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Subsections === Summary ===
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=== Summary === 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.

TableOfContents(5)

Call for Observing Proposals on the 30m Telescope

Summary

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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