| M25BP001 |
Sheng-Jun Lin |
12.7 |
JW |
12.7 |
|
|
|
|
JCMT-APEX-ASTHROS survey: Unveiling cold chemistry by H2D+ and D2H+ spin isomers |
| M25BP002 |
Sheng-Jun Lin |
13 |
JW |
13 |
|
|
|
|
Probing Cosmic-Ray Ionization Rates: H2D+ Observations toward Orion Starless Cores |
| M25BP003 |
Peter Scicluna |
24 |
NO |
|
|
|
|
24 |
HCN and SiO in nearby AGB stars |
| M25BP006 |
Yongming Liang |
18 |
HP |
18 |
|
|
|
|
Interplay between Galaxies and the Most Extremely Concentrated Quasars |
| M25BP011 |
Li-Hwai Lin |
72 |
HP |
|
|
|
|
72 |
Environmental Effects on Molecular Gas in Virgo Dwarf Galaxies: Completing the JCMT Pilot CO Survey |
| M25BP012 |
Stephen Serjeant |
13.5 |
HP |
|
|
13.5 |
|
|
SPOTLESS2: Submm-selected PrOTocLustEr Survey using SCUBA-2 |
| M25BP013 |
Janik Karoly |
16.1 |
NO |
16.1 |
|
|
|
|
Tracing the Magnetic Field in the Filamentary Structure G111 |
| M25BP019 |
Alik Panja |
1.3 |
JW |
|
1.3 |
|
|
|
Deciphering massive clump formation at the hub of merging filaments with SCUBA-2 |
| M25BP021 |
Doris Arzoumanian |
11.8 |
HP |
|
11.8 |
|
|
|
Role of the magnetic field in the evolution of the star-cluster forming Serpens South hub-filament network |
| M25BP026 |
Kyriakos Trakakis |
11.8 |
JW |
|
|
|
11.8 |
|
Molecular Cloud 9... lines - Complete CO coverage for a sample of molecular clouds |
| M25BP027 |
Tania Pereira Dominici |
14.5 |
HP |
|
|
|
7.4 |
7.1 |
Sub-mm blazar variability: a pilot program for LLAMA |
| M25BP030 |
David Eden |
10.5 |
JW |
|
10.5 |
|
|
|
The conditions for star formation in the Outer Galaxy |
| M25BP031 |
Mike Peel |
3 |
HP |
0.3 |
0.3 |
0.3 |
0.3 |
2 |
Thermal emission from large Low Earth Orbit satellites |
| M25BP032 |
Mike Peel |
18.4 |
HP |
3 |
6.4 |
9 |
|
|
Characterising submm transient sources detected by Simons Observatory |
| M25BP033 |
Manuel Fernández-López |
4.6 |
JW |
|
|
4.6 |
|
|
Revamping the observations on the HH270/HH110 deflected jet |
| M25BP040 |
Ram K. Yadav |
32.3 |
JW |
|
32.3 |
|
|
|
SCUBA-2/POL-2 observation of a collision-induced filament G178.2-00.6 |
| M25BP041 |
Daniel Perley |
15 |
HP |
3 |
5 |
5 |
2 |
|
SCUBA-2 ToO Observations of Gamma-Ray Bursts |
| M25BP042 |
Janik Karoly |
2.8 |
NO |
|
|
|
|
2.8 |
CO Observations in L1616 to Better Characterize the Conditions of Star Formation |
| M25BP043 |
Kate Pattle |
2.2 |
SL |
|
2.2 |
|
|
|
Observing scattering in Saturn's rings with POL-2 |
| M25BP044 |
Gary Fuller |
20 |
JW |
|
|
|
|
20 |
The Giant Outflow in M17 |
| M25BP045 |
Travis J. Thieme |
37 |
HP |
|
|
37 |
|
|
Is there a relationship between the Cosmic-Ray Ionization Rate and Protostellar Disk Radius? |
| M25BP046 |
Kim Ngan Nhat Nguyen |
8.5 |
SL |
|
|
8.5 |
|
|
Deciphering Radio Feedback in AGNs: The Crucial Role of Low-to-High Luminosity Sample |
| M25BP048 |
Ming-Kang Lim |
21 |
JW |
|
21 |
|
|
|
SCUBA-2/POL-2 Observations of Dense Clumps in W40's Bipolar HII Region |
| M25BP050 |
Seamus D. Clarke |
8.2 |
NO |
|
8.2 |
|
|
|
STREAMS: linking turbulent, magnetic and gravitational energies across scales with fragmentation in high-mass clumps |
| M25BP054 |
Daniel Harsono |
30 |
NO |
|
|
30 |
|
|
The JCMT Transient Survey: A search for variable protostars |
| M25BP060 |
Miyu Kido |
39.4 |
NO |
|
|
|
24.2 |
15.2 |
Wide Field Imaging of the Accretion Streamers in Young Protostars |
| M25BP061 |
Jia-Wei Wang |
12 |
JW |
|
12 |
|
|
|
Magnetic Fields in an Early Phase Cloud-Cloud Collision system |
| M25BP065 |
Nicolas Peretto |
32.9 |
NO |
|
32.9 |
|
|
|
Magnetic field orientation as a probe of the dynamical decoupling of cluster-forming clumps |
| M25BP066 |
Zacariyya Khan |
10.7 |
NO |
|
10.7 |
|
|
|
Magnetic Fields in the S255N Cloud |
| M25BP069 |
Chian-Chou Chen |
24 |
HP |
12 |
12 |
|
|
|
Growing in concert: The co-evolution of dusty star-forming galaxies and quasars at z~3 |
| M25BP070 |
Kuiyun Huang |
9 |
HP |
3 |
3 |
3 |
|
|
SCUBA-2 Follow-up of Neutrino events |
| M25BP072 |
Seyma Mercimek |
17 |
JW |
|
|
|
17 |
|
Revealing infall in IRDCs for STREAMS- Mapping HCO$^{+}$ |
| M25BP075 |
Sandhyarani Panigrahy |
7.5 |
NO |
7.5 |
|
|
|
|
Revealing the imprints of cloud-cloud collision on the magnetic field morphology |