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WASP-52 b
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WASP-52
Stellar parameters and planets on the system

Host Star: WASP-52 WASP-52 System planets
RA 348.49484
Teff 5000
Radius 0.79
Mass 0.87
DEC 8.761278
Spectral Type EU K2V
V Mag 12
I Mag 0
Distance 140
J Mag 0
H Mag 0
K Mag 0
Planet Name Planet Mass Planet Radius Semi Major Axis Orbital Period Eccentricity Inclination
WASP-52 b 0.46 1.27 0.0272 1.7497798 0 85.35
Photosferic properties via VOSA

Photometric data catalogues and tools:

TESS OBSERVATIONS

No observations availables in Tess archives for this object (yet)

Spectroscopic data catalogues:

 

OHP archives:
Available observations data for WASP-52

Spectra timeseries observations in SOPHIE OHP archive.

Cross correlation functions in SOPHIE archive, with Radial velocity

List of Spectra timeseries observations in ELODIE archive

Cross correlation functions in ELODIE archive, with Radial velocity

La Palma, CAHA, Keck, ESO archives

WASP-52 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-52 b 0.46 1.27 0.0272 1.7497798 0 85.35 0 2455793.68143 0 Na 140

Direct access and visualization for NASA archive

 

SHOW ERRORBARS Y/N

RefTypeFacilityInstrum.NptComments
Chen et al. 2017 spec Gran Telescopio CANARIAS 10.4m telescopeOSIRIS26CHEN ET AL 2017 We observed one transit of the hot Jupiter WASP-52b on thenight of August 28, 2015, using the Optical System for Imag-ing and low-Intermediate-Resolution Integrated Spectroscopy(OSIRIS; Sánchez et al. 2012) mounted at the Nasmyth-B fo-cal station of the GTC.
Louden et al. 2017 spec Isaac Newton Groups William Herschel TelescopeACAM19LOUDEN ET AL 2017 WASP-52 was observed for 2 full nights on August 22 and 29th 2014 using the auxiliary-port camera (ACAM) on the William Herschel Telescope (WHT). ACAM was used in single slit spectroscopy mode with a custom made extra wideslit of 27”. A slit of 27” arcseconds was chosen after an earlier analysis of the Point Spread Function (PSF) of the instrument in an earlier dataset, with the goal of there being less than 0.1%slit losses
Exoplanets-A (CASCADe) spec HSTWFC325Exoplanets-A reduction
CASCADE v. 1.0.0
Created:2021_2_18:11_21_46
Obs.Type:transit
Transit models (Exoplanets-A: CASCADe reduction):