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pro vyhledávání: '"Rigley, Jessica"'
Autor:
Walton, Craig R., Rigley, Jessica K., Lipp, Alexander, Law, Robert, Suttle, Martin D., Schonbachler, Maria, Wyatt, Mark, Shorttle, Oliver
Publikováno v:
Earth. Nat Astron (2024)
Earth's surface is deficient in available forms of many elements considered limiting for prebiotic chemistry. In contrast, many extraterrestrial rocky objects are rich in these same elements. Limiting prebiotic ingredients may, therefore, have been d
Externí odkaz:
http://arxiv.org/abs/2402.12310
Autor:
Rigley, Jessica K., Wyatt, Mark C.
Models of the zodiacal cloud's thermal emission and sporadic meteoroids suggest Jupiter-family comets (JFCs) as the dominant source of interplanetary dust. However, comet sublimation is insufficient to sustain the quantity of dust presently in the in
Externí odkaz:
http://arxiv.org/abs/2111.14860
Autor:
Rigley, Jessica K., Wyatt, Mark C.
The SEDs of some nearby stars show mid-infrared excesses from warm habitable zone dust, known as exozodiacal dust. This dust may originate in collisions in a planetesimal belt before being dragged inwards. This paper presents an analytical model for
Externí odkaz:
http://arxiv.org/abs/2007.01313
Autor:
Bewley, Alex, Rigley, Jessica, Liu, Yuxuan, Hawke, Jeffrey, Shen, Richard, Lam, Vinh-Dieu, Kendall, Alex
Simulation can be a powerful tool for understanding machine learning systems and designing methods to solve real-world problems. Training and evaluating methods purely in simulation is often "doomed to succeed" at the desired task in a simulated envi
Externí odkaz:
http://arxiv.org/abs/1812.03823
Autor:
Rigley, Jessica Kathryn, Wyatt, Mark C
Warm exozodiacal dust clouds (known as exozodis) reside in the habitable zones of stars, and provide an opportunity to study the inner planetary system. An understanding of exozodis is also crucial to the detection of Earth-like planets, as they will
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::38eb8b6ed6b462e7d1e9ab395b54663f
Autor:
Rigley, Jessica
Many stars show excess mid-infrared emission which is attributed to warm dust in the habitable zone of the star, known as exozodiacal dust, or exozodis for short. Such dust will be a source of noise and confusion when attempting to detect and charact
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c1424abcfb4916376a5deeb8cb0cae4d
Akademický článek
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Autor:
Rigley, Jessica K, Wyatt, Mark C
Publikováno v:
Monthly Notices of the Royal Astronomical Society; Sep2020, Vol. 497 Issue 1, p1143-1165, 23p
