Geert Barentsen

@dhomeier @texadactyl Thank you both! This is very helpful! 👍👍👍

We use MAST's name resolver behind the scenes, which returns incorrect coordinates for `beta pic`: ```python >>> from astroquery.mast import MastClass >>> crd1 = MastClass().resolve_object('beta pic') >>> crd1.to_string('hmsdms') '05h47m16.392s -51d04m01.74s'...

(/cc @scfleming)

Thank you for opening this issue @hippke, and congratulations with your work on `transitleastsquares`. It looks like a very innovative and valuable piece of work! I'd like to answer in...

@stefano-rgc Thank you for opening this issue! A little-known fact is that there is a tiny overlap between different TESS cameras. In this specific case, TIC 306772650 falls on science...

@ceb8 From memory, I think all cameras have a tiny tiny overlap with each other in every sector, but I'm not able to find anything about this in the TESS...

> if we change the behavior to show only one TESS Cut per sector, we might want to change search_lightcurvefile() There's a subtle difference: every result returned by `search_lightcurvefile()` is...

> I mistakenly believed there would be two cuts from two FFIs, one from each camera. This may still be the case in the future, should TESSCut add a feature...

:+1:

A new result on the frequency of circumbinary planets was recently published by Asensio-Torres et al using direct imaging: http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:1807.08687