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WASP-101 b
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CPD-23 1329
Stellar parameters and planets on the system

Host Star: CPD-23 1329 CPD-23 1329 System planets
RA 98.35111
Teff 6400
Radius 1.29
Mass 1.34
DEC -23.486193
Spectral Type EU F6
V Mag 10.3
I Mag 0
Distance 0
J Mag 0
H Mag 0
K Mag 0
Planet Name Planet Mass Planet Radius Semi Major Axis Orbital Period Eccentricity Inclination
WASP-101 b 0.5 1.41 0.0506 3.585722 0 85
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-101 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-101 b 0.5 1.41 0.0506 3.585722 0 85 0 2456164.6934 1560 0

Direct access and visualization for NASA archive

 

SHOW ERRORBARS Y/N

RefTypeFacilityInstrum.NptComments
Wakeford et al. 2017 spec Hubble Space Telescope satelliteWide Field Camera 315WAKEFORD ET AL 2017 Observations of WASP-101 were conducted with HST WFC3 G141 grism as part of the HST PanCET program GO-14767 (PIs Sing and Lopez-Morales) on October 2nd 2016. Observations were conducted in forward spatial scan mode, using the 512 x 512 subarray, in SPARS25, wih 7 reads per exposure, resulting in a exposure time of 138.38 seconds. We use a scan rate of 0.65 pixels per seconds with a final spatial scan covering 90 pixels in the cross-dispersion directionon the detector. This results in a maximun count rate of 22000 e per pixel, which is quite low but importantly does not enter the non-linearity regime of the detector. We use the IMA output files from the CalWF3 pipeline.
Exoplanets-A (CASCADe) spec HSTWFC325Exoplanets-A reduction
CASCADE v. 1.0.0
Created:2021_2_18:7_22_26
Obs.Type:transit
Transit models (Exoplanets-A: CASCADe reduction):