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个人简介
Anna Ho's primary interests are in energetic transients and time-domain astronomy. Her overarching goal is to connect the final stages of massive-star evolution and the formation of compact objects to the observed characteristics of supernovae, transients, and compact-object remnants. To that end, she makes heavy use of wide-field surveys (ZTF, DESI) and targeted observations spanning the electromagnetic spectrum (Swift, Chandra, Gemini, Keck, SMA, NOEMA, ALMA, VLA), and works to understand the physical processes governing the observed emission. She is an active member of the ZTF, CMB-S4, and DESI collaborations, and serves as co-chair of the CMB-S4 Sources & Transients Working Group.
研究兴趣
论文共 94 篇作者统计合作学者相似作者
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Maayane T. Soumagnac,Peter Nugent,Robert A. Knop,Anna Y. Q. Ho, William Hohensee,Autumn Awbrey,Alexis Andersen,Greg Aldering, Matan Ventura,Jessica N. Aguilar,Steven Ahlen,Segev Y. Benzvi,
arxiv(2024)
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Yuhan Yao,Wenbin Lu,Fiona Harrison, S. R. Kulkarni,Suvi Gezari,Muryel Guolo,S. Bradley Cenko,Anna Y. Q. Ho
ASTROPHYSICAL JOURNALno. 1 (2024): 39
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETYno. 3 (2024): 3020-3034
The Astrophysical Journalno. 1 (2024)
arXiv (Cornell University) (2023)
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#Papers: 93
#Citation: 2580
H-Index: 25
G-Index: 50
Sociability: 7
Diversity: 2
Activity: 120
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