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WASP-80 b
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TYC 5165-481-1
Stellar parameters and planets on the system

Host Star: TYC 5165-481-1 TYC 5165-481-1 System planets
RA 303.16736
Teff 4145
Radius 0.63
Mass 0.58
DEC -2.1442206
Spectral Type EU K7V
V Mag 11.881
I Mag 10.279
Distance 60
J Mag 9.218
H Mag 8.513
K Mag 8.351
Planet Name Planet Mass Planet Radius Semi Major Axis Orbital Period Eccentricity Inclination
WASP-80 b 0.554 0.952 0.0346 3.0678504 0.07 89.92
Photosferic properties via VOSA

Photometric data catalogues and tools:

TESS OBSERVATIONS

No observations availables in Tess archives for this object (yet)

Spectroscopic data catalogues:

 

OHP archives:
Available observations data for TYC 5165-481-1

Spectra timeseries observations in SOPHIE OHP archive.

Cross correlation functions in SOPHIE archive, with Radial velocity

List of Spectra timeseries observations in ELODIE archive

Cross correlation functions in ELODIE archive, with Radial velocity

La Palma, CAHA, Keck, ESO archives

WASP-80 b
Planet parameters

Planet Name Planet Mass Planet Radius Semi Major Axis Orbital Period Eccentricity Inclination Tidally Locked Angular Distance Primary Transit Source (JD) Calculated Planet Temperature(K) Molecules Star Distance
WASP-80 b 0.554 0.952 0.0346 3.0678504 0.07 89.92 0 2456125.41751 0 CH4, CO, H, H2O, He, K, Na 60

Direct access and visualization for NASA archive

 

SHOW ERRORBARS Y/N

RefTypeFacilityInstrum.NptComments
Fukui et al. 2014 phot Infrared Survey FacilitySIRIUS9FUKUI ET AL 2014 :We observed three primary transits of WASP-80b with the Simultaneous Infrared Imager for Unbiased Survey camera mounted on the Infrared Survey Facility (IRSF) 1.4 m telescope at the South African Astronomical Observatory on 2013 July 16, August 22, and October 7 (UT). SIRIUS has three detectors, enabling us to obtain J- ,H- , and Ks- band images simultaneously
Fukui et al. 2014 phot National Astronomical Observatory of Japans Okayama Astrophysical Observatory 0.5m Telescope6FUKUKI ET AL 2014 We observed two primary transits of WASP-80b by simultaneously using two instruments at Okayama Astrophysical Observatory (OAO) on 2013 August 13 and September 22 (UT); One is the NIR imaging and spectroscopic instrument ISLE (Yanagisawa et al. 2006, 2008) mounted on the 188 cm cope and the other is a multicolor imager mounted on the 50 cm telescope which is one of Multicolor Imaging Telescopes for Survey and Monstrous Explosions (MITSuME;Kotani et al. 2005; Yanagisawa et al. 2010). We used J-band filter and set the exposure time to 45 s on both nights.
Fukui et al. 2014 phot National Astronomical Observatory of Japans Okayama Astrophysical Observatory 1.88m TelescopeISLE2KIRK ET AL 2018 Two transits of WASP-80b were observed on the nights of2016 August 18 and 2016 August 21 using the ACAM instrument
Kirk et al. 2018 spec Isaac Newton Group William Herschel TelescopeACAM34TRIAUD ET AL 2015 : TABLE A1 : 6 Jun 2013 Danish/DFOSC Bessell I
Triaud et al. 2015 phot Danish 1.54m telescope at European Southern ObservatoryDFOSC1TRIAUD ET AL 2015 : TABLE A1 16 Jun 2013 2.2m/GROND Sloan z' 16 Jun 2013 2.2m/GROND Sloan r' 16 Jun 2013 2.2m/GROND Sloan i' 16 Jun 2013 2.2m/GROND Sloan g'
Triaud et al. 2015 phot Max Planck Gesellschaft 2.2 meter Telescope at European Southern ObservatoryGROND2TRIAUD ET AL 2015 : TABLE A1
Triaud et al. 2015 phot Multiple ObservatoriesMultiple Instruments2TRIAUD ET AL 2015 : We obtained data covering one transit and two occultations at 3.6 microns and one transit and two occultations at 4.5 microns. The scheduling of these observations was based on the orbital solution presented by Triaud et al. (2013). We used the subarray mode with exposure times of 0.4s (3.6) and 2s (4.5). The resulting sets of 64 individual subarray images were calibrated by the Spitzer pipeline version S 19.1.0 and are available on the Spitze rHeritage Archive Database
Triaud et al. 2015 phot Spitzer Space Telescope satelliteInfrared Array Camera (IRAC)2FUKUI ET AL 2014 :We observed three primary transits of WASP-80b with the Simultaneous Infrared Imager for Unbiased Survey camera mounted on the Infrared Survey Facility (IRSF) 1.4 m telescope at the South African Astronomical Observatory on 2013 July 16, August 22, and October 7 (UT). SIRIUS has three detectors, enabling us to obtain J- ,H- , and Ks- band images simultaneously
Exoplanets-A (CASCADe) spec HSTWFC325Exoplanets-A reduction
CASCADE v. 1.0.0
Created:2021_2_18:10_33_48
Obs.Type:transit
Transit models (Exoplanets-A: CASCADe reduction):