|
|
|
|
Single-dish approved proposals for the 40m telescope in 2025
Proposals are evaluated by scientific merit and are classifed in ranks A, B and C. Proposals in rank A are guaranteed to be observed, proposals in rank B may be observed if there is available telescope time and proposals in rank C do not have enough quality to be observed.
First Semester - 2025A
| Proposal ID |
Rank |
Title |
PI |
| 25A002 |
A |
SiO maser monitoring in post-AGB disks. Part II |
Iván Gallardo Cava |
| 25A004 |
B |
A Q-band line survey towards supernova remnant W28 |
Tianyu Tu |
| 25A005 |
A |
Studies on the inheritance of large carbon species to the next-generation star-forming regions -a case study for WR140- |
Kotomi Taniguchi |
| 25A006 |
A |
Simultaneous measurements on the isotope ratios of 12C/13C, 14N/15N and 18O/17O in our Galaxy |
Jialiang Chen |
| 25A008 |
A |
Towards Tracking Binary SMBH Orbits Using Global K/Q/W Simultaneous VLBI |
Hyunwook Ro |
| 25A010 |
A |
Linking the fragmentation of clumps to the evolutionary stages |
Han-Tsung Lee |
| 25A012 |
A |
From Droplets to Dense Cores - a Chemical and Kinematic Analysis of Future Star Formation in the Taurus Molecular Cloud |
Lucille Steffes |
| 25A018 |
A |
Sulphur isotopic fractionation in low-mass star-forming regions |
Gisela Esplugues |
| 25A019 |
B |
Is the widely-distributed narrow SiO tracing different molecular cloud formation scenarios? |
Wonju Kim |
| 25A020 |
A |
Constraining gas and grain sulfur chemistry in star forming regions |
Angèle Taillard |
| 25A024 |
A |
On the origin of the extended velocity features in the Milky Way (resubmission) |
Yan Gong |
| 25A025 |
B |
Where and when are PAHs formed in evolved stars? |
Jose Cernicharo |
| 25A026 |
A |
Exploration of the diffuse interstellar gas composition : a confirmation |
gerin |
| 25A028 |
A |
Accurate measurements of the atmospheric spectrum accessible to the Yebes-40m for model improvements |
Juan Ramón Pardo Carrión |
| 25A029 |
A |
A high-sensitivity molecular spectral survey of young stellar objects at 7 mm: a pilot study |
Pablo Rivière |
| 25A030 |
B |
Investigatinting the chemical composition evolution of high-mass star-forming regions |
Jialiang Chen |
|