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pro vyhledávání: '"Birkmann, SM"'
Autor:
Birkmann, SM, Ferruit, P, Giardino, G, Nielsen, LD, García Munoz, A, Kendrew, S, Rauscher, BJ, Beck, TL, Keyes, C, Valenti, JA, Jakobsen, P, Dorner, B, Alves De Oliveira, C, Arribas, S, Boker, T, Bunker, AJ, Charlot, S, De Marchi, G, Kumari, N, López-Caniego, M, Lutzgendorf, N, Maiolino, R, Manjavacas, E, Marston, A, Moseley, SH, Prizkal, N, Proffitt, C, Rawle, T, Rix, HW, Te Plate, M, Sabbi, E, Sirianni, M, Willott, CJ, Zeidler, P
Publikováno v:
Birkmann, S M, Ferruit, P, Giardino, G, Nielsen, L D, García Muñoz, A, Kendrew, S, Rauscher, B J, Beck, T L, Keyes, C, Valenti, J A, Jakobsen, P, Dorner, B, Alves De Oliveira, C, Arribas, S, Böker, T, Bunker, A J, Charlot, S, De Marchi, G, Kumari, N, López-caniego, M, Lützgendorf, N, Maiolino, R, Manjavacas, E, Marston, A, Moseley, S H, Prizkal, N, Proffitt, C, Rawle, T, Rix, H, Te Plate, M, Sabbi, E, Sirianni, M, Willott, C J & Zeidler, P 2022, ' The Near-Infrared Spectrograph (NIRSpec) on the James Webb Space Telescope IV. Capabilities and predicted performance for exoplanet characterization ', Astronomy & Astrophysics, vol. 661, A83 . https://doi.org/10.1051/0004-6361/202142592
Astronomy & Astrophysics
Astronomy & Astrophysics
The Near-Inrared Spectrograph (NIRSpec) on the James Webb Space Telescope (JWST) is a very versatile instrument, offering multiobject and integral field spectroscopy with varying spectral resolution ($\sim$30 to $\sim$3000) over a wide wavelength ran
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Autor:
T. Böker, T. L. Beck, S. M. Birkmann, G. Giardino, C. Keyes, N. Kumari, J. Muzerolle, T. Rawle, P. Zeidler, Y. Abul-Huda, C. Alves de Oliveira, S. Arribas, K. Bechtold, R. Bhatawdekar, N. Bonaventura, A. J. Bunker, A. J. Cameron, S. Carniani, S. Charlot, M. Curti, N. Espinoza, P. Ferruit, M. Franx, P. Jakobsen, D. Karakla, M. López-Caniego, N. Lützgendorf, R. Maiolino, E. Manjavacas, A. P. Marston, S. H. Moseley, P. Ogle, M. Perna, M. Peña-Guerrero, N. Pirzkal, R. Plesha, C. R. Proffitt, B. J. Rauscher, H.-W. Rix, B. Rodríguez del Pino, Z. Rustamkulov, E. Sabbi, D. K. Sing, M. Sirianni, M. te Plate, L. Úbeda, G. M. Wahlgren, E. Wislowski, R. Wu, Chris J. Willott
Publikováno v:
Boker, T, Beck, T L, Birkmann, S M, Giardino, G, Keyes, C, Kumari, N, Muzerolle, J, Rawle, T, Zeidler, P, Abul-Huda, Y, de Oliveira, C A, Arribas, S, Bechtold, K, Bhatawdekar, R, Bonaventura, N, Bunker, A J, Cameron, A J, Carniani, S, Charlot, S, Curti, M, Espinoza, N, Ferruit, P, Franx, M, Jakobsen, P, Karakla, D, Lopez-Caniego, M, Lutzgendorf, N, Maiolino, R, Manjavacas, E, Marston, A P, Moseley, S H, Ogle, P, Perna, M, Pena-Guerrero, M, Pirzkal, N, Plesha, R, Proffitt, C R, Rauscher, B J, Rix, H-W, del Pino, B R, Rustamkulov, Z, Sabbi, E, Sing, D K, Sirianni, M, Plate, M T, ubeda, L, Wahlgren, G M, Wislowski, E, Wu, R & Willott, C J 2023, ' In-orbit Performance of the Near-infrared Spectrograph NIRSpec on the James Webb Space Telescope ', Publications of the Astronomical Society of the Pacific, vol. 135, no. 1045, 038001 . https://doi.org/10.1088/1538-3873/acb846
The Near-Infrared Spectrograph (NIRSpec) is one of the four focal plane instruments on the James Webb Space Telescope. In this paper, we summarize the in-orbit performance of NIRSpec, as derived from data collected during its commissioning campaign a
Autor:
Sing DK; Department of Earth and Planetary Sciences, Johns Hopkins University, Baltimore, MD, USA. dsing@jhu.edu.; Department of Physics and Astronomy, Johns Hopkins University, Baltimore, MD, USA. dsing@jhu.edu., Rustamkulov Z; Department of Earth and Planetary Sciences, Johns Hopkins University, Baltimore, MD, USA., Thorngren DP; Department of Physics and Astronomy, Johns Hopkins University, Baltimore, MD, USA., Barstow JK; School of Physical Sciences, The Open University, Milton Keynes, UK., Tremblin P; Université Paris-Saclay, UVSQ, CNRS, CEA, Maison de la Simulation, Gif-sur-Yvette, France.; Université Paris-Saclay, Université Paris Cité, CEA, CNRS, AIM, Gif-sur-Yvette, France., Alves de Oliveira C; European Space Agency, European Space Astronomy Centre, Madrid, Spain., Beck TL; Space Telescope Science Institute, Baltimore, MD, USA., Birkmann SM; European Space Agency, European Space Astronomy Centre, Madrid, Spain., Challener RC; Department of Astronomy and Carl Sagan Institute, Cornell University, Ithaca, NY, USA., Crouzet N; Leiden Observatory, Leiden University, Leiden, The Netherlands., Espinoza N; Space Telescope Science Institute, Baltimore, MD, USA., Ferruit P; European Space Agency, European Space Astronomy Centre, Madrid, Spain., Giardino G; ATG Europe for the European Space Agency, ESTEC, Noordwijk, The Netherlands., Gressier A; Space Telescope Science Institute, Baltimore, MD, USA., Lee EKH; Center for Space and Habitability, University of Bern, Bern, Switzerland., Lewis NK; Department of Astronomy and Carl Sagan Institute, Cornell University, Ithaca, NY, USA., Maiolino R; The Old Schools, University of Cambridge, Cambridge, UK., Manjavacas E; Department of Physics and Astronomy, Johns Hopkins University, Baltimore, MD, USA.; AURA for the European Space Agency (ESA), Space Telescope Science Institute, Baltimore, MD, USA., Rauscher BJ; NASA Goddard Space Flight Center, Greenbelt, MD, USA., Sirianni M; European Space Agency (ESA) Office, Space Telescope Science Institute, Baltimore, MD, USA., Valenti JA; Space Telescope Science Institute, Baltimore, MD, USA.
Publikováno v:
Nature [Nature] 2024 Jun; Vol. 630 (8018), pp. 831-835. Date of Electronic Publication: 2024 May 20.
Autor:
Krause O; Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany. krause@mpia.de, Birkmann SM, Usuda T, Hattori T, Goto M, Rieke GH, Misselt KA
Publikováno v:
Science (New York, N.Y.) [Science] 2008 May 30; Vol. 320 (5880), pp. 1195-7.