| Proposal ID |
Period (*) |
Time (h) |
Title |
PI |
| 22A002 |
22A |
26.0 |
Probing the Jet Base of M87 in the Time Domain |
Jongho Park |
| 22A005 |
22A |
336.0 |
Monitoring of SiO masers in evolved stars (Continuation) |
Miguel Gómez Garrido |
| 22A007 |
22A |
115.4 |
A high sensitivity map at different spatial scales of the molecular emission in TMC-1 |
Jose Cernicharo |
| 22A008 |
22A |
72.1 |
A Carbon-Chain Survey toward Intermediate-Mass Young Stellar Objects |
Kotomi Taniguchi |
| 22A010 |
22A |
69.0 |
Yebes survey of complex organic molecules in Orion cold cores |
Liu Xunchuan |
| 22A011 |
22A |
81.0 |
Searching fullerene-related species towards IC 418 |
Domingo Anibal Garcia Hernandez |
| 22A012 |
22A |
137.6 |
Physical conditions of the expanding bubbles around Orion's massive stars:
Quantifying stellar feedback processes.
|
Javier R. Goicoechea |
| 22A013 |
22A |
40.0 |
CHIPS (Chemistry in Outflows of Post-AGB Stars): The ARIES Survey I |
Luis Velilla-Prieto |
| 22A018 |
22A |
57.0 |
Cold does not mean poor in organics: a chemical survey of galactic cold cores
|
Charlotte VASTEL |
| 22A019 |
22A |
160.0 |
Limits to chemical complexity in UV-illuminated regions IV |
Sara Cuadrado |
| 22A020 |
22A |
29.3 |
Probing infall and shocks in Nearby IRDCs |
Xie |
| 22A021 |
22A |
72.0 |
Improving the K-band Celestial Reference Frame |
Aletha de Witt |
| 22A022 |
22A |
72.0 |
COM Survey of 'Typical' Starless Cores in the Taurus, Perseus and Aquila Molecular Clouds |
Samantha Scibelli |
| 22A024 |
22A |
30.0 |
A molecular cloud almost without turbulence? |
Shu Liu |
| 22A025 |
22A |
125.0 |
The search for chemical complexity in a prestellar cold core: a line survey of TMC-1 in the W band |
Jose Cernicharo |
| 22A028 |
22A |
65.0 |
Unveiling the chemical complexity in hot corinos: the case of B1-a |
Gisela Esplugues |
| 22A029 |
22A |
90.0 |
Disentangling glycine presence and formation through its precursors in G10.47+0.03 |
Gisela Esplugues |
| 22B002 |
22B |
216.0 |
Monitoring of SiO masers in evolved stars (Continuation) |
Miguel Gómez Garrido |
| 22B005 |
22B |
120.2 |
Carbon-Chain Survey toward Seven Intermediate-Mass Young Stellar Objects |
Kotomi Taniguchi |
| 22B006 |
22B |
26.1 |
Stars in the Wind: unveiling the effects of stellar winds on the parental molecular cloud. |
Giuliana Cosentino |
| 22B007 |
22B |
31.4 |
Core shift probes magnetic fields in AGN within 10 000 gravitational radii |
Aleksei Nikonov |
| 22B009 |
22B |
20.0 |
Ionisation triggered by the HB3 supernova remnant: combining FERMI and Yebes 40m telescope |
Aimie Clément |
| 22B012 |
22B |
29.8 |
A Yebes 40m full spectral scan of bright comet C/2022 E3 (ZTF) |
Susanne Wampfler |
| 22B013 |
22B |
8.4 |
Search for Si-bearing molecules in L1157-B1 with Yebes |
Xuefang Xu |
| 22B015 |
22B |
29.5 |
Molecular characterisation of the Integral Shape Filament |
Andrea Socci |
| 22B016 |
22B |
51.0 |
Characterizing the physical and chemical properties of the Sgr B2 east region with the Yebes 40m telescope |
Juan Li |
| 22B017 |
22B |
33.1 |
Abundance ratio of HOCN and HNCO in star formation regions |
Zheng |
| 22B018 |
22B |
10.5 |
Extended SiO Emission in IRDCs: Tracing the Assembly of Massive Clumps? |
Gary Fuller |
| 22B019 |
22B |
26.6 |
A Glimpse to VELLA – Very Low Luminosity/Mass Ratio Clumps |
Ke Wang |
| 22B023 |
22B |
150.0 |
Confirmation of interstellar anions |
Marcelino Agundez |
| 22B025 |
22B |
57.5 |
Yebes W-band survey of complex organic molecules in Orion cold cores |
Liu Xunchuan |
| 22B027 |
22B |
72.0 |
Improving the K-band Celestial Reference Frame |
Aletha de Witt |
| 22B028 |
22B |
40.0 |
3mm spectroscopic mapping observation toward S255 to S257 region |
Shu Liu |
| 22B029 |
22B |
200.0 |
SANCHO: a high sensitivity map of the molecular emission in TMC-1 complementary to QUIJOTE |
Jose Cernicharo |
| 22D011 |
22D |
26.0 |
Probing the Jet Base of M87 in the Time Domain |
Jongho Park |
A: First semestre (1st Feb 2022 - 31st Jul 2022).
B: Second semestre (1st Aug 2022 - 31st Jan 2023).
D: Director's Discretionary Time (1st Feb 2022 - 31st Jan 2023).