E-viri
Recenzirano
Odprti dostop
-
Bond, I. A; Bennett, D. P; Sumi, T; Udalski, A; Suzuki, D; Rattenbury, N. J; Bozza, V; Koshimoto, N; Abe, F; Asakura, Y; Barry, R. K; Bhattacharya, A; Donachie, M; Evans, P; Fukui, A; Hirao, Y; Itow, Y; Li, M. C. A; Ling, C. H; Masuda, K; Matsubara, Y; Muraki, Y; Nagakane, M; Ohnishi, K; Ranc, C; Saito, To; Sharan, A; Sullivan, D. J; Tristram, P. J; Yamada, T; Yamada, T; Yonehara, A; Skowron, J; Szymański, M. K; Poleski, R; Mróz, P; Soszyński, I; Pietrukowicz, P; Kozłowski, S; Ulaczyk, K; Pawlak, M
Monthly Notices of the Royal Astronomical Society, 08/2017, Letnik: 469, Številka: 2Journal Article
Abstract We report discovery of the lowest mass ratio exoplanet to be found by the microlensing method in the light curve of the event OGLE 2016–BLG–1195. This planet revealed itself as a small deviation from a microlensing single lens profile from an examination of the survey data. The duration of the planetary signal is ∼2.5 h. The measured ratio of the planet mass to its host star is q = 4.2 ± 0.7 × 10−5. We further estimate that the lens system is likely to comprise a cold ∼3 Earth mass planet in an ∼2 au wide orbit around a 0.2 Solar mass star at an overall distance of 7.1 kpc.
Avtor
Vnos na polico
Trajna povezava
- URL:
Faktor vpliva
Dostop do baze podatkov JCR je dovoljen samo uporabnikom iz Slovenije. Vaš trenutni IP-naslov ni na seznamu dovoljenih za dostop, zato je potrebna avtentikacija z ustreznim računom AAI.
Leto | Faktor vpliva | Izdaja | Kategorija | Razvrstitev | ||||
---|---|---|---|---|---|---|---|---|
JCR | SNIP | JCR | SNIP | JCR | SNIP | JCR | SNIP |
Baze podatkov, v katerih je revija indeksirana
Ime baze podatkov | Področje | Leto |
---|
Povezave do osebnih bibliografij avtorjev | Povezave do podatkov o raziskovalcih v sistemu SICRIS |
---|
Vir: Osebne bibliografije
in: SICRIS
To gradivo vam je dostopno v celotnem besedilu. Če kljub temu želite naročiti gradivo, kliknite gumb Nadaljuj.