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WASP-43 b
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GSC 05490-00141
Stellar parameters and planets on the system

Host Star: GSC 05490-00141 GSC 05490-00141 System planets
RA 154.90837
Teff 4520
Radius 0.667
Mass 0.717
DEC -9.806275
Spectral Type EU K7V
V Mag 12.4
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-43 b 2.052 1.036 0.01526 0.81347753 0.0035 82.33
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-43 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-43 b 2.052 1.036 0.01526 0.81347753 0.0035 82.33 0 2455726.54336 0 C, CH4, CO, CO2, H2O, NH3, O I 0

Direct access and visualization for NASA archive

 

SHOW ERRORBARS Y/N

 

SHOW ERRORBARS Y/N

RefTypeFacilityInstrum.NptComments
Chen et al. 2014 spec Max Planck Gesellschaft 2.2 meter Telescope at European Southern ObservatoryGROND7CHEN ET AL 2014 We observed one primary transit and one secondary eclipse events of WASP-43b with the GROND instrument mounted on the MPG/ESO 2.2-meter telescope at La Silla in Chile. GROND is an imaging instrument primarily designed for the investigation of gamma-ray burst afterglows and other transients simultaneously in seven bands: Sloan g′,r′,i′,z′and near-infrared J,H,K.
Hoyer et al. 2016 phot LCOGT 1m telescope at Cerro Tololo Inter-American ObservatorySinistro2HOYER ET AL 2016 Of these, 6 events were observed simultaneously in the i' and g' filters with the 1.0-m LCOGT Network, other two transits were observed only with the g' or the i' filter also at the 1.0-m LCOGT
Hoyer et al. 2016 phot Observatorio del Teides 0.8 meter TelescopeCAMELOT1HOYER ET AL 2016 The transit at IAC80 telescope was observed using the CAMELOT instrument. CAMELOT has a collector area of 2048 x 2048 pixels 2 with two readout amplifier channels, a FoV of 10.4 x 10.4 arcmin 2 and a pixel scale of 0.304 arcsec. The observation was performed using the 500 KHz read-out speed in both channels without binning, having thus a readout time of 4.4s TABLE 1 doc https://arxiv.org/pdf/1603.01144.pdf
Kreidberg et al. 2014 spec Hubble Space Telescope satelliteWide Field Camera 322KREIDBERG ET AL 2014 We observed three full-orbit phase curves, three primary transits, and two secondary eclipses of WASP-43b with 61 HST orbits. During the observations, we obtained low-resolution time series spectroscopy with the WFC3 G141 grism over the wavelength range 1.1 to 1.7μm.
Murgas et al. 2014 spec Gran Telescopio CANARIAS 10.4m telescopeOSIRIS36MURGAS ET AL 2014 We used OSIRIS in its long-slit spectroscopic mode, selecting the grism R1000R which covers the spectral range of 520-1040 nm, and a custom built slit of 12 arc-sec of width. With such a wide slit, the spectral resolution is dominated by the seeing during the observations, which varied between 0.8 and 1.8 arcsec. This translates in an effective spectral resolution of R=374-841 at 751 nm.
Ricci et al. 2015 phot Observatorio Astronomico Nacionals 0.84m TelescopeMexman3RICCI ET AL 2015 WASP-43b was observed in V R I with the 2.12m telescope and in the i filter with the robotic 1.50m telescope
Ricci et al. 2015 phot Observatorio Astronomico Nacionals Harold Johnson TelescopeRATIR1RICCI ET AL 2015 WASP-43b was observed in V R I with the 2.12m telescope and in the i filter with the robotic 1.50m telescope
Exoplanets-A (CASCADe) spec HSTWFC325Exoplanets-A reduction
CASCADE v. 1.0.0
Created:2021_2_18:15_48_25
Obs.Type:transit
Exoplanets-A (CASCADe) spec HSTWFC325Exoplanets-A reduction
CASCADE v. 1.0.0
Created:2021_2_18:15_51_7
Obs.Type:eclipse
Transit models (Exoplanets-A: CASCADe reduction):

Eclipse models (Exoplanets-A: CASCADe reduction):