Differences between revisions 26 and 28 (spanning 2 versions)
Revision 26 as of 2017-02-25 11:46:14
Size: 4400
Editor: PabloGarcia
Comment:
Revision 28 as of 2017-02-25 11:57:44
Size: 4648
Editor: PabloGarcia
Comment:
Deletions are marked like this. Additions are marked like this.
Line 35: Line 35:
{{attachment:E1_BBC1_s16.png|E1_BBC1_s16|width=500}} {{attachment:E1_BBC2_s16.png|E1_BBC2_s16|width=500}} {{attachment:E1_BBC3_s16.png|E1_BBC3_s16|width=500}} {{attachment:E1_BBC4_s16.png|E1_BBC4_s16|width=500}}
{{attachment:E1_NBC5_s16.png|E1_NBC5_s16|width=500}} {{attachment:E1_NBC6_s16.png|E1_NBC6_s16|width=500}}
{{attachment:E1_BBC1_25FEB2017_s16-2.png|E1_BBC1_s16|width=500}} {{attachment:E1_BBC2_25FEB2017_s16-2.png|E1_BBC2_s16|width=500}} {{attachment:E1_BBC3_25FEB2017_s16-2.png|E1_BBC3_s16|width=500}} {{attachment:E1_BBC4_25FEB2017_s16-2.png|E1_BBC4_s16|width=500}} {{attachment:E1_NBC5_25FEB2017_s16-2.png|E1_NBC5_s16|width=500}} {{attachment:E1_NBC6_25FEB2017_s16-2.png|E1_NBC6_s16|width=500}}
Line 40: Line 39:
{{attachment:E1_BBC1_s18.png|E1_BBC1_s18|width=500}} {{attachment:E1_BBC2_s18.png|E1_BBC2_s18|width=500}} {{attachment:E1_BBC3_s18.png|E1_BBC3_s18|width=500}} {{attachment:E1_BBC4_s18.png|E1_BBC4_s18|width=500}}
{{attachment:E1_NBC5_s18.png|E1_NBC5_s18|width=500}} {{attachment:E1_NBC6_s18.png|E1_NBC6_s18|width=500}}
{{attachment:E1_BBC1_25FEB2017_s18.png|E1_BBC1_s18|width=500}} {{attachment:E1_BBC2_25FEB2017_s18.png|E1_BBC2_s18|width=500}} {{attachment:E1_BBC3_25FEB2017_s18.png|E1_BBC3_s18|width=500}} {{attachment:E1_BBC4_25FEB2017_s18.png|E1_BBC4_s18|width=500}} {{attachment:E1_NBC5_25FEB2017_s18.png|E1_NBC5_s18|width=500}} {{attachment:E1_NBC6_25FEB2017_s18.png|E1_NBC6_s18|width=500}}
Line 45: Line 43:
{{attachment:E2_BBC1_s11.png|E2_BBC1_s11|width=500}} {{attachment:E2_BBC2_s11.png|E2_BBC2_s11|width=500}} {{attachment:E2_BBC3_s11.png|E2_BBC3_s11|width=500}} {{attachment:E2_BBC4_s11.png|E2_BBC4_s11|width=500}}
{{attachment:E2_NBC5_s11.png|E2_NBC5_s11|width=500}} {{attachment:E2_NBC6_s11.png|E2_NBC6_s11|width=500}}
{{attachment:E2_BBC1_25FEB2017_s11.png|E2_BBC1_s11|width=500}} {{attachment:E2_BBC2_25FEB2017_s11.png|E2_BBC2_s11|width=500}} {{attachment:E2_BBC3_25FEB2017_s11.png|E2_BBC3_s11|width=500}} {{attachment:E2_BBC4_25FEB2017_s11.png|E2_BBC4_s11|width=500}} {{attachment:E2_NBC5_25FEB2017_s11.png|E2_NBC5_s11|width=500}} {{attachment:E2_NBC6_25FEB2017_s11.png|E2_NBC6_s11|width=500}}
Line 50: Line 47:
{{attachment:E2_BBC1_s13.png|E2_BBC1_s13|width=500}} {{attachment:E2_BBC2_s13.png|E2_BBC2_s13|width=500}} {{attachment:E2_BBC3_s13.png|E2_BBC3_s13|width=500}} {{attachment:E2_BBC4_s13.png|E2_BBC4_s13|width=500}}
{{attachment:E2_NBC5_s13.png|E2_NBC5_s13|width=500}} {{attachment:E2_NBC6_s13.png|E2_NBC6_s13|width=500}}
{{attachment:E2_BBC1_25FEB2017_s13.png|E2_BBC1_s13|width=500}} {{attachment:E2_BBC2_25FEB2017_s13.png|E2_BBC2_s13|width=500}} {{attachment:E2_BBC3_25FEB2017_s13.png|E2_BBC3_s13|width=500}} {{attachment:E2_BBC4_25FEB2017_s13.png|E2_BBC4_s13|width=500}} {{attachment:E2_NBC5_25FEB2017_s13.png|E2_NBC5_s13|width=500}} {{attachment:E2_NBC6_25FEB2017_s13.png|E2_NBC6_s13|width=500}}

Go to the Run9 page.


Skydip Observations with EMIR

General Procedure: two skydips are performed in both bands E1 & E2. The central frequency for each band is set to 151.60 GHz USB and 256.68 GHz USB (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 recorded bands are 4 BBCs (LSB & USB in HORIZONTAL & VERTICAL polarizations) and 2 NBC (USB in HORIZONTAL & VERTICAL polarizations). The scans are reduced in MIRA following the procedure outlined here. Opacity results are given in the plots.

2017-02-22, Skydip Azimuth = 134.05°: weather conditions were very similar for both measurements with pwv ~ 7 [mm]. A pointing (dAz = 3.7", dEl = 6.1") and focus (dFz = -2.0 mm) was performed on Mars to check the EMIR settings. Scan numbers for the bands are: 26, 28 for E1 and 32, 34 for E2. WARNING: the E2 frequency used in this day was 256.0 GHz instead of 256.68 GHz due to a typo in the NIKA2.lin file.

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

2017-02-25, Skydip Azimuth = 128.70°: weather conditions for both measurements with pwv ~ 3 [mm] but VERY UNSTABLE. A pointing (dAz = 4.0", dEl = -1.0") and focus (dFz = -2.4 mm) was performed on Jupiter to check the EMIR settings. A focus was done after the skydip measurements to check that the focus correction first applied using the E2 tuning was also adequate for E1 (dFz = -2.5 mm, consistent). Scan numbers for the bands are: 16, 18 for E1 and 11, 13 for E2.

Results E1, s16:

E1_BBC1_s16 E1_BBC2_s16 E1_BBC3_s16 E1_BBC4_s16 E1_NBC5_s16 E1_NBC6_s16

Results E1, s18:

E1_BBC1_s18 E1_BBC2_s18 E1_BBC3_s18 E1_BBC4_s18 E1_NBC5_s18 E1_NBC6_s18

Results E2, s11:

E2_BBC1_s11 E2_BBC2_s11 E2_BBC3_s11 E2_BBC4_s11 E2_NBC5_s11 E2_NBC6_s11

Results E2, s13:

E2_BBC1_s13 E2_BBC2_s13 E2_BBC3_s13 E2_BBC4_s13 E2_NBC5_s13 E2_NBC6_s13

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