Zobrazeno 1 - 10
of 6 270
pro vyhledávání: '"Johnson, Luke A"'
Autor:
Johnson, Luke
Publikováno v:
Prairie Schooner. Fall2022, Vol. 96 Issue 3, p121-124. 4p.
Autor:
Raut, Sanket, Mellor, Rebecca, Meurk, Carla, Lam, Michael, Lane, Jonathan, Khoo, Andrew, Cronin, Andrew, Smith, Steve, Heffernan, Ed, Johnson, Luke
Publikováno v:
In Journal of Affective Disorders 15 January 2025 369:411-420
Autor:
Johnson, Luke
Publikováno v:
Prairie Schooner. Fall2022, Vol. 96 Issue 3, p119-121. 3p.
Autor:
Vasilev, Olivia, Hayles, Andrew, Campbell, David, Jaarsma, Ruurd, Johnson, Luke, Vasilev, Krasimir
Publikováno v:
In Materials Today Chemistry October 2024 41
Autor:
Olson, Stan1
Publikováno v:
Currents in Theology & Mission. Jul2024, Vol. 51 Issue 3, p75-76. 2p.
Publikováno v:
Interpretation: A Journal of Bible & Theology. Oct2022, Vol. 76 Issue 4, p369-385. 17p.
Autor:
Johnson, Luke J., Norris, Charlotte N., Unruh, Yvonne C., Solanki, Sami K., Krivova, Natalie, Witzke, Veronika, Shapiro, Alexander I.
Variability observed in photometric lightcurves of late-type stars (on timescales longer than a day) is a dominant noise source in exoplanet surveys and results predominantly from surface manifestations of stellar magnetic activity, namely faculae an
Externí odkaz:
http://arxiv.org/abs/2104.11544
Autor:
Wu, Jun, Chen, Nu, Grau, Elizabeth, Johnson, Luke, Liu, Yongqing, Li, Chi, Scott, Patrick A., Kim, Chang, Sun, Deming, Kaplan, Henry J., Shao, Hui
Publikováno v:
In The Ocular Surface April 2024 32:48-57
Autor:
Gordon, Daniel F., Grugan, Patrick, Kupfer, Rotem, Chen, Yu-hsin, Ting, Antonio, Mamonau, Aliaksandr, Johnson, Luke A., Babzien, Marcus
Two color laser pulses are used to form an air plasma and generate broadband infrared radiation suitable as a seed for backward Raman amplification of CO2 laser pulses. Broadband radiation in the atmospheric window from 8-14 microns is observed. The
Externí odkaz:
http://arxiv.org/abs/2009.13481
A new generation of exoplanet research beckons and with it the need for simulation tools that accurately predict signal and noise in transit spectroscopy observations. We developed ExoSim: an end-to-end simulator that models noise and systematics in
Externí odkaz:
http://arxiv.org/abs/2002.03739