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27 April 2024
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313
for query "
G. Peres
". (0.00 sec.)
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1.
X-ray spectral and timing characteristics of the stars in the young open cluster IC 2391
A. Marino
;
G. Micela
;
G. Peres
;
I. Pillitteri
;
S. Sciortino
;
5 Oct 2004
2.
X-ray spectral and timing characteristics of the stars in the young open cluster IC 2391
A. Marino
;
G. Micela
;
G. Peres
;
I. Pillitteri
;
S. Sciortino
;
5 Oct 2004
3.
Reply to `Comment on "Gapless Spin-1 Neutral Collective Mode Branch for Graphite"' by Peres et al
G. Baskaran
;
S.A. Jafari
;
10 Dec 2003
4.
ROSAT-HRI investigation of the NGC 507 X-ray halo
M. Paolillo
;
G. Fabbiano
;
G. Peres
;
D.-W. Kim
;
20 Nov 2002
/ Astrophys.J. 586 (2003) 850-867
5.
Atmospheric neutrinos: LMA oscillations, Ue3 induced interference and CP-violation
O. L. G. Peres
;
A. Yu. Smirnov
;
27 Sep 2003
/ Nucl.Phys. B680 (2004) 479-509
6.
Probing the LSND scale and four neutrino scenarios with a neutrino telescope
H. Nunokawa
;
O. L. G. Peres
;
R. Zukanovich Funchal
;
5 Feb 2003
/ Phys.Lett. B562 (2003) 279-290
7.
LMA parameters and non-zero $U_{e3}$ effects on atmospheric $ u$ data?
O. L. G. Peres
;
A. Yu. Smirnov
;
9 Dec 2001
/ Nucl.Phys.Proc.Suppl. 110 (2002) 355-357
8.
Global Analysis of the post-SNO Solar Neutrino Data for Standard and Non-Standard Oscillation Mechanisms
A. M. Gago
;
M. M. Guzzo
;
P. C. de Holanda
;
H. Nunokawa
;
O. L. G. Peres
;
V. Pleitez
;
R. Zukanovich Funchal
;
4 Dec 2001
/ Phys.Rev. D65 (2002) 073012
9.
Constraining the $3-3-1$ model with heavy neutral leptons using $(g-2)_{mu}$ and dark matter observables
C. E. Alvarez-Salazar
;
O. L. G. Peres
;
15 Jun 2019
10.
Coronal properties of G-type stars in different evolutionary phases
L. Scelsi
;
A. Maggio
;
G. Peres
;
R. Pallavicini
;
28 Dec 2004
11.
Anchored expansion, percolation and speed
Dayue Chen
;
Yuval Peres
;
Gabor Pete
;
26 Mar 2003
/ Annals of Probability 2004, Vol. 32, No. 4, 2978-2995 DOI: 10.1214/009117904000000586
12.
Finite-Temperature Transport in Finite-Size Hubbard Rings in the Strong-Coupling Limit
N. M. R. Peres
;
R. G. Dias
;
P. D. Sacramento
;
J. M. P. Carmelo
;
19 Nov 1999
13.
Density modulo 1 of sublacunary sequences: application of Peres-Schlag's argument
Nikolai G. Moshchevitin
;
21 Sep 2007
14.
A version of the proof for Peres-Schlag's theorem on lacunary sequence
Nikolai G. Moshchevitin
;
15 Aug 2007
15.
Are coronae of late type stars made of solar-like structures? The Fx-HR diagram and the pressure-temperature correlation
G. Peres
;
S. Orlando
;
F. Reale
;
14 May 2004
/ Astrophys.J. 612 (2004) 472-480
16.
Comment on "Gapless Spin-1 Neutral Collective Mode Branch for Graphite"
N. M. R. Peres
;
M. A. N. Araujo
;
A. H. Castro Neto
;
10 Dec 2003
17.
The distribution of emission measure, and of heating budget, among the loops in the corona
G. Peres
;
S. Orlando
;
F. Reale
;
R. Rosner
;
9 Nov 2001
18.
On the massless "just-so" solution to the solar neutrino problem
M. M. Guzzo
;
H. Nunokawa
;
P. C. de Holanda
;
O. L. G. Peres
;
7 Dec 2000
/ Phys.Rev. D64 (2001) 097301
19.
(3+1)-spectrum of neutrino masses: A chance for LSND?
O. L. G. Peres
;
A. Yu. Smirnov
;
3 Nov 2000
/ Nucl.Phys. B599 (2001) 3
20.
Quantum and classical descriptions of a measuring apparatus
Ori Hay
;
Asher Peres
;
19 Dec 1997
/ Phys.Rev. A58 (1998) 116
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