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The NAOC’s ISM group is pleased to announce the 2021 NAOC/ISM Spring Science Forum, which will bee hold at A408 at the NAOC campus on Friday, April 30 from 9:30 AM to 5:00 PM, Beijing Standard Time. Oral presentations will be given and broadcasted from NAOC. The online e-posters will be presented on the Forum website.
The Forum will allow the ISM group’s postdocs, junior faculty members, selected senior graduate students, and invited speakers to give formal oral presentation about their recent work with focus on the proposal ideas. The speakers are encouraged to include 3-5min discussions in the presentation on the possible FAST proposal ideas related to his/her currecnt research projects. Advanced graduate students will also be presenting e-posters on their research. This forum will be open to the NAOC community and invited outside researchers and scientists to attend.
The Online attendence please use Zoom to connect:
https://zoom.com.cn/j/89277150211
SOC:
Di Li (Chair, NAOC)
Chao-Wei Tsai (co-Chair, NAOC)
Jingwen Wu (NAOC)
Weiwei Zhu (NAOC)
Ran Duan (NAOC)
Zheng Zheng (NAOC)
LOC:
Chen-Hui Niu (Chair, NAOC)
Chao-Wei Tsai (co-Chair, NAOC)
Hualei Lyu (NAOC)
Contact:
Chen-Hui Niu (peterniu@nao.cas.cn)
Chao-Wei Tsai (cwtsai@nao.cas.cn)
Forum Opening Remarks
Prof. Di Li
Interstellar scintillation and polarization of PSR B0656+14 in the Monogem ring
uwb survey about known pulsars with special behavior in time domain
Confirmation and Monitoring of Pulsar Candidates in Globular Cluster M5 and M15
Southern Pulsar Census and Polarimetric Studies with the Murchison Widefield Array
The FAST FRBs and the new repeaters
Opportunities with FAST and FASTA (A few brief notes)
Infall streamers to individual stars
Dynamics and Excitation Environment in the rho-Oph Molecular Cloud
A Robust Approach to Estimate Stellar Mass and Stellar Formation Rate of Galaxies Using Empirical SED Templates and Machine Learning
The HI Gas between M83 and NGC5253
Hyperfine Group Ratio (HFGR): A New Recipe for Deriving Temperature from Ammonia Inversion
The Stochastic Nature of FRB121102
Searching for Hot DOGs at low redshifts
Lunch Break
Multi-Scale Coherent Magnetic Field from Atomic Medium to L1544 Molecular Core
Search for molecules toward Orion KL by FAST
Searching for the radio pulse signal in the double neutron star system
Why the magnetic fields become complex even in the quiescent low-mass star forming cores?
Proposed HI observations of low metallicity galaxies by FAST
The abundance ratio X(13CO) /X(C18O) in molecular clouds
A Radio Recombination Line Survey in C Band and Future Perspective of Observations on HI Lines from AGN-Host Dwarf Galaxies with FAST
Forum Summary and Closing Remarks
（Di Li, Zheng Zheng）
Forum Opening Remarks
Interstellar scintillation and polarization of PSR B0656+14 in the Monogem ring
uwb survey about known pulsars with special behavior in time domain
Confirmation and Monitoring of Pulsar Candidates in Globular Cluster M5 and M15
Southern Pulsar Census and Polarimetric Studies with the Murchison Widefield Array
The FAST FRBs and the new repeaters
Opportunities with FAST and FASTA (A few brief notes)
Infall streamers to individual stars
Dynamics and Excitation Environment in the rho-Oph Molecular Cloud
A Robust Approach to Estimate Stellar Mass and Stellar Formation Rate of Galaxies Using Empirical SED Templates and Machine Learning
The HI Gas between M83 and NGC5253
Hyperfine Group Ratio (HFGR): A New Recipe for Deriving Temperature from Ammonia Inversion
The Stochastic Nature of FRB121102
Searching for Hot DOGs at low redshifts
Lunch Break
Multi-Scale Coherent Magnetic Field from Atomic Medium to L1544 Molecular Core
Search for molecules toward Orion KL by FAST
Searching for the radio pulse signal in the double neutron star system
Why the magnetic fields become complex even in the quiescent low-mass star forming cores?
Proposed HI observations of low metallicity galaxies by FAST
The abundance ratio X(13CO) /X(C18O) in molecular clouds
A Radio Recombination Line Survey in C Band and Future Perspective of Observations on HI Lines from AGN-Host Dwarf Galaxies with FAST
Forum Summary and Closing Remarks
（Di Li, Zheng Zheng）
