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The detected Na/Mg ratio in a sample of 17 Na-enhanced and Na-rich meteors is investigated based on obtained spectral, orbital and structural data. We utilize the meteor observations of the AMOS network obtained within a survey of…

Earth and Planetary Astrophysics · Physics 2020-04-24 Pavol Matlovič , Juraj Tóth , Leonard Kornoš , Stefan Loehle

We demonstrate a new statistical method of determining the global photometric properties of the Milky Way (MW) to an unprecedented degree of accuracy, allowing our Galaxy to be compared directly to objects measured in extragalactic surveys.…

Astrophysics of Galaxies · Physics 2015-08-20 Timothy C. Licquia , Jeffrey A. Newman , Jarle Brinchmann

Cryogenic calorimeters, also known as bolometers, are among the leading technologies for searching for rare events. The CUPID experiment is exploiting this technology to deploy a tonne-scale detector to search for neutrinoless double-beta…

Instrumentation and Detectors · Physics 2025-03-07 The CUPID Collaboration , K. Alfonso , A. Armatol , C. Augier , F. T. Avignone , O. Azzolini , A. S. Barabash , G. Bari , A. Barresi , D. Baudin , F. Bellini , G. Benato , L. Benussi , V. Berest , M. Beretta , M. Bettelli , M. Biassoni , J. Billard , F. Boffelli , V. Boldrini , E. D. Brandani , C. Brofferio , C. Bucci , M. Buchynska , J. Camilleri , A. Campani , J. Cao , C. Capelli , S. Capelli , V. Caracciolo , L. Cardani , P. Carniti , N. Casali , E. Celi , C. Chang , M. Chapellier , H. Chen , D. Chiesa , D. Cintas , M. Clemenza , I. Colantoni , S. Copello , O. Cremonesi , R. J. Creswick , A. D'Addabbo , I. Dafinei , F. A. Danevich , F. De Dominicis , M. De Jesus , P. de Marcillac , S. Dell'Oro , S. Di Domizio , S. Di Lorenzo , V. Dompè , A. Drobizhev , L. Dumoulin , G. Fantini , M. El Idrissi , M. Faverzani , E. Ferri , F. Ferri , F. Ferroni , E. Figueroa-Feliciano , J. Formaggio , A. Franceschi , S. Fu , B. K. Fujikawa , J. Gascon , S. Ghislandi , A. Giachero , M. Girola , L. Gironi , A. Giuliani , P. Gorla , C. Gotti , C. Grant , P. Gras , P. V. Guillaumon , T. D. Gutierrez , K. Han , E. V. Hansen , K. M. Heeger , D. L. Helis , H. Z. Huang , M. T. Hurst , L. Imbert , A. Juillard , G. Karapetrov , G. Keppel , H. Khalife , V. V. Kobychev , Yu. G. Kolomensky , R. Kowalski , H. Lattaud , M. Lefevre , M. Lisovenko , R. Liu , Y. Liu , P. Loaiza , L. Ma , F. Mancarella , N. Manenti , A. Mariani , L. Marini , S. Marnieros , M. Martinez , R. H. Maruyama , Ph. Mas , D. Mayer , G. Mazzitelli , E. Mazzola , Y. Mei , M. N. Moore , S. Morganti , T. Napolitano , M. Nastasi , J. Nikkel , C. Nones , E. B. Norman , V. Novosad , I. Nutini , T. O'Donnell , E. Olivieri , M. Olmi , B. T. Oregui , S. Pagan , M. Pageot , L. Pagnanini , D. Pasciuto , L. Pattavina , M. Pavan , Ò. Penek , H. Peng , G. Pessina , V. Pettinacci , C. Pira , S. Pirro , O. Pochon , D. V. Poda , T. Polakovic , O. G. Polischuk , E. G. Pottebaum , S. Pozzi , E. Previtali , A. Puiu , S. Puranam , S. Quitadamo , A. Rappoldi , G. L. Raselli , A. Ressa , R. Rizzoli , C. Rosenfeld , P. Rosier , M. Rossella , J. A. Scarpaci , B. Schmidt , R. Serino , A. Shaikina , K. Shang , V. Sharma , V. N. Shlegel , V. Singh , M. Sisti , P. Slocum , D. Speller , P. T. Surukuchi , L. Taffarello , S. Tomassini , C. Tomei , A. Torres , J. A. Torres , D. Tozzi , V. I. Tretyak , D. Trotta , M. Velazquez , K. J. Vetter , S. L. Wagaarachchi , G. Wang , L. Wang , R. Wang , B. Welliver , J. Wilson , K. Wilson , L. A. Winslow , F. Xie , M. Xue , J. Yang , V. Yefremenko , V. I. Umatov , M. M. Zarytskyy , T. Zhu , A. Zolotarova , S. Zucchelli

We aim to study the dust ejected by main-belt comet (MBC) (300163) 2006 VW139 to obtain information on the ejection mechanism and the spectral properties of the object, to see if they are compatible with those of "normal" comets. Images in…

Earth and Planetary Astrophysics · Physics 2015-06-12 J. Licandro , F. Moreno , J. de León , G. P. Tozzi , L. M. Lara , A. Cabrera-Lavers

Using the Monte Carlo code, SEDONA, multiband photometry and spectra are calculated for supernovae derived from stripped helium stars with presupernova masses from 2.2 to 10.0 $M_\odot$. The models are representative of evolution in close…

High Energy Astrophysical Phenomena · Physics 2021-06-23 Stan Woosley , Tuguldur Sukhbold , Daniel Kasen

We study a sample of 16 Type Ia supernovae (SNe Ia) having both spectroscopic and photometric observations within 2 $-$ 3 days after the first light. The early $B-V$ colors of such a sample tends to show a continuous distribution. For…

From the Sun we know that coronal mass ejections (CMEs) are a transient phenomenon, often correlated with flares. They have an impact on solar mass- and angular momentum loss, and therefore solar evolution, and make a significant part of…

Solar and Stellar Astrophysics · Physics 2022-05-25 Martin Leitzinger , Petra Odert , Petr Heinzel

Recent observations of asteroidal surfaces indicate the presence of materials that do not match the bulk lithology of the body. A possible explanation for the presence of these exogenous materials is that they are products of inter-asteroid…

Earth and Planetary Astrophysics · Physics 2016-01-27 C. Avdellidou , M. C. Price , M. Delbo , P. Ioannidis , M. J. Cole

The measurement of type Ia supernovae magnitudes provides cosmological distances, which can be used to constrain dark energy parameters. Large photometric surveys require a substantial improvement in the calibration precision of their…

A blowout jet occurred within the south coronal hole on 9 February 2011 at 09:00 UT and was observed by the Atmospheric Imaging Assembly (AIA) and Helioseismic and Magnetic Imager (HMI) onboard the Solar Dynamics Observatory, and the EUV…

Solar and Stellar Astrophysics · Physics 2015-06-17 Peter Young , Karin Muglach

As fireball networks grow, the number of events observed becomes unfeasible to manage by manual efforts. Reducing and analysing big data requires automated data pipelines. Triangulation of a fireball trajectory can swiftly provide…

The CoRoT satellite is collecting precise time-resolved photometry for tens of asteroseismology targets. To ensure a correct interpretation of the CoRoT data, the atmospheric parameters, chemical compositions, and rotational velocities of…

Solar and Stellar Astrophysics · Physics 2015-05-13 E. Niemczura , T. Morel , C. Aerts

The discovery of `Oumuamua and CNEOS 2014-01-08 allowed for a calibration of the impact rate of interstellar objects. We propose a new telescope in lunar orbit to study in real-time interstellar meteoroid impacts and to serve as a…

Earth and Planetary Astrophysics · Physics 2020-05-20 Amir Siraj , Abraham Loeb

Discovery of periodic maser emission was an unexpected result from monitoring observations of methanol transitions in high-mass young stellar objects. We report on the detection of five new periodic sources from a monitoring program with…

Solar and Stellar Astrophysics · Physics 2020-01-08 Mateusz Olech , Marian Szymczak , Paweł Wolak , Rafał Sarniak , Anna Bartkiewicz

Distance estimates based on low-resolution spectroscopy and Two Micron All Sky Survey (2MASS) J magnitudes are presented for a large sample of 322 nearby candidates from Luyten's NLTT catalogue. Mainly relatively bright (typically 7 < K_s <…

Astrophysics · Physics 2009-11-13 Ralf-Dieter Scholz , Helmut Meusinger , Hartmut Jahreiß

On October 8th, 2011 the Earth crossed the dust trails left by comet 21P/Giacobini-Zinner during its XIX and XX century perihelion approaches with the comet being close to perihelion. The geometric circumstances of that encounter were thus…

Context: We use phase curves of small bodies to measure absolute magnitudes and, together with complementary theoretical and laboratory results, to understand their surfaces' micro and macroscopic properties. Although we can observe…

Earth and Planetary Astrophysics · Physics 2022-11-09 A. Alvarez-Candal , S. Jiménez Corral , M. Colazo

Apparent stellar magnitudes observed at Maidanak observatory for SN2017ein - peculiarly faint core-collapse supernova rumored to have images of progenitor - are processed to get exact photometric data. Technique of photometry is described…

High Energy Astrophysical Phenomena · Physics 2018-07-24 Pulat Tadjimuratov , Davron Mirzakulov

Metallic bodies that were the cores of differentiated bodies are sources of iron meteorites and are considered to have formed early in the terrestrial planet region before migrating to the main asteroid belt. Surface temperatures and mutual…

Earth and Planetary Astrophysics · Physics 2021-03-31 Ryo Ogawa , Akiko M. Nakamura , Ayako I. Suzuki , Sunao Hasegawa

We present a new methodology to discriminate between light and heavy ultra-high energy cosmic-ray primaries on an event-by-event basis using information from the radio detection of extensive air showers at MHz frequencies. Similarly to…

High Energy Astrophysical Phenomena · Physics 2019-03-18 Washington R. Carvalho , Jaime Alvarez-Muñiz