Angular power spectra of the COBE dirbe maps

The angular power spectra of the infrared maps obtained by the DIRBE (Diffuse InfraRed Background Experiment) instrument on the COBE satellite have been obtained by two methods: the Hauser-Peebles method previously applied to the DMR maps, and by Fourier transforming portions of the all-sky maps projected onto a plane. The two methods give consistent results, and the power spectrum of the high-latitude dust emission is C_\ell \propto \ell^{-3} in the range 2 < \ell < 300.

References(8)

Figures(0)

The Wiener filtered COBE DMR data and predictions for the Tenerife experiment

- Astrophys.J. 464 (1996) 1
•
e-Print:
- astro-ph/9509045
•
DOI:
- 10.1086/177294

The COBE mission - Its design and performance two years after launch

et al.

- Astrophys.J. 397 (1992) 420-429
•
DOI:
- 10.1086/171797

- Nature 312 505

- Astron.J. 103 1313

- Astrophys.J. 185 757

Weighing the universe with the cosmic microwave background

Gerard Jungman
(
- Syracuse U.
)
,
Marc Kamionkowski
(
- Columbia U.
)
,
Arthur Kosowsky
(
- Harvard-Smithsonian Ctr. Astrophys. and
- Harvard U.
)
,
David N. Spergel
(
- Princeton U.
)

- Phys.Rev.Lett. 76 (1996) 1007-1010
•
e-Print:
- astro-ph/9507080
•
DOI:
- 10.1103/PhysRevLett.76.1007

- Astrophys.J. 460 1

- Astrophys.J. 278 L19