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| 2 | entering extended mode |
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| 3 | **campagne.tex |
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| 115 | [1 |
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| 117 | ] |
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| 122 | Underfull \hbox (badness 10000) in paragraph at lines 152--163 |
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| 123 | |
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| 124 | [] |
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| 125 | |
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| 126 | |
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| 127 | Overfull \hbox (65.94304pt too wide) in paragraph at lines 175--175 |
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| 128 | [][]\T1/cmr/m/n/8 PACS num-bers: 13.30.a,14.20.Dh,14.60.Pq,26.65.t+,29.40.Gx,29.40.Ka,29.40.Mc,95.55.Vj,95.85.Ry, |
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| 129 | [] |
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| 130 | |
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| 131 | [2] [3] [4] [5] |
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| 132 | File: Fig1-T100K_3d.eps Graphic file (type eps) |
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| 133 | <Fig1-T100K_3d.eps> [6] |
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| 134 | File: Fig2-LenaPictureNov06.eps Graphic file (type eps) |
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| 135 | <Fig2-LenaPictureNov06.eps> [7] |
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| 136 | File: Fig3-MEMPHYS.eps Graphic file (type eps) |
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| 137 | <Fig3-MEMPHYS.eps> [8] |
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| 138 | Underfull \hbox (badness 2573) in paragraph at lines 486--501 |
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| 139 | [][]\T1/cmr/m/n/10 The presently identified worldwide candidate sites are located in three |
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| 140 | [] |
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| 142 | |
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| 143 | Underfull \hbox (badness 10000) detected at line 535 |
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| 144 | [] |
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| 145 | [] |
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| 146 | |
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| 147 | [9] [10] |
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| 148 | File: Fig4-PavelMajoranaNew.eps Graphic file (type eps) |
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| 149 | <Fig4-PavelMajoranaNew.eps> [11] |
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| 150 | File: Fig5-epi0-WC-Shiozawa.eps Graphic file (type eps) |
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| 151 | <Fig5-epi0-WC-Shiozawa.eps> [12] |
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| 152 | File: Fig6-limit_pdk_expo.eps Graphic file (type eps) |
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| 153 | <Fig6-limit_pdk_expo.eps> [13] [14] |
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| 154 | File: Fig7-Knu-WC-Shiozawa.eps Graphic file (type eps) |
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| 155 | |
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| 156 | <Fig7-Knu-WC-Shiozawa.eps> [15] [16] |
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| 157 | Overfull \hbox (12.0817pt too wide) in paragraph at lines 922--958 |
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| 158 | [][][] |
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| 159 | [] |
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| 160 | |
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| 161 | [17] [18] [19] |
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| 162 | Overfull \hbox (2.27449pt too wide) in paragraph at lines 1135--1135 |
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| 163 | [][]\T1/cmr/m/n/10 0.5 Mton year |
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| 164 | [] |
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| 165 | |
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| 166 | |
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| 167 | Overfull \hbox (2.27449pt too wide) in paragraph at lines 1140--1140 |
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| 168 | [][]\T1/cmr/m/n/10 0.4 Mton year |
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| 169 | [] |
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| 170 | |
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| 171 | |
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| 172 | Overfull \hbox (2.27449pt too wide) in paragraph at lines 1145--1145 |
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| 173 | [][]\T1/cmr/m/n/10 0.7 Mton year |
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| 174 | [] |
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| 175 | |
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| 176 | [20] |
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| 177 | File: Fig8-dsnspec1.eps Graphic file (type eps) |
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| 178 | <Fig8-dsnspec1.eps> |
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| 179 | File: Fig9-GdSKtemp-expect-bis.eps Graphic file (type eps) |
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| 180 | <Fig9-GdSKtemp-expect-bis.eps> [21] [22] [23] [24] |
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| 181 | File: Fig10-fig.octant.eps Graphic file (type eps) |
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| 182 | <Fig10-fig.octant.eps> |
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| 183 | Underfull \hbox (badness 1642) in paragraph at lines 1394--1414 |
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| 184 | [][]\T1/cmr/m/n/10 Historically, the atmospheric neutrino problem originated in the 80's as |
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| 185 | [] |
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| 186 | |
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| 187 | |
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| 188 | Underfull \hbox (badness 1189) in paragraph at lines 1394--1414 |
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| 189 | \T1/cmr/m/n/10 a discrepancy between the atmospheric neutrino flux measured with different |
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| 190 | [] |
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| 191 | |
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| 192 | [25] [26] |
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| 193 | File: Fig11-SPLBBMEMPHYS-fig16.eps Graphic file (type eps) |
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| 194 | <Fig11-SPLBBMEMPHYS-fig16.eps> |
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| 195 | File: Fig12-theta13.eps Graphic file (type eps) |
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| 196 | <Fig12-theta13.eps> [27] [28] |
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| 197 | Overfull \hbox (2.97217pt too wide) in paragraph at lines 1568--1580 |
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| 198 | [][][] |
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| 199 | [] |
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| 200 | |
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| 201 | |
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| 202 | Underfull \hbox (badness 1533) in paragraph at lines 1602--1605 |
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| 203 | [][]\T1/cmr/m/n/10 The pdf $\OML/cmm/m/it/10 f[]$ \T1/cmr/m/n/10 and $\OML/cmm/m/it/10 f[]$ \T1/cmr/m/n/10 are integrate |
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| 204 | d over the whole spectrum of possible |
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| 205 | [] |
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| 206 | |
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| 207 | [29] [30] |
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| 208 | File: Fig13-wimp_senal_fondo_10gev.eps Graphic file (type eps) |
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| 209 | <Fig13-wimp_senal_fondo_10gev.eps> |
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| 210 | File: Fig14-jasp_dislimit_10gev.eps Graphic file (type eps) |
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| 211 | <Fig14-jasp_dislimit_10gev.eps> [31] [32] |
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| 212 | File: Fig15-LENAMEMPHYS-reac-histogram.eps Graphic file (type eps) |
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| 213 | |
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| 214 | <Fig15-LENAMEMPHYS-reac-histogram.eps> [33] |
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| 215 | File: Fig16-memphys-sk-sol-lena.eps Graphic file (type eps) |
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| 216 | <Fig16-memphys-sk-sol-lena.eps> |
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| 217 | Underfull \hbox (badness 1097) in paragraph at lines 1876--1884 |
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| 218 | [][]\T1/cmr/m/n/10 Anyhow, the accuracy in the knowledge of the solar neutrino oscillation |
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| 219 | [] |
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| 220 | |
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| 221 | File: Fig17-MEMPHYSGdreactorthreshold.eps Graphic file (type eps) |
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| 222 | <Fig17-MEMPHYSGdreactorthreshold.eps> [34] [35] |
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| 223 | File: Fig18-CNGS_Fraction_th13Disc_NH.eps Graphic file (type eps) |
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| 224 | <Fig18-CNGS_Fraction_th13Disc_NH.eps> |
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| 225 | File: Fig19-CNGS850_1050_Fraction_excMass_NH.eps Graphic file (type eps) |
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| 226 | |
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| 227 | <Fig19-CNGS850_1050_Fraction_excMass_NH.eps> [36] [37] |
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| 228 | File: Fig20-SPLBBMEMPHYS-fig8.eps Graphic file (type eps) |
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| 229 | <Fig20-SPLBBMEMPHYS-fig8.eps> [38] |
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| 230 | File: Fig21-SPLBBMEMPHYS-fig9.eps Graphic file (type eps) |
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| 231 | <Fig21-SPLBBMEMPHYS-fig9.eps> |
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| 232 | File: Fig22-SPLBBMEMPHYS-fig11.eps Graphic file (type eps) |
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| 233 | |
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| 234 | <Fig22-SPLBBMEMPHYS-fig11.eps> [39] [40] |
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| 235 | File: Fig23-SPLBBMEMPHYS-fig14.eps Graphic file (type eps) |
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| 236 | <Fig23-SPLBBMEMPHYS-fig14.eps> [41] |
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| 237 | File: Fig24-SPLBBMEMPHYS-fig7.eps Graphic file (type eps) |
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| 238 | <Fig24-SPLBBMEMPHYS-fig7.eps> [42] |
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| 239 | File: Fig25-s2_l7400_sensi_t13.eps Graphic file (type eps) |
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| 240 | |
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| 241 | <Fig25-s2_l7400_sensi_t13.eps> [43] |
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| 242 | File: Fig26-CPsensi.eps Graphic file (type eps) |
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| 243 | <Fig26-CPsensi.eps> [44] |
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| 244 | Underfull \hbox (badness 10000) detected at line 2359 |
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| 245 | [] |
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| 246 | [] |
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| 247 | |
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| 248 | [45] [46] (campagne.bbl [47] [48] [49] [50] [51]) [52] (campagne.aux) ) |
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| 249 | Here is how much of TeX's memory you used: |
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| 250 | 2016 strings out of 95305 |
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| 252 | 76797 words of memory out of 1500000 |
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| 254 | 16206 words of font info for 45 fonts, out of 3000000 for 5000 |
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| 255 | 14 hyphenation exceptions out of 8191 |
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| 256 | 25i,15n,24p,672b,405s stack positions out of 5000i,500n,10000p,200000b,50000s |
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| 257 | |
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| 258 | Output written on campagne.dvi (52 pages, 239068 bytes). |
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