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RECEIVER CHOICE next up previous
Next: OBSERVING PROCEDURES Up: Spectral-Line Observing at AO Previous: INTRODUCTION to Spectral Line


RECEIVER CHOICE

The majority of the receivers at Arecibo are housed in the new Gregorian Dome. The exceptions are the 47-MHz and 430CH receivers attached to the old Carriage House. As these receivers are not commonly used for spectral line work they will not be discussed here. Detailed information on the Carriage House receivers can be found both on the relevant receivers' web page and in the pulsar observing handbook.

The available Gregorian receivers are listed in Table 1. In most cases, only one receiver will be available which will meet your frequency requirements. (REMEMBER - At present only one receiver can be used at a time.) In a few cases, such as in the L and S bands, more than one receiver may be available which suit your needs. In these cases, you probably want to choose the receiver with the narrowest frequency range which fits your need. Alternatively, you may wish to choose the most sensitive (lowest SEFD - system equivalent flux density) receiver. Conveniently, these two choices often lead to the same receiver (i.e. using the L-narrow over the L-wide, when possible). The most up-to-date information on the receivers can be found on the Arecibo web pages at http://www.naic.edu/$\sim$astro/RXstatus/.


Table 1: Gregorian Receivers
Frequency Range Receiver Name Native Pol. Sensitivity System
      (K/Jy) Temp (K)
0.312 - 0.342 327 Dual Linear 5-6 160
0.425 - 0.435 430 Dual Circular   55
0.609 - 0.614 610 Dual Linear 8 130
1.12 - 1.73 L-wide Dual Linear 8-11 35-40
1.28 - 1.50 L-narrow Dual Circular$\dag $ 08-10 25-30
l .8 - 3.1 S-low Dual Linear 7 40
2.33 - 2.43 S-Radar Dual Circular 9-10 25-30
3.85-6.00 C Dual Circular 4-8 32-34
8.0 - 10.0 X Dual Circular 1.5-3* 43.48*
$\dag $The L-narrow is circularly polarized only at 1420MHz
and becomes increasingly elliptically polarized away from this frequency.
*Receiver still being calibrated. These numbers are very preliminary.

L-Wide Receiver Options: If you choose to use the L-wide receiver, a number of options not available to the other receivers must be decided. In particular, you must choose your polarization type and r.f. filter.

NOTE: A smaller filter bank will soon be available for both the L-Narrow and S-Wide receivers as well.


next up previous
Next: OBSERVING PROCEDURES Up: Spectral-Line Observing at AO Previous: INTRODUCTION to Spectral Line
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