IC 5287
2MIG 3128
AGN is labelled “AGN”; comparison stars are labelled
1, 2, 3… to match the table. Click a marker for details.
One 3.0 h sequence on 2025 June 30/July 1; 90 s exposures; 101 frames retained.
Reference-star use.
Comparison star 1 was adopted as the primary statistical reference.
The variability classification was unchanged when stars 2 or 3
were used instead.
Validation.
Three local comparison stars from APASS DR9 were used.
Leave-one-out stability tests were applied, and the adopted
aperture minimized seeing dependence.
Comparison-star sequence
| ID | RA (deg) | Dec (deg) | V | σV | Catalogue | |
|---|---|---|---|---|---|---|
| 1 | 347.296561 | 0.724682 | 15.319 | 0.079 | APASS DR9 | |
| 2 | 347.278866 | 0.755341 | 15.371 | 0.071 | APASS DR9 | |
| 3 | 347.266787 | 0.734029 | 15.007 | 0.051 | APASS DR9 |
Observing log
| Night | Exposure | Duration | Frames |
|---|---|---|---|
| 2025-06-30/07-01 | 90 s | 3.00 h | 101 used / 102 acquired |
Source:
Izviekova et al. (2026, manuscript) —
The 2MIG isolated AGNs – 5. Hot-dust reverberation and
spectroscopic constraints on BLR–dust scales in IC 5287 and Mrk 845
Public article link will be added after release.
Public article link will be added after release.