Removal of point source leakage from time-order data filtering episode artwork

EPISODE · Nov 27, 2022 · 0 MIN

Removal of point source leakage from time-order data filtering

from Astro arXiv | all categories · host Corentin Cadiou

Removal of point source leakage from time-order data filtering by Zhaoxuan Zhang et al. on Sunday 27 November Time-ordered data (TOD) from ground-based CMB experiments are generally filtered before map-making to remove or reduce the contamination from the ground and the atmospheric emissions. However, when the observation region contains strong point sources, the filtering process will result in considerable leakage around the point sources in a measured CMB map, and leave spurious polarization signals. Therefore, such signals need to be assessed and removed before CMB science exploitation. In this work, we present a new method that we call "template fitting" and can effectively remove these leakage signals in pixel domain, not only satisfying the requirement for measuring primordial gravitational waves from CMB-$B$ modes, but also avoiding time-consuming operations on TOD. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2211.13870v1

Episode metadata supplied by the publisher feed · Published Nov 27, 2022

Embed this episode

NOW PLAYING

Removal of point source leakage from time-order data filtering

0:00 0:31

No transcript for this episode yet

We transcribe on demand. Request one and we'll notify you when it's ready — usually under 10 minutes.

No similar episodes found.

No similar podcasts found.

Frequently Asked Questions

How long is this episode of Astro arXiv | all categories?

This episode is 0 minutes long.

When was this Astro arXiv | all categories episode published?

This episode was published on November 27, 2022.

Can I download this Astro arXiv | all categories episode?

Yes. Use the download control on the episode player to save the publisher-provided media file.
URL copied to clipboard!