This project has received funding from the European Union's Seventh Framework Programme (FP7-SPACE-2013-1) for research, technological development and demonstration under grant agreement no. 606740
HAT-P-7 b
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BD+47 2846
Stellar parameters and planets on the system

Host Star: BD+47 2846 BD+47 2846 System planets
RA 292.2473
Teff 6259
Radius 2
Mass 1.51
DEC 47.96951
Spectral Type EU
V Mag 10.5
I Mag 0
Distance 320
J Mag 0
H Mag 0
K Mag 0
Planet Name Planet Mass Planet Radius Semi Major Axis Orbital Period Eccentricity Inclination
HAT-P-7 b 1.741 1.431 0.0379 2.204735471 0 84.1
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.
Observation id: 17000982027

Plot from LIGHTCURVE FITS file


Auxiliary Products:


tess2019227203528-s0015-s0015-0000000424865156-00245_dvm.pdf
tess2019227203528-s0015-s0015-0000000424865156-00245_dvr.pdf
tess2019227203528-s0015-s0015-0000000424865156-00297_dvm.pdf
tess2019227203528-s0015-s0015-0000000424865156-00297_dvr.pdf
tess2019227203528-s0015-s0015-0000000424865156-01-00245_dvs.pdf
tess2019227203528-s0015-s0015-0000000424865156-01-00297_dvs.pdf
Observation id: 17001055104

There is no LIGHTCURVE FITS file for this observation on Tess Archives

Auxiliary Products:


tess2019199201929-s0014-s0016-0000000424865156-00253_dvm.pdf
tess2019199201929-s0014-s0016-0000000424865156-00253_dvr.pdf
tess2019199201929-s0014-s0016-0000000424865156-01-00253_dvs.pdf
Observation id: 17000941028

Plot from LIGHTCURVE FITS file


Auxiliary Products:


tess2019199201929-s0014-s0014-0000000424865156-00240_dvm.pdf
tess2019199201929-s0014-s0014-0000000424865156-00240_dvr.pdf
tess2019199201929-s0014-s0014-0000000424865156-00290_dvm.pdf
tess2019199201929-s0014-s0014-0000000424865156-00290_dvr.pdf
tess2019199201929-s0014-s0014-0000000424865156-01-00240_dvs.pdf
tess2019199201929-s0014-s0014-0000000424865156-01-00290_dvs.pdf

HAT-P-7 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
HAT-P-7 b 1.741 1.431 0.0379 2.204735471 0 84.1 0.000118 2454731.68039 2121 320

Direct access and visualization for NASA archive

 

SHOW ERRORBARS Y/N

 

SHOW ERRORBARS Y/N

RefTypeFacilityInstrum.NptComments
Wong et al. 2016 phot Spitzer Space Telescope satelliteInfrared Array Camera (IRAC)2WONG ET AL 2016: We analyze full-orbit phase curve observations of the transiting hot Jupiters WASP-19b and HAT-P-7b at 3.6 and 4.5 microns obtained using the Spitzer Space Telescope.
Exoplanets-A (CASCADe) spec HSTWFC325Exoplanets-A reduction
CASCADE v. 1.0.0
Created:2021_2_28:13_21_13
Obs.Type:eclipse

Eclipse models (Exoplanets-A: CASCADe reduction):