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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
    • 0128-new r constraint
    • 0311-MCA
    • 0331-PSM simulation
  • 2024
    • 0209-Linux and git basic command
    • 0213-How to take notes for research
    • 0214-Scientific method
    • 0215-Scientific method
    • 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
    • 0305-constrained realization and CMB S4
    • 0306-BICEP setup
    • 0307-Bicep setup
    • 0308-QUIJOTE
    • 0311-SPT point source catelogue
    • 0312-Jaffe Thesis: Foreground Challenge to CMB Polarization: Present Methodologies and New Concepts
    • 0314-python logger
    • 0318-The radio source counts at 15 GHz and their implications for cm-wave CMB imaging
    • 0320-Component separation methods for the PLANCK mission
    • 0326-Low-$\ell$ CMB analysis and inpainting Starck 2013
    • 0328-Sparsity
    • 0329-Morphological component analysis on the sphere
    • 0410-Planck 2018 V Planck 2015 IX
    • 0411- Fan region and Gum nebula, Coma and Virgo cluster
    • 0417-vec.ctypes.data
    • 0419-Stokes parameter
    • 0430-PBH
    • 0520-ACT Extragalactic Point Sources in the Southern Surveys at 150, 220 and 280 GHz
    • 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
    • 0619-EB noise level
    • 0703-bias from wrong covariance matrix estimation
    • 0718-np.random.choice
    • 0807-ps rmv brainstorm
    • 0814-test-inline-formula
    • 0814-healpy lon lat scope
    • 0816-change $ to $$
    • 0821-len() for np.ndarray
    • 0821-angdist snippets and hp.ang2pix lonlat range
    • 0823-same name of some variable
    • 0828-purity and completeness
    • 0904-template fitting advantage over matched filter
    • 0910-FUTURE CODE
    • 0911-EB leakage test
    • 0918-add prior to chi square fitting
    • 0929-PS results comparison
    • 1002-apodization
    • 1011-power spectrum estimation for partial sky
    • 1015-215GHz and 95GHz / th noise power spectrum
    • 1015-conference
    • 1020-compare different method pipeline-star
    • 1029-mask small scale structure
    • 1030-smoothing maps precautions
    • 1031-inpainting debug
    • 1031-unit test
    • 1105-inpainting steps
    • 1108-git tag
    • 1114-cut how many number PS can give good estimate of other components
    • 1118-nested title in markdown
    • 1122-some markdown format
    • 1202-lmax for maps
    • 1203-theory noise level
    • 1205-python local variable
    • 1210-BAO
    • 1217-pandas index
    • 1225-multiunion and reduce lists
  • Biophysics
    • Claycomb
      • Terminology
  • QUATA
    • term
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