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{{attachment:E1_BBC1_s28.png|E1_BBC1_s28|width=400}} {{attachment:E1_BBC2_s28.png|E1_BBC2_s28|width=400}} {{attachment:E1_BBC3_s28.png|E1_BBC3_s28|width=400}} {{attachment:E1_BBC4_s28.png|E1_BBC4_s28|width=400}}
{{attachment:E1_NBC5_s28.png|E1_NBC5_s28|width=400}} {{attachment:E1_NBC6_s28.png|E1_NBC6_s28|width=400}} 		{{attachment:E1_BBC1_s28.png|E1_BBC1_s28|width=500}} {{attachment:E1_BBC2_s28.png|E1_BBC2_s28|width=500}} {{attachment:E1_BBC3_s28.png|E1_BBC3_s28|width=500}} {{attachment:E1_BBC4_s28.png|E1_BBC4_s28|width=500}}
{{attachment:E1_NBC5_s28.png|E1_NBC5_s28|width=500}} {{attachment:E1_NBC6_s28.png|E1_NBC6_s28|width=500}}
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{{attachment:E2_BBC1_s32.png|E2_BBC1_s32|width=400}} {{attachment:E2_BBC2_s32.png|E2_BBC2_s32|width=400}} {{attachment:E2_BBC3_s32.png|E2_BBC3_s32|width=400}} {{attachment:E2_BBC4_s32.png|E2_BBC4_s32|width=400}}
{{attachment:E2_NBC5_s32.png|E2_NBC5_s32|width=400}} {{attachment:E2_NBC6_s32.png|E2_NBC6_s32|width=400}} 		{{attachment:E2_BBC1_s32.png|E2_BBC1_s32|width=500}} {{attachment:E2_BBC2_s32.png|E2_BBC2_s32|width=500}} {{attachment:E2_BBC3_s32.png|E2_BBC3_s32|width=500}} {{attachment:E2_BBC4_s32.png|E2_BBC4_s32|width=500}}
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{{attachment:E2_BBC1_s34.png|E2_BBC1_s34|width=400}} {{attachment:E2_BBC2_s34.png|E2_BBC2_s34|width=400}} {{attachment:E2_BBC3_s34.png|E2_BBC3_s34|width=400}} {{attachment:E2_BBC4_s34.png|E2_BBC4_s34|width=400}}
{{attachment:E2_NBC5_s34.png|E2_NBC5_s34|width=400}} {{attachment:E2_NBC6_s34.png|E2_NBC6_s34|width=400}} 		{{attachment:E2_BBC1_s34.png|E2_BBC1_s34|width=500}} {{attachment:E2_BBC2_s34.png|E2_BBC2_s34|width=500}} {{attachment:E2_BBC3_s34.png|E2_BBC3_s34|width=500}} {{attachment:E2_BBC4_s34.png|E2_BBC4_s34|width=500}}
{{attachment:E2_NBC5_s34.png|E2_NBC5_s34|width=500}} {{attachment:E2_NBC6_s34.png|E2_NBC6_s34|width=500}}

Skydip Observations with EMIR

Go to the NIKA2 main page.

Skydip Observations with EMIR

2017-02-22: two skydips were performed in both bands E1 & E2. The central frequency for each band was set to 151.60 GHz and 256.68 GHz (average of A1 & A3) after calculations of the effective frequency for the NIKA2 bands by J. Macias (A1 => 255.53 GHz, A2 => 151.60 GHZ, A3 => 257.84). The weather conditions were very similar for both measurements with pwv = 7 [mm]. Scan numbers for the bands are: 26, 28 for E1 and 32, 34 for E2. The recorded bands are 4 BBCs (LSB & USB in HORIZONTAL & VERTICAL polarizations) and 2 NBC (USB in HORIZONTAL & VERTICAL polarizations). Opacity results are given in the plots.

Results E1, s26:

E1_BBC1_s26 E1_BBC2_s26 E1_BBC3_s26 E1_BBC4_s26 E1_NBC5_s26 E1_NBC6_s26

Results E1, s28:

E1_BBC1_s28 E1_BBC2_s28 E1_BBC3_s28 E1_BBC4_s28 E1_NBC5_s28 E1_NBC6_s28

Results E2, s32:

E2_BBC1_s32 E2_BBC2_s32 E2_BBC3_s32 E2_BBC4_s32 E2_NBC5_s32 E2_NBC6_s32

Results E2, s34:

E2_BBC1_s34 E2_BBC2_s34 E2_BBC3_s34 E2_BBC4_s34 E2_NBC5_s34 E2_NBC6_s34

OffProcNika2Run9 (last edited 2017-03-02 09:51:11 by NikaBolometer)