Zobrazeno 1 - 10
of 71
pro vyhledávání: '"Harald Nicklas"'
Autor:
Richard Davies, João Alves, Yann Clénet, Veronika Hörmann, Florian Kerber, Florian Lang-Bardl, Harald Nicklas, Jörg-Uwe Pott, Sebastian Rabien, Eckhard Sturm, Eline Tolstoy, Benedetta Vulcani, Jari Kotilainen
Publikováno v:
Ground-based and Airborne Instrumentation for Astronomy IX.
Publikováno v:
Ground-based and Airborne Instrumentation for Astronomy IX.
Autor:
S. J. González Manrique, Christoph Kuckein, David Schmidt, N. Bello González, J. Staude, A. Hofmann, Dirk Soltau, Harald Nicklas, Manuel Collados, Andreas Lagg, Franz Kneer, Meetu Verma, Wolfgang Schmidt, Alex Feller, O. von der Lühe, D. Orozco Suárez, P. Gömöry, Andrea Diercke, C. E. Fischer, S. Hoch, Rolf Schlichenmaier, Sami K. Solanki, M. Sobotka, Horst Balthasar, Klaus G. Strassmeier, Michael Sigwarth, Th. Berkefeld, T. Waldmann, Reiner Volkmer, C. Denker, A. Pastor Yabar
Publikováno v:
Astronomische Nachrichten. 337:1057-1063
Autor:
T. Waldmann, Reza Rezaei, Thomas Berkefeld, J. Kavka, Klaus G. Strassmeier, Harald Nicklas, Axel Hofmann, D. Orozco Suárez, M. Collados Vera, R. Vasková, W. Schmidt, Michael Sigwarth, Peter Gömöry, Carsten Denker, Andreas Lagg, Alex Feller, Michal Sobotka, O. von der Lühe, S. J. González Manrique, Christoph Kuckein, P. Schwartz, Sami K. Solanki, Rolf Schlichenmaier, A. Pastor Yabar, A. Kučera, D. Soltau, H. Balthasar, Dirk Schmidt, Reiner Volkmer, J. Staude
Publikováno v:
Astronomische Nachrichten. 337:1050-1056
Arch filament systems occur in active sunspot groups, where a fibril structure connects areas of opposite magnetic polarity, in contrast to active region filaments that follow the polarity inversion line. We used the GREGOR Infrared Spectrograph (GRI
Autor:
C. Denker, Alex Feller, C. E. Fischer, Andrea Diercke, O. von der Lühe, Th. Berkefeld, M. Sobotka, F. Böhm, Rolf Schlichenmaier, S. J. González Manrique, Harald Nicklas, Dirk Soltau, Axel Hofmann, A. Pator Yabar, C. Kuckein, Klaus G. Strassmeier, D. Orozco Suárez, H. Balthasar, Reza Rezaei, T. Waldmann, Michael Sigwarth, J. Staude, N. Bello González, Andreas Lagg, Sami K. Solanki, David Schmidt, Wolfgang Schmidt, Reiner Volkmer, Manuel Collados, M. Verma
Publikováno v:
Astronomische Nachrichten. 337:1090-1098
Autor:
Lennart Schmidt, Harald Nicklas, Amon Richter, P. Rhode, Karen Disseau, Katja Hauptner, H. Anwand-Heerwart
Publikováno v:
Ground-based and Airborne Instrumentation for Astronomy VII.
The MICADO instrument support structure has to fulfill two purposes, a) the positioning of the camera in a stand-alone mode with SCAO wavefront sensing at the First Light, and b) when it will be mounted at a later stage downstream of its MCAO facilit
Autor:
Thomas Jahn, Maximilian Fabricius, Edmundo Balderrama, Taft Armandroff, Darren L. DePoy, Andreas Kelz, Stephen C. Odewahn, Harald Nicklas, Greg C. Smith, Renny Spencer, Jan Snigula, Gavin Dalton, Gary J. Hill, Cynthia S. Froning, Daniel J. Farrow, Jennifer L. Marshall, John M. Good, Ralf Bender, James R. Fowler, Karl Gebhardt, Andrew M. Peterson, Travis Prochaska, Matthias Steinmetz, Matthew Shetrone, Taylor S. Chonis, Greg Zeimann, George Damm, S. I. Rostopchin, Niv Drory, Sarah Tuttle, Dionne M. Haynes, Herman Kriel, Phillip J. MacQueen, Francesco Montesano, Hanshin Lee, Jerry Martin, Trent Peterson, Jason Ramsey, Eva Noyola, Emily Mrozinski, Amy Westfall, Brian L. Vattiat, Brent Buetow, Randy Bryant, Briana L. Indahl
Publikováno v:
Ground-based and Airborne Instrumentation for Astronomy VII.
The Visible Integral-field Replicable Unit Spectrograph (VIRUS) consists of 156 identical spectrographs (arrayed as 78 pairs, each with a pair of spectrographs) fed by 35,000 fibers, each 1.5 arcsec diameter, at the focus of the upgraded 10 m Hobby-E
Autor:
Joao Alves, Davide Massari, Maximilian Fabricius, Wilfried Boland, O. Dupuis, R.-R. Rohloff, Piercarlo Bonifacio, Sebastian Rabien, U. Neumann, M. Manhart, Gérard Rousset, N. M. Förster Schreiber, Hans Gemperlein, Eckhard Sturm, Florian Lang-Bardl, Josef A. Richter, Roberto Ragazzoni, Florian Kerber, V. Hörmann, Arnaud Sevin, Matthias Rosensteiner, Suzanne Ramsay, Ralf Bender, Ronny Ramlau, Kieran Leschinski, M. Hauser, Peter Bizenberger, R. Genzel, B. Borgo, H.-J. Hess, Vincent Garrel, Markus Plattner, K. Disseau, J. M. Huet, A. Monna, L. Barl, Jens Thomas, Willem Jellema, P. Baudoz, Bodo L. Ziegler, Martin Glück, Christopher Mandla, Niels Tromp, Tristan Buey, Stefan Dreizler, J. Schlichter, Ulrich Hopp, Eline Tolstoy, Ramón Navarro, Stefan Gillessen, Frank Grupp, N. Muench, E. Huby, Simona Mei, H. W. Rix, J. Ramos, Wolfgang Kausch, F. Merlin, Mathieu Cohen, D. Ives, P. Rhode, Roland Wagner, P. Fedou, Gérard Zins, Josef Schubert, Fabrice Vidal, G. Musters, F. Chapron, Renato Falomo, Naidu Bezawada, H. Kravcar, Michael Wegner, Santiago Barboza, Amon Richter, Lars Mohr, Remko Stuik, G. Rodeghiero, G. Verdoes-Kleijn, Harald Nicklas, Paola Amico, A. Janssen, J. Ziegleder, Victoria Hutterer, Norbert Przybilla, W. Zeilinger, N. Neumayer, Ralph Hofferbert, Eric Gendron, F. Müller, Jörg-Uwe Pott, H. Anwand-Heerwart, O. Czoske, Michael Hartl, Fanny Chemla, B. Le Ruyet, Z. Hubert, Yann Clénet, Ric Davies, Jenny Niebsch, N. Geis, V. Déo
Publikováno v:
Proceedings Volume 10702, Ground-based and Airborne Instrumentation for Astronomy VII, 10702
MICADO will enable the ELT to perform diffraction limited near-infrared observations at first light. The instrument's capabilities focus on imaging (including astrometric and high contrast) as well as single object spectroscopy. This contribution loo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c1b51302bc4cc071f4ff5b1977b86754
Autor:
Ian Parry, C. Lovis, Valentina D'Odorico, Marco Riva, Alistair Glasse, Andrea Chiavassa, Lars A. Buchhave, Artie P. Hatzes, Nelson J. Nunes, Nuno C. Santos, Erik Zackrisson, Andrzej Niedzielski, Martin Fisher, Willy Benz, Francesco Pepe, François Bouchy, P. Di Marcantonio, Piotr Masłowski, H. C. Stempels, Ernesto Oliva, David F. Buscher, Harald Nicklas, Alexandre Cabral, Johan P. U. Fynbo, Richard A. McCracken, S. G. Sousa, Mário J. P. F. G. Monteiro, V. Adibekyan, Filippo Maria Zerbi, Pedro Figueira, Phil Parr-Burman, J. R. De Medeiros, P. Huke, R. Rebolo Lopez, Isabelle Boisse, Alessandro Marconi, V. C. Parro, I. C. Leão, Andreas J. Korn, I. Matute, Christopher A. Haniff, Camilla Juul Hansen, Nikolai Piskunov, I. Di Varano, Didier Queloz, Andreas Quirrenbach, C. Allende Prieto, Carlos Martins, Enric Palle, Jochen Liske, Luca Valenziano, E. Delgado-Mena, Michael Weber, B. L. Canto Martins, Simon L. Morris, João Coelho, Martin G. Haehnelt, Derryck T. Reid, Stéphane Udry, Ansgar Reiners, Walter Seifert, Lise Christensen, Pedro J. Amado, Manuel Abreu, Leonardo Vanzi, Klaus G. Strassmeier, Roberto Maiolino, X. Bonfils, Stefano Cristiani, Tim Morris, Marianne Vestergaard, Livia Origlia, Xin Sun
Publikováno v:
NASA Astrophysics Data System
ResearcherID
ResearcherID
The first generation of E-ELT instruments will include an optical-infrared High Resolution Spectrograph, conventionally indicated as EELT-HIRES, which will be capable of providing unique breakthroughs in the fields of exoplanets, star and planet form
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f9d8b3634a90a1624dd207c39ef24fca
http://arxiv.org/abs/1609.00497
http://arxiv.org/abs/1609.00497
Autor:
Heiko Anwad, Guillermo A. Blanc, Andreas Kelz, Thomas Jahn, Darren L. DePoy, Gary J. Hill, Karl Gebhardt, Travis Prochaska, Brian L. Vattiat, Martin Landriau, Hermanus Kriel, Briana L. Indahl, Jennifer L. Marshall, Daniel J. Farrow, Niv Drory, Markus Roth, Sarah Tuttle, Gavin Dalton, Taylor S. Chonis, Maximilian Fabricius, Richard D. Allen, Francesco Montesano, Steve Finkelstein, Hanshin Lee, Ralf Bender, Jason Ramsey, Jan Snigula, Trent Peterson, Eva Noyola, Richard Savage, Harald Nicklas, Dionne M. Haynes, John M. Good, Phillip J. MacQueen
Publikováno v:
SPIE Proceedings.
The Visible Integral-field Replicable Unit Spectrograph (VIRUS) consists of 156 identical spectrographs (arrayed as 78 pairs) fed by 35,000 fibers, each 1.5 arcsec diameter, at the focus of the upgraded 10 m Hobby-Eberly Telescope (HET). VIRUS has a