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Table 3
List of observations of β Pic b used for our simulations.
Instrument | Band | Technique | Wavelength (µm) | R | Reference |
---|---|---|---|---|---|
VLT/SPHERE/IFS | Y–H | LRS | 0.96–1.63 | 30 | … |
VLTI/GRAVITY | K | LRS | 1.97–2.49 | 500 | Nowak et al. (2020) |
VLT/SINFONI | K | MRCCS | 2.09–2.45 | 4000 | Hoeijmakers et al. (2018) |
LCO/VisAO | Ys | PHOT | 0.99 | … | Males et al. (2014) |
VLT/NACO | J | PHOT | 1.28 | … | Currie et al. (2013) |
Gemini/NICI | ED286 | PHOT | 1.59 | … | Males et al. (2014) |
VLT/NACO | H | PHOT | 1.67 | … | Currie et al. (2013) |
VLT/SPHERE/IRDIS | K12.1 | PHOT | 2.11 | … | Lagrange et al. (2020) |
VLT/NACO | Ks | PHOT | 2.15 | … | Bonnefoy et al. (2011) |
VLT/SPHERE/IRDIS | K12.2 | PHOT | 2.26 | … | Lagrange et al. (2020) |
VLT/NACO | NB374 | PHOT | 3.74 | … | Stolker et al. (2020) |
VLT/NACO | Lp | PHOT | 3.81 | … | Stolker et al. (2019) |
VLT/NACO | NB405 | PHOT | 4.07 | … | Stolker et al. (2020) |
VLT/NACO | Mp | PHOT | 4.79 | … | Stolker et al. (2019) |
Notes. The VLT/SPHERE/IFS spectrum is not public and therefore we do not put a reference next to it, however we do refer to Langlois et al. (2021) to estimate the errorbars of our synthetic spectra.
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