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WASP-29 b
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TYC 8015-1020-1
Stellar parameters and planets on the system

Host Star: TYC 8015-1020-1 TYC 8015-1020-1 System planets
RA 357.87952
Teff 4800
Radius 0.846
Mass 0.825
DEC -39.90674
Spectral Type EU K4V
V Mag 11.3
I Mag 0
Distance 80
J Mag 0
H Mag 0
K Mag 0
Planet Name Planet Mass Planet Radius Semi Major Axis Orbital Period Eccentricity Inclination
WASP-29 b 0.2428971463 0.8412897516 0.0457 3.922727 0.03 88.8
Photosferic properties via VOSA

Photometric data catalogues and tools:

TESS OBSERVATIONS

Light curve files contain flux time series data and are produced for each target using simple aperture photometry. These are used to search for transiting planets and other astrophysical phenomena. The flux and uncertainties are provided at each cadence, with NaNs filling in any missing data values. TESS light curves are FITS format files that contain the output of the photometric extraction and subsequent systematics removal (cotrending) performed by the SPOC algorithms. A single light curve file contains the data for one target for on observing sector. If a target was observed in more than one TESS sector, multiple light curve files will be created but they may be made available on the MAST in separate deliveries.
Here there are the plotted Light Curves from each Observation Fits file whit the Data validation auxiliary products created by the Tess pipeline.

WASP-29 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-29 b 0.2428971463 0.8412897516 0.0457 3.922727 0.03 88.8 0.000571 2455320.2431 0 80

Direct access and visualization for NASA archive

 

SHOW ERRORBARS Y/N

RefTypeFacilityInstrum.NptComments
Gibson et al. 2013 spec Gemini South TelescopeGMOS15
Exoplanets-A (CASCADe) spec HSTWFC325Exoplanets-A reduction
CASCADE v. 1.0.0
Created:2021_2_20:15_22_15
Obs.Type:transit
Transit models (Exoplanets-A: CASCADe reduction):