Differences between revisions 4 and 9 (spanning 5 versions)
Revision 4 as of 2015-10-07 14:03:41
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Revision 9 as of 2015-10-13 21:34:34
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||112 || 12h10m || Mars || otf 400X220 arcsec || 200 || 45 || 0,0,-1.3 || 0.2-0.3 ||All the scan are not reconized from Elvin. It appears as _I_|| ||112 || 12h10m || Mars || otf 400X220 arcsec || 200 || 45 || 0,0,-1.3 || 0.2-0.3 ||All the scans are not reconized from Elvin. It appears as _I_||
Line 28: Line 28:
||114 || 12h21m || Mars || beam-map1 otf 300X300 arcsec || 200 || 35 || 0,0,-1.3 || 0.2-0.3 ||||
||115 || 12h21m || Mars || beam-map2 otf 300X300 arcsec || 200 || 35 || 0,0,-1.3 || 0.2-0.3 ||||
||116 || 12h21m || Mars || beam-map3 otf 300X300 arcsec || 200 || 35 || 0,0,-1.3 || 0.2-0.3 ||||
||114 || 12h21m || Mars || beam-map1 otf 300X300 arcsec || 200 || 35 || 0,0,-1.3 || 0.2-0.3 || 13/10: we need to check that it was in fact 600x225 !||
||115 || 12h21m || Mars || beam-map2 otf 300X300 arcsec || 200 || 35 || 0,0,-1.3 || 0.2-0.3 || 13/10: we need to check that it was in fact 600x225 !||
||116 || 12h21m || Mars || beam-map3 otf 300X300 arcsec || 200 || 35 || 0,0,-1.3 || 0.2-0.3 || 13/10: we need to check that it was in fact 600x225 !||
Line 32: Line 32:
||120 || 12h21m || 3C273 || otf 240X240 arcsec || 200 || 42 || 0,0,-1.3 || 0.2-0.3 |||| ||121 || 12h21m || 3C273 || otf 240X240 arcsec || 200 || 42 || 0,0,-1.3 || 0.2-0.3 ||||
||122 || 12h21m || 3C273 || otf 240X240 arcsec || 200 || 42 || 0,0,-2 || 0.2-0.3 ||changing focus||
||126 || 12h21m || Mercury || otf 240X240 arcsec || 200 || 30 || 0,0,-1.3 || 0.2-0.3 ||||
||127 || 12h21m || Mercury || otf 240X240 arcsec || 200 || 30 || 0,0,-2 || 0.2-0.3 ||||
||128 || 12h21m || Mercury || otf 240X240 arcsec || 200 || 30 || 0,0,-0.6 || 0.2-0.3 ||||

NIKA October 7th, 2015 / S1

Back to list of day to day logbook of observations

2015-10-07


Following not updated

.Cryostat Temperature: 170mK cooling down slowly

  • Arrays status tonight: full 2mm array - 1-3 Hz noise; 2 feed lines on 1mm array 3-5Hz noise

Modulation frequency: 10kHz 1mm, 5kHz 2mm

Opacity is measured with the new taumeter at 225 GHz

Nasmyth offsets : 0, 0

Set Focus : -1.3 mm (not at all optimised)

  • Quick description of the session: Test the Pako sequences and data flows.


Data Repository: /home/nika2/NIKA/Data/run13_mirror_1m_X/

Scan

UT

Source

Command

Az

El

Pointing X, Y, Focus

Tau225

Comment

112

12h10m

Mars

otf 400X220 arcsec

200

45

0,0,-1.3

0.2-0.3

All the scans are not reconized from Elvin. It appears as _I_

113

12h21m

Mars

otf 400X400 arcsec

200

40

0,0,-1.3

0.2-0.3

114

12h21m

Mars

beam-map1 otf 300X300 arcsec

200

35

0,0,-1.3

0.2-0.3

13/10: we need to check that it was in fact 600x225 !

115

12h21m

Mars

beam-map2 otf 300X300 arcsec

200

35

0,0,-1.3

0.2-0.3

13/10: we need to check that it was in fact 600x225 !

116

12h21m

Mars

beam-map3 otf 300X300 arcsec

200

35

0,0,-1.3

0.2-0.3

13/10: we need to check that it was in fact 600x225 !

119

12h21m

Mercury

otf 400X400 arcsec

200

43

0,0,-1.3

0.2-0.3

121

12h21m

3C273

otf 240X240 arcsec

200

42

0,0,-1.3

0.2-0.3

122

12h21m

3C273

otf 240X240 arcsec

200

42

0,0,-2

0.2-0.3

changing focus

126

12h21m

Mercury

otf 240X240 arcsec

200

30

0,0,-1.3

0.2-0.3

127

12h21m

Mercury

otf 240X240 arcsec

200

30

0,0,-2

0.2-0.3

128

12h21m

Mercury

otf 240X240 arcsec

200

30

0,0,-0.6

0.2-0.3

NK2015_Oct07 (last edited 2015-10-13 21:34:34 by NikaBolometer)