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TrES-4 b
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NAME TrES-4 Parent Star
Stellar parameters and planets on the system

Host Star: NAME TrES-4 Parent Star NAME TrES-4 Parent Star System planets
RA 268.3044
Teff 6200
Radius 1.798
Mass 1.388
DEC 37.211765
Spectral Type EU F
V Mag 11.592
I Mag 0
Distance 479
J Mag 0
H Mag 0
K Mag 0
Planet Name Planet Mass Planet Radius Semi Major Axis Orbital Period Eccentricity Inclination
TrES-4 b 0.917 1.706 0.05084 3.5539268 0 82.81
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: 17001256119

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

Auxiliary Products:


tess2019199201929-s0014-s0026-0000000159742538-00353_dvm.pdf
tess2019199201929-s0014-s0026-0000000159742538-00353_dvr.pdf
tess2019199201929-s0014-s0026-0000000159742538-01-00353_dvs.pdf
Observation id: 17001133786

Plot from LIGHTCURVE FITS file


Auxiliary Products:


tess2020135030118-s0025-s0025-0000000159742538-00344_dvm.pdf
tess2020135030118-s0025-s0025-0000000159742538-00344_dvr.pdf
tess2020135030118-s0025-s0025-0000000159742538-01-00344_dvs.pdf

TrES-4 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
TrES-4 b 0.917 1.706 0.05084 3.5539268 0 82.81 0.000106 2454230.90524 0 479

Direct access and visualization for NASA archive

 

SHOW ERRORBARS Y/N

RefTypeFacilityInstrum.NptComments
Ranjan et al. 2014 spec Hubble Space Telescope satelliteWFC310RANJAN ET AL 2014 We probe the structure and composition of the atmospheres of 5 hot Jupiter exoplanets using the Hubble Space Telescope Wide Field Camera 3 (WFC3) instrument. We use the G141 grism (1.1-1.7 microns) to study TrES-2b, TrES-4b, and CoRoT-1b in transit, TrES-3b in secondary eclipse, and WASP-4b in both. This wavelength region includes a predicted absorption feature from water at 1.4 microns, which we expect to be non degenerate with the other molecules that are likely to be abundant for hydrocarbon-poor (e.g. solar composition) hot Jupiter atmospheres. We divide our wavelength regions into 10 bins. For each bin we produce a spectrophotometric light curve spanning the time of transit and/or eclipse. We correct these light curves for instrumental systematics without reference to an instrument model.
Exoplanets-A (CASCADe) spec HSTWFC325Exoplanets-A reduction
CASCADE v. 1.0.0
Created:2021_2_28:10_45_31
Obs.Type:transit
Transit models (Exoplanets-A: CASCADe reduction):