MISCLASSIFIED
    MILKY WAY
 
  | 
    
| OX Cyg | IRAS - | GSC2.4.2 N2J1006733 | AAVSO 000-BDN-399 | 
| SIMBAD V* OX Cyg | Pan-STARRS 155102986640930591 | SAO - | VSX 11231 | 
| GAIA DR3 2072638040396339456 | SkyMapper - | WRAY - | GCVS OX Cyg | 
| 2MASS J19543937+3914598 | HIP - | Hen - | BD - | 
| WISE J195439.36+391459.8 | TYC - | ESO - | HD - | 
| Bidelman (1954) | - | Allen (1984) | - | Belzcyński et al. (2001) | - | 
| Gaposchkin (1957) | - | Kenyon (1986) | - | Akras et al. (2019) | - | 
| Boyarchuk (1969) | - | Vaidis (1988, 1991) | OX Cyg (Susp.) | 
| Right ascension (°) | 298.6641Ref | Parallax (mas) | 0.648±0.020Ref | Reddening E(B-V) (mag) | 0.36±0.02Ref, Note | 
| Declination (°) | 39.2499Ref | Distance (kpc) | 1.49Ref, Note, 1.48Ref, Note | ||
| Galactic longitude (°) | 74.4339Ref | Proper motion in α (mas/yr) | -0.73±0.02Ref | ||
| Galactic latitude (°) | 5.7849Ref | Proper motion in δ (mas/yr) | -2.65±0.02Ref | 
First mentioned in Hoffleit (1975) and included as a symbiotic candidate in Vaidis (1988). The star studied by Hoffleit (1975), however, corresponds to OY Cyg according to Kazarovets & Samus (1998). In Heinze et al. (2018), this object is classified as a close binary with a period of around 0.36 days, which is well consistent with the ZTF data.