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OTF Test Observation ---NGC2264

1. Observation Time:2011-4-21 ~ 2011-4-23 8 hours.

   2011-5-7 7 hours.

System Temperature:

2011-4-21 ~ 2011-4-23 Tsys of Lower Band: 160 K ~ 239 K;

Tsys of Uper Band: 260 K ~ 441 K

2011-5-7              Tsys of Lower Band: 175 K ~ 235 K;

Tsys of Uper Band : 270 K ~ 390 K

2. Observation Parameter:

SOURCE

NGC2264

Observation Center

RA(B1950) : 06:38:10.00

DEC(B1950): +09:40:00.0

Scans Repeat

4

THETAROW (arcsec)

15

WIDTH(arcsec)

1200

HEIGHT(arcsec)

6000

RAMP(acccleratingrcgion)【second of arc】

10

SCANRATE (arcsec/sec)

75

TDUMP (sec)

0.2

CALRATE Interval (minute)

3

OFFINTTIME (sec)

1.3

CALINTTIME(sec)

2

3. Results:

Fig. 1 left panel:integral intensity (Unit in K km s-1) for CO(1-0), velocity range from -4 to -20 km/s;right panel: line noise (Unit in K) per channel for CO(1-0).

Fig. 2 left panel:integral intensity for 13CO(1-0), velocity range from -4 to -20 km/s;right panel: line noise per channel for 13CO(1-0).

 

 

(image or by WU Yuan Wei)

Fig. 3 left panel:integral intensity for C18O(1-0), velocity range from -4 to -20 km/s;right panel: line noise per channel for C18O(1-0).

 

(image or by WU Yuan Wei)

Fig.4: Top, middle and bellows are Spectra map for 12CO(1-0)、13CO(1-0) and C18O(1-0).

 

(image or by WU Yuan Wei)

Fig.5 Top, middle and below are rms distributions for 12CO(1-0)、13CO(1-0) and C18O(1-0). The reason for the double peak profile is that rms in the bottom region of NGC2264 are larger than the middle and top region.

 

 
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