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System - General

The 30-m telescope is now operating using the New Control System (NCS)

NCS supports only source coordinates in Equatorial J2000.0 system. (More systems will be made available as soon as possible)

Observations near and towards the Sun are not yet supported.

NCS supports observing modes and source offsets in:

All 4 Switching Modes are supported by the NCS (total power, beam switching, wobbler switching, frequency switching.)

Observing modes supported by the NCS:

Automatic calibration and processing of heterodyne data using the MIRA software is in operation for all observing modes. MIRA can also be used manually and offline.

/!\ Online data processing, in some circumstances, still may have problems with scans extending over midnight. Please check data and report problems to Albrecht Sievers. It may be safer to avoid long scans extending over midnight.

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Antenna

(./) OK

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Wobbler

(./) OK

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Pointing Model and Focus

The Pointing Model is maintained with respect to the receiver B100. The misalignment and focus error (D-focus) of the other receivers with respect to B100 is the following: 

  Rx       misal.(")       date            D_focus(mm)       date
 A100     0.16 ±0.06     27-Feb-07,        +0.09 ±0.03     13-Mar-07
 A230     1.34 ±0.18     27-Feb-07,        +0.43 ±0.02     13-Mar-07
 B100     0.00                              0.00
 B230     1.74 ±0.16     27-Feb-07,        +0.40 ±0.10     17-Apr-07
 C150     1.26 ±0.24      5-Feb-07,        +0.64 ±0.13     17-Apr-07
 C270     0.78 ±0.18      5-Feb-07,        +0.36 ±0.15     17-Apr-07
 D150     1.03 ±0.13     12-Mar-07,        +0.26 ±0.02     12-Mar-07
 D270     1.40 ±0.19     12-Mar-07,        +0.18 ±0.05     12-Mar-07

heterodyne: last model update: 2007-10-23, 40 points, previous rms = 3.44", new rms = 1.69"

bolometer: last model update: 2007-11-16, 36 points, new rms < 1.5"

/!\ Pointing on spectral line sources like SiO masers is not yet supported by the data processing.

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SIS Receivers

(./) A, B, C, D receivers are supported by NCS for observations.

(./) Image/Signal gain-ratio calibration is supported by NCS, processing in MIRA. It is highly recommended to use this.

(./) A standard table of T_cold calibration temperatures for A, B, C, D receivers is implemented in NCS. This built-in table covers most frequencies. /!\ Outside this range, T_cold has to be set manually.

(./) Tables and plots are now at http://gra-lx1/mainWiki/ReceiverGroupColdLoadPlotsCurrent 2007-10-11 dj

/!\ Receiver C150 shows low continuum signal at the higher frequencies (>168 GHz). It has to be fully checked. Use D150 instead. (2005-11-16)

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HERA

(./) HERA is supported by the NCS. (2006-02 HU)

Second polarization installed. BR SSB tuning tables for standard frequencies. BR Sideband rejections not determined (2004-12-01 AW). Use standard value of 0.1! BR

(./) For HERA calibration, measured values of the load temperatures are automatically used!

/!\ Watch the computer control of the derotator closely (2002-12-22). BR /!\ Make sure the derotator tracking is stopped after observations, i.e., set to zero degrees in "frame". BR

/!\ The automatic tuning of both HERA1 and 2 can be improved by manually changing the mixer current according to DJ; HERA Pool managers should be aware of this, and operators will receive training (2007-09-19 RM)

HERA 2 is more noisy than HERA 1, limiting HERA2's useful frequency range to below about 242 GHz (2006-09-27 HU according to info from SN)BR

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Pointing and Flux monitoring with SIS receivers:

Continuum instability ("ripple") can occur with all receivers, making pointing and focusing difficult.

In general some receivers are better than others in this respect as summarized here:

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Bolometers

Bolometer Observations are supported by the NCS.

Mambo1: OFFLINE

Mambo2 was re-installed and commissioned the week 13.11.2007/20.11.2007

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Backends

Support by NCS:

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Computer/Software

/!\ The 30-m telescope is now operating using the New Control System (NCS) (2005-11-30 HU). Note that the NCS supports most essential features, but still has some limitations! See the NCS documentation for details, in particular links from the Wiki [https://mrt-lx1.iram.es/mainWiki/OperationNotesObservers NCS Operation Notes for Observers]

/!\ Online data processing, in some circumstances, still may have problems with scans extending over midnight. Please check data and report problems to Albrecht Sievers. It may be safer to avoid long scans extending over midnight.

/!\ Pako does not run under the default gildas version on mrt-lx3, mrt-lx2. Use gag_aug06 before starting pako (2008-01-15 AS). Note: the instructions to start pako explicitly say to run it on mrt-lx1. The 'tricksuggested by AS for mrt-lx2, mrt-lx3 may work, but it is not guaranteed.

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Other Items

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Updates/History

To see the changes between the actual and the last version, please see Show Changes in the Wiki Interface. If you want to see the Revision History of this page, please see Get Info in the Wiki Interface.

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Legend

(./) : OKBR /!\ : WarningBR {X} : ErrorBR

The wiki markup of these icons is: 

(./) : OK
/!\ : Warning
{X} : Error

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