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Tests of the Observing Modes

Tests made on 20151021

On 20151021, the atmospheric conditions where poor (tau 225 GHz in the range 0.5-1.0), with fog. We were unable to obtain a proper focus, so we moved to test the observing modes. For this we used Jupiter + Ganymede with maps large enough normally to see both targets and check that the observing modes actually perform as expected. No skydip corrections where available at the time.

Observations where done between 04:24 and 06:16 UT.

From the positions of Jupiter and satellites according to JPL Horizon, here are the derived distances and position angles.

In the Azimuth-Elevation reference frame

Time

dist.

P.A.

dist.

P.A.

dist

P.A.

dist.

P.A.

(arcsec)

(degree)

(arcsec)

(degree)

(arcsec)

(degree)

(arcsec)

(degree)

Io

Europa

Ganymede

Callisto

2015-Oct-21 04:00 UT

4

38

83

-167

184

12

244

10

2015-Oct-21 04:30 UT

3

152

78

-166

182

12

247

10

2015-Oct-21 05:00 UT

10

-178

74

-165

178

13

249

11

2015-Oct-21 05:30 UT

17

-172

68

-164

176

15

252

12

2015-Oct-21 06:00 UT

23

-167

64

-161

173

17

255

14

2015-Oct-21 06:30 UT

30

-164

59

-158

169

20

257

17

2015-Oct-21 07:00 UT

37

-159

53

-153

166

24

260

22

In the ICRS (e.g. RA, Dec) Reference frame

2015-Oct-21 04:00 UT

4

-91

83

113

184

-65

244

-63

2015-Oct-21 04:30 UT

3

150

78

113

182

-65

247

-63

2015-Oct-21 05:00 UT

10

126

73

113

179

-66

249

-63

2015-Oct-21 05:30 UT

17

121

69

113

176

-66

252

-63

2015-Oct-21 06:00 UT

24

119

64

112

173

-66

255

-63

2015-Oct-21 06:30 UT

30

118

58

112

169

-66

257

-63

2015-Oct-21 07:00 UT

37

117

53

112

166

-66

260

-63

nkliss

  • Pako command: nkliss 6
  • Scan number: 20151021s22

  • Note: None
  • pipeline param:
    • param.map_xsize = 650
    • param.map_ysize = 650
    • param.map_proj: = ‘azel’
    • param.decor_cm_dmin = 40.

nkotf_square

  • Pako command: nkotf_square 10
  • Scan number: 20151021s24 et 20151021s25

  • Note: The observation produced 2 scan files. The pipeline does not find Antenna imbfits for scan 25, so only scan 24 was reduced.
  • pipeline param:
    • param.map_xsize = 700
    • param.map_ysize = 700
    • param.map_proj: = ‘azel’
    • param.decor_cm_dmin = 60.
    • param.decor_method = ‘COMMON_MODE_KIDS_OUT’
  • results:
    • Ganymede and Callisto are both seen at 1mm (left) and 2mm (right) images. The measured distances are 181 arcsec for Ganymede, 250 arcsec for Callisto, and position angle (from top, leftward) of 13 degree and 11 degree respectively, a good match for this observation taken close to 05:00 UT . (Not the that the images are displayed with IDL !order = 1 so that the pixel (0, 0) of the maps are at the top, left of the displayed image. With such !order, the results are as expected. The expected position of Europa is also marked, put it is too close from jupiter.

20151021s24_i1_with_satellites.png 20151021s24_i2_with_satellites.png

  • The coverage at 2mm (grid.nhits_2) is displayed below. The total map is 11.6 x 11.6 arc min on a side. The white square shows the 10 x 10 arc min area indicated by the pako command. Within this area, the coverage is not homogenous, from 130 hits on the edge to 330 in the middle. The dashed area correspond to 250 hits and above, and is 40 square arcmin (6.3 x 6.3 arc min). Maybe we should add a Pako message saying that the homogenous coverage is closer to 6’ x 6’.

20151021s24_nhits2.png

  • Observation mode seems OK, except for the remark of the coverage map.

nkotf in azel reference

  • Pako command: nkotf 3 10 0 0 30 50azel
  • Scan number: 20151021s27

  • Note: None
  • pipeline param:
    • param.map_xsize = 700
    • param.map_ysize = 700
    • param.map_proj: = ‘azel’
    • param.decor_cm_dmin = 60.
    • param.decor_method = ‘COMMON_MODE_KIDS_OUT’
  • results:
    • In the 2mm image (left), Ganymede is found at 180”, PA=13, Callisto at 254”, PA = 10. This is in good agreement with Horizon. (again, with convention !order = 1).
    • In the array 2 nhits map (right), the scanning at constant elevation is clear. The coverage is inhomogenous. The 3 x 10 arc min expected from the scan is shown by the white rectangle. The coverage in this rectangle goes from 80 to 240 hits...

20151021s27_i2_with_satellites.png 20151021s27_nhits2.png

OffProcNika2Run1ObsModeTests20151021 (last edited 2015-10-22 19:56:12 by NikaBolometer)