Scientific Report 2007-2009 Dissemination Astronomy & Astrophysics: 2007-2009 Publications 2009 [1] R.A. Capuzzo Dolcetta, Galactic Nuclei Activity Powered by Globular Cluster Mass Accretion, Astrophys. J., 1, (2009), pp. 1 [2] G.S. Bisnovatyi-Kogan et al., Spherically symmetric relativistic stellar clusters with anisotropy and cutoff energy in momentum distribution. I. The Newtonian regime., Astrophys. J., 703, (2009), pp. 628 [3] A.A. Abdo et al., Early Fermi Gamma-ray Space Telescope Observations of the Quasar 3C 454.3, Astrophys. J., 699, (2009), pp. 817 [4] A.A. Abdo et al., Bright Active Galactic Nuclei Source List from the First Three Months of the Fermi Large Area Telescope All-Sky Survey, Astrophys. J., 700, (2009), pp. 597 [5] J. H. Groh et al., On the Nature of the Prototype Luminous Blue Variable Ag Carinae. I. Fundamental Parameters During Visual Minimum Phases and Changes in the Bolometric Luminosity During the S-Dor Cycle, Astrophys. J., 698, (2009), pp. 1698 [6] V.A. Acciari et al., Multiwavelength Observations of a TeV-Flare from W Comae, Astrophys. J., 707, (2009), pp. 612 [7] G. Luzzi et al., Redshift dependence of the Cosmic Microwave Background temperature from Sunyaev- Zel’dovich measurements, Astrophys. J., 705, (2009), pp. 1122 [8] M. Veneziani et al., Subdegree Sunyaev-Zel’dovich Signal from Multifrequency BOOMERANG Observations, Astrophys. J. Let., 702, (2009), pp. L61 [9] G. Gubitosi et al., A constraint on Planck-scale modifications to electrodynamics with CMB polarization data, J. Cosmol. Astropart. Phys., 08, (2009), pp. 21 [10] A. Melchiorri et al., Sterile Neutrinos in Light of Recent Cosmological and Oscillation Data: a Multi-Flavor Scheme Approach, J. Cosmol. Astropart. Phys., 0901, (2009), pp. 36 [11] R. Capuzzo Dolcetta et al., Dynamical friction in cuspy galaxies, Mon. Not. R. Astron. Soc., 1, (2009), pp. 1 [12] F. Antonini et al., A Counterpart to the Radial Orbit Instability in Triaxial Stellar Systems, Mon. Not. R. Astron. Soc., 399, (2009), pp. 671 [13] M. Merafina, Gravothermal instability in globular clusters., Mon. Not. R. Astron. Soc., XX, (2009), pp. x [14] I. Flores-Cacho et al., The Sunyaev-Zeldovich effect in superclusters of galaxies using gasdynamical simulations: the case of Corona Borealis, Mon. Not. R. Astron. Soc., 400, (2009), pp. 1868 [15] P. Serra et al., Lensed Cosmic Microwave Background Constraints on Post-General Relativity Parameters, Phys. Rev. D: Part. Fields, 79, (2009), pp. 101301 [16] F. De Bernardis et al., Delayed recombination and standard rulers, Phys. Rev. D: Part. Fields, 79, (2009), pp. 043503 [17] M. Martinelli et al., Cosmological constraints on the Hu-Sawicki modified gravity scenario, Phys. Rev. D: Part. Fields, 79, (2009), pp. 123516 [18] S.F. Daniel et al., A Multi-Parameter Investigation of Gravitational Slip, Phys. Rev. D: Part. Fields, 80, (2009), pp. 023532 [19] S. Galli et al., CMB constraints on Dark Matter models with large annihilation cross-section, Phys. Rev. D: Part. Fields, 80, (2009), pp. 023505 [20] S. Galli et al., From Cavendish to PLANCK: Constraining Newton’s Gravitational Constant with CMB Temperature and Polarization Anisotropy, Phys. Rev. D: Part. Fields, 80, (2009), pp. 023508 [21] F. De Bernardis et al., Determining the Neutrino Mass Hierarchy with Cosmology, Phys. Rev. D: Part. Fields, 80, (2009), pp. 123509 [22] E. Calabrese et al., CMB Lensing Constraints on Dark Energy and Modified Gravity Scenarios, Phys. Rev. D: Part. Fields, 80, (2009), pp. 103516 [23] P. Serra et al., No Evidence for Dark Energy Dynamics from a Global Analysis of Cosmological Data, Phys. Rev. D: Part. Fields, 80, (2009), pp. 121302 [24] E. Menegoni et al., New Constraints on variations of the fine structure constant from CMB anisotropies., Phys. Rev. D: Part. Fields, 80, (2009), pp. 087302 [25] E. Calabrese et al., Cosmological constraints on the matter equation of state, Phys. Rev. D: Part. Fields, 80, (2009), pp. 063539 [26] L. Pagano et al., CMB Polarization Systematics, Cosmological Birefringence and the Gravitational Waves Background., Phys. Rev. D: Part. Fields, d80, (2009), pp. 043522 [27] F. Lamareille et al., Physical properties of galaxies and their evolution in the VIMOS VLT Deep Survey. I. The evolution of the mass-metallicity relation up to z 0.9, Astron. Astrophys., 495, (2009), pp. 53 [28] E. Massaro et al., Roma-BZCAT: a multifrequency catalogue of blazars, Astron. Astrophys., 495, (2009), pp. 691 [29] R.A. Capuzzo Dolcetta et al., Globular cluster system erosion in elliptical galaxies., Astron. Astrophys., 507, (2009), pp. 183 [30] R. Campana et al., The multicomponent model of the Crab pulsar at energies above 25 GeV (Research Note), Astron. Astrophys., 499, (2009), pp. 847 [31] K. Boutsia et al., Spectroscopic follow-up of variabilityselected active galactic nuclei in the Chandra Deep Field South, Astron. Astrophys., 497, (2009), pp. 81 [32] S. Salimbeni et al., A comprehensive study of largescale structures in the GOODS-SOUTH field up to z 2.5, Astron. Astrophys., 501, (2009), pp. 865 [33] P. de Bernardis et al., The Cosmic Microwave Background in the Light of Planck, Nucl. Phys. B, 188, (2009), pp. 9 [34] P. de Bernardis et al., B-Pol: Detecting Primordial Gravitational Waves Generated During Inflation, Exp. Astron., 23, (2009), pp. 5 [35] A. Maselli et al., Are symmetric radio spectra of some GPS/HFP sources related to a statistical acceleration mechanism?, Astron. Nachr., 330, (2009), pp. 295 <strong>Sapienza</strong> Università di Roma 247 Dipartimento di Fisica
Scientific Report 2007-2009 Dissemination [36] C. Rossi et al., Oxygen and Carbon rich stars in the Cepheus region: classification of selected objects from the KP2001 catalogue, Astrophysics, 52, (2009), pp. 523 [37] R. Nesci et al., Spectra in the Digitized First Byurakan Survey, Baltic Astronomy, 18, (2009), pp. 383 [38] M. Laurenza et al., Search for periodicities in the IMP-8 Charged Particle Measurement Experiment proton fluxes in the energy bands 0.50-0.96 MeV and 190-440 MeV, J. Geophys. Res., 114, (2009), pp. 1103-1 [39] P. de Bernardis et al., Dal Big bang ai Buchi Neri, Le Scienze, 494, (2009), pp. 72 [40] R. Briguglio et al., The Small IRAIT telescope. Photometric time-series during the polar night, Mem. S. A. It., 80, (2009), pp. 147 [41] A. Melchiorri et al., Determination of Cosmological Parameters from Cosmic Microwave Background Anisotropies, Lect. Notes Phys., 665, (2009), pp. 320 Publications 2008 [1] F. De Bernardis et al., The cosmic neutrino background and the age of the Universe, J. Cosmol. Astropart. Phys., 03, (2008), pp. 20 [2] F. De Bernardis et al., Anisotropies in the Cosmic Neutrino Background after WMAP 5-year Data, J. Cosmol. Astropart. Phys., 06, (2008), pp. 13 [3] K. Kohri et al., Black hole formation and slow-roll inflation, J. Cosmol. Astropart. Phys., 0804, (2008), pp. 38 [4] L. Pagano et al., Red Density Perturbations and Inflationary Gravitational Waves, J. Cosmol. Astropart. Phys., 0804, (2008), pp. 9 [5] J. Hamann et al., Nonlinear corrections to the cosmological matter power spectrum and scale-dependent galaxy bias: implications for parameter estimation, J. Cosmol. Astropart. Phys., 07, (2008), pp. 17 [6] R.A. Capuzzo Dolcetta et al., Merging of globular clusters within inner galactic regions. II. The nuclear star cluster formation., Astrophys. J., 681, (2008), pp. 1136 [7] R.A. Capuzzo Dolcetta, Galactic Nuclei Activity Powered by Globular Cluster Mass Accretion, Astrophys. J., 1, (2008), pp. 1 [8] F. Gastaldello et al., XMM-Newton Observations of the Cluster of galaxies Zw 1305.4+2941 in the Field SA 57, Astrophys. J., 673, (2008), pp. 176 [9] R. Campana et al., A Minimal Spanning Tree algorithm for source detection in gamma-ray images, Mon. Not. R. Astron. Soc., 383, (2008), pp. 1166 [10] R.A. Capuzzo Dolcetta et al., Self-consistent simulations of nuclear cluster formation through globular cluster orbital decay and merging., Mon. Not. R. Astron. Soc., 388, (2008), pp. 69 [11] R. Campana et al., X-ray observations of the Large Magellanic Cloud pulsar PSR B0540-69 and its pulsar wind nebula, Mon. Not. R. Astron. Soc., 389, (2008), pp. 691 [12] S. Galli et al., Delayed Recombination and Cosmic Parameters, Phys. Rev. D: Part. Fields, 78, (2008), pp. 063532 [13] A. Cooray et al., The trispectrum of 21-cm background anisotropies as a probe of primordial non-Gaussianity, Phys. Rev. D: Part. Fields, 77, (2008), pp. 103506 [14] E. Calabrese et al., Cosmic Microwave Weak lensing data as a test for the dark universe, Phys. Rev. D: Part. Fields, 77, (2008), pp. 123531 [15] P.S. Corasaniti et al., Testing Cosmology with Cosmic Sound Waves, Phys. Rev. D: Part. Fields, 77, (2008), pp. 103507 [16] R. Camerini et al., Is Cosmology Compatible with Blue Gravity Waves ?, Phys. Rev. D: Part. Fields, 77, (2008), pp. 101301 [17] S.F. Daniel et al., Large Scale Structure as a Probe of Gravitational Slip, Phys. Rev. D: Part. Fields, 77, (2008), pp. 103513 [18] T.D. Kitching et al., Finding Evidence for Massive Neutrinos using 3D Weak Lensing, Phys. Rev. D: Part. Fields, 77, (2008), pp. 103008 [19] G.L. Fogli et al., Observables sensitive to absolute neutrino masses. II, Phys. Rev. D: Part. Fields, 78, (2008), pp. 033010 <strong>Sapienza</strong> Università di Roma 248 Dipartimento di Fisica
- Page 2 and 3:
Sapienza Università di Roma Dipart
- Page 4 and 5:
Scientific Report 2007-2009 Introdu
- Page 6 and 7:
Scientific Report 2007-2009 Introdu
- Page 8 and 9:
Scientific Report 2007-2009 Introdu
- Page 10 and 11:
Scientific Report 2007-2009 Organiz
- Page 12 and 13:
Scientific Report 2007-2009 Organiz
- Page 14 and 15:
Scientific Report 2007-2009 Organiz
- Page 16 and 17:
Scientific Report 2007-2009 Organiz
- Page 18 and 19:
Scientific Report 2007-2009 Organiz
- Page 20 and 21:
Scientific Report 2007-2009 Theoret
- Page 22 and 23:
Scientific Report 2007-2009 Theoret
- Page 24 and 25:
Scientific Report 2007-2009 Theoret
- Page 26 and 27:
Scientific Report 2007-2009 Theoret
- Page 28 and 29:
Scientific Report 2007-2009 Theoret
- Page 30 and 31:
Scientific Report 2007-2009 Theoret
- Page 32 and 33:
Scientific Report 2007-2009 Theoret
- Page 34 and 35:
Scientific Report 2007-2009 Theoret
- Page 36 and 37:
Scientific Report 2007-2009 Theoret
- Page 38 and 39:
Scientific Report 2007-2009 Theoret
- Page 40 and 41:
Scientific Report 2007-2009 Theoret
- Page 42 and 43:
Scientific Report 2007-2009 Theoret
- Page 44 and 45:
Scientific Report 2007-2009 Theoret
- Page 46 and 47:
Scientific Report 2007-2009 Theoret
- Page 48 and 49:
Scientific Report 2007-2009 Condens
- Page 50 and 51:
Scientific Report 2007-2009 Condens
- Page 52 and 53:
Scientific Report 2007-2009 Condens
- Page 54 and 55:
Scientific Report 2007-2009 Condens
- Page 56 and 57:
Scientific Report 2007-2009 Condens
- Page 58 and 59:
Scientific Report 2007-2009 Condens
- Page 60 and 61:
Scientific Report 2007-2009 Condens
- Page 62 and 63:
Scientific Report 2007-2009 Condens
- Page 64 and 65:
Scientific Report 2007-2009 Condens
- Page 66 and 67:
Scientific Report 2007-2009 Condens
- Page 68 and 69:
Scientific Report 2007-2009 Condens
- Page 70 and 71:
Scientific Report 2007-2009 Condens
- Page 72 and 73:
Scientific Report 2007-2009 Condens
- Page 74 and 75:
Scientific Report 2007-2009 Condens
- Page 76 and 77:
Scientific Report 2007-2009 Condens
- Page 78 and 79:
Scientific Report 2007-2009 Condens
- Page 80 and 81:
Scientific Report 2007-2009 Condens
- Page 82 and 83:
Scientific Report 2007-2009 Condens
- Page 84 and 85:
Scientific Report 2007-2009 Condens
- Page 86 and 87:
Scientific Report 2007-2009 Condens
- Page 88 and 89:
Scientific Report 2007-2009 Condens
- Page 90 and 91:
Scientific Report 2007-2009 Condens
- Page 92 and 93:
Scientific Report 2007-2009 Condens
- Page 94 and 95:
Scientific Report 2007-2009 Condens
- Page 96 and 97:
Scientific Report 2007-2009 Condens
- Page 98 and 99:
Scientific Report 2007-2009 Condens
- Page 100 and 101:
Scientific Report 2007-2009 Condens
- Page 102 and 103:
Scientific Report 2007-2009 Particl
- Page 104 and 105:
Scientific Report 2007-2009 Particl
- Page 106 and 107:
Scientific Report 2007-2009 Particl
- Page 108 and 109:
Scientific Report 2007-2009 Particl
- Page 110 and 111:
Scientific Report 2007-2009 Particl
- Page 112 and 113:
Scientific Report 2007-2009 Particl
- Page 114 and 115:
Scientific Report 2007-2009 Particl
- Page 116 and 117:
Scientific Report 2007-2009 Particl
- Page 118 and 119:
Scientific Report 2007-2009 Particl
- Page 120 and 121:
Scientific Report 2007-2009 Particl
- Page 122 and 123:
Scientific Report 2007-2009 Particl
- Page 124 and 125:
Scientific Report 2007-2009 Particl
- Page 126 and 127:
Scientific Report 2007-2009 Particl
- Page 128 and 129:
Scientific Report 2007-2009 Particl
- Page 130 and 131:
2 2 2 Scientific Report 2007-2009 P
- Page 132 and 133:
Scientific Report 2007-2009 Particl
- Page 134 and 135:
Scientific Report 2007-2009 Particl
- Page 136 and 137:
Scientific Report 2007-2009 Particl
- Page 138 and 139:
Scientific Report 2007-2009 Particl
- Page 140 and 141:
Scientific Report 2007-2009 Particl
- Page 142 and 143:
Scientific Report 2007-2009 Particl
- Page 144 and 145:
Scientific Report 2007-2009 Astrono
- Page 146 and 147:
Scientific Report 2007-2009 Astrono
- Page 148 and 149:
Scientific Report 2007-2009 Astrono
- Page 150 and 151:
Scientific Report 2007-2009 Astrono
- Page 152 and 153:
Scientific Report 2007-2009 Astrono
- Page 154 and 155:
Scientific Report 2007-2009 Astrono
- Page 156 and 157:
Scientific Report 2007-2009 Astrono
- Page 158 and 159:
Scientific Report 2007-2009 Astrono
- Page 160 and 161:
Scientific Report 2007-2009 Astrono
- Page 162 and 163:
Scientific Report 2007-2009 Astrono
- Page 164 and 165:
Scientific Report 2007-2009 Astrono
- Page 166 and 167:
Scientific Report 2007-2009 Geophys
- Page 168 and 169:
Scientific Report 2007-2009 Geophys
- Page 170 and 171:
Scientific Report 2007-2009 Geophys
- Page 172 and 173:
Scientific Report 2007-2009 History
- Page 174 and 175:
Scientific Report 2007-2009 History
- Page 176 and 177:
Scientific Report 2007-2009 Laborat
- Page 178 and 179:
Scientific Report 2007-2009 Laborat
- Page 180 and 181:
Scientific Report 2007-2009 Laborat
- Page 182 and 183:
Scientific Report 2007-2009 Laborat
- Page 184 and 185:
Scientific Report 2007-2009 Laborat
- Page 186 and 187:
Scientific Report 2007-2009 Laborat
- Page 188 and 189:
Scientific Report 2007-2009 Laborat
- Page 190 and 191:
Scientific Report 2007-2009 Laborat
- Page 192 and 193:
Scientific Report 2007-2009 Laborat
- Page 194 and 195:
Scientific Report 2007-2009 Laborat
- Page 196 and 197:
Scientific Report 2007-2009 Laborat
- Page 198 and 199: Scientific Report 2007-2009 Laborat
- Page 200 and 201: Scientific Report 2007-2009 Laborat
- Page 202 and 203: Scientific Report 2007-2009 Grants
- Page 204 and 205: Scientific Report 2007-2009 Grants
- Page 206 and 207: Scientific Report 2007-2009 Grants
- Page 208 and 209: Scientific Report 2007-2009 Grants
- Page 210 and 211: Scientific Report 2007-2009 Dissemi
- Page 212 and 213: Scientific Report 2007-2009 Dissemi
- Page 214 and 215: Scientific Report 2007-2009 Dissemi
- Page 216 and 217: Scientific Report 2007-2009 Dissemi
- Page 218 and 219: Scientific Report 2007-2009 Dissemi
- Page 220 and 221: Scientific Report 2007-2009 Dissemi
- Page 222 and 223: Scientific Report 2007-2009 Dissemi
- Page 224 and 225: Scientific Report 2007-2009 Dissemi
- Page 226 and 227: Scientific Report 2007-2009 Dissemi
- Page 228 and 229: Scientific Report 2007-2009 Dissemi
- Page 230 and 231: Scientific Report 2007-2009 Dissemi
- Page 232 and 233: Scientific Report 2007-2009 Dissemi
- Page 234 and 235: Scientific Report 2007-2009 Dissemi
- Page 236 and 237: Scientific Report 2007-2009 Dissemi
- Page 238 and 239: Scientific Report 2007-2009 Dissemi
- Page 240 and 241: Scientific Report 2007-2009 Dissemi
- Page 242 and 243: Scientific Report 2007-2009 Dissemi
- Page 244 and 245: Scientific Report 2007-2009 Dissemi
- Page 246 and 247: Scientific Report 2007-2009 Dissemi
- Page 250 and 251: Scientific Report 2007-2009 Dissemi
- Page 252 and 253: Scientific Report 2007-2009 Dissemi
- Page 254 and 255: Scientific Report 2007-2009 Dissemi
- Page 256 and 257: Scientific Report 2007-2009 Dissemi
- Page 258 and 259: Scientific Report 2007-2009 Dissemi
- Page 260: Scientific Report 2007-2009 Dissemi