| Filed | Form | Description | |
|---|---|---|---|
| 12/19/25 | 424B5 | 424B5 | → |
| 12/17/25 | 424B5 | 424B5 | → |
| 12/11/25 | F-3 | F-3 | → |
| 7/15/25 | 424B4 | 424B4 | → |
| 7/3/25 | F-1 | F-1 | → |
| 9/25/24 | 424B4 | 424B4 | → |
| ↓ | |||
| Filed | Form | Description | |
|---|---|---|---|
| 2/6/23 | SC 13D/A | AMENDMENT NO. 2 TO SCHEDULE 13D | → |
| 12/1/22 | SC 13D/A | AMENDMENT NO. 1 TO SCHEDULE 13D | → |
| 10/25/22 | SC 13D | SCHEDULE 13D | → |
| 5/27/22 | SC 13G/A | AMENDMENT NO. 1 TO SCHEDULE 13G | → |
| 5/26/22 | SC 13G | SCHEDULE 13G | → |
| Filed | Form | Description | |
|---|---|---|---|
| 12/17/25 | EFFECT | EFFECT | → |
| 11/21/25 | DRS | DRS | → |
| 10/1/25 | SCHEDULE 13G/A | SCHEDULE 13G/A | → |
| 9/30/25 | SCHEDULE 13G/A | SCHEDULE 13G/A | → |
| 9/22/25 | SCHEDULE 13G/A | SCHEDULE 13G/A | → |
| 8/14/25 | SCHEDULE 13G/A | SCHEDULE 13G/A | → |
| ↓ | |||
A nova is a transient astronomical event that causes the sudden appearance of a bright, apparently "new" star that slowly fades over weeks or months. All observed novae involve white dwarfs in close binary systems, but causes of the dramatic appearance of a nova vary, depending on the circumstances of the two progenitor stars.