Sunday April 05, 2026 04:17 EDT
** The project ID links in the below schedule will bring the user to the appropriate page in the DSS (login required)**
| 2026-04-05 (ET) | Type | Project ID | Project Title | PI | Friend | Rcvrs | Frequency (GHz) |
|---|---|---|---|---|---|---|---|
| 00:00 - 02:00 | A | GBT26A-556 | Measuring M Dwarf Flare Rates with GBT | MacGregor | Salas | C | 3.85 - 8.00 |
| 02:00 - 02:45 | A | GBT26A-556 | Measuring M Dwarf Flare Rates with GBT | MacGregor | Salas | C | 3.85 - 8.00 |
| 02:45 - 08:30 | A | GBT26A-998 | Space Research | Armentrout | Minter | C | 3.85 - 8.00 |
| 08:30 - 12:30 | A | GBT26A-573 | How Clumpy is the Warm Ionized Medium? | Anderson | Armentrout | C | 3.85 - 8.00 |
| 12:30 - 14:30 | A | GBT26A-556 | Measuring M Dwarf Flare Rates with GBT | MacGregor | Salas | C | 3.85 - 8.00 |
| 14:30 - 15:00 | A | GBT26A-556 | Measuring M Dwarf Flare Rates with GBT | MacGregor | Salas | C | 3.85 - 8.00 |
| 15:00 - 17:30 | A | GBT26A-544 | Direct Measurement of the Cosmic Acceleration: A Quarter-Century GBT Baseline | Darling | Gregory | 800 | 0.68 - 0.92 |
| 17:30 - 18:15 | T | TGBT22A_604 | RFI Scan C static | O'Neil | O'Neil | C | |
| 18:15 - 20:15 | A | GBT26A-580 | A Search for Luminous Radio Bursts from a Repeating Tidal Disruption Event | Pearlman | Lynch | C | 3.85 - 8.00 |
| 20:15 - 00:00+ | T | TGBT22A_604 | RFI Scan C static | O'Neil | O'Neil | C | |
| 2026-04-06 (ET) | Type | Project ID | Project Title | PI | Friend | Rcvrs | Frequency (GHz) |
| +00:00 - 00:30 | T | TGBT22A_604 | RFI Scan C static | O'Neil | O'Neil | C | |
| 00:30 - 02:30 | A | GBT26A-556 | Measuring M Dwarf Flare Rates with GBT | MacGregor | Salas | C | 3.85 - 8.00 |
| 02:30 - 03:00 | A | GBT26A-556 | Measuring M Dwarf Flare Rates with GBT | MacGregor | Salas | C | 3.85 - 8.00 |
| 03:00 - 08:30 | A | GBT26A-998 | Space Research | Armentrout | Minter | C | 3.85 - 8.00 |
| 08:00 - 16:30 | M | Maintenance | Maintenance Period A- No receiver changes | Chestnut | Minter | 800, L, C, X, Q, KFPA, W, ARGUS, MBA2 | |
| 08:00 - 16:30 | M | Maintenance | Maintenance Period B- No receiver changes | Chestnut | Minter | 800, L, C, X, Q, KFPA, W, ARGUS, MBA2 | |
| 08:30 - 10:30 | A | GBT26A-376 | Giant Pulse Emission from an Isolated MSP | Tabassum | Lynch | 800 | 0.68 - 0.92 |
| 10:30 - 13:30 | A | GBT26A-293 | Detecting Radio Pulsations from Optically Variable Spider Candidates | Deneva | Gregory | 800 | 0.68 - 0.92 |
| 13:30 - 18:30 | A | GBT26A-556 | Measuring M Dwarf Flare Rates with GBT | MacGregor | Salas | C | 3.85 - 8.00 |
| 18:30 - 21:45 | T | TGBT22A_604 | RFI Scan C static | O'Neil | O'Neil | C | |
| 21:45 - 00:00+ | A | GBT26A-556 | Measuring M Dwarf Flare Rates with GBT | MacGregor | Salas | C | 3.85 - 8.00 |
| 2026-04-07 (ET) | Type | Project ID | Project Title | PI | Friend | Rcvrs | Frequency (GHz) |
| +00:00 - 00:45 | A | GBT26A-556 | Measuring M Dwarf Flare Rates with GBT | MacGregor | Salas | C | 3.85 - 8.00 |
| 00:45 - 02:45 | A | GBT26A-556 | Measuring M Dwarf Flare Rates with GBT | MacGregor | Salas | C | 3.85 - 8.00 |
| 02:45 - 08:30 | A | GBT26A-998 | Space Research | Armentrout | Minter | C | 3.85 - 8.00 |
| 2026-04-08 (ET) | Type | Project ID | Project Title | PI | Friend | Rcvrs | Frequency (GHz) |
| 03:00 - 08:30 | A | GBT26A-998 | Space Research | Armentrout | Minter | C | 3.85 - 8.00 |
| 2026-04-09 (ET) | Type | Project ID | Project Title | PI | Friend | Rcvrs | Frequency (GHz) |
| 20:00 - 22:00 | A | TYUE000N | LOVEX NRAO Test | Yang | Gregory | X | 7.80 - 12.00 |