DeLingHa13
my home upper gernal Observation ARO HHT ARO 12M ASTE CSO DeLingHa13 IRAM 30M KOSMA LSST Nobeyama 45M YNAO40m SESHAN25 Herschel

Caution!! Although I am happy to share my research notes below with all visitors to my webpages, these pages are mainly designed for my own use and subject to change without warning. I do not guarantee the correctness of all contents as well.


 

PMO (De Ling Ha) 13.7 m millimeter telescope (DeLingHa telescope webpage )


 

Location: (back to top)

De Ling Ha observation stating
                Longitude: 97d 33.6m east;
                Lattitude:  37d 22.4m  north;
                Elevation: 3200m above sea level.
Basic facts: (back to top)

Diameter: 13.7 m
Support system: azimuth system (limited to elevation >= 30deg)
Focus: Cassegrain
Surface rms: 70um
Pointing: tracking error = 1.42" (1"~3" for most sky area);
             elevation error = 1.44";
             pointing error = 5"
Beam size: AZ=59"+-9",EL=66"+-8" (@ LO = 112GHz), as a function of wavelength: beam = k * lambda / D.

Efficiencies: eta_Moon = 66.1(+-2.6)%
                  aperture efficiency: eta_A = 25%
                   beam efficiency: eta* = 67% (at zenith), as a function of elevation due to gravity deformation and the change of optical path coupling:
                         eta*(el) = 0.61(+-0.10) - 0.16 (+-0.16) cos(el)   for 12CO line
                         eta*(el) = 0.55(+-0.10) - 0.06 (+-0.14) cos(el)   for 13CO line
Calibration accuracy: Trms = 0.56 K for 60 integration; relative accuracy  = 3.5%.

Receivers: (back to top)

  • Single beam: 3mm SiS receiver (85-115 GHz), Trx = 70~123 K (DSB), Tsys = 250 K (112 GHz)
  • 3x3 multi-beam: beam separation ~ 200";

       (Note: observe 90 GHz bands during summer and 113 GHz bands during winter.)

Backends(back to top)

FFTS: bandwidth: 1000, 500, 250, 200 MHz bandwidths, 16384 channels;

Band Width

Channel Width (theory)

Channel Width (measured)

Notes

200 MHz

12.2 kHz

12.2 kHz

基带变换1000 MHz

250 MHz

15.3 kHz

15.3 kHz

1000 MHz

61.0 kHz

61.0 kHz

500 MHz

30.5 kHz

30.5 kHz

基带变换500 MHz

AOS: 3-line system(12CO, 13CO, C18O, 1-0). See below:

Backends

Bandwidth(MHz)

Central freq. (MHz)

Channels

Channel

Width(KHz)

Frequency

Resolution(KHz)

AOS-I(13CO)
(
110.201353 GHz)

42.691

70.01294

1024

41.73

79.3±2.5

AOS-II(C18O)
(109.782183 GHz)

43.077

70.00898

1024

42.13

80.7±4.2

AOS-III(12CO)
(115.271204 GHz)

145.337

225.4101

1024

142.06

212.7±5.9


The measured antenna temperature is T_A*, after the correction of atmospheric absorption and Omic loss. 

 

Observation modes: beam switch, position switch, grid mapping, on-the-fly (OTF) mapping, sky dip.

Proposal: (back to top)

Proposal submission via email to proposal@mail.pmodlh.ac.cn at any time. Application form (Chinese) can be download from here

To use AOS backends, download and run software: AOSfreqset (download here: http://www.pmodlh.ac.cn/AOSfreqset.rar)

To use FFTS backends, download and run software: FFTSfreqset (download here: http://www.pmodlh.ac.cn/FFTSfreqset.rar)

To do mapping, download and run software: dtg.tcl (download here: http://www.pmodlh.ac.cn/dtg6.2.rar)

Download the Chinese version of telescope manual here: http://www.pmodlh.ac.cn/13.7guanceshouce2007-10-18.pdf

 

(back to top)

 

 [ previous ] [ upper ] [ next ] Welcome comments to me: jinhuaheynao.ac.cn [back to my Home]