarization heterodyne receivers centered at wavelengths of 3, 2, 1.3, and 1.1 mm.
- the 9 pixel dual-polarization heterodyne receiver array, HERA, operating at 1.3 mm wavelength
- The MAMBO-2 bolometer array with 117 pixels operating at 1.2 mm; the smaller MAMBO-1 array with 37 pixels is kept as a backup.
Emphasis will be put on observations at the shorter wavelengths, but 3mm proposals are also encouraged inasmuch as they are suited for medium or low quality weather backup onservations. About 2000 hours of observing time are expected to be available.
What is new?
Applications
Reminders
Observing time estimates
Pooled observing
Service observing
Remote observing
Technical Information about the 30m Telescope
HERA
The single pixel heterodyne receivers
Extended tuning range: 72 - 80 GHz.
General point about receiver operations.
Polarimeter XPOL
MPIfR Bolometer arrays
The Telescope
Beam and Efficiencies
Pointing and Focusing
===== Wobbling Secondary =====