Table 1
List of ERIS data.
| Epoch | ID | NDIT | DIT [s] | PS [mas] | S/N | FWHMx [mas] | FWHMy [mas] | Seeing [mas] |
|---|---|---|---|---|---|---|---|---|
| 2023.279 | 111.24H0.002 | 3 | 600 | 12.5 | 5.4 | 62.37±2.25 | 61.25±2.12 | 0.5-0.6 |
| 2023.435 | 111.24H0.003 | 3 | 600 | 12.5 | 3.7 | 66.27±1.40 | 68.75±1.43 | 0.3-0.7 |
| 2024.221 | 0112.B-2117(A) | 3 | 600 | 12.5 | 4.3 | 80.12±5.37 | 74.00±4.25 | 0.5-0.8 |
| 2024.224 | 0113.B-0111(A) | 3 | 600 | 12.5 | 4.1 | 66.75±1.87 | 67.00±1.95 | 0.3-1.0 |
| 2023.443 | 111.24H0.003 | 14 | 30 | 100 | 5.8 | 107.10±4.45 | 82.26±4.71 | 0.3-0.7 |
| 2023.443 | 111.24H0.003 | 7 | 10 | 250 | 6.1 | 333.86±6.81 | 267.33±5.56 | 0.3-0.7 |
Notes. We measured the Doppler-shifted Brγ line of G2/DSO against the continuum emission to derive the S/N for the data with a spatial plate scale of 12.5 mas. For the data with a spatial plate scale of 100 and 250 mas, we used the bow-shock source X3 because of crowding effects in the dense S cluster. Hence, the indicated quantities describe a signal-to-continuum ratio and are a lower limit to describe the data quality. We refer to Appendix C, where we outline the spectral analysis we used to derive the S/N. Furthermore, the FWHM of S2 indicates a qualitative parameter to compare the 12.5 mas data quality. For the 100 mas and 250 mas data, we list the FWHM of IRS 16NW and IRS 1W, respectively. The listed seeing in arcseconds was taken from www.eso.org and indicates the DIMM-Seeing-at-start-time.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.