First results from viper: Detection of small scale anisotropy at 40 GHZ - INSPIRE

DataBETA

First results from viper: Detection of small scale anisotropy at 40 GHZ

J.B. Peterson
(
- Carnegie Mellon U.
)
,
G.S. Griffin
(
- Carnegie Mellon U.
)
,
M.G. Newcomb
(
- Carnegie Mellon U.
)
,
D.L. Alvarez
(
- Carnegie Mellon U.
)
,
C.M. Cantalupo
(
- Carnegie Mellon U.
)

Oct, 1999

5 pages

Published in:

Astrophys.J.Lett. 532 (2000) L83

e-Print:

astro-ph/9910503 [astro-ph]

DOI:

10.1086/312576

View in:

ADS Abstract Service

reference search48 citations

Citations per year

Abstract: (arXiv)

Results of a search for small-scale anisotropy in the cosmic microwave background (CMB) are presented. Observations were made at the South Pole using the Viper telescope, with a .26 degree (FWHM) beam and a passband centered at 40 GHz. Anisotropy band-power measurements in bands centered at l = 108, 173, 237, 263, 422 and 589 are reported. Statistically significant anisotropy is detected in all bands.

References(13)

Figures(0)

Estimating the power spectrum of the cosmic microwave background

- Phys.Rev.D 57 (1998) 2117-2137
•
e-Print:
- astro-ph/9708203
•
DOI:
- 10.1103/PhysRevD.57.2117

An Upper limit to arcminute scale anisotropy in the cosmic microwave background radiation at 142-GHz

S.E. Church
(
- Caltech
)
,
K.M. Ganga
(
- Caltech
)
,
P.A.R. Ade
(
- Queen Mary, U. of London
)
,
W.L. Holzapfel
(
- Caltech and
- UC, Berkeley
)
,
P.D. Mauskopf
(
- Caltech and
- UC, Berkeley
)

et al.

- Astrophys.J. 484 (1997) 523
•
e-Print:
- astro-ph/9702196
•
DOI:
- 10.1086/304362

Anisotropy in the cosmic microwave background at degree angular scales: Python V results

K. Coble
(
- Chicago U., EFI
)
,
M. Dragovan
(
- Chicago U., EFI
)
,
J. Kovac
(
- Chicago U., EFI
)
,
N.W. Halverson
(
- Chicago U., EFI and
- Caltech
)
,
W.L. Holzapfel
(
- Chicago U., EFI
)

et al.

- Astrophys.J.Lett. 519 (1999) L5-8
•
e-Print:
- astro-ph/9902195
•
DOI:
- 10.1086/312093

- Astron.J. 105 1666

The Physics of microwave background anisotropies

Wayne Hu
(
)
,
Naoshi Sugiyama
(
- UC, Berkeley, Astron. Dept. and
- UC, Berkeley, CfPA and
- Tokyo U. and
- Tokyo U., RESCEU
)
,
Joseph Silk
(
)

- Nature 386 (1997) 37-43
•
e-Print:
- astro-ph/9604166
•
DOI:
- 10.1038/386037a0

Small scale cosmic microwave background anisotropies as a probe of the geometry of the universe

Marc Kamionkowski
(
- Princeton, Inst. Advanced Study
)
,
David N. Spergel
(
- Princeton U. Observ.
)
,
Naoshi Sugiyama
(
- UC, Berkeley, CfPA and
- Tokyo U.
)

- Astrophys.J.Lett. 426 (1994) L57
•
e-Print:
- astro-ph/9401003
•
DOI:
- 10.1086/187339

Correlated Errors in the COBE DMR Sky Maps

et al.

- Astrophys.J. 436 (1994) 452
•
e-Print:
- astro-ph/9403021
•
DOI:
- 10.1086/174920

What can cosmic microwave background observations already say about cosmological parameters in open and critical density cold dark matter models?

Charles H. Lineweaver
(
- Strasbourg, CRN
)
,
Domingos Barbosa
(
- Porto U.
)

- Astrophys.J. 496 (1998) 624
•
e-Print:
- astro-ph/9706077
•
DOI:
- 10.1086/305408

- Astrophys.J. 474 4766

CMB anisotropy constraints on open and flat lambda CDM cosmogonies from UCSB south pole, ARGO, MAX, white dish, and SuZIE data

Bharat Ratra
(
- Kansas State U.
)
,
Radoslaw Stompor
(
- Cambridge U. and
- Warsaw, Copernicus Astron. Ctr.
)
,
Ken Ganga
(
- Caltech
)
,
Graca Rocha
(
- Warsaw, Copernicus Astron. Ctr.
)
,
Naoshi Sugiyama
(
- Kyoto U., RIMS
)

et al.

- Astrophys.J. 517 (1999) 549
•
e-Print:
- astro-ph/9901014
•
DOI:
- 10.1086/307236

A Line of sight integration approach to cosmic microwave background anisotropies

- Astrophys.J. 469 (1996) 437-444
•
e-Print:
- astro-ph/9603033
•
DOI:
- 10.1086/177793

Anisotropies in the cosmic microwave background

Martin J. White
(
- UC, Berkeley, CfPA
)
,
Douglas Scott
(
- UC, Berkeley, CfPA
)
,
Joseph Silk
(
- UC, Berkeley, CfPA
)

- Ann.Rev.Astron.Astrophys. 32 (1994) 319-370
•
DOI:
- 10.1146/annurev.aa.32.090194.001535

- Astrophys.J.Suppl. 91 111