| Rank | ESO Prog. ID | Investigator | Instrument | Title and link to proposal | Time | Sky | Airmass | |||
|---|---|---|---|---|---|---|---|---|---|---|
| (link to ESO) | (username) | (link to proposal) | (h) | moon | transp. | seeing | ||||
| MPIA/DDT | 0103.A-9033(A) | Régis Lachaume | GROND | Characterizing the variable cloud bands of the binary brown dwarf Luhman 16AB | 7.0 | bright | thin | 2.0 | 2.0 | |
| MPIA/P102 | 0102.A-9008(A) | Olga Zakhozhay | FEROS | Monitoring: Radial Velocity Survey for Planets around Young stars (RVSPY) | 8.0 | bright | thin | 2.0 | 1.8 | |
| MPIA/P102 | 0102.A-9006(A) | Paula Sarkis | FEROS | Monitoring: RV confirmation of TESS warm giant candidates | 8.0 | bright | thin | 2.5 | 1.9 | |
| MPIA/A | 0103.A-9008(A) | Paula Sarkis | FEROS | Monitoring: RV confirmation of TESS warm giant candidates | 208.0 | bright | thin | 2.5 | 1.9 | |
| MPIA/A | 0103.A-9009(A) | Wolfgang Brandner | FEROS | Towards a consistent age scale for the bPic moving group | 80.0 | bright | thin | 1.0 | 3.0 | |
| MPIA/A | 0103.A-9010(A) | Olga Zakhozhay | FEROS | Monitoring: Radial Velocity Survey for Planets around Young stars (RVSPY) | 216.0 | bright | thin | 2.0 | 1.8 | |
| MPIA/A | 0103.A-9011(A) | Trifon Trifonov | FEROS | Monitoring: Eccentric loner or a resonant couple? | 64.0 | bright | thin | 2.5 | 2.5 | |
| MPIA/A | 0103.A-9012(A) | Jan Rybizki | FEROS | Finding close encounters to the solar system using Gaia and FEROS | 64.0 | bright | thin | 2.5 | 2.0 | |
| MPIA/A | 0103.A-9013(A) | Theodora Xylaki-Dornbusch | FEROS | Preparing for the discovery of metal-poor stars in wide-field surveys | 40.0 | bright | thin | 1.2 | 1.5 | |
| MPIA/A | 0103.A-9014(A) | Luigi Mancini | GROND | Physical characterization of the Exoplanetary System WASP-174 | 6.0 | bright | clear | 3.0 | 2.0 | |
| External | 0103.A-9001(A) | Frédéric Courbin | WFI | QSO monitoring programme | 360.0 | bright | thin | 1.8 | 1.5 | |
| Opticon | 0103.A-9007(A) | Daniel Bayliss | FEROS | Probing the Neptune Desert | 48.0 | bright | thick | 1.3 | ||
| MPE | 0103.A-9006(A) | Arne Rau | GROND | Monitoring: RRM/ToO | 0.0 | |||||
| MPE | 0103.A-9005(A) | Janet Chen | GROND | Do superluminous supernovae preferentially occur in group environments | 0.0 | |||||
| CNTAC | 0103.A-9002(A) | Lorenzo Monaco | WFI | Globular clusters in the Gaia era | 24.0 | gray | ||||
| CNTAC | 0103.A-9003(A) | Mercedes Hernández | FEROS | Towards solving the SN Ia progenitor problem | 32.0 | bright | ||||
| CNTAC | 0103.A-9004(A) | James Jenkis | FEROS | Characterising hot Saturns and Jupiters from the Next Generation Transit Survey | 48.0 | bright | ||||
| ToO | 0103.A-9099(A) | Arne Rau | GROND | MPE ToO/RRM GROND run | 0.0 | |||||
| Calib | 60.A-9080(A) | N/A | GROND | GROND calibration | 0.0 | |||||
| Calib | 60.A-9700(A) | N/A | FEROS | FEROS calibration | 0.0 | |||||
| Calib | 60.A-9120(A) | N/A | WFI | WFI calibration | 0.0 | |||||