2017A&A...598A..83W


C.D.S. - SIMBAD4 rel 1.7 - 2020.07.04CEST02:36:43

2017A&A...598A..83W - Astronomy and Astrophysics, volume 598A, 83-83 (2017/2-1)

VLT/SPHERE robust astrometry of the HR8799 planets at milliarcsecond-level accuracy Orbital architecture analysis with PyAstrOFit.

WERTZ O., ABSIL O., GOMEZ GONZALEZ C.A., MILLI J., GIRARD J.H., MAWET D. and PUEYO L.

Abstract (from CDS):

Context. HR8799 is orbited by at least four giant planets, making it a prime target for the recently commissioned Spectro-Polarimetric High-contrast Exoplanet REsearch (VLT/SPHERE). As such, it was observed on five consecutive nights during the SPHERE science verification in December 2014.
Aims. We aim to take full advantage of the SPHERE capabilities to derive accurate astrometric measurements based on H-band images acquired with the Infra-Red Dual-band Imaging and Spectroscopy (IRDIS) subsystem, and to explore the ultimate astrometric performance of SPHERE in this observing mode. We also aim to present a detailed analysis of the orbital parameters for the four planets.
Methods. We performed thorough post-processing of the IRDIS images with the Vortex Imaging Processing (VIP) package to derive a robust astrometric measurement for the four planets. This includes the identification and careful evaluation of the different contributions to the error budget, including systematic errors. Combining our astrometric measurements with the ones previously published in the literature, we constrain the orbital parameters of the four planets using PyAstrOFit, our new open-source python package dedicated to orbital fitting using Bayesian inference with Monte-Carlo Markov Chain sampling.
Results. We report the astrometric positions for epoch 2014.93 with an accuracy down to 2.0 mas, mainly limited by the astrometric calibration of IRDIS. For each planet, we derive the posterior probability density functions for the six Keplerian elements and identify sets of highly probable orbits. For planet d, there is clear evidence for nonzero eccentricity (e∼0.35), without completely excluding solutions with smaller eccentricities. The three other planets are consistent with circular orbits, although their probability distributions spread beyond e = 0.2, and show a peak at e~=0.1 for planet e. The four planets have consistent inclinations of approximately 30° with respect to the sky plane, but the confidence intervals for the longitude of the ascending node are disjointed for planets b and c, and we find tentative evidence for non-coplanarity between planets b and c at the 2σ level.

Abstract Copyright: © ESO, 2017

Journal keyword(s): planetary systems - stars: individual: HR8799 - methods: data analysis

Simbad objects: 6

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Number of rows : 6

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2020
#notes
1 * bet Pic b Pl 05 47 17.0876901 -51 03 59.441135           ~ 338 1
2 * alf PsA b Pl 22 57 39.04625 -29 37 20.0533           ~ 179 1
3 HD 218396b Pl 23 07 28.7156905667 +21 08 03.302133882           ~ 199 1
4 HD 218396d Pl 23 07 28.7156905667 +21 08 03.302133882           ~ 171 1
5 HD 218396c Pl 23 07 28.7156905667 +21 08 03.302133882           ~ 187 1
6 HD 218396e Pl 23 07 28.7156905667 +21 08 03.302133882           ~ 124 1

    Equat.    Gal    SGal    Ecl

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2020.07.04-02:36:43

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