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information_for_astronomers:rx:s60mm [2013/10/21 15:40]
bwinkel [Spectroscopy modes and resolution]
information_for_astronomers:rx:s60mm [2025/05/28 16:50] (current)
akraus
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 ====== 6-cm secondary focus receiver (4600-5100 MHz) ====== ====== 6-cm secondary focus receiver (4600-5100 MHz) ======
  
-This is a 4-channel ​2-horn ​system for sensitive continuum, polarimetry,​ VLBI, and pulsar observations. ​+This is a 4-channel system for sensitive continuum, polarimetry,​ VLBI, and pulsar observations. ​ 
 + 
 +==== Overview ==== 
 + 
 +^ RX Name ^ [[information_for_astronomers:​rx:​bands|Band]] ^ Frequency range [GHz] ^ Polarisation^Nr. of Horns ^Horn position relativ to center of focus cabin^ 
 +| **S60mm** | C | 4.6-5.1 | dual-circular| 1 | Az: 236.6, arcsec, Elv: -1336.0 arcsec| 
  
 ==== Calibration Information ==== ==== Calibration Information ====
  
 ^ Frequency [GHz] ^ Channel ^ Polarisation ^ Tcal [K] ^ Tsys [K] ^ Sensitivity [K/Jy] ^ SEFD [Jy] ^ Aperture Eff. [%] ^ TMB/S [K/Jy] ^ Main Beam Eff. [%] ^ FWHM [arcsec] ^ Last update ^ ^ Frequency [GHz] ^ Channel ^ Polarisation ^ Tcal [K] ^ Tsys [K] ^ Sensitivity [K/Jy] ^ SEFD [Jy] ^ Aperture Eff. [%] ^ TMB/S [K/Jy] ^ Main Beam Eff. [%] ^ FWHM [arcsec] ^ Last update ^
-|4.850 |A / B | LCP / RCP |1.8 |27 |1.55 |18 |53 |2.4 |63 |146 |June 2008|+|4.850 |A / B |LCP / RCP |1.8 |27 |1.55 |18 |53 |2.4 |63 |146 |June 2008|
  
 ^ normalized Gain curve (G = A0 + A1·Elv + A2·Elv2)^^^ Observed in ^ confirmed ^ ^ normalized Gain curve (G = A0 + A1·Elv + A2·Elv2)^^^ Observed in ^ confirmed ^
-|A0 = 0.97323|A1 = 1.2702E-3|A2 = -1.5059E-5|May ​2004|  | +|A0 = 0.9870|A1 = 8.692E-4|A2 = -1.453E-5|Aug 2023|May 2025  |
-|A0 = 0.995|A1 = 5.2022E-4|A2 = -1.27874e-05|Feb 2008|  |+
  
 **Comments:​** **Comments:​**
   * The values for LCP and RCP do not differ significantly.   * The values for LCP and RCP do not differ significantly.
-  * The new gain curve (Feb 2007) was corrected for opacity. +  * The opacity is usually very small. Typical ​zenith tau values are < 0.01. 
-  * If no other information about the opacity is available a typical ​zenith tau value of about 0.016 should do a good job+ 
 +==== Available receiver versions (for OBSINP) ==== 
 + 
 +^Version^Description^Details^ 
 +|BB_continuum|standard continuum backend with internal polarimeter|bandwidth 500 MHz| 
 +|EDDPOL_MULTIFIBA | spectro-polarimeter backend | | 
 + 
 + 
 +**Below here: Information is currently updated.** 
  
 ==== Version description for OBSINP ==== ==== Version description for OBSINP ====
  
 ^ RX Name ^ Wavelength [cm] ^ Frequency (center) [GHz] ^ Nr. of Horns ^ ^ RX Name ^ Wavelength [cm] ^ Frequency (center) [GHz] ^ Nr. of Horns ^
-| **S60mm Double Beam** | 6 | 4.6-5.1 (4.85) | +| **S60mm Double Beam** | 6 | 4.6-5.1 (4.85) | 
 | **Version:​** |   ​**Comment** ​  ||| | **Version:​** |   ​**Comment** ​  |||
 |1. Continuum (BW: 500 MHz) | Broad Band Continuum + Polarimeter ||| |1. Continuum (BW: 500 MHz) | Broad Band Continuum + Polarimeter |||
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 ==== Tcal and Tsys measurements ==== ==== Tcal and Tsys measurements ====
-{{:​information_for_astronomers:​rx:​s60mm-xffts-tcal.png?900|Tcal}} +{{:​information_for_astronomers:​rx:​s60mmb_tcal_from_specpointing_using_tau_spec.png?675 |}} 
- +{{:​information_for_astronomers:​rx:​s60mmb_tsys0_from_specpointing_using_tau_spec.png?​675 |}} 
-{{:​information_for_astronomers:​rx:​s60mm-xffts-tsys.png?900|Tsys}}+{{:​information_for_astronomers:​rx:​s60mmb_tau_from_specpointing_using_tau_spec.png?​675 |}} 
 +{{:​information_for_astronomers:​rx:​s60mmb_hpbw_from_specpointing.png?675 |}}
  
-{{:​information_for_astronomers:​rx:​s60mm-xffts-trms.png?​900|Trms}} 
  
  
information_for_astronomers/rx/s60mm.1382362810.txt.gz · Last modified: 2013/10/21 15:40 by bwinkel