Yeah, that link doesn't work for me either. Here's a link to the abstract from the Monthly Notices of the RAS:
VVV-WIT-08: the giant star that blinked | Monthly Notices of the Royal Astronomical Society | Oxford Academic (oup.com)
Apparently, several such objects have been observed. The suggestion is that the occulting object might be an optically opaque disc around a second star orbiting the first.
ETA: Found the preprint:
2106.05300.pdf (arxiv.org)
Have other stars in the same location of VVV-WIT-08 been determined to be close enough to orbit VVV-WIT-08?
Most likely the case as a Jupiter or even a Super Gas Giant orbiting the star might not register as a dip in the light curve from 23,000 light years away.
At that range, there would be a lot of other objects to think about first, rogue planets or large rogue asteroid fields passing across the stars line of sight to Earth where the object could be 15,000 light years away. But if rogue celestial objects were the cause, then the dip wouldn't repeat itself.
If the object causing the dip in the light curve of VVV-WIT-08 is a planet, most likely a Super Gas Giant, then the planet would be at a distance of somewhere between the distance that Jupiter and Saturn are from our own Sun. The dip of VVV-WIT-08 happens once every 17 years, meaning that the object has taken 17 years to make one full revolution around VVV-WIT-08. Jupiter takes 12 years from any transit point to return to that point.