Zobrazeno 1 - 10
of 110
pro vyhledávání: '"Robert L. Kurucz"'
Autor:
Ruth C. Peterson, Robert L. Kurucz
The spectrum of neutral iron is critical to astrophysics, yet furnace laboratory experiments cannot reach many high-lying Fe I levels. Instead, Peterson & Kurucz (2015) and Peterson, Kurucz & Ayres (2017) turned to UV and optical spectra of warm star
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a130ec429855b270feb341466b8fc40c
http://arxiv.org/abs/2112.14742
http://arxiv.org/abs/2112.14742
Autor:
N. Buchschacher, Fabien Alesina, Damien Ségransan, Andrea Guzmán-Mesa, Chloe Fisher, Kevin Heng, Matej Malik, João M. Mendonça, H. Jens Hoeijmakers, Daniel Kitzmann, Sergey N. Yurchenko, Jonathan Tennyson, Julien Burnier, Simon L. Grimm, Robert L. Kurucz
Publikováno v:
Grimm, S L, Malik, M, Kitzmann, D, Guzmán-Mesa, A, Hoeijmakers, H J, Fisher, C, Mendonça, J M, Yurchenko, S N, Tennyson, J, Alesina, F, Buchschacher, N, Burnier, J, Segransan, D, Kurucz, R L & Heng, K 2021, ' HELIOS-K 2.0 Opacity Calculator and Open-source Opacity Database for Exoplanetary Atmospheres ', Astrophysical Journal Supplement Series, vol. 253, no. 1, 30 . https://doi.org/10.3847/1538-4365/abd773
Grimm, Simon L; Malik, Matej; Kitzmann, Daniel; Guzmán-Mesa, Andrea; Hoeijmakers, H. Jens; Fisher, Chloe; Mendonça, João M.; Yurchenko, Sergey N.; Tennyson, Jonathan; Alesina, Fabien; Buchschacher, Nicolas; Burnier, Julien; Segransan, Damien; Kurucz, Robert L.; Heng, Kevin (2021). HELIOS-K 2.0 Opacity Calculator and Open-source Opacity Database for Exoplanetary Atmospheres. Astrophysical journal-supplement series, 253(1), p. 30. Institute of Physics Publishing IOP 10.3847/1538-4365/abd773
Grimm, Simon L; Malik, Matej; Kitzmann, Daniel; Guzmán-Mesa, Andrea; Hoeijmakers, H. Jens; Fisher, Chloe; Mendonça, João M.; Yurchenko, Sergey N.; Tennyson, Jonathan; Alesina, Fabien; Buchschacher, Nicolas; Burnier, Julien; Segransan, Damien; Kurucz, Robert L.; Heng, Kevin (2021). HELIOS-K 2.0 Opacity Calculator and Open-source Opacity Database for Exoplanetary Atmospheres. Astrophysical journal-supplement series, 253(1), p. 30. Institute of Physics Publishing IOP 10.3847/1538-4365/abd773
Computing and using opacities is a key part of modeling and interpreting data of exoplanetary atmospheres. Since the underlying spectroscopic line lists are constantly expanding and currently include up to ~ 10^10 - 10^11 transition lines, the opacit
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::393c8ace32e2b12cc9dd96d0b1dcafd8
http://arxiv.org/abs/2101.02005
http://arxiv.org/abs/2101.02005
The helium-enriched (He-enriched) metal-rich red giants of Omega Centauri, discovered by Hema and Pandey using the low-resolution spectra from the Vainu Bappu Telescope (VBT) and confirmed by the analyses of the high-resolution spectra obtained from
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::025ca8a9ab229b065127ed1c00cf2d81
http://arxiv.org/abs/2005.06807
http://arxiv.org/abs/2005.06807
Autor:
Gerrit C. Groenenboom, Rainer Volkamer, Brian J. Drouin, Keeyoon Sung, A.A. Vigasin, Tijs Karman, Iouli E. Gordon, Magnus Gustafsson, Jean-Michel Hartmann, Laurence S. Rothman, Wim J. van der Zande, Robert L. Kurucz, Ad van der Avoird, Edward H. Wishnow, Robin Wordsworth, Yury Baranov, Ryan Thalman, Ha Tran, Kang Sun, Christian Boulet
Publikováno v:
Icarus, 328, 160-175
Icarus
Icarus, Elsevier, 2019, 328, pp.160-175. ⟨10.1016/j.icarus.2019.02.034⟩
Icarus, 328, pp. 160-175
Icarus
Icarus, Elsevier, 2019, 328, pp.160-175. ⟨10.1016/j.icarus.2019.02.034⟩
Icarus, 328, pp. 160-175
Correct parameterization of the Collision-induced Absorption (CIA) phenomena is essential for accurate modeling of planetary atmospheres. The HITRAN spectroscopic database provides these parameters in a dedicated section. Here, we significantly revis
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2852592aa7df8a41940302c99c85254e
http://hdl.handle.net/2066/204360
http://hdl.handle.net/2066/204360
Autor:
Robert L. Kurucz
Publikováno v:
Canadian Journal of Physics. 95:825-827
I present a progress report on including all the lines in the line lists, including all the lines in the opacities, and including all the lines in the model atmosphere and spectrum synthesis calculations. The increased opacity will improve stellar at
Autor:
Paul D. Feldman, Randy A. Kimble, Jason Hansen, Grant O. Peacock, Susana E. Deustua, Edward L. Wright, Mary Elizabeth Kaiser, Ralph C. Bohlin, Saul Perlmutter, Joe D. Orndorff, Robert L. Kurucz, Jeffrey W. Kruk, Adam G. Riess, H. Warren Moos, Russell Pelton, Stephan R. McCandliss, David J. Sahnow, Bernard J. Rauscher, Lauren Nicole Aldoroty, Jonathan P. Gardner, William V. Dixon, Matthew J. Morris
Publikováno v:
UV/Optical/IR Space Telescopes and Instruments: Innovative Technologies and Concepts VIII.
Establishing improved spectrophotometric standards is important for a broad range of missions and is relevant to many astrophysical problems. ACCESS, “Absolute Color Calibration Experiment for Standard Stars”, is a series of rocket-borne sub-orbi
Autor:
Eugene F. Milone, Andrew T. Young, Roger A. Bell, Michael Bessell, Richard P. Boyl, Brian Carter, T. Alan Clark, Martin Cohen, David J.I. Fry, Robert Garrison, Ian S. Glass, John Graham, Anahi Granada, Lynn Hillenbrand, Robert L. Kurucz, Ian McLean, Matthew Mountain, George Riecke, Rogerio Riffel, Ronald G. Samec, Stephen J. Schiller, Douglas Simons, Michael Skrutskie, C. Russell Stagg, Christiaan L. Sterken, Roger I. Thompson, Alan Tokunaga, Kevin Volk, Robert Wing
Publikováno v:
Transactions of the International Astronomical Union Series B
Autor:
Robert L. Kurucz
Publikováno v:
Canadian Journal of Physics. 89:417-428
I present a progress report on including all the lines in the line lists, including all the lines in the opacities, and including all the lines in the model atmosphere and spectrum synthesis calculations. The increased opacity will improve stellar at
Autor:
Kelly Chance, Robert L. Kurucz
Publikováno v:
Journal of Quantitative Spectroscopy and Radiative Transfer. 111:1289-1295
We have developed an improved solar reference spectrum for use in the analysis of atmospheric spectra from vacuum wavelengths of 200.07 through 1000.99 nm. The spectrum is developed by combining high spectral resolution ground-based and balloon-based