Proposal ID |
Period (*) |
Time (h) |
Title |
PI |
24A001 |
24A |
14.0 |
Searching for DCN 1-0, DNC 1-0 and DCO+ 1-0 in early-stage massive star-forming regions |
Yuqiang li |
24A002 |
24A |
157.0 |
How widespread are aromatics in cold clouds? |
Marcelino Agundez |
24A003 |
24A |
30.5 |
Molecular Chemistry Induced by J-shock in Supernova Remnant W51C |
Tianyu Tu |
24A004 |
24A |
60.0 |
Further Investigation of the extended ultra-hot gas in the Galactic center with the Yebes 40m telescope |
Juan Li |
24A005 |
24A |
0.7 |
Dynamical state and deuterium fractionation of the infrared dark cloud G1.75-0.08 near the Galactic Centre |
Oskari Miettinen |
24A006 |
24A |
92.8 |
Cataloging the Complex Chemistry towards the Highly-Deuterated Prestellar Core IRAS 16293 E |
Samantha Scibelli |
24A008 |
24A |
10.4 |
Astrochemical Insight: Q Band Line Survey of High Mass Star-Forming Regions with Yebes 40m Telescope
|
suman kumar mondal |
24A009 |
24A |
69.0 |
Linking core and cloud chemistry in the chemically rich star-forming region G31.41+0.31 |
Maria Teresa Beltran |
24A010 |
24A |
86.0 |
Expanding the dominions of the RNA prebiotic feedstock in the Galactic Center |
David San Andrés de Pedro |
24A011 |
24A |
107.5 |
Is the extended, narrow SiO tracing different molecular cloud formation scenarios? |
Wonju Kim |
24A012 |
24A |
192.0 |
Monitoring of SiO masers in evolved stars (Continuation) |
Miguel Gómez Garrido |
24A014 |
24A |
98.0 |
Discovering the chemical complexity towards the outer Galaxy source WB89-621 |
Laura Colzi |
24A019 |
24A |
72.9 |
Chemical Inventory of a Molecular Cloud Interacting with a Supernova Remnant |
Giuliana Cosentino |
24A020 |
24A |
39.0 |
Origin of DCO+ in cold molecular clouds |
Junzhi Wang |
24A021 |
24A |
40.0 |
3mm spectroscopic mapping observation toward S255 to S257 region |
Shu Liu |
24A023 |
24A |
50.0 |
Exploration of the diffuse interstellar gas composition |
gerin |
24A024 |
24A |
72.1 |
Investigating Massive Protostars: A High-Sensitivity Q Band Line Survey with RT40m Telescope |
Prasanta Gorai |
24A025 |
24A |
25.9 |
A Q Band Astrochemical Survey of Extended Green Objects |
Ankan Das |
24A026 |
24A |
120.0 |
Improving the K-band Celestial Reference Frame: Cycle 4 |
Aletha de Witt |
24A028 |
24A |
40.0 |
Effect of ionized gas on massive clumps and ``lobe'' structure in M17 northern cloud |
Zhu Feng-Yao |
24A029 |
24A |
113.7 |
Mapping chemistry in TMC-1: Improving the sensitivity of SANCHO to map rare species and isotopologues |
Jose Cernicharo |
24B001 |
24B |
144.0 |
SiO maser monitoring in post-AGB disks |
Iván Gallardo Cava |
24B002 |
24B |
24.0 |
Tracking SMBH binary orbits using K/Q/W simultaneous VLBI |
Hyunwook Ro |
24B003 |
24B |
57.0 |
Does X-ray/far-UV emission from companions destroy molecules in the envelope of AGB stars? |
José Jairo Díaz Luis |
24B004 |
24B |
135.0 |
New potentially aromatic-rich sources |
Marcelino Agundez |
24B006 |
24B |
22.5 |
A systematic molecular spectral line survey towards mixed chemistry planetary nebulae |
Xujia Ouyang |
24B007 |
24B |
34.1 |
The Infall Motion of Potential Episodic Accretion Sources |
Song Shi-Min |
24B008 |
24B |
24.0 |
High-precision AGN Core-shift Measurements using Triple-band Source-frequency Phase-referencing |
Guang-Yao Zhao |
24B009 |
24B |
768.0 |
Monitoring of SiO masers in evolved stars (Continuation) |
Miguel Gómez Garrido |
24B010 |
24B |
36.5 |
Chemistry induced by cosmic rays towards supernova remnant Kes79 |
Tianyu Tu |
24B011 |
24B |
50.0 |
Q-band survey of CO-emitting post-AGB disks |
Iván Gallardo Cava |
24B012 |
24B |
54.6 |
Complex organics and their precursor radicals in an evolved prestellar core B10-1/L1495 |
Anna Punanova |
24B013 |
24B |
172.0 |
Investigatinting the chemical composition evolution of high-mass star-forming regions |
Jialiang Chen |
24B014 |
24B |
10.0 |
Examining Molecular Gas Chemistry in Dust-Lane
Collisions in the Central Molecular Zone |
Veena Vadamattom Shaji |
24B015 |
24B |
34.0 |
Gas ionisation in M17 |
Andrea Socci |
24B016 |
24B |
60.0 |
Chemical evolution in the early stages of the formation of intermediate-mass protostars (IMs) |
Patricia Fernández Ruiz |
24B019 |
24B |
43.5 |
Is spatially-extended, narrow line-width SiO emission caused by accretion shocks onto molecular clouds? |
Seamus Clarke |
24B020 |
24B |
58.3 |
Mapping chemical complexity and deuteration in the IRAS 16293 E pre-stellar core |
Judit Ferrer Asensio |
24B021 |
24B |
34.3 |
Cold Carbon-Chain Molecules in Barnard 5 |
Anna Punanova |
24B024 |
24B |
145.0 |
Mapping the emission of COMs toward the L1544 pre-stellar core |
Izaskun Jiménez |
24B025 |
24B |
576.0 |
Improving the K-band Celestial Reference Frame: Cycle 5 |
Aletha de Witt |
A: First semestre (1st Feb 2024 - 31st Jul 2024).
B: Second semestre (1st Aug 2024 - 31st Jan 2025).
D: Director's Discretionary Time (1st Feb 2024 - 31st Jan 2025).