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相关论文: Meteor colorimetry with CMOS cameras

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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…

地球与行星天体物理 · 物理学 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.…

星系天体物理 · 物理学 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…

仪器与探测器 · 物理学 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…

地球与行星天体物理 · 物理学 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…

高能天体物理现象 · 物理学 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…

太阳与恒星天体物理 · 物理学 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…

地球与行星天体物理 · 物理学 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…

太阳与恒星天体物理 · 物理学 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…

太阳与恒星天体物理 · 物理学 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…

地球与行星天体物理 · 物理学 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…

太阳与恒星天体物理 · 物理学 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 <…

天体物理学 · 物理学 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…

地球与行星天体物理 · 物理学 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…

高能天体物理现象 · 物理学 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…

地球与行星天体物理 · 物理学 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…

高能天体物理现象 · 物理学 2019-03-18 Washington R. Carvalho , Jaime Alvarez-Muñiz