D
Di Li
Researcher at Chinese Academy of Sciences
Publications - 726
Citations - 20998
Di Li is an academic researcher from Chinese Academy of Sciences. The author has contributed to research in topics: Molecular cloud & Star formation. The author has an hindex of 57, co-authored 617 publications receiving 15824 citations. Previous affiliations of Di Li include Space Science Institute & Max Planck Society.
Papers
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Journal ArticleDOI
The overview of FAST real-time Fast Radio Burst searching system
Xinxin Zhang,R. Duan,Vishal Gajjar,Hai-yan Zhang,Pei Wang,C. H. Niu,Dan Werthimer,Jeff Cobb,Shi-Yu Li,Xin Pei,Yan Zhu,Di Li +11 more
TL;DR: In this paper , a real-time fast radio burst (FRB) searching system has been successfully installed on the 19-beam receiver of FAST, which can detect the FRBs in real time and allows high-time resolution spectro-temporal studies among the repeated bursts.
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Molecular Cloud Cores with High Deuterium Fractions: Nobeyama Mapping Survey
Ken'ichi Tatematsu,Ken'ichi Tatematsu,Gwanjeong Kim,Gwanjeong Kim,Tie Liu,Neal J. Evans,Hee-Weon Yi,Jeong-Eun Lee,Yuefang Wu,Naomi Hirano,Sheng-Yuan Liu,Somnath Dutta,Dipen Sahu,Patricio Sanhueza,Kee-Tae Kim,Mika Juvela,L. Viktor Tóth,O. Fehér,Jinhua He,J. X. Ge,Siyi Feng,Minho Choi,Miju Kang,Mark Thompson,Gary A. Fuller,Di Li,Isabelle Ristorcelli,Ke Wang,James Di Francesco,David Eden,Satoshi Ohashi,Ryo Kandori,Charlotte Vastel,Tomoya Hirota,Takeshi Sakai,Xing Lu,Quang Nguyen Luong,Hiroko Shinnaga,Jungha Kim +38 more
TL;DR: In this article, the results of on-the-fly mapping observations of 44 fields containing 107 SCUBA-2 cores in the emission lines of molecules, N$_2$H$^+$, HC$_3$N, and CCS at 82$-$94 GHz using the Nobeyama 45m telescope were presented.
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Deep Learning for Day Forecasts from Sparse Observations
Marcin Andrychowicz,Lasse Espeholt,Di Li,Samier Merchant,Alexander Merose,Fred Zyda,Shreya Agrawal,Nal Emmerich Kalchbrenner +7 more
TL;DR: MetNet-3 as discussed by the authors extends the lead time to 24 hours by using both dense and sparse data sensors and makes predictions for precipitation, wind, temperature, and dew point.
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H i Self-absorption toward the Cygnus X North: From Atomic Filament to Molecular Filament
TL;DR: In this article , the authors investigated the transition from atomic filament to molecular filament in the Cygnus X North region and found that the most remarkable H i cloud is characterized by a filamentary structure associated in space and in velocity with the principal molecular filament.
Journal ArticleDOI
Discovery of a New Molecular Bubble–Outflow Structure in the Taurus B18 Cloud
Yan Duan,Di Li,Paul F. Goldsmith,Laurent Pagani,Tao-Chung Ching,Shu Liu,Jinjin Xie,Cheng Wang +7 more
TL;DR: In this paper , the identification of a new molecular bubble with an outflow, and a Herbig-Haro object, HH 319, located at the bubble center was reported.