The Cautionary Tale of HD 131399 Ab

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The Cautionary Tale of HD 131399 Ab Jason Wang (UC Berkeley) Nielsen, De Rosa, Rameau, Wang, et al., AJ, in press, 2017 The Gemini Planet Imager The Gemini Planet Imager Credit: Rob De Rosa GPI Exoplanet Survey Updates New Team Photo New Logo GPIES Spectral Library Credit: Julien Rameau HD 131399 VLT/SPHERE This candidate passed all of the standard false positive tests Wagner+ 2016 HD 131399 Ab with GPI Reduced with two separate pipelines: pyKLIP (J. Wang) and cADI (J. Rameau) HD 131399 Ab with GPI Beware of Correlated Noise HD 131399 Ab Spectra Beware of Correlated Noise HD 131399 Ab Spectral Type Not an L- or T-type spectrum HD 131399 Ab Astrometry If bound, HD 131399 Ab is moving faster than escape velocity Escape velocity cone HD 131399 Ab Astrometry Fiing an orbit gives unrealistic parameters for the system Background Objects � Adapted from Eric Nielsen Background Objects � Adapted from Eric Nielsen Doesn’t Follow the Background Track But also not in the cone of possible orbits! Parallax Relative PM Background Objects � Not infinity Infinity Adapted from Eric Nielsen Background Objects � Not infinity Also not infinity Adapted from Eric Nielsen A Non-zero Proper Motion Background Object ~12 mas/yr! HD 131399 Ab is a Background Object Non-zero Proper Motion M-dwarf Spectra Lessons Learned for Following Up Candidates • Pipeline systematics exist • Use multiple data reduction pipelines on faint sources • Spectral noise is correlated • Data with broad spectral coverage or from multiple instruments is needed • We can measure nonstationary background objects • Need to rule out both stationary and non-stationary background objects • Otherwise, need to be very confident on spectral typing Color Magnitude Diagram JGPI - HGPI .

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