Recommended time allocation by the CAT

Semester 2024A

William Herschel Telescope

Ref. CATBandPIAwarded hoursInstrumentLarge programTitle
SW2024a11A Jorge Sánchez Almeida 35.7 WEAVE/LIFU - First Halpha detection of a fossil starless dark-mater halo
SW2024a07B Jesús Maíz Apellániz 48.6 WEAVE/LIFU - A multiplicity survey of stellar clusters with O stars
SW2024a13B Ignacio Negueruela 9.0 WEAVE/LIFU - A massive young cluster in the Outer Milky Way
SW2024a12B Martín Guerrero 9.0 WEAVE/LIFU - Unveiling the Ejecta 3D structure of Nova Remnants
SW2024a09B Ignacio Trujillo 9.0 WEAVE/LIFU - A precise distance estimation to Nube
SW2024a14B Anelise Audibert 10.8 WEAVE/LIFU - WEAVEing insights into jet-ISM interaction: a pilot study of radio-loug galaxies
SW2024a15BC MariCruz Gálvez-Ortiz 36.0 (B:19, C:17) WEAVE/LIFU - Characterization of low-mass eclipsing binaries with WEAVE
SW2024a10C Francesca Pinna 24.3 WEAVE/LIFU - WEAVE-GECKOS: unveiling the assembly of young cold disks in spiral galaxies

*) Oversuscription factor in 2024A = 1.3.
*) Band A corresponds to 25% of CAT A+B time. *) A-band proposals have very high priority and all possible efforts will be made to execute all of the required/approved observations in the requested semester. Unfinished A-band proposals will have a "carry-over status" during two additional semesters, or until their completion, whichever comes first. Unfinished A-band proposals do not have to be re-submitted in the following two semesters because of their carry-over status.
*) B-band proposals will be executed on a best-effort basis during the requested semester, and do not have a carry-over status.
*) C-band proposals have lower priority and no guaranteee that the program will start in the current semester.
*) Recommended telescope time has been increased by a factor of 1.8 (all proposals but one) to account for overheads following the Observatory technical recommendation.