Научные публикации в Scopus: Recent submissions

  • Mechanistic Basis for the Binding of RGD- and AGDV-Peptides to the Platelet Integrin αIIbβ3 
    Kononova O.; Litvinov R.; Blokhin D.; Klochkov V.; Weisel J.; Bennett J.; Barsegov V. (2017)
    © 2017 American Chemical Society.Binding of soluble fibrinogen to the activated conformation of the integrin αIIbβ3 is required for platelet aggregation and is mediated exclusively by the C-terminal AGDV-containing ...
  • Interaction of different statins with model membranes by NMR data 
    Galiullina L.; Aganova O.; Latfullin I.; Musabirova G.; Aganov A.; Klochkov V. (2017)
    © 2016 Elsevier B.V.Hydroxy-methyl-glutaryl-coenzyme A (HMG-CoA) reductase inhibitors or statins reduce the amount of low-density lipoprotein (LDL) cholesterol, which is known as a well-established risk factor for ...
  • High-energy Gamma-Ray Activity from V404 Cygni Detected by AGILE during the 2015 June Outburst 
    Piano G.; Munar-Adrover P.; Verrecchia F.; Tavani M.; Trushkin S. (2017)
    © 2017. The American Astronomical Society. All rights reserved.The AGILE satellite detected transient high-energy γ-ray emission from the X-ray binary V404 Cygni, during the 2015 June outburst observed in radio, optical, ...
  • NuSTAR and Swift Observations of the Ultraluminous X-Ray Source IC 342 X-1 in 2016: Witnessing Spectral Evolution 
    Shidatsu M.; Ueda Y.; Fabrika S. (2017)
    © 2017. The American Astronomical Society. All rights reserved.We report on an X-ray observing campaign of the ultraluminous X-ray source IC 342 X-1 with NuSTAR and Swift in 2016 October, in which we captured the very ...
  • Variability and Period Analysis for BL Lac AO 0235+164 
    Fan J.; Kurtanidze O.; Liu Y.; Liu X.; Yang J.; Richter G.; Nikolashvili M.; Kurtanidze S.; Wang H.; Sasada M.; Zhou A.; Lin C.; Yuan Y.; Zhang Y.; Costantin D. (2017)
    © 2017. The American Astronomical Society. All rights reserved.Variability is one of the extreme observational properties of BL Lacertae objects. AO 0235+164 is a well-studied BL Lac throughout allelectromagnetic wavebands. ...
  • M31N 2008-12a - The REMARKABLE RECURRENT NOVA in M31: PANCHROMATIC OBSERVATIONS of the 2015 ERUPTION 
    Darnley M.; Henze M.; Bode M.; Hachisu I.; Hernanz M.; Hornoch K.; Hounsell R.; Kato M.; Ness J.; Osborne J.; Page K.; Ribeiro V.; Rodríguez-Gil P.; Shafter A.; Shara M.; Steele I.; Williams S.; Arai A.; Arcavi I.; Barsukova E.; Boumis P.; Chen T.; Fabrika S.; Figueira J.; Gao X.; Gehrels N.; Godon P.; Goranskij V.; Harman D.; Hartmann D.; Hosseinzadeh G.; Horst J.; Itagaki K.; José J.; Kabashima F.; Kaur A.; Kawai N.; Kennea J.; Kiyota S.; Kučáková H.; Lau K.; Maehara H.; Naito H.; Nakajima K.; Nishiyama K.; O'Brien T.; Quimby R.; Sala G.; Sano Y.; Sion E.; Valeev A.; Watanabe F.; Watanabe M.; Williams B.; Xu Z. (2016)
    © 2016. The American Astronomical Society. All rights reserved.The Andromeda Galaxy recurrent nova M31N 2008-12a had been observed in eruption 10 times, including yearly eruptions from 2008 to 2014. With a measured recurrence ...
  • MULTIFREQUENCY PHOTO-POLARIMETRIC WEBT OBSERVATION CAMPAIGN on the BLAZAR S5 0716+714: SOURCE MICROVARIABILITY and SEARCH for CHARACTERISTIC TIMESCALES 
    Bhatta G.; Stawarz; Ostrowski M.; Markowitz A.; Akitaya H.; Arkharov A.; Bachev R.; Benítez E.; Borman G.; Carosati D.; Cason A.; Chanishvili R.; Damljanovic G.; Dhalla S.; Frasca A.; Hiriart D.; Hu S.; Itoh R.; Jableka D.; Jorstad S.; Jovanovic M.; Kawabata K.; Klimanov S.; Kurtanidze O.; Larionov V.; Laurence D.; Leto G.; Marscher A.; Moody J.; Moritani Y.; Ohlert J.; Paola A.; Raiteri C.; Rizzi N.; Sadun A.; Sasada M.; Sergeev S.; Strigachev A.; Takaki K.; Troitsky I.; Ui T.; Villata M.; Vince O.; Webb J.; Yoshida M.; Zola S. (2016)
    © 2016. The American Astronomical Society. All rights reserved..Here we report on the results of the Whole Earth Blazar Telescope photo-polarimetric campaign targeting the blazar S5 0716+71, organized in 2014 March to ...
  • The accretion flow-discrete ejection connection in GRS 1915+105 
    Punsly B.; Rodriguez J.; Trushkin S. (2016)
    © 2016. The American Astronomical Society. All rights reserved.The microquasar GRS 1915+105 is known for its spectacular discrete ejections. They occur unexpectedly, thus their inception has escaped direct observation. It ...
  • MULTIWAVELENGTH STUDY OF QUIESCENT STATES OF MRK 421 WITH UNPRECEDENTED HARD X-RAY COVERAGE PROVIDED BY NuSTAR IN 2013 
    Baloković M.; Paneque D.; Madejski G.; Furniss A.; Chiang J.; Ajello M.; Alexander D.; Barret D.; Blandford R.; Boggs S.; Christensen F.; Craig W.; Forster K.; Giommi P.; Grefenstette B.; Hailey C.; Harrison F.; Hornstrup A.; Kitaguchi T.; Koglin J.; Madsen K.; Mao P.; Miyasaka H.; Mori K.; Perri M.; Pivovaroff M.; Puccetti S.; Rana V.; Stern D.; Tagliaferri G.; Urry C.; Westergaard N.; Zhang W.; Zoglauer A.; Archambault S.; Archer A.; Barnacka A.; Benbow W.; Bird R.; Buckley J.; Bugaev V.; Cerruti M.; Chen X.; Ciupik L.; Connolly M.; Cui W.; Dickinson H.; Dumm J.; Eisch J.; Falcone A.; Feng Q.; Finley J.; Fleischhack H.; Fortson L.; Griffin S.; Griffiths S.; Grube J.; Gyuk G.; Huetten M.; Håkansson N.; Holder J.; Humensky T.; Johnson C.; Kaaret P.; Kertzman M.; Khassen Y.; Kieda D.; Krause M.; Krennrich F.; Lang M.; Maier G.; McArthur S.; Meagher K.; Moriarty P.; Nelson T.; Nieto D.; Ong R.; Park N.; Pohl M.; Popkow A.; Pueschel E.; Reynolds P.; Richards G.; Roache E.; Santander M.; Sembroski G.; Shahinyan K.; Smith A.; Staszak D.; Telezhinsky I.; Todd N. (2016)
    © 2016. The American Astronomical Society. All rights reserved.We present coordinated multiwavelength observations of the bright, nearby BL Lacertae object Mrk 421 taken in 2013 January-March, involving GASP-WEBT, Swift, ...
  • Planck intermediate results: XL. the Sunyaev-Zeldovich signal from the Virgo cluster 
    Ade P.; Aghanim N.; Arnaud M.; Ashdown M.; Aumont J.; Baccigalupi C.; Banday A.; Barreiro R.; Bartolo N.; Battaner E.; Benabed K.; Benoit-Lévy A.; Bernard J.; Bersanelli M.; Bielewicz P.; Bonaldi A.; Bonavera L.; Bond J.; Borrill J.; Bouchet F.; Burigana C.; Butler R.; Calabrese E.; Cardoso J.; Catalano A.; Chamballu A.; Chiang H.; Christensen P.; Churazov E.; Clements D.; Colombo L.; Combet C.; Comis B.; Couchot F.; Coulais A.; Crill B.; Curto A.; Cuttaia F.; Danese L.; Davies R.; Davis R.; De Bernardis P.; De Rosa A.; De Zotti G.; Delabrouille J.; Dickinson C.; Diego J.; Dolag K.; Dole H.; Donzelli S.; Doré O.; Douspis M.; Ducout A.; Dupac X.; Efstathiou G.; Elsner F.; Enßlin T.; Eriksen H.; Finelli F.; Forni O.; Frailis M.; Fraisse A.; Franceschi E.; Galeotta S. (2016)
    © ESO, 2016.The Virgo cluster is the largest Sunyaev-Zeldovich (SZ) source in the sky, both in terms of angular size and total integrated flux. Planck's wide angular scale and frequency coverage, together with its high ...
  • Planck intermediate results: XLV. Radio spectra of northern extragalactic radio sources 
    Ade P.; Aghanim N.; Aller H.; Aller M.; Arnaud M.; Aumont J.; Baccigalupi C.; Banday A.; Barreiro R.; Bartolo N.; Battaner E.; Benabed K.; Benoit-Lévy A.; Bernard J.; Bersanelli M.; Bielewicz P.; Bonaldi A.; Bonavera L.; Bond J.; Borrill J.; Bouchet F.; Burigana C.; Calabrese E.; Catalano A.; Chiang H.; Christensen P.; Clements D.; Colombo L.; Couchot F.; Crill B.; Curto A.; Cuttaia F.; Danese L.; Davies R.; Davis R.; De Bernardis P.; De Rosa A.; De Zotti G.; Delabrouille J.; Dickinson C.; Diego J.; Dole H.; Donzelli S.; Doré O.; Ducout A.; Dupac X.; Efstathiou G.; Elsner F.; Eriksen H.; Finelli F.; Forni O.; Frailis M.; Fraisse A.; Franceschi E.; Galeotta S.; Galli S.; Ganga K.; Giard M.; Giraud-Héraud Y.; Gjerløw E.; González-Nuevo J.; Górski K.; Gruppuso A.; Gurwell M.; Hansen F.; Harrison D.; Henrot-Versillé S. (2016)
    © ESO, 2016.Continuum spectra covering centimetre to submillimetre wavelengths are presented for a northern sample of 104 extragalactic radio sources, mainly active galactic nuclei, based on four-epoch Planck data. The ...
  • Planck intermediate results: XLI. A map of lensing-induced B -modes 
    Ade P.; Aghanim N.; Ashdown M.; Aumont J.; Baccigalupi C.; Banday A.; Barreiro R.; Bartolo N.; Basak S.; Battaner E.; Benabed K.; Benoit-Lévy A.; Bernard J.; Bersanelli M.; Bielewicz P.; Bock J.; Bonaldi A.; Bonavera L.; Bond J.; Borrill J.; Bouchet F.; Boulanger F.; Burigana C.; Butler R.; Calabrese E.; Cardoso J.; Catalano A.; Chiang H.; Christensen P.; Clements D.; Colombi S.; Colombo L.; Combet C.; Crill B.; Curto A.; Cuttaia F.; Danese L.; Davis R.; De Bernardis P.; De Zotti G.; Delabrouille J.; Dickinson C.; Diego J.; Doré O.; Ducout A.; Dupac X.; Elsner F.; Enßlin T.; Eriksen H.; Finelli F.; Forni O.; Frailis M.; Fraisse A.; Franceschi E.; Galeotta S.; Galli S.; Ganga K.; Ghosh T.; Giard M.; Giraud-Héraud Y.; Gjerløw E.; González-Nuevo J.; Górski K.; Gruppuso A. (2016)
    © ESO, 2016.The secondary cosmic microwave background (CMB) B-modes stem from the post-decoupling distortion of the polarization E-modes due to the gravitational lensing effect of large-scale structures. These lensing-induced ...
  • Planck intermediate results: XLII. Large-scale Galactic magnetic fields 
    Adam R.; Ade P.; Alves M.; Ashdown M.; Aumont J.; Baccigalupi C.; Banday A.; Barreiro R.; Bartolo N.; Battaner E.; Benabed K.; Benoit-Lévy A.; Bernard J.; Bersanelli M.; Bielewicz P.; Bonavera L.; Bond J.; Borrill J.; Bouchet F.; Boulanger F.; Bucher M.; Burigana C.; Butler R.; Calabrese E.; Cardoso J.; Catalano A.; Chiang H.; Christensen P.; Colombo L.; Combet C.; Couchot F.; Crill B.; Curto A.; Cuttaia F.; Danese L.; Davis R.; De Bernardis P.; De Rosa A.; De Zotti G.; Delabrouille J.; Dickinson C.; Diego J.; Dolag K.; Doré O.; Ducout A.; Dupac X.; Elsner F.; Enßlin T.; Eriksen H.; Ferrière K.; Finelli F.; Forni O.; Frailis M.; Fraisse A.; Franceschi E.; Galeotta S.; Ganga K.; Ghosh T.; Giard M.; Gjerløw E.; González-Nuevo J.; Górski K. (2016)
    © ESO, 2016.Recent models for the large-scale Galactic magnetic fields in the literature have been largely constrained by synchrotron emission and Faraday rotation measures. We use three different but representative models ...
  • Planck intermediate results: XXXIX. the Planck list of high-redshift source candidates 
    Ade P.; Aghanim N.; Arnaud M.; Aumont J.; Baccigalupi C.; Banday A.; Barreiro R.; Bartolo N.; Battaner E.; Benabed K.; Benoit-Lévy A.; Bernard J.; Bersanelli M.; Bielewicz P.; Bonaldi A.; Bonavera L.; Bond J.; Borrill J.; Bouchet F.; Boulanger F.; Burigana C.; Butler R.; Calabrese E.; Catalano A.; Chiang H.; Christensen P.; Clements D.; Colombo L.; Couchot F.; Coulais A.; Crill B.; Curto A.; Cuttaia F.; Danese L.; Davies R.; Davis R.; De Bernardis P.; De Rosa A.; De Zotti G.; Delabrouille J.; Dickinson C.; Diego J.; Dole H.; Doré O.; Douspis M.; Ducout A.; Dupac X.; Elsner F.; Enßlin T.; Eriksen H.; Falgarone E.; Finelli F.; Flores-Cacho I.; Frailis M.; Fraisse A.; Franceschi E.; Galeotta S.; Galli S.; Ganga K.; Giard M.; Giraud-Héraud Y.; Gjerløw E.; González-Nuevo J.; Górski K.; Gregorio A.; Gruppuso A. (2016)
    © ESO, 2016.The Planck mission, thanks to its large frequency range and all-sky coverage, has a unique potential for systematically detecting the brightest, and rarest, submillimetre sources on the sky, including distant ...
  • Planck intermediate results: XLIII. Spectral energy distribution of dust in clusters of galaxies 
    Adam R.; Ade P.; Aghanim N.; Ashdown M.; Aumont J.; Baccigalupi C.; Banday A.; Barreiro R.; Bartolo N.; Battaner E.; Benabed K.; Benoit-Lévy A.; Bersanelli M.; Bielewicz P.; Bikmaev I.; Bonaldi A.; Bond J.; Borrill J.; Bouchet F.; Burenin R.; Burigana C.; Calabrese E.; Cardoso J.; Catalano A.; Chiang H.; Christensen P.; Churazov E.; Colombo L.; Combet C.; Comis B.; Couchot F.; Crill B.; Curto A.; Cuttaia F.; Danese L.; Davis R.; De Bernardis P.; De Rosa A.; De Zotti G.; Delabrouille J.; Désert F.; Diego J.; Dole H.; Doré O.; Douspis M.; Ducout A.; Dupac X.; Elsner F.; Enßlin T.; Finelli F.; Forni O.; Frailis M.; Fraisse A.; Franceschi E.; Galeotta S.; Ganga K.; Génova-Santos R.; Giard M.; Giraud-Héraud Y.; Gjerløw E.; González-Nuevo J.; Górski K. (2016)
    © ESO 2016.Although infrared (IR) overall dust emission from clusters of galaxies has been statistically detected using data from the Infrared Astronomical Satellite (IRAS), it has not been possible to sample the spectral ...
  • Planck 2015 results: IV. Low Frequency Instrument beams and window functions 
    Ade P.; Aghanim N.; Ashdown M.; Aumont J.; Baccigalupi C.; Banday A.; Barreiro R.; Bartolo N.; Battaner E.; Benabed K.; Benoît A.; Benoit-Lévy A.; Bernard J.; Bersanelli M.; Bielewicz P.; Bock J.; Bonaldi A.; Bonavera L.; Bond J.; Borrill J.; Bouchet F.; Bucher M.; Burigana C.; Butler R.; Calabrese E.; Cardoso J.; Catalano A.; Chamballu A.; Christensen P.; Colombi S.; Colombo L.; Crill B.; Curto A.; Cuttaia F.; Danese L.; Davies R.; Davis R.; De Bernardis P.; De Rosa A.; De Zotti G.; Delabrouille J.; Dickinson C.; Diego J.; Dole H.; Donzelli S.; Doré O.; Douspis M.; Ducout A.; Dupac X.; Efstathiou G.; Elsner F.; Enßlin T.; Eriksen H.; Fergusson J.; Finelli F.; Forni O.; Frailis M.; Franceschi E.; Frejsel A.; Galeotta S.; Galli S.; Ganga K.; Giard M.; Giraud-Héraud Y. (2016)
    © ESO, 2016.This paper presents the characterization of the in-flight beams, the beam window functions, and the associated uncertainties for the Planck Low Frequency Instrument (LFI). The structure of the paper is similar ...
  • Planck 2015 results: X. Diffuse component separation: Foreground maps 
    Adam R.; Ade P.; Aghanim N.; Alves M.; Arnaud M.; Ashdown M.; Aumont J.; Baccigalupi C.; Banday A.; Barreiro R.; Bartlett J.; Bartolo N.; Battaner E.; Benabed K.; Benoît A.; Benoit-Lévy A.; Bernard J.; Bersanelli M.; Bielewicz P.; Bock J.; Bonaldi A.; Bonavera L.; Bond J.; Borrill J.; Bouchet F.; Boulanger F.; Bucher M.; Burigana C.; Butler R.; Calabrese E.; Cardoso J.; Catalano A.; Challinor A.; Chamballu A.; Chary R.; Chiang H.; Christensen P.; Clements D.; Colombi S.; Colombo L.; Combet C.; Couchot F.; Coulais A.; Crill B.; Curto A.; Cuttaia F.; Danese L.; Davies R.; Davis R.; De Bernardis P.; De Rosa A.; De Zotti G.; Delabrouille J.; Désert F.; Dickinson C.; Diego J.; Dole H.; Donzelli S.; Doré O.; Douspis M.; Ducout A.; Dupac X.; Efstathiou G. (2016)
    © 2016 ESO.Planck has mapped the microwave sky in temperature over nine frequency bands between 30 and 857 GHz and in polarization over seven frequency bands between 30 and 353 GHz in polarization. In this paper we consider ...
  • Planck 2015 results: V. LFI calibration 
    Ade P.; Aghanim N.; Ashdown M.; Aumont J.; Baccigalupi C.; Banday A.; Barreiro R.; Bartolo N.; Battaglia P.; Battaner E.; Benabed K.; Benoît A.; Benoit-Lévy A.; Bernard J.; Bersanelli M.; Bielewicz P.; Bock J.; Bonaldi A.; Bonavera L.; Bond J.; Borrill J.; Bouchet F.; Bucher M.; Burigana C.; Butler R.; Calabrese E.; Cardoso J.; Catalano A.; Chamballu A.; Christensen P.; Colombi S.; Colombo L.; Crill B.; Curto A.; Cuttaia F.; Danese L.; Davies R.; Davis R.; De Bernardis P.; De Rosa A.; De Zotti G.; Delabrouille J.; Dickinson C.; Diego J.; Dole H.; Donzelli S.; Doré O.; Douspis M.; Ducout A.; Dupac X.; Efstathiou G.; Elsner F.; Enßlin T.; Eriksen H.; Fergusson J.; Finelli F.; Forni O.; Frailis M.; Franceschi E.; Frejsel A.; Galeotta S.; Galli S.; Ganga K.; Giard M. (2016)
    © 2016 ESO.We present a description of the pipeline used to calibrate the Planck Low Frequency Instrument (LFI) timelines into thermodynamic temperatures for the Planck 2015 data release, covering four years of uninterrupted ...
  • Planck 2015 results: XV. Gravitational lensing 
    Ade P.; Aghanim N.; Arnaud M.; Ashdown M.; Aumont J.; Baccigalupi C.; Banday A.; Barreiro R.; Bartlett J.; Bartolo N.; Basak S.; Battaner E.; Benabed K.; Benoît A.; Benoit-Lévy A.; Bernard J.; Bersanelli M.; Bielewicz P.; Bock J.; Bonaldi A.; Bonavera L.; Bond J.; Borrill J.; Bouchet F.; Boulanger F.; Bucher M.; Burigana C.; Butler R.; Calabrese E.; Cardoso J.; Catalano A.; Challinor A.; Chamballu A.; Chiang H.; Christensen P.; Church S.; Clements D.; Colombi S.; Colombo L.; Combet C.; Couchot F.; Coulais A.; Crill B.; Curto A.; Cuttaia F.; Danese L.; Davies R.; Davis R.; De Bernardis P.; De Rosa A.; De Zotti G.; Delabrouille J.; Désert F.; Diego J.; Dole H.; Donzelli S.; Doré O.; Douspis M.; Ducout A.; Dunkley J.; Dupac X.; Efstathiou G.; Elsner F. (2016)
    © 2016 EDP Sciences.We present the most significant measurement of the cosmic microwave background (CMB) lensing potential to date (at a level of 40σ), using temperature and polarization data from the Planck 2015 full-mission ...
  • Planck 2015 results: II. Low Frequency Instrument data processings 
    Ade P.; Aghanim N.; Ashdown M.; Aumont J.; Baccigalupi C.; Ballardini M.; Banday A.; Barreiro R.; Bartolo N.; Basak S.; Battaglia P.; Battaner E.; Benabed K.; Benoît A.; Benoit-Lévy A.; Bernard J.; Bersanelli M.; Bielewicz P.; Bock J.; Bonaldi A.; Bonavera L.; Bond J.; Borrill J.; Bouchet F.; Bucher M.; Burigana C.; Butler R.; Calabrese E.; Cardoso J.; Castex G.; Catalano A.; Chamballu A.; Christensen P.; Colombi S.; Colombo L.; Crill B.; Curto A.; Cuttaia F.; Danese L.; Davies R.; Davis R.; De Bernardis P.; De Rosa A.; De Zotti G.; Delabrouille J.; Dickinson C.; Diego J.; Dole H.; Donzelli S.; Doré O.; Douspis M.; Ducout A.; Dupac X.; Efstathiou G.; Elsner F.; Enßlin T.; Eriksen H.; Fergusson J.; Finelli F.; Forni O.; Frailis M.; Franceschet C. (2016)
    © ESO, 2016.We present an updated description of the Planck Low Frequency Instrument (LFI) data processing pipeline, associated with the 2015 data release. We point out the places where our results and methods have remained ...

Search DSpace


Advanced Search

Browse

My Account