Zobrazeno 1 - 10
of 33
pro vyhledávání: '"Paul Kuin"'
Autor:
Marina Manganaro, Giovanna Pedaletti, Marlene Doert, Denis Bastieri, Vandad Fallah Ramazani, Dario Gasparrini, Elina Lindfors, Benoit Lott, Mireia Nievas, Bindu Rani, David J. Thompson, Emmanouil Angelakis, George Borman, Mark Gurwell, Talvikki Hovatta, Ryosuke Itoh, Svetlana Jorstad, Alex Kraus, Thomas P. Krichbaum, Paul Kuin, Anne Lähteenmäki, Valeri Larionov, Amy Yarleen Lien, Ioannis Myserlis, Merja Tornikoski, Ivan Troitsky, J. Anton Zensus, the MAGIC and -LAT Collaborations
Publikováno v:
Galaxies, Vol 4, Iss 4, p 69 (2016)
S5 0716+714 is a well known BL Lac object, and one of the brightest and most active blazars. The discovery in the Very High Energy band (VHE, E > 100 GeV) by MAGIC happened in 2008. In January 2015, the source went through the brightest optical state
Externí odkaz:
https://doaj.org/article/3e822faa25894e19b9a9f51250d9203a
Autor:
Natalie A. Webb, Francisco J. Carrera, Axel Schwope, Christian Motch, Jean Ballet, Mike Watson, Mat Page, Michael Freyberg, Ioannis Georgantopoulos, Mickael Coriat, Didier Barret, Zoe Massida, Maitrayee Gupta, Hugo Tranin, Erwan Quintin, M. Teresa Ceballos, Silvia Mateos, Amalia Corral, Rosa Dominguez, Holger Stiele, Iris Traulsen, Adriana Pires, Ada Nebot, Laurent Michel, François Xavier Pineau, Jere Kuuttila, Pierre Maggi, Sudip Chakroborty, Keir Birchall, Paul Kuin, Athanassios Akylas, Angel Ruiz, Ektoras Pouliasis, Antonis Georgakakis
Publikováno v:
Astronomische Nachrichten.
A novel method is presented which can pin down the time the accretion disk re-established itself in the RS Oph system after it experienced a nova disruption. The method is based on the re-ionisation of the ejecta by photoionisation from the radiation
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e141a52ad94611e92584c788308162b7
Autor:
Vladimir Yershov, Mónica Tress, Gustavo Bruzual, Ignacio Ferreras, Daisuke Kawata, Mat Page, Stéphane Charlot, Paul Kuin, Mark Cropper
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 505 (1), pp.283-292. ⟨10.1093/mnras/stab1270⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 505 (1), pp.283-292. ⟨10.1093/mnras/stab1270⟩
We explore variations of the dust extinction law of the Milky Way by selecting stars from the Swift/UVOT Serendipitous Source Catalogue, cross-matched with Gaia DR2 and 2MASS to produce a sample of 10,452 stars out to ~4kpc with photometry covering a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d2238e2f2456561e697551e650708e42
Autor:
Łukasz Wyrzykowski, Giorgos Leloudas, Kate D. Alexander, M. Dennefeld, Matt Nicholl, I. Irani, Sebastian Gomez, S. J. Smartt, Giacomo Cannizzaro, B. E. Tucker, Curtis McCully, Lluís Galbany, Harrison Abbot, P. Short, Andy Lawrence, Sergio Campana, P. Charalampopoulos, Thomas Wevers, Steve Schulze, Anders Jerkstrand, C. Pellegrino, Cosimo Inserra, Iair Arcavi, Javier Pineda, Mariusz Gromadzki, S. R. Oates, Tao Chen, D. R. Young, Daichi Hiramatsu, Rupak Roy, Paul Kuin, P. K. Blanchard, N. Ihanec, Joseph P. Anderson, D. A. Howell, Nicholas P. Ross, Jamison Burke, Santiago González-Gaitán, Ilya Mandel, Francesca Onori, T. E. Müller-Bravo, Edo Berger, K. W. Smith, Peter G. Jonker, Griffin Hosseinzadeh
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 499, 482-504
Monthly Notices of the Royal Astronomical Society, 499, 1, pp. 482-504
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2020, 499 (1), pp.482-504. ⟨10.1093/mnras/staa2824⟩
Monthly Notices of the Royal Astronomical Society
Nicholl, M, Wevers, T, Oates, S R, Alexander, K D, Leloudas, G, Onori, F, Jerkstrand, A, Gomez, S, Campana, S, Arcavi, I, Charalampopoulos, P, Gromadzki, M, Ihanec, N, Jonker, P G, Lawrence, A, Mandel, I, Schulze, S, Short, P, Burke, J, McCully, C, Hiramatsu, D, Howell, D A, Pellegrino, C, Abbot, H, Anderson, J P, Berger, E, Blanchard, P K, Cannizzaro, G, Chen, T-W, Dennefeld, M, Galbany, L, Gonzalez-Gaitan, S, Hosseinzadeh, G, Inserra, C, Irani, I, Kuin, P, Muller-Bravo, T, Pineda, J, Ross, N P, Roy, R, Smartt, S J, Smith, K W, Tucker, B, Wyrzykowski, L & Young, D R 2020, ' An outflow powers the optical rise of the nearby, fast-evolving tidal disruption event AT2019qiz ', Monthly Notices of the Royal Astronomical Society, vol. 499, no. 1, pp. 482-504 . https://doi.org/10.1093/mnras/staa2824
Digibug. Repositorio Institucional de la Universidad de Granada
instname
Nicholl, M, Wevers, T, Oates, S R, Alexander, K D, Leloudas, G, Onori, F, Jerkstrand, A, Gomez, S, Campana, S, Arcavi, I, Charalampopoulos, P, Gromadzki, M, Ihanec, N, Jonker, P G, Lawrence, A, Mandel, I, Schulze, S, Short, P, Burke, J, McCully, C, Hiramatsu, D, Howell, D A, Pellegrino, C, Abbot, H, Anderson, J P, Berger, E, Blanchard, P K, Cannizzaro, G, Chen, T-W, Dennefeld, M, Galbany, L, González-Gaitán, S, Hosseinzadeh, G, Inserra, C, Irani, I, Kuin, P, Müller-Bravo, T, Pineda, J, Ross, N P, Roy, R, Smartt, S J, Smith, K W, Tucker, B, Wyrzykowski, Ł & Young, D R 2020, ' An outflow powers the optical rise of the nearby, fast-evolving tidal disruption event AT2019qiz ', Monthly Notices of the Royal Astronomical Society, vol. 499, no. 1, pp. 482-504 . https://doi.org/10.1093/mnras/staa2824
Digibug: Repositorio Institucional de la Universidad de Granada
Universidad de Granada (UGR)
Monthly Notices of the Royal Astronomical Society, 499, 1, pp. 482-504
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2020, 499 (1), pp.482-504. ⟨10.1093/mnras/staa2824⟩
Monthly Notices of the Royal Astronomical Society
Nicholl, M, Wevers, T, Oates, S R, Alexander, K D, Leloudas, G, Onori, F, Jerkstrand, A, Gomez, S, Campana, S, Arcavi, I, Charalampopoulos, P, Gromadzki, M, Ihanec, N, Jonker, P G, Lawrence, A, Mandel, I, Schulze, S, Short, P, Burke, J, McCully, C, Hiramatsu, D, Howell, D A, Pellegrino, C, Abbot, H, Anderson, J P, Berger, E, Blanchard, P K, Cannizzaro, G, Chen, T-W, Dennefeld, M, Galbany, L, Gonzalez-Gaitan, S, Hosseinzadeh, G, Inserra, C, Irani, I, Kuin, P, Muller-Bravo, T, Pineda, J, Ross, N P, Roy, R, Smartt, S J, Smith, K W, Tucker, B, Wyrzykowski, L & Young, D R 2020, ' An outflow powers the optical rise of the nearby, fast-evolving tidal disruption event AT2019qiz ', Monthly Notices of the Royal Astronomical Society, vol. 499, no. 1, pp. 482-504 . https://doi.org/10.1093/mnras/staa2824
Digibug. Repositorio Institucional de la Universidad de Granada
instname
Nicholl, M, Wevers, T, Oates, S R, Alexander, K D, Leloudas, G, Onori, F, Jerkstrand, A, Gomez, S, Campana, S, Arcavi, I, Charalampopoulos, P, Gromadzki, M, Ihanec, N, Jonker, P G, Lawrence, A, Mandel, I, Schulze, S, Short, P, Burke, J, McCully, C, Hiramatsu, D, Howell, D A, Pellegrino, C, Abbot, H, Anderson, J P, Berger, E, Blanchard, P K, Cannizzaro, G, Chen, T-W, Dennefeld, M, Galbany, L, González-Gaitán, S, Hosseinzadeh, G, Inserra, C, Irani, I, Kuin, P, Müller-Bravo, T, Pineda, J, Ross, N P, Roy, R, Smartt, S J, Smith, K W, Tucker, B, Wyrzykowski, Ł & Young, D R 2020, ' An outflow powers the optical rise of the nearby, fast-evolving tidal disruption event AT2019qiz ', Monthly Notices of the Royal Astronomical Society, vol. 499, no. 1, pp. 482-504 . https://doi.org/10.1093/mnras/staa2824
Digibug: Repositorio Institucional de la Universidad de Granada
Universidad de Granada (UGR)
We thank the anonymous referee for their many suggestions that improved this paper. We thank Miguel Perez-Torres for helpful discussions. MN is supported by a Royal Astronomical Society Research Fellowship. TW is funded in part by European Research C
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9bd07a9b6af7e568fbca5f004268437f
http://hdl.handle.net/2066/225657
http://hdl.handle.net/2066/225657
Publikováno v:
Astronomy & Astrophysics. 649:A28
Context.Classical nova progenitors are cataclysmic variables and very old novae are observed to match systems with high mass transfer rates and (relatively) long orbital periods. However, the aftermath of a classical nova has never been studied in de
Publikováno v:
Research Notes of the AAS. 4:142
The latest eruption of the recurrent nova LMC 1968 was extensively observed by Swift with its X-ray Telescope instrument. A comparison with the Swift data set from the 2016 eruption shows that the X-ray evolution was remarkably similar just as the ev
Publikováno v:
Astronomy & Astrophysics. 635:A115
Some transients, although classified as novae based on their maximum and early decline optical spectra, cast doubts on their true nature and whether nova impostors might exist. We monitored a candidate nova which displayed a distinctly unusual light
A fraction of classical novae form dust during the early stages of their outbursts. The classical CO nova V5668 Sgr (Nova Sgr. 2015b) underwent a deep photometric minimum about 100 days after outburst that was covered across the spectrum. A similar e
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e6d28917dc9540ee1a3b770ffef03961
Autor:
Nobuyuki Kawai, Stefano Covino, A. S. Trotter, Om Sharan Salafia, Jochen Greiner, Lorraine Hanlon, D. B. Malesani, F. Nappo, J. Japelj, Aaron P. LaCluyze, M. G. Bernardini, Robert J. Smith, Paul Kuin, Sergio Campana, K. M. Ivarsen, Giancarlo Ghirlanda, Daisuke Kuroda, Gianpiero Tagliaferri, P. D'Avanzo, Ruben Salvaterra, B. E. Cobb, Javier Gorosabel, F. J. Virgili, Valerio D'Elia, Dino Fugazza, H. Hanayama, J. Bolmer, C. Guidorzi, Shiho Kobayashi, Josh Haislip, M. Topinka, A. Gomboc, Martin Jelínek, Iain A. Steele, Antonio Martin-Carrillo, Carole Mundell, Jae Woo Kim, B. Sbarufatti, Drejc Kopač, Daniel E. Reichart, A. Melandri, E. Zaninoni, S. D. Vergani, Myungshin Im, David Murphy
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astron.Astrophys.
Astron.Astrophys., 2017, 607, pp.A29. ⟨10.1051/0004-6361/201731759⟩
Melandri, A, Covino, S, Zaninoni, E, Campana, S, Bolmer, J, Cobb, B E, Gorosabel, J, Kim, J W, Kuin, N P M, Kuroda, D, Malesani, D, Mundell, C G, Nappo, F, Sbarufatti, B, Smith, R J, Steele, I A, Topinka, M, Trotter, A S, Virgili, F J, Bernardini, M G, D’avanzo, P, D’elia, V, Fugazza, D, Ghirlanda, G, Gomboc, A, Greiner, J, Guidorzi, C, Haislip, J B, Hanayama, H, Hanlon, L, Im, M, Ivarsen, K M, Japelj, J, Jelínek, M, Kawai, N, Kobayashi, S, Kopac, D, Lacluyzé, A P, Martin-carrillo, A, Murphy, D, Reichart, D E, Salvaterra, R, Salafia, O S, Tagliaferri, G & Vergani, S D 2017, ' Colour variations in the GRB 120327A afterglow ', Astronomy & Astrophysics, vol. 607, pp. A29 . https://doi.org/10.1051/0004-6361/201731759
NASA Astrophysics Data System
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2017, 607, pp.A29. ⟨10.1051/0004-6361/201731759⟩
Astron.Astrophys., 2017, 607, pp.A29. 〈10.1051/0004-6361/201731759〉
instname
Astron.Astrophys.
Astron.Astrophys., 2017, 607, pp.A29. ⟨10.1051/0004-6361/201731759⟩
Melandri, A, Covino, S, Zaninoni, E, Campana, S, Bolmer, J, Cobb, B E, Gorosabel, J, Kim, J W, Kuin, N P M, Kuroda, D, Malesani, D, Mundell, C G, Nappo, F, Sbarufatti, B, Smith, R J, Steele, I A, Topinka, M, Trotter, A S, Virgili, F J, Bernardini, M G, D’avanzo, P, D’elia, V, Fugazza, D, Ghirlanda, G, Gomboc, A, Greiner, J, Guidorzi, C, Haislip, J B, Hanayama, H, Hanlon, L, Im, M, Ivarsen, K M, Japelj, J, Jelínek, M, Kawai, N, Kobayashi, S, Kopac, D, Lacluyzé, A P, Martin-carrillo, A, Murphy, D, Reichart, D E, Salvaterra, R, Salafia, O S, Tagliaferri, G & Vergani, S D 2017, ' Colour variations in the GRB 120327A afterglow ', Astronomy & Astrophysics, vol. 607, pp. A29 . https://doi.org/10.1051/0004-6361/201731759
NASA Astrophysics Data System
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2017, 607, pp.A29. ⟨10.1051/0004-6361/201731759⟩
Astron.Astrophys., 2017, 607, pp.A29. 〈10.1051/0004-6361/201731759〉
Aims. We present a comprehensive temporal and spectral analysis of the long Swift GRB 120327A afterglow data to investigate possible causes of the observed early-time colour variations. Methods. We collected data from various instruments and telescop
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c8a63ce769c2a09747fe7c2229f33e30
http://hdl.handle.net/11392/2378464
http://hdl.handle.net/11392/2378464