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The mass of the $\tau$-lepton has been measured in the decay modes $\tau \to 3\pi \nu_\tau$ and $\tau \to 3\pi \pi^0\nu_\tau$ using a pseudomass technique. The preliminary result is $1776.71\pm 0.25 {(stat)} \pm 0.62 {(syst)}$ MeV. The…

High Energy Physics - Experiment · Physics 2012-08-27 Belle Collaboration

Objects gravitationally captured by the Earth-Moon system are commonly called temporarily captured orbiters (TCOs), natural Earth satellites, or minimoons. TCOs are a crucially important subpopulation of near-Earth objects (NEOs) to…

Earth and Planetary Astrophysics · Physics 2019-12-05 P. M. Shober , T. Jansen-Sturgeon , E. K. Sansom , H. A. R. Devillepoix , P. A. Bland , M. Cupák , M. C. Towner , R. M. Howie , B. A. D. Hartig

We report high resolution multi-station observations of meteors by the Canadian Automated Meteor Observatory (CAMO) recorded from June 2009 to August 2010. Our survey has a limiting detection magnitude of +5 mag in R-band, equivalent to a…

Earth and Planetary Astrophysics · Physics 2015-05-30 R. Musci , R. J. Weryk , P. Brown , M. D. Campbell-Brown , P. A. Wiegert

The French FRIPON (Fireball Recovery and Interplanetary Observation Network) programme relies on a video cameras network associated to radio sensors running in a radar multistatic configuration to observe fireballs and to determine…

A limit on the mass of the tau neutrino is derived from 4.5 million tau pairs produced in an integrated luminosity of 5.0 fb^{-1} of electron-positron annihilation to tau pairs at center of mass energies near 10.6 GeV. The measurement…

High Energy Physics - Experiment · Physics 2010-04-08 R. Ammar , CLEO Collaboration et al

Aims. Lightning mapper sensors on board weather satellites can be successfully used to observe fireballs. These sensors use a very narrow spectral band at 777nm, which is only a small fraction of the total fireball radiation. In this…

Earth and Planetary Astrophysics · Physics 2022-12-14 V. Vojáček , J. Borovička , P. Spurný

We have analysed the orbits and ablation characteristics in the atmosphere of 59 earth-impacting fireballs, produced by meteoroids one meter in diameter or larger, described here as meter-scale. Using heights at peak luminosity as a proxy…

Earth and Planetary Astrophysics · Physics 2015-12-23 P. Brown , P. Wiegert , D. Clark , E. Tagliaferri

We present the result from a precision measurement of the mass of the $\tau$ lepton, $M_\tau$, based on $423 fb^{-1}$ of data recorded at the $\Upsilon(4S)$ resonance with the BaBar detector. Using a pseudomass endpoint method, we determine…

High Energy Physics - Experiment · Physics 2010-04-12 The BaBar Collaboration , B. Aubert

Meteoroids are pieces of asteroids and comets. They serve as unique probes to the physical and chemical properties of their parent bodies. We can derive some of these properties when meteoroids collide with the atmosphere of Earth and…

Earth and Planetary Astrophysics · Physics 2023-03-08 Tomáš Henych , Jiří Borovička , Pavel Spurný

A limit on the tau neutrino mass is obtained using all the $Z^{0} \to \tau^{+} \tau^{-}$ data collected at LEP by the DELPHI detector between 1992 and 1995. In this analysis events in which one of the taus decays into one charged particle,…

High Energy Physics - Experiment · Physics 2019-08-16 Davide Perego

The reconstruction of tau-pair production, $e^{+}e^{-} \to \tau^{+}\tau^{-}$, from the subsequent 3-prong ($\tau^{+} \rightarrow \pi^{+} \pi^{-} \pi^{+} \bar{\nu}_{\tau}$) and 1-prong ($\tau^{-} \to \ell^{-} \bar{\nu}_{\ell} \nu_{\tau}$,…

High Energy Physics - Experiment · Physics 2021-03-10 Belle II Collaboration , F. Abudinén , I. Adachi , R. Adak , K. Adamczyk , P. Ahlburg , J. K. Ahn , H. Aihara , N. Akopov , A. Aloisio , F. Ameli , L. Andricek , N. Anh Ky , D. M. Asner , H. Atmacan , V. Aulchenko , T. Aushev , V. Aushev , T. Aziz , V. Babu , S. Bacher , S. Baehr , S. Bahinipati , A. M. Bakich , P. Bambade , Sw. Banerjee , S. Bansal , M. Barrett , G. Batignani , J. Baudot , A. Beaulieu , J. Becker , P. K. Behera , M. Bender , J. V. Bennett , E. Bernieri , F. U. Bernlochner , M. Bertemes , M. Bessner , S. Bettarini , V. Bhardwaj , B. Bhuyan , F. Bianchi , T. Bilka , S. Bilokin , D. Biswas , A. Bobrov , A. Bondar , G. Bonvicini , A. Bozek , M. Bračko , P. Branchini , N. Braun , R. A. Briere , T. E. Browder , D. N. Brown , A. Budano , L. Burmistrov , S. Bussino , M. Campajola , L. Cao , G. Caria , G. Casarosa , C. Cecchi , D. Červenkov , M. -C. Chang , P. Chang , R. Cheaib , V. Chekelian , Y. Q. Chen , Y. -T. Chen , B. G. Cheon , K. Chilikin , K. Chirapatpimol , H. -E. Cho , K. Cho , S. -J. Cho , S. -K. Choi , S. Choudhury , D. Cinabro , L. Corona , L. M. Cremaldi , D. Cuesta , S. Cunliffe , T. Czank , N. Dash , F. Dattola , E. De La Cruz-Burelo , G. De Nardo , M. De Nuccio , G. De Pietro , R. de Sangro , B. Deschamps , M. Destefanis , S. Dey , A. De Yta-Hernandez , A. Di Canto , F. Di Capua , S. Di Carlo , J. Dingfelder , Z. Doležal , I. Domínguez Jiménez , T. V. Dong , K. Dort , D. Dossett , S. Dubey , S. Duell , G. Dujany , S. Eidelman , M. Eliachevitch , D. Epifanov , J. E. Fast , T. Ferber , D. Ferlewicz , G. Finocchiaro , S. Fiore , P. Fischer , A. Fodor , F. Forti , A. Frey , M. Friedl , B. G. Fulsom , M. Gabriel , N. Gabyshev , E. Ganiev , M. Garcia-Hernandez , R. Garg , A. Garmash , V. Gaur , A. Gaz , U. Gebauer , M. Gelb , A. Gellrich , J. Gemmler , T. Geßler , D. Getzkow , R. Giordano , A. Giri , A. Glazov , B. Gobbo , R. Godang , P. Goldenzweig , B. Golob , P. Gomis , P. Grace , W. Gradl , E. Graziani , D. Greenwald , Y. Guan , C. Hadjivasiliou , S. Halder , K. Hara , T. Hara , O. Hartbrich , T. Hauth , K. Hayasaka , H. Hayashii , C. Hearty , M. Heck , M. T. Hedges , I. Heredia de la Cruz , M. Hernández Villanueva , A. Hershenhorn , T. Higuchi , E. C. Hill , H. Hirata , M. Hoek , M. Hohmann , S. Hollitt , T. Hotta , C. -L. Hsu , Y. Hu , K. Huang , T. Iijima , K. Inami , G. Inguglia , J. Irakkathil Jabbar , A. Ishikawa , R. Itoh , M. Iwasaki , Y. Iwasaki , S. Iwata , P. Jackson , W. W. Jacobs , I. Jaegle , D. E. Jaffe , E. -J. Jang , M. Jeandron , H. B. Jeon , S. Jia , Y. Jin , C. Joo , K. K. Joo , I. Kadenko , J. Kahn , H. Kakuno , A. B. Kaliyar , J. Kandra , K. H. Kang , P. Kapusta , R. Karl , G. Karyan , Y. Kato , H. Kawai , T. Kawasaki , T. Keck , C. Ketter , H. Kichimi , C. Kiesling , B. H. Kim , C. -H. Kim , D. Y. Kim , H. J. Kim , J. B. Kim , K. -H. Kim , K. Kim , S. -H. Kim , Y. -K. Kim , Y. Kim , T. D. Kimmel , H. Kindo , K. Kinoshita , B. Kirby , C. Kleinwort , B. Knysh , P. Kodyš , T. Koga , S. Kohani , I. Komarov , T. Konno , S. Korpar , N. Kovalchuk , T. M. G. Kraetzschmar , P. Križan , R. Kroeger , J. F. Krohn , P. Krokovny , H. Krüger , W. Kuehn , T. Kuhr , J. Kumar , M. Kumar , R. Kumar , K. Kumara , T. Kumita , T. Kunigo , M. Künzel , S. Kurz , A. Kuzmin , P. Kvasnička , Y. -J. Kwon , S. Lacaprara , Y. -T. Lai , C. La Licata , K. Lalwani , L. Lanceri , J. S. Lange , K. Lautenbach , P. J. Laycock , F. R. Le Diberder , I. -S. Lee , S. C. Lee , P. Leitl , D. Levit , P. M. Lewis , C. Li , L. K. Li , S. X. Li , Y. M. Li , Y. B. Li , J. Libby , K. Lieret , L. Li Gioi , J. Lin , Z. Liptak , Q. Y. Liu , Z. A. Liu , D. Liventsev , S. Longo , A. Loos , P. Lu , M. Lubej , T. Lueck , F. Luetticke , T. Luo , C. MacQueen , Y. Maeda , M. Maggiora , S. Maity , R. Manfredi , E. Manoni , S. Marcello , C. Marinas , A. Martini , M. Masuda , T. Matsuda , K. Matsuoka , D. Matvienko , J. McNeil , F. Meggendorfer , J. C. Mei , F. Meier , M. Merola , F. Metzner , M. Milesi , C. Miller , K. Miyabayashi , H. Miyake , H. Miyata , R. Mizuk , K. Azmi , G. B. Mohanty , H. Moon , T. Moon , J. A. Mora Grimaldo , A. Morda , T. Morii , H. -G. Moser , M. Mrvar , F. Mueller , F. J. Müller , Th. Muller , G. Muroyama , C. Murphy , R. Mussa , K. Nakagiri , I. Nakamura , K. R. Nakamura , E. Nakano , M. Nakao , H. Nakayama , H. Nakazawa , T. Nanut , Z. Natkaniec , A. Natochii , M. Nayak , G. Nazaryan , D. Neverov , C. Niebuhr , M. Niiyama , J. Ninkovic , N. K. Nisar , S. Nishida , K. Nishimura , M. Nishimura , M. H. A. Nouxman , B. Oberhof , K. Ogawa , S. Ogawa , S. L. Olsen , Y. Onishchuk , H. Ono , Y. Onuki , P. Oskin , E. R. Oxford , H. Ozaki , P. Pakhlov , G. Pakhlova , A. Paladino , T. Pang , A. Panta , E. Paoloni , S. Pardi , C. Park , H. Park , S. -H. Park , B. Paschen , A. Passeri , A. Pathak , S. Patra , S. Paul , T. K. Pedlar , I. Peruzzi , R. Peschke , R. Pestotnik , M. Piccolo , L. E. Piilonen , P. L. M. Podesta-Lerma , G. Polat , V. Popov , C. Praz , E. Prencipe , M. T. Prim , M. V. Purohit , N. Rad , P. Rados , R. Rasheed , M. Reif , S. Reiter , M. Remnev , P. K. Resmi , I. Ripp-Baudot , M. Ritter , M. Ritzert , G. Rizzo , L. B. Rizzuto , S. H. Robertson , D. Rodríguez Pérez , J. M. Roney , C. Rosenfeld , A. Rostomyan , N. Rout , M. Rozanska , G. Russo , D. Sahoo , Y. Sakai , D. A. Sanders , S. Sandilya , A. Sangal , L. Santelj , P. Sartori , J. Sasaki , Y. Sato , V. Savinov , B. Scavino , M. Schram , H. Schreeck , J. Schueler , C. Schwanda , A. J. Schwartz , B. Schwenker , R. M. Seddon , Y. Seino , A. Selce , K. Senyo , I. S. Seong , J. Serrano , M. E. Sevior , C. Sfienti , V. Shebalin , C. P. Shen , H. Shibuya , J. -G. Shiu , B. Shwartz , A. Sibidanov , F. Simon , J. B. Singh , S. Skambraks , K. Smith , R. J. Sobie , A. Soffer , A. Sokolov , Y. Soloviev , E. Solovieva , S. Spataro , B. Spruck , M. Starič , S. Stefkova , Z. S. Stottler , R. Stroili , J. Strube , J. Stypula , M. Sumihama , K. Sumisawa , T. Sumiyoshi , D. J. Summers , W. Sutcliffe , K. Suzuki , S. Y. Suzuki , H. Svidras , M. Tabata , M. Takahashi , M. Takizawa , U. Tamponi , S. Tanaka , K. Tanida , H. Tanigawa , N. Taniguchi , Y. Tao , P. Taras , F. Tenchini , D. Tonelli , E. Torassa , K. Trabelsi , T. Tsuboyama , N. Tsuzuki , M. Uchida , I. Ueda , S. Uehara , T. Ueno , T. Uglov , K. Unger , Y. Unno , S. Uno , P. Urquijo , Y. Ushiroda , Y. Usov , S. E. Vahsen , R. van Tonder , G. S. Varner , K. E. Varvell , A. Vinokurova , L. Vitale , V. Vorobyev , A. Vossen , E. Waheed , H. M. Wakeling , K. Wan , W. Wan Abdullah , B. Wang , C. H. Wang , M. -Z. Wang , X. L. Wang , A. Warburton , M. Watanabe , S. Watanuki , I. Watson , J. Webb , S. Wehle , M. Welsch , C. Wessel , J. Wiechczynski , P. Wieduwilt , H. Windel , E. Won , L. J. Wu , X. P. Xu , B. Yabsley , S. Yamada , W. Yan , S. B. Yang , H. Ye , J. Yelton , I. Yeo , J. H. Yin , M. Yonenaga , Y. M. Yook , T. Yoshinobu , C. Z. Yuan , G. Yuan , W. Yuan , Y. Yusa , L. Zani , J. Z. Zhang , Y. Zhang , Z. Zhang , V. Zhilich , Q. D. Zhou , X. Y. Zhou , V. I. Zhukova , V. Zhulanov , A. Zupanc

Any predictive theory of star formation must explain observed variations (or lack thereof) in the initial mass function. Recent work suggests that we might expect quantitative variations in the IMF as a function of metallicity (Larson 2005)…

The disruption of asteroids and comets produces cm-sized meteoroids that end up impacting the Earth's atmosphere and producing bright fireballs that might have associated shock waves or, in geometrically-favorable occasions excavate craters…

Earth and Planetary Astrophysics · Physics 2024-05-29 Eloy Peña-Asensio , Josep Maria Trigo-Rodríguez , Maria Gritsevich , Albert Rimola

Material arriving at our solar system from the Galaxy may be detected at Earth in the form of meteors ablating in our atmosphere. Here we report on a search for interstellar meteors within the highest-quality events in the Global Meteor…

Earth and Planetary Astrophysics · Physics 2025-03-26 Paul Wiegert , Vanessa Tran , Cole Gregg , Denis Vida , Peter Brown

Mass ($M$) and luminosity ($L$) are fundamental parameters of stars but can only be measured indirectly. Typically, effective temperature ($T_{\rm eff}$), surface gravity (${\rm log}\ g$) and metallicity ([M/H]) are derived from stellar…

Solar and Stellar Astrophysics · Physics 2025-04-04 Qida Li , Jianping Xiong , Jiao Li , Yanjun Guo , Zhanwen Han , Xuefei Chen , Chao Liu

Fireball light curves can give insight into the meteor ablation process which can be used to improve fireball trajectory and mass modelling. To this aim, the Desert Fireball Network (DFN) is developing a low cost add-on fireball radiometer…

Instrumentation and Methods for Astrophysics · Physics 2019-07-31 Stuart R. G. Buchan , Robert M. Howie , Jonathan Paxman , Hadrien A. R. Devillepoix

Near-Earth asteroid (3200) Phaethon is notable for its association to a strong annual meteor shower, the Geminids, indicative of one or more episodes of mass ejection in the past. The mechanism of Phaethon's past activity is not yet…

Earth and Planetary Astrophysics · Physics 2018-09-05 Quanzhi Ye , Paul A. Wiegert , Man-To Hui

The luminosity function (LF) statistics applied to the BATSE GRBs (sources of GUSBAD catalog) is the theme approached in this work. The LF is a strong statistical tool to extract useful information from astrophysical samples, where the key…

High Energy Astrophysical Phenomena · Physics 2013-09-16 L. J. Rangel Lemos , C. Bianco , R. Ruffini , M. Malheiro

The nature of turbulence in molecular clouds is one of the key parameters that control star formation efficiency: compressive motions, as opposed to solenoidal motions, can trigger the collapse of cores, or mark the expansion of Hii…