{"_facts":{"companion":"","deep":"","dossier":"","gaia_eb":"","impression":"yes","period":"2.6149075","planet":"Probably noise or an instrument effect","toi":""},"ai_model":"DreamShaperXL_Turbo_v2.safetensors","amplitude":"1.2%","bp_rp":"0.82","cover":"0_illustration.png","data_used":"TESS sector 1 (QLP)","date":"2026-10-02","dec":"-58.5873","depth":"4.1%","distance_pc":"631 (~2,058 light years)","found_by":"hunt.py (automatic)","gaia_dr3":"6411304738818677120","gaia_gmag":"12.60","gaia_lum":"2.69 x the Sun","gaia_mass":"1.06 x the Sun","gaia_radius":"1.75 x the Sun","gaia_rv":"speed changes by 147 km/s - likely an orbiting pair","gaia_teff":"5,592 K","history":[{"date":"2026-10-02","text":"Found by the automatic search in TESS sector 1"},{"date":"2026-10-02","text":"Planet check: Probably noise or an instrument effect"},{"date":"2026-10-02","text":"Artist's impression added"},{"date":"2026-10-02","text":"Period refined to 2.6149075 days using all TESS sectors"}],"hr":[0.818,3.603],"illustration_note":"Painted by an image AI (DreamShaper XL, a Stable Diffusion XL model) running locally on a home PC, over a 3D layout built from the measured data. No cloud services.","last_update":"2026-10-02","nearest_variable":"Gaia DR3 6411304154703125504 (ROT), 168\" away","nearest_variable_id":"Gaia DR3 6411304154703125504","notes":"Probably noise or an instrument effect.\n\nFound automatically by hunt.py in TESS sector 1 (flagged in 1 sector(s)). Detection score 315.0.\nNot in VSX, ASAS-SN or ZTF variable catalogues at the time of the search; not in Gaia DR3's variable lists.\nUnchecked by hand yet: verify the period, nearby stars and a wider catalogue search.\n\nUpdates:\n2026-10-02  Period refined to 2.6149075 days using all TESS sectors\n2026-10-02  Artist's impression added\n2026-10-02  Planet check: Probably noise or an instrument effect\n2026-10-02  Found by the automatic search in TESS sector 1","period_days":"2.6149075","period_source":"eclipse fit to TESS sectors [1, 27, 28, 67, 102, 103, 104]","planet_check":"Probably noise or an instrument effect","planet_size":"~38.8 Earth radii (~3.46 Jupiter) - too big for a planet","planet_verdict":"fa","ra":"331.972","ruwe":"1.09 - fits a single star","score":"315.0","sector":1,"simbad_id":"UCAC4 158-218247","simbad_name":"UCAC4 158-218247 [*]","status":"Probably noise","summary":"Artist's impression of an UNCONFIRMED candidate, based on its measured data. Two stars of about 5,600 K and 2,900 K (1.8 and 1.2 times the Sun's radius, ~1.0 and ~0.6 solar masses) orbit each other every 62.8 hours, 6.5 million km apart (the Sun-Mercury distance is 58 million km). We see the orbit at 74 degrees (90 = exactly edge-on), close enough to edge-on that they eclipse each other. Sizes, separation, tilt and colours come from fitting the TESS eclipses (see the model-fit plot) plus Gaia's temperature; masses assume normal main-sequence stars. The painted look, surface detail and background were added by a locally run image AI; the stars' sizes, colours and spacing follow the measured data. The secondary eclipse arrives 131 minutes later than half an orbit after the primary, a sign of a slightly oval (eccentric) orbit: e*cos(omega) = +0.0546.","tic":"265592269","title":"TIC 265592269","tmag":"12.12","type":"Transit candidate"}