cosmic microwave background And NotKarl Glazebrook
List of bibliographic references
Number of relevant bibliographic references: 9.| Ident. | Authors (with country if any) | Title |
|---|---|---|
| 000339 | Gayoung Chon ; Anthony Challinor ; Simon Prunet [France] ; Eric Hivon [États-Unis] ; István Szapudi [États-Unis] | Fast estimation of polarization power spectra using correlation functions |
| 000340 | Gayoung Chon [Royaume-Uni] ; Anthony Challinor ; Simon Prunet [France] ; Eric Hivon [États-Unis] ; István Szapudi [États-Unis] | Fast estimation of polarization power spectra using correlation functions |
| 000345 | T. Poutanen [Finlande] ; D. Maino [Italie] ; H. Kurki-Suonio [Finlande] ; E. Keih Nen [Finlande] ; E. Hivon [États-Unis] | Cosmic microwave background power spectrum estimation with the destriping technique |
| 000353 | S. Peng Oh [États-Unis] ; Asantha Cooray [États-Unis] ; Marc Kamionkowski [États-Unis] | Sunyaev—Zeldovich fluctuations from the first stars? |
| 000359 | Xuelei Chen [États-Unis] ; Asantha Cooray [États-Unis] ; Naoki Yoshida [Japon] ; Naoshi Sugiyama [Japon] | Can non-Gaussian cosmological models explain the WMAP high optical depth for reionization? |
| 000372 | S. Peng Oh ; Asantha Cooray [États-Unis] ; Marc Kamionkowski [États-Unis] | Sunyaev–Zeldovich fluctuations from the first stars? |
| 000387 | Xuelei Chen [États-Unis] ; Asantha Cooray [États-Unis] ; Naoki Yoshida [Japon] ; Naoshi Sugiyama [Japon] | Can non‐Gaussian cosmological models explain the WMAP high optical depth for reionization? |
| 000416 | G. Efstathiou [États-Unis] | Principal‐component analysis of the cosmic microwave background anisotropies: revealing the tensor degeneracy |
| 000417 | G. Efstathiou [États-Unis, Royaume-Uni] | Principal-component analysis of the cosmic microwave background anisotropies: revealing the tensor degeneracy |
| This area was generated with Dilib version V0.6.32. |  |