Friday March 13, 2026 15:43 EDT
** The project ID links in the below schedule will bring the user to the appropriate page in the DSS (login required)**
| 2026-03-13 (ET) | Type | Project ID | Project Title | PI | Friend | Rcvrs | Frequency (GHz) |
|---|---|---|---|---|---|---|---|
| +00:00 - 02:00 | A | GBT25A-504 | GBT chemical survey of the newly discovered interstellar comet 3I/ATLAS | Hsieh | Armentrout | ARGUS | 75.00 - 115.50 |
| 02:00 - 07:30 | A | GBT26A-317 | Testing a CR-IC origin to the cooling flow problem with MUSTANG-2 and Chandra | Silich | Moravec | MBA2 | 80.00 - 100.00 |
| 07:30 - 09:15 | A | GBT26A-120 | GBT Diffuse Ionized Gas Survey at Low frequencies -- GDIGS-Low | Salas | Salas | 342 | 0.29 - 0.40 |
| 09:15 - 10:45 | A | GBT26A-436 | Confirming pulsar candidates from a reprocessing of the GBNCC survey | Sengar | Lynch | 342 | 0.29 - 0.40 |
| 10:15 - 11:00 | Maintenance | Incidental non-observational activity | Chestnut | Minter | |||
| 10:45 - 16:15 | A | GBT26A-208 | Magnetoionic properties of persistent radio sources around fast radio bursts | Pandhi | Bautista | L | 1.15 - 1.73 |
| 16:15 - 23:30 | A | GBT25B-093 | Broadband Analysis of TMC-1: Composition and Astrochemical Variety Explored | Remijan | Morgan | X | 7.80 - 12.00 |
| 23:30 - 00:00+ | A | VLBA25B-252 | Observing the real-time evolution of the jet base in M87 | Tiede | Salas | Q, W | 39.20 - 49.80, 68.00 - 92.00 |
| 2026-03-14 (ET) | Type | Project ID | Project Title | PI | Friend | Rcvrs | Frequency (GHz) |
| +00:00 - 07:30 | A | VLBA25B-252 | Observing the real-time evolution of the jet base in M87 | Tiede | Salas | Q, W | 39.20 - 49.80, 68.00 - 92.00 |
| 07:30 - 09:15 | A | GBT26A-120 | GBT Diffuse Ionized Gas Survey at Low frequencies -- GDIGS-Low | Salas | Salas | 342 | 0.29 - 0.40 |
| 09:15 - 10:30 | A | GBT26A-436 | Confirming pulsar candidates from a reprocessing of the GBNCC survey | Sengar | Lynch | 342 | 0.29 - 0.40 |
| 10:30 - 11:45 | A | GBT26A-436 | Confirming pulsar candidates from a reprocessing of the GBNCC survey | Sengar | Lynch | 342 | 0.29 - 0.40 |
| 11:45 - 13:45 | A | GBT26A-556 | Measuring M Dwarf Flare Rates with GBT | MacGregor | Salas | C | 3.85 - 8.00 |
| 13:45 - 15:45 | A | GBT26A-556 | Measuring M Dwarf Flare Rates with GBT | MacGregor | Salas | C | 3.85 - 8.00 |
| 15:45 - 23:15 | A | GBT24B-077 | A Quest for More GLUCOSE: the GBT L1544 Unbiased Complex Organics SurvEy | Scibelli | Morgan | Q | 39.20 - 49.80 |
| 23:15 - 00:00+ | A | GBT26A-388 | Do Quenched Satellite Galaxies Retain Gas? Measuring HI in SAGA Satellites | Asali | Smith | L | 1.15 - 1.73 |
| 2026-03-15 (ET) | Type | Project ID | Project Title | PI | Friend | Rcvrs | Frequency (GHz) |
| +00:00 - 03:00 | A | GBT26A-388 | Do Quenched Satellite Galaxies Retain Gas? Measuring HI in SAGA Satellites | Asali | Smith | L | 1.15 - 1.73 |
| 03:00 - 06:15 | A | GBT26A-224 | Mapping Cool Clouds in the Milky Way's Nuclear Wind | Bordoloi | Bautista | L | 1.15 - 1.73 |
| 06:15 - 09:15 | A | GBT26A-120 | GBT Diffuse Ionized Gas Survey at Low frequencies -- GDIGS-Low | Salas | Salas | 342 | 0.29 - 0.40 |
| 2026-03-16 (ET) | Type | Project ID | Project Title | PI | Friend | Rcvrs | Frequency (GHz) |
| 08:00 - 16:30 | M | Maintenance | Maintenance Period A- No receiver changes | Chestnut | Minter | 342, L, C, X, Q, KFPA, W, ARGUS, MBA2 | |
| 08:00 - 16:30 | M | Maintenance | Maintenance Period B- No receiver changes | Chestnut | Minter | 342, L, C, X, Q, KFPA, W, ARGUS, MBA2 | |
| 09:00 - 01:00 | Maintenance | Incidental non-observational activity | Chestnut | Minter | |||
| 2026-03-17 (ET) | Type | Project ID | Project Title | PI | Friend | Rcvrs | Frequency (GHz) |