References
All excluded regions are at 90% CL unless noted otherwise. Most of
the contours were read off from the original postscript files. The
topdrawer files used to generate the plot is here.
- BNL E776
- Excluded region on numubar to nuebar appearance is
from L. Borodovsky et al., Phys. Rev.
Lett. 68, 274-277 (1992).
- Bugey
-
Limit is on nuebar disappearance from B. Achkar et al.,
Nucl. Phys.
B434, 503-534 (1995).
- CDHSW
- Excluded region on numu disappearance is from F. Dydak et
al., Phys. Lett. B134, 281 (1984).
- CHOOZ
- Limit is on nuebar disappearance from M. Apollonio et
al., hep-ex/0301017,
Eur. Phys. J. C27, 331-374 (2003), Fig. 55, Analysis A.
- CHORUS
- Excluded region on nue to nutau or numu to nutau appearance
is from E. Eskut et al., Phys. Lett.
B497, 8-22 (2001).
- Cl (Homestake)
- Preferred region on nue disappearance is based on hep-ex/0208004 by
Michael Smy.
- Ga (SAGE and GALLEX)
- Preferred region on nue disappearance at 95% CL is based on G.L. Fogli
et al., hep-ph/0506083,
adapted to 2 dof for this figure.
- KamLAND (NEW)
- Preferred region on nuebar disappearance at 95% CL, from hep-ex/0801.4589.
- KARMEN2
- Excluded region on numubar to nuebar appearance is from
A. Armbruster et al., hep-ex/0203021, Phys. Rev.
D65, 112001 (2002).
- K2K (NEW)
- Excluded region on numu to nue appearance at 90% CL, from hep-ex/0603004, Phys.
Rev. Lett. 96 181801 (2006).
- Preferred region on numu disappearance at 90% CL, from hep-ex/0606032, Phys.
Rev. D 74 072003 (2006).
- LSND
- Preferred region on numubar to nuebar appearance is from
A. Aguilar et al., hep-ex/0104049, Phys. Rev.
D64, 112007 (2001), at 90% and 99% CL.
- Mini-BooNE
- Excluded region on numu to nue appearance is from
A.A. Aguilar-Arevalo et al., arXiv:0704.1500,
Phys. Rev. Lett. 98, 231801 (2007).
- MINOS (NEW)
- Preferred region on numu disappearance from hep-ex/0708.1495v2
- NOMAD
- Excluded region on nue to nutau or numu to nutau appearance
is from P. Astier et al., hep-ex/0106102, Nucl. Phys.
B611, 3-39 (2001).
- Excluded region on numu to nue appearance
is from P. Astier et al., hep-ex/0306037, Phys. Lett.
B570, 19-31 (2003).
- Palo Verde
- Limit is on nuebar disappearance from F. Boehm et al.,
hep-ex/0107009, Phys. Rev.
D64, 112001 (2001), Fig. 7, solid curve.
- SNO
- Preferred region on nue disappearance at 95% CL is from nucl-ex/0502021,
Fig. 34.
- Super-Kamiokande (solar neutrino, NEW)
- Preferred region on nue disappearance at the 95% CL is based on hep-ex/0803.4312, Fig. 15,
center. The combination of all solar neutrino data at the 95% CL
from Fig. 15, right.
- Super-Kamiokande (atmospheric neutrino)
- Preferred region on numu disappearance at the 90% and 99% CL,
from the talk presented by Masato Shiozawa at International
School of Nuclear Physics, 27th Course, "Neutrinos in
Cosmology, in Astro, Particle, and Nuclear Physics," Erice, Sicily,
16-24 September, 2005.