| Ref. CAT | Band | PI | Awarded time (h) | Instrument | Large program | Title |
| SW2025b19 | A | <Pablo Sánchez Alarcón | 3 | WEAVE | - | Confirming the first Nuclear Star Cluster in formation with WEAVE |
| SW2025b20 | A(20h)+B(29h) | <Jairo Méndez Abreu | 49 | WEAVE | - | Constraining the formation of Milky-Way analogues with WEAVE-LIFU |
| SW2025b26 | B | <Anelise Audibert | 11 | WEAVE | - | WEAVEing Insights into Jet- ISM Interaction |
| SW2025b18 | B | <Maria Kopsacheili | 12.7 | WEAVE | - | Investigation of Supernova Remnants and Ultra-Luminous X-ray nebulae in IC 342 |
| SW2025b24 | B(15h)+C(12h) | <Sara Rodríguez-Berlanas | 27 | WEAVE | - | A multiplicity survey of stellar clusters with O stars |
| SW2025b17 | C | <Sébastien Comerón | 6 | WEAVE | - | NGC1277: a massive galaxy lacking dark matter? |
| SW2025b23 | C | <Sara Rodríguez-Berlanas | 23 | WEAVE | - | Combining the ALS and Villafranca projects: OB stars in clusters |
| SW2025b21 | C | <Rubén García Benito | 37 | WEAVE | - | Illuminating Stellar Relics: WHT/WEAVE Deep Spectroscopy of Galactic Planetary |
| SW2025b27 | C | <Artemi Camps-Fariñao | 5.4 | WEAVE | - | A burst of star formation triggered by a galaxy entering the Coma supercluster |
| SW2025b25 | C | <Sébastien Comerón | 30.3 | WEAVE | - | Constraining the Ionization Mechanism of eDIG in Low- SFR Galaxies |
| SW2025b22 | C | <Cecilia Farina | 9 | WEAVE | - | The impact of Be Stars in open clusters's integrated spectra |