Deutsch
 
Hilfe Datenschutzhinweis Impressum
  DetailsucheBrowse

Datensatz

DATENSATZ AKTIONENEXPORT
Zur Ablage hinzufügen
 Lokale TagsFreigabegeschichteDetailsÜbersicht
  Searching for transiting cold Jupiters around bright stars with ASTEP South at Dome C, Antarctica

Crouzet, N., Mékarnia, D., Guillot, T., Bayliss, D., Deeg, H., Palle, E., et al. (2019). Searching for transiting cold Jupiters around bright stars with ASTEP South at Dome C, Antarctica. In AAS/Division for Extreme Solar Systems Abstracts.

Item is

 

einblenden: alle ausblenden: alle

Basisdaten

einblenden: ausblenden:
Datensatz-Permalink: https://hdl.handle.net/21.11116/0000-0005-D3CB-8 Versions-Permalink: https://hdl.handle.net/21.11116/0000-0005-D3CC-7
Genre: Konferenzbeitrag

Externe Referenzen

einblenden:
ausblenden:
externe Referenz:
https://ui.adsabs.harvard.edu/abs/2019ESS.....430210C (beliebiger Volltext)
Beschreibung:
-
OA-Status:

Urheber

einblenden:
ausblenden:
 Urheber:
Crouzet, Nicolas1, Autor
Mékarnia, Djamel1, Autor
Guillot, Tristan1, Autor
Bayliss, Daniel1, Autor
Deeg, Hans1, Autor
Palle, Enric1, Autor
Abe, Lyu1, Autor
Agabi, Abdelkrim1, Autor
Rivet, Jean-Pierre1, Autor
Murgas, Felipe1, Autor
Gillon, Michaël1, Autor
Delrez, Laetitia1, Autor
Jehin, Emmanuël1, Autor
Espinoza, Néstor1, Autor
Affiliations:
1Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners, ou_2421692              

Inhalt

einblenden:
ausblenden:
Schlagwörter: -
 Zusammenfassung: Much of our understanding of gas giant exoplanets come from those transiting in front of bright stars at small orbital separations (P 3 days, a 0.05 au). These hot Jupiters are coupled to their host star: stellar irradiation impacts the chemistry and temperature structure of their atmospheres and tidal interactions affects the orbital dynamics and may even impact the star itself. In contrast, gas giant exoplanets with long orbital periods and large separations (P > 30 days, a > 0.2 au) are much less coupled to their host star and provide ideal benchmarks to study gas giant planets in general. However, only a few transiting "cold Jupiters" orbiting bright stars are known to date. In the past years, we conducted the ASTEP experiment (Antarctica Search for Transiting ExoPlanets) to search and characterize transiting exoplanets from Dome C, Antarctica and to qualify this site for photometry in the visible. One instrument, ASTEP South, is a 10 cm diameter lens equipped with a CCD camera in a thermalised box pointing continuously towards the celestial South pole. We analysed four winters of data collected with this instrument and identified about 30 transit candidates around relatively bright stars (9 < V < 13) with orbital periods up to 80 days. We performed photometric follow-up with the Las Cumbres Observatory (LCO) 0.4m telescopes to investigate these signals. Most of these stars are also observed by TESS and their lightcurves can be extracted from the full frame images. In this poster, we present our set of candidates, the first results of the photometric follow-up, and discuss the use of TESS data to investigate these objects.

Details

einblenden:
ausblenden:
Sprache(n):
 Datum: 2019
 Publikationsstatus: Erschienen
 Seiten: -
 Ort, Verlag, Ausgabe: -
 Inhaltsverzeichnis: -
 Art der Begutachtung: -
 Identifikatoren: -
 Art des Abschluß: -

Veranstaltung

einblenden:
ausblenden:
Titel: AAS/Division for Extreme Solar Systems Abstracts
Veranstaltungsort: -
Start-/Enddatum: 2019

Entscheidung

einblenden:

Projektinformation

einblenden:

Quelle 1

einblenden:
ausblenden:
Titel: AAS/Division for Extreme Solar Systems Abstracts
Genre der Quelle: Konferenzband
 Urheber:
Affiliations:
Ort, Verlag, Ausgabe: -
Seiten: - Band / Heft: - Artikelnummer: - Start- / Endseite: - Identifikator: -