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K. Ng

4 papers hereh-index 474 citations8 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author3

Across the 3 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph4
same name
  • K. Ng — 96 papers, h 26
  • K. Ng — 59 papers, h 34
  • K. Ng — 19 papers, h 10
  • K. Ng — 17 papers, h 5
  • K. Ng — 11 papers, h 13
  • K. Ng — 10 papers, h 13

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
19931996
most citedLarge-angle Polarization of the Cosmic Microwave Background Radiation and Reionization

26 citations · 64 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph1996★ 2 cited

Stokes Parameters in Cosmic Microwave Background Measurements

Ka Lok Ng, Kin-Wang Ng

We compute numerically the scalar- and tensor-mode induced Stokes parameters of the cosmic microwave background, by taking into account the basis rotation effects. It is found that…

astro-ph1994★ 26 cited

Large-angle Polarization of the Cosmic Microwave Background Radiation and Reionization

Ka Lok Ng, Kin-Wang Ng, 19 pages +3

We discuss the effect of matter reionization on the large-angular-scale anisotropy and polarization of the cosmic microwave background radiation (CMBR) in the standard CDM model. W…

astro-ph1994★ 19 cited

Gravitational Wave Induced Large-scale Polarization of \\Cosmic Microwave Background Radiation

Ka Lok Ng, Kin-Wang Ng

We discuss the contribution of gravitational wave to the cosmic microwave background radiation (CMBR) anisotropy and polarization. It is found that the large-scale polarization of…

astro-ph1993★ 17 cited

Large-scale Polarization of the Cosmic Microwave Background Radiation

Ka Lok Ng, Kin-Wang Ng

The anisotropy and polarization of the cosmic microwave background radiation (CMBR) induced by the scalar and tensor metric perturbations are computed in the long-wavelength limit.…

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