Diff for "OffProcNika2Run9" - www.iram.es Main Wiki

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Go to the Run9 page.

Skydip Observations with EMIR

General Procedure: two skydips were performed in both bands E1 & E2. The central frequency for each band was 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 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 perdormed on Mars to check the EMIR settings. 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). The scans were reduced in MIRA following the procedure outlined here. Opacity results are given in the plots.

2017-02-22:

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

-  ⇤ ← Revision 2 as of 2017-02-22 19:22:24 → 
  Size: 1119
  Editor: PabloGarcia
  Comment:
+   ← Revision 19 as of 2017-02-25 11:14:39 → ⇥
  Size: 2409
  Editor: PabloGarcia
  Comment:
-Deletions are marked like this.
+Additions are marked like this.
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-= Skydip Observations with EMIR =



'''Go to the [[http://www.iram.es/IRAMES/mainWiki/Continuum/NIKA2/Main| NIKA2]] main page.'''
+'''Go to the [[http://www.iram.es/IRAMES/mainWiki/Nika2Run9| Run9]] page.'''
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-= Skydip Observations with EMIR =
+== Skydip Observations with EMIR ==
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--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]. Sccan numbers for the bands are: 26, 27 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).
+'''General Procedure:''' two skydips were performed in both bands E1 & E2. The central frequency for each band was 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 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 perdormed on Mars to check the EMIR settings. 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). The scans were reduced in MIRA following the procedure outlined [[http://www.iram.es/IRAMES/mainWiki/ListOfAstroTargetNika2Run9/test/ | here]]. Opacity results are given in the plots.
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-Results E1, s25:
+'''2017-02-22''':
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-||[[attachment:E1_BBC1_s26.png|E1_BBC1_s26|width=500]] || [[attachment:E1_BBC2_s26.png|E1_BBC1_s26|width=500]] || [[attachment:E1_BBC3_s26.png|E1_BBC1_s26|width=500]] || [[attachment:E1_BBC4_s26.png|E1_BBC1_s26]|width=500] || 
||[[attachment:E1_NBC5_s26.png|E1_BBC1_s26|width=500]] || [[attachment:E1_NBC6_s26.png|E1_BBC1_s26|width=500]]
+Results E1, s26:

{{attachment:E1_BBC1_s26.png|E1_BBC1_s26|width=500}} {{attachment:E1_BBC2_s26.png|E1_BBC2_s26|width=500}} {{attachment:E1_BBC3_s26.png|E1_BBC3_s26|width=500}} {{attachment:E1_BBC4_s26.png|E1_BBC4_s26|width=500}}
{{attachment:E1_NBC5_s26.png|E1_NBC5_s26|width=500}} {{attachment:E1_NBC6_s26.png|E1_NBC6_s26|width=500}} 

Results E1, s28:

{{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}} 

Results E2, s32:

{{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}}
{{attachment:E2_NBC5_s32.png|E2_NBC5_s32|width=500}} {{attachment:E2_NBC6_s32.png|E2_NBC6_s32|width=500}} 

Results E2, s34:

{{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}}