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-32 b
<- Back to Exoplanets DataBase

TYC 3281-800-1
Stellar parameters and planets on the system

Host Star: TYC 3281-800-1 TYC 3281-800-1 System planets
RA 31.04283
Teff 6001
Radius 1.387
Mass 1.176
DEC 46.68784
Spectral Type EU F/G
V Mag 11.29
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-32 b 0.86 1.789 0.0343 2.150008 0.0072 88.9
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 TYC 3281-800-1

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

HAT-P-32 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-32 b 0.86 1.789 0.0343 2.150008 0.0072 88.9 0.000108 2455855.57877 0 320

Direct access and visualization for NASA archive

 

SHOW ERRORBARS Y/N

 

SHOW ERRORBARS Y/N

RefTypeFacilityInstrum.NptComments
Gibson et al. 2013 spec Gillett Gemini North TelescopeGMOS29GIBSON ET AL 2013 Observations used the R400 grism + OG515 filter with a central wavelength of 725 nm in 2 x 2 binning. The dispersion is 0.14 nm per (binned) pixel, giving wavelength coverage from about 510 to 930 nm
Mallonn & Strassmeier 2016 spec Large Binocular Telescope ObservatoryMODS12MALLONN AMP STRASSMEIER 2016 We observed a transit of the inflated hot Jupiter HAT-P-32b with the Multi-Object Double Spectrograph atthe Large Binocular Telescope to characterize its atmosphere from 3300 to 10000
Mallonn et al. 2016 phot Calar Alto Observatorys 2.2 meter TelescopeBUSCA1One transit was observed with BUSCA, the four-channel imager at the Calar Alto Observatory 2.2 m telescope. Table 3 Filter I
Mallonn et al. 2016 phot Fred Lawrence Whipple Observatorys 1.2 meter TelescopeKeplerCam1MALLONN ET 2016 table 3 Filter z prime
Mallonn et al. 2016 phot Isaac Newton Groups William Herschel TelescopeULTRACAM2MALLONN ET 2016 table 3 Filter u prime, NaI
Mallonn et al. 2016 phot Multiple ObservatoriesMultiple Instruments5MALLONN ET 2016 Table 3 Filter B, g prime + Gunn g , V , r prime + Gunn r, R
Nortmann et al. 2016 spec Gran Telescopio CANARIAS 10.4m telescopeOSIRIS20NORTMANN ET AL 2016 We observed HAT-P-32Ab twice during transit on 2012 September 15 (JD 2456185.5, Run 1) and on 2012 September 30 (JD 2456200.5, Run 2) with the OSIRIS instrument. We chose the method of long slit spec-troscopy, in which the planet host star and a suitable referencestar are both placed inside one long slit. The grism R1000R was used to disperse the light over the range from 518 to 918 nm
Exoplanets-A (CASCADe) spec HSTWFC325Exoplanets-A reduction
CASCADE v. 1.0.0
Created:2021_2_18:11_31_53
Obs.Type:transit
Exoplanets-A (CASCADe) spec HSTWFC325Exoplanets-A reduction
CASCADE v. 1.0.0
Created:2021_2_18:11_32_50
Obs.Type:eclipse
Transit models (Exoplanets-A: CASCADe reduction):

Eclipse models (Exoplanets-A: CASCADe reduction):