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  • Crowrite
  • 2025
    • 0225-TODO
    • 0107-Convolution
    • 0115-file saving
    • 0118-recycling method factor
    • 0121-constraints on tensor-scalar ratio
    • 0122-better way to use my own code
    • 0124-r constraint
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  • 2024
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    • 0221-Statistical properties of polarized radio sources at high frequency... arxiv:1003.5846
    • 0223-Primordial B-mode Diagnostics and Self Calibrating the CMB Polarization arxiv:0912.3532
    • 0226-it is customary to mask detected point sources in order to eliminate this spurious contribution
    • 0227-(WMAP) Observations: Foreground Emission arxiv:0302208
    • 0228-Ali-first light
    • 0229-Masking versus removing point sources in CMB data: arxiv:1207.2315
    • 0301-Galactic cold Clump
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    • 0521-Astrometry
    • 0522-AGN Two-season ACTPol Extragalactic Point Sources and their Polarization properties
    • 0523-classmethod and static method
    • 0528-ACT DR5 maps of 18 000 square degrees of the microwave sky from ACT 2008-2018 data
    • 0619-Gaussian profile
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  1. 2025

0225-TODO

GMCA inpaint?

https://github.com/sriniraghunathan/inpainting

https://arxiv.org/abs/2405.06820

inpaint using m3 method

matched filter lon lat coordinate.

A METHOD FOR INDIVIDUAL SOURCE BRIGHTNESS ESTIMATION IN SINGLE- AND MULTI-BAND

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