Table 1
Binary stars observed with separation at or below the resolution limit of 2.56 m NOT or 1.52 m TCS.
| WDS | Discover Comp | HIP | Date/Time | Telescope | Magnitudes |
|---|---|---|---|---|---|
| (α,δ,J2000.0) | Pri Sec | ||||
| (1) | (2) | (3) | (4) | (5) | (6) |
| 08585+3548 | COU 1897 | 44064 | 2024-01-24T03:35 | NOT | 6.84,8.73 |
| 08585+3548 | COU 1897 | 44064 | 2024-03-17T22:39 | TCS | 6.84,8.73 |
| 10083+3136 | KUI 48AB | 49658 | 2024-01-24T04:38 | NOT | 6.90,7.20 |
| 10083+3136 | KUI 48AB | 49658 | 2024-02-28T23:56 | TCS | 6.90,7.20 |
| 10116+1321 | HU 874 | 49929 | 2024-01-24T04:05 | NOT | 6.90,7.87 |
| 10116+1321 | HU 874 | 49929 | 2024-02-28T23:24 | TCS | 6.90,7.87 |
| 15245+3723 | CHR 181Aa,Ab | 75411 | 2023-05-10T01:38 | NOT | 4.31,- |
| 15245+3723 | CHR 181Aa,Ab | 75411 | 2023-04-12T03:38 | TCS | 4.31,- |
Notes. The data for these objects have been used to test the LIST algorithm. All objects were observed at zenith distances of less than 25° and with λ = 825 nm and ∆λ = l20nm.The first three columns (1)–(3), are different designations for the objects, (4) is the date and time in UT of the observations with (5) the telescope used. In (6) the magnitudes from the WDS catalogue are listed. Note: for object 15245+3723, only the magnitude of the main object is given because the source this catalogue is based on does not include both measurements.
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