Scientific Report 2007-2009 Dissemination [20] P. Serra et al., Impact of Point Source Clustering on Cosmological Parameters with CMB Anisotropies, Phys. Rev. D: Part. Fields, 78, (2008), pp. 043004 [21] F. De Bernardis et al., An improved limit on the neutrino mass with CMB and redshift-dependent halo biasmass relations from SDSS, DEEP2, and Lyman-Break Galaxies, Phys. Rev. D: Part. Fields, 78, (2008), pp. 083535 [22] W.H. Kinney et al., Latest inflation model constraints from cosmic microwave background measurements, Phys. Rev. D: Part. Fields, 78, (2008), pp. 087302 [23] S. Salimbeni et al., The red and blue galaxy population in the GOODS field: evidence for an excess of red dwarfs, Astron. Astrophys., 477, (2008), pp. 763 [24] D. Trevese et al., Optical spectroscopy of active galactic nuclei in SA57, Astron. Astrophys., 477, (2008), pp. 473 [25] L. Fu et al., Very weak lensing in the CFHTLS wide: cosmology from cosmic shear in the linear regime, Astron. Astrophys., 479, (2008), pp. 9 [26] A. Maselli et al., The 26 year-long X-ray light curve and the X-ray spectrum of the BL Lacertae object 1E 1207.9+3945 in its brightest state, Astron. Astrophys., 479, (2008), pp. 35 [27] C. M. Raiteri et al., Radio-to-UV monitoring of AO 0235+164 by the WEBT and Swift during the 2006-2007 outburst, Astron. Astrophys., 480, (2008), pp. 339 [28] R. Gonzalez-Riestra et al., AG Draconis observed with XMM-Newton, Astron. Astrophys., 481, (2008), pp. 725 [29] F. Massaro et al., Swift observations of IBL and LBL objects, Astron. Astrophys., 489, (2008), pp. 1047 [30] C.M. Raiteri et al., The high activity of 3C 454.3 in autumn 2007. Monitoring by the WEBT during the AGILE detection, Astron. Astrophys., 485, (2008), pp. 17 [31] C.M. Raiteri et al., A new activity phase of the blazar 3C 454.3. Multifrequency observations by the WEBT and XMM-Newton in 2007-2008, Astron. Astrophys., 491, (2008), pp. 755 [32] G. Muratorio et al., Analysis of the variability of the luminous emission line star MWC 314, Astron. Astrophys., 487, (2008), pp. 673 [33] M. Radovich et al., A weak-lensing analysis of the Abell 2163 cluster, Astron. Astrophys., 487, (2008), pp. 55 [34] D. Trevese et al., Variability-selected active galactic nuclei from supernova search in the Chandra deep field south, Astron. Astrophys., 488, (2008), pp. 73 [35] F. De Bernardis et al., New constraints on the reheating temperature of the universe after WMAP-5, Astropart. Phys., 30, (2008), pp. 192 Publications 2007 [1] B. Lanzoni et al., The Surface Density Profile of NGC 6388: A Good Candidate for Harboring an Intermediate- Mass Black Hole, Astrophys. J., 668, (2007), pp.139 [2] A. Vicari et al., Consequences of Triaxiality for Gravitational Wave Recoil of Black Holes, Astrophys. J., 662, (2007), pp.797 [3] G. De Troia et al., Searching for non Gaussian signals in the BOOMERanG 2003 CMB maps, Astrophys. J., 670, (2007), pp.73 [4] B. R. Johnson et al., MAXIPOL: Cosmic Microwave Background Polarimetry Using a Rotating Half-Wave Plate, Astrophys. J., 665, (2007), pp.42 [5] R.A. Capuzzo Dolcetta et al., Self consistent models of triaxial cuspy galaxies with dark matter haloes, Astrophys. J., 666, (2007), pp.165 [6] M. Castellano et al., A Photometrically Detected Forming Cluster of Galaxies at Redshift 1.6 in the GOODS Field, Astrophys. J., 671, (2007), pp.1497 [7] M. Montuori et al., Tidal Tails around Globular Clusters: Are They a Good Tracer of Cluster Orbits?, Astrophys. J., 659, (2007), pp.1212 [8] G. Mangano et al., Present bounds on the relativistic energy density in the Universe from cosmological observables., J. Cosmol. Astropart. Phys., 0703, (2007), pp.6 [9] P. Serra et al., Bayesian Evidence for a Cosmological Constant using new High-Redshift Supernovae Data, Mon. Not. R. Astron. Soc., 379, (2007), pp.169 [10] P. Miocchi, The presence of intermediate-mass black holes in globular clusters and their connection with extreme horizontal branch stars, Mon. Not. R. Astron. Soc., 381, (2007), pp.103 [11] R.A. Capuzzo Dolcetta et al., Dynamical friction in cuspy galaxies, Mon. Not. R. Astron. Soc., 1, (2007), pp.1 [12] R. Nesci et al., Optical Variability of the Strong-lined and X-Ray-bright Source 1WGA J0447.9-0322, Astron. J., 133, (2007), pp.965 [13] R. Bean et al., Cosmological constraints in the presence of ionizing and resonance radiation at recombination., Phys. Rev. D: Part. Fields, 75, (2007), pp.063505 [14] P.S. Corasaniti et al., Exploring the Dark Energy Redshift Desert with the Sandage-Loeb Test., Phys. Rev. D: Part. Fields, 75, (2007), pp.062001 [15] G.L. Fogli et al., Observables sensitive to absolute neutrino masses: A Reappraisal after WMAP-3y and first MINOS results, Phys. Rev. D: Part. Fields, 75, (2007), pp.053001 [16] A. Melchiorri et al., Improved cosmological bound on the thermal axion mass, Phys. Rev. D: Part. Fields, 76, (2007), pp.041303 [17] A. Melchiorri et al., When did cosmic acceleration start?, Phys. Rev. D: Part. Fields, 76, (2007), pp.041301 [18] R. Caldwell et al., Constraints on a New Post-General Relativity Cosmological Parameter, Phys. Rev. D: Part. Fields, 76, (2007), pp.023507 [19] J. Hamann et al., New Constraints on Oscillations in the Primordial Spectrum of Inflationary Perturbations, Phys. Rev. D: Part. Fields, 76, (2007), pp.023503 [20] P. Giommi et al., ROXA J081009.9+384757.0: a 10 4 7 erg s − 1 blazar with hard X-ray synchrotron peak or a <strong>Sapienza</strong> Università di Roma 249 Dipartimento di Fisica
Scientific Report 2007-2009 Dissemination new type of radio loud AGN?, Astron. Astrophys., 468, (2007), pp.97 [21] M. Perri et al., Swift XRT and UVOT deep observations of the high-energy peaked BL Lacertae object PKS 0548- 322 close to its brightest state, Astron. Astrophys., 462, (2007), pp.889 [22] D. Trevese et al., A new (2+1)D cluster finding algorithm based on photometric redshifts: large scale structure in the Chandra deep field south, Astron. Astrophys., 463, (2007), pp.853 [23] F. Giovannelli et al., HeI doubled emission lines from A0535+26 HDE 245770. A possible interpretation, Astron. Astrophys., 275, (2007), pp.651 [24] P. Giommi et al., Swift detection of all previously undetected blazars in a micro-wave flux-limited sample of WMAP foreground sources, Astron. Astrophys., 468, (2007), pp.571 [25] R.F. Viotti et al., The 2006 hot phase of Romano’s star (GR 290) in M 33, Astron. Astrophys., 464, (2007), pp.53 [26] A. Tramacere et al., SWIFT observations of TeV BL Lacertae objects, Astron. Astrophys., 467, (2007), pp.501 [27] D. Trevese et al., Line and continuum variability of two intermediate-redshift, high-luminosity quasars, Astron. Astrophys., 470, (2007), pp.491 [28] L. Vetere et al., The complete catalogue of GRBs observed by the wide field cameras on board BeppoSAX, Astron. Astrophys., 473, (2007), pp.347 [29] J.F. Macias-Perez et al., Archeops In-flight Performance, Data Processing and Map Making, Astron. Astrophys., 467, (2007), pp.1313 [30] D. Trevese et al., An X-ray survey in SA 57 with XMM- Newton, Astron. Astrophys., 469, (2007), pp.1211 [31] A.M. Mickaelian et al., The digitized first Byurakan survey - DFBS, Astron. Astrophys., 464, (2007), pp.1177 [32] S. Colafrancesco et al., Direct probes of Dark Matter in the cluster 1ES0657-556 through microwave observations, Astron. Astrophys., 467, (2007), pp.1 [33] A. Melchiorri et al., New bounds on millicharged particles from cosmology, Phys. Lett. B, 650, (2007), pp.416 [34] A. De La Macorra et al., The impact of neutrino masses on the determination of dark energy properties, Astropart. Phys., 27, (2007), pp.406 [35] F. Nati et al., The OLIMPO experiment, New Astron. Rev., 51, (2007), pp.385 [36] L. Lamagna et al., S-Z constraints on the dependence of the CMB temperature on redshift, New Astron. Rev., 51, (2007), pp.381 [37] E.S. Battistelli et al., SZ effect from Corona Borealis supercluster, New Astron. Rev., 51, (2007), pp.374 [38] M. De Petris et al., MITO: a ”creative approach” for Sunyaev-Zel’dovich effect observations from ground, New Astron. Rev., 51, (2007), pp.368 [39] G. Polenta et al., The BRAIN CMB polarization experiment, New Astron. Rev., 51, (2007), pp.256 [40] G. De Troia et al., Searching for non Gaussian signals in the BOOMERanG 2003 CMB map: preliminary results, New Astron. Rev., 51, (2007), pp.250 [41] F. Piacentini et al., CMB polarization with Boomerang 2003, New Astron. Rev., 51, (2007), pp.244 [42] S. Masi et al., The millimeter sky as seen with BOOMERanG, New Astron. Rev., 51, (2007), pp.236 [43] A. Melchiorri et al., New constraints on neutrino masses from cosmology., New Astron. Rev., 50, (2007), pp.1020 [44] P. de Bernardis et al., From BOOMERanG to B-Pol, Nuovo Cimento Soc. Ital. Fis., B, 122, (2007), pp.1327 [45] S. De Gregori et al., New data for the X, y, z, T-CMB reference frame, Nuovo Cimento Soc. Ital. Fis., B, 122, (2007), pp.1239 [46] M. Castellano et al., Large-scale structures at high redshift in the GOODS field, Nuovo Cimento Soc. Ital. Fis., B, 122, (2007), pp.1235 [47] S. Salimbeni et al., The red and blue galaxy luminosity function in the GOODS field: Evidence for an excess of red-dwarf galaxies, Nuovo Cimento Soc. Ital. Fis., B, 122, (2007), pp.1183 [48] P. de Bernardis, Un nobel per il fondo cosmico a microonde, Il Nuovo Saggiatore, 22, (2007), pp.87 <strong>Sapienza</strong> Università di Roma 250 Dipartimento di Fisica
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