30 November 2020 to 3 December 2020
Kavli IPMU, Kashiwa, Japan
Asia/Tokyo timezone

Session

2. Systematics requirement toward the next generation CMB B-mode experiment

30 Nov 2020, 19:30
Remote access (Kavli IPMU, Kashiwa, Japan)

Remote access

Kavli IPMU, Kashiwa, Japan

Kashiwa, Japan

Presentation materials

There are no materials yet.

  1. Dr Eirik Gjerløw (University of Oslo)
    30/11/2020, 19:30

    The BeyondPlanck collaboration recently published the results from mapping out the global Bayesian posterior of instrumental and observational parameters jointly for LFI time-ordered data. These results are the first of their kind, providing an unique new perspective on the calibration process, and in this talk I will share some of the things we learned, and how that can be applied to future...

    Go to contribution page
  2. Dr Silvia Galli (IAP)
    30/11/2020, 19:55

    Accurate cosmological parameters estimates using polarization data put stringent requirements on maps calibration, as highlighted in the recent results of the Planck collaboration. In this talk, I will present the new results of a paper where we point out that a model-dependent determination of polarization calibration parameters can be achieved by the joint fit of the TE and EE CMB power...

    Go to contribution page
  3. Prof. Enrique Martínez-González (Instituto de Física de Cantabria (CSIC-UC))
    30/11/2020, 20:20

    A methodology to provide the polarization angle requirements for the different frequency channels of a given CMB B-mode experiment is presented. The component separation procedure used to separate the CMB from the foreground signals is considered in order to establish those requirements. In addition, it is also considered possible instrumental correlations among the different measured...

    Go to contribution page
  4. Dr Max Abitbol (University of Oxford)
    30/11/2020, 20:45

    I will discuss foreground and instrument systematic modeling for upcoming ground-based B-mode searches with the Simons Observatory (SO). I will begin by summarizing the power-spectrum domain foreground and systematic cleaning pipeline for SO. Using this framework we have quantified calibration requirements on bandpass and polarization angle systematics for the SO target of $\sigma_r\approx...

    Go to contribution page
  5. 30/11/2020, 21:10
Building timetable...