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Table 1.
Details of the INT IDS spectroscopic observations of Y Gem.
Start Time | Grating | λ0 | Spectral range | Spectral Dispersion | Slit Width | R | Exposure Time |
---|---|---|---|---|---|---|---|
(UTC) | (Å) | (Å) | (Å) | (arcsec) | (s) | ||
2024-02-17T21:36 | R1200B | 4050 | 3200 – 4120 | 0.48 | 1.055 | 4220 | 5 × 120 |
2024-02-17T21:56 | R1200B | 4950 | 4130 – 5640 | 0.48 | 1.055 | 5430 | 5 × 80 |
2024-02-16T22:52 | R1200V | 5850 | 5650 – 6180 | 0.48 | 1.055 | 6960 | 5 × 50 |
2024-02-16T22:38 | R1200V | 6750 | 6170 – 7320 | 0.48 | 1.055 | 8790 | 5 × 50 |
2024-02-16T22:24 | R1200V | 7650 | 7320 – 8290 | 0.48 | 1.055 | 9660 | 5 × 50 |
Notes. The spectral range corresponds to the effective spectral range when the segments of the spectra severely affected by the optics vignetting are excised. R denotes the average spectral resolution, R = λ0/Δλ.
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