Describe GoalsPrepStaffNika2TestRun54 here.

NIKA2 technical run #54 / September 2021

Back to the NIKA2 Run 54 main page

Goals

Do a complete setup of NIKA2 in advance of the science runs starting in October 2021.

TO BE UPDATED

-- Sweep

-- beam map

-- skydip

-- secondary calibrators

Test polarization setup

TO BE UPDATED

-- planets and quasars

Test the external calibrator

TO BE UPDATED

The previous test was successful and we have learned a lot. The signal is well detected (Pi-Pq) 100 Hz @ 1mm and 800Hz @ 2mm. Using the HWP, it is polarized (80%) at 1mm. In order to exclude various scenarios, we need to repeat the tests, essentially made of skydips. A session of 2-3 hours max will be necessary that should be contiguous with the polarisation session so as to be in the fast acquisition mode. Skydip should be modified so as to include 90 degrees step. Others should include the 0 degree elevation if the Kid tuning is ok.

-- Do a skydip without the source on but with the pi-pq mode, in order to test if we find 0

-- Do a skydip with source @1mm on

-- Do a skydip with source @2mm on

-- Do a skydip with both sources on.

See this data analysis page

Sources

• Visibilities of science sources:

• Strongly polarized quasars (>10% with POLAMI@1mm in past month):

TO BE CHECKED

-- The usual 3C286.

-- 0219+428 (I=0.5Jy, 12% on Sept. 29)= J0222+4302

-- 0851+202 (I=2.7Jy, 11% on Oct. 14)= OJ287

-- 1127-145 (I=0.4Jy, 12% on Oct. 14)= J1130-1449

• NOEMA has only observed 1044+719 at 1mm the past 2weeks (and gives 2% polar)

• Visibilities of quasars:

Observers and Schedule

TO BE UPDATED

• Telescope Schedule
  

• Due to the Covid pandemic there's no travel at the telescope, observations will be on remote with the help of the remote AOD and Operators at the telescope. List of the remote observers and the shifts:
  

TO BE DEFINED

• Angel is the AoD, see IRAM's http://www.iram.es/IRAMES/mainWiki/AstronomersOnDutySchedule.