دورية أكاديمية
No random transits in CHEOPS observations of HD 139139
العنوان: | No random transits in CHEOPS observations of HD 139139 |
---|---|
المؤلفون: | Alonso, R., Hoyer, S., Deleuil, M., Simon, A. E., Beck, M., Benz, W., Florén, H. -G., Guterman, P., Borsato, L., Brandeker, A., Gandolfi, D., Wilson, T. G., Zingales, T., Alibert, Y., Anglada, G., Bárczy, T., Barrado Navascues, D., S. C. C. Barros, Baumjohann, W., Beck, T., Billot, N., Bonfils, X., Broeg, Ch., Charnoz, S., Collier Cameron, A., Corral van Damme, C., Sz., Csizmadia, Cubillos, P. E., Davies, M. B., Deline, A., Delrez, Laetitia, O. D. S. Demangeon, Demory, B. -O., Ehrenreich, D-, Erikson, A., Fortier, A., Fossati, L., Fridlund, M., Gillon, Michaël, Güdel, M., Günther, M. N., Heitzmann, A., Helling, Ch., Isaak, K. G., Kiss, L. L., Kopp, E., K. W. F. Lam, Laskar, J., Lecavelier des Etangs, A., Lendl, M., Magrin, D., P. F. L. Maxted, Mordasini, Ch., Nascimbeni, V., Olofsson, G., Ottensamer, R., Pagano, I., Pallé, E., Peter, G., Piotto, G., Pollacco, D., Queloz, D., Ragazzoni, R., Rando, N., Rauer, H., Ribas, I., Santos, N. C., Scandariato, G., Ségransan, D., A. M. S. Smith, Sousa, S. G., Stalport, Manu, Szabó, Gy. M., Thomas, N., Udry, S., Ulmer, B., Van Grootel, Valérie, Venturini, J., Verrecchia, F., Walton, N. A. |
المصدر: | Astronomy and Astrophysics, 680, A78 (2023-12) |
بيانات النشر: | EDP Sciences |
سنة النشر: | 2023 |
المجموعة: | University of Liège: ORBi (Open Repository and Bibliography) |
مصطلحات موضوعية: | astro-ph.EP, astro-ph.SR, Space and Planetary Science, Astronomy and Astrophysics, Physical, chemical, mathematical & earth Sciences, Space science, astronomy & astrophysics, Physique, chimie, mathématiques & sciences de la terre, Aérospatiale, astronomie & astrophysique |
الوصف: | peer reviewed ; HD 139139 (a.k.a. 'The Random Transiter') is a star that exhibited enigmatic transit-like features with no apparent periodicity in K2 data. The shallow depth of the events ($\sim$200 ppm -- equivalent to transiting objects with radii of $\sim$1.5 R$_\oplus$ in front of a Sun-like star), and their non-periodicity, constitutes a challenge for the photometric follow-up of this star. The goal of this study is to confirm with independent measurements the presence of shallow, non-periodic transit-like features on this object. We performed observations with CHEOPS, for a total accumulated time of 12.75 d, distributed in visits of roughly 20 h in two observing campaigns in years 2021 and 2022. The precision of the data is sufficient to detect 150 ppm features with durations longer than 1.5 h. We use the duration and times of the events seen in the K2 curve to estimate how many should have been detected in our campaigns, under the assumption that their behaviour during the CHEOPS observations would be the same as in the K2 data of 2017. We do not detect events with depths larger than 150 ppm in our data set. If the frequency, depth, and duration of the events were the same as in the K2 campaign, we estimate the probability of having missed all events due to our limited observing window would be 4.8 %. We suggest three different scenarios to explain our results: 1) Our observing window was not long enough, and the events were missed with the estimated 4.8 % probability. 2) The events recorded in the K2 observations were time critical, and the mechanism producing them was either not active in the 2021 and 2022 campaigns or created shallower events under our detectability level. 3) The enigmatic events in the K2 data are the result of an unidentified and infrequent instrumental noise in the original data set or its data treatment. |
نوع الوثيقة: | article in journal/newspaper |
اللغة: | English |
تدمد: | 0004-6361 1432-0746 |
العلاقة: | https://www.aanda.org/10.1051/0004-6361/202347779/pdfTest; urn:issn:0004-6361; urn:issn:1432-0746; https://orbi.uliege.be/handle/2268/310094Test; info:hdl:2268/310094; https://orbi.uliege.be/bitstream/2268/310094/1/2310.10332.pdfTest; scopus-id:2-s2.0-85180601746; arXiV:2310.10332v2 |
DOI: | 10.1051/0004-6361/202347779 |
الإتاحة: | https://doi.org/10.1051/0004-6361/202347779Test https://doi.org/10.1051/0004-6361/202347779/pdfTest https://orbi.uliege.be/handle/2268/310094Test https://orbi.uliege.be/bitstream/2268/310094/1/2310.10332.pdfTest |
حقوق: | open access ; http://purl.org/coar/access_right/c_abf2Test ; info:eu-repo/semantics/openAccess |
رقم الانضمام: | edsbas.CDD6F2C9 |
قاعدة البيانات: | BASE |
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A.</searchLink> ) Array ( [Name] => TitleSource [Label] => Source [Group] => Src [Data] => Astronomy and Astrophysics, 680, A78 (2023-12) ) Array ( [Name] => Publisher [Label] => Publisher Information [Group] => PubInfo [Data] => EDP Sciences ) Array ( [Name] => DatePubCY [Label] => Publication Year [Group] => Date [Data] => 2023 ) Array ( [Name] => Subset [Label] => Collection [Group] => HoldingsInfo [Data] => University of Liège: ORBi (Open Repository and Bibliography) ) Array ( [Name] => Subject [Label] => Subject Terms [Group] => Su [Data] => <searchLink fieldCode="DE" term="%22astro-ph%2EEP%22">astro-ph.EP</searchLink><br /><searchLink fieldCode="DE" term="%22astro-ph%2ESR%22">astro-ph.SR</searchLink><br /><searchLink fieldCode="DE" term="%22Space+and+Planetary+Science%22">Space and Planetary Science</searchLink><br /><searchLink fieldCode="DE" term="%22Astronomy+and+Astrophysics%22">Astronomy and Astrophysics</searchLink><br /><searchLink fieldCode="DE" term="%22Physical%22">Physical</searchLink><br /><searchLink fieldCode="DE" term="%22chemical%22">chemical</searchLink><br /><searchLink fieldCode="DE" term="%22mathematical+%26+earth+Sciences%22">mathematical & earth Sciences</searchLink><br /><searchLink fieldCode="DE" term="%22Space+science%22">Space science</searchLink><br /><searchLink fieldCode="DE" term="%22astronomy+%26+astrophysics%22">astronomy & astrophysics</searchLink><br /><searchLink fieldCode="DE" term="%22Physique%22">Physique</searchLink><br /><searchLink fieldCode="DE" term="%22chimie%22">chimie</searchLink><br /><searchLink fieldCode="DE" term="%22mathématiques+%26+sciences+de+la+terre%22">mathématiques & sciences de la terre</searchLink><br /><searchLink fieldCode="DE" term="%22Aérospatiale%22">Aérospatiale</searchLink><br /><searchLink fieldCode="DE" term="%22astronomie+%26+astrophysique%22">astronomie & astrophysique</searchLink> ) Array ( [Name] => Abstract [Label] => Description [Group] => Ab [Data] => peer reviewed ; HD 139139 (a.k.a. 'The Random Transiter') is a star that exhibited enigmatic transit-like features with no apparent periodicity in K2 data. The shallow depth of the events ($\sim$200 ppm -- equivalent to transiting objects with radii of $\sim$1.5 R$_\oplus$ in front of a Sun-like star), and their non-periodicity, constitutes a challenge for the photometric follow-up of this star. The goal of this study is to confirm with independent measurements the presence of shallow, non-periodic transit-like features on this object. We performed observations with CHEOPS, for a total accumulated time of 12.75 d, distributed in visits of roughly 20 h in two observing campaigns in years 2021 and 2022. The precision of the data is sufficient to detect 150 ppm features with durations longer than 1.5 h. We use the duration and times of the events seen in the K2 curve to estimate how many should have been detected in our campaigns, under the assumption that their behaviour during the CHEOPS observations would be the same as in the K2 data of 2017. We do not detect events with depths larger than 150 ppm in our data set. If the frequency, depth, and duration of the events were the same as in the K2 campaign, we estimate the probability of having missed all events due to our limited observing window would be 4.8 %. We suggest three different scenarios to explain our results: 1) Our observing window was not long enough, and the events were missed with the estimated 4.8 % probability. 2) The events recorded in the K2 observations were time critical, and the mechanism producing them was either not active in the 2021 and 2022 campaigns or created shallower events under our detectability level. 3) The enigmatic events in the K2 data are the result of an unidentified and infrequent instrumental noise in the original data set or its data treatment. ) Array ( [Name] => TypeDocument [Label] => Document Type [Group] => TypDoc [Data] => article in journal/newspaper ) Array ( [Name] => Language [Label] => Language [Group] => Lang [Data] => English ) Array ( [Name] => ISSN [Label] => ISSN [Group] => ISSN [Data] => 0004-6361<br />1432-0746 ) Array ( [Name] => NoteTitleSource [Label] => Relation [Group] => SrcInfo [Data] => https://www.aanda.org/10.1051/0004-6361/202347779/pdf; urn:issn:0004-6361; urn:issn:1432-0746; https://orbi.uliege.be/handle/2268/310094; info:hdl:2268/310094; https://orbi.uliege.be/bitstream/2268/310094/1/2310.10332.pdf; scopus-id:2-s2.0-85180601746; arXiV:2310.10332v2 ) Array ( [Name] => DOI [Label] => DOI [Group] => ID [Data] => 10.1051/0004-6361/202347779 ) Array ( [Name] => URL [Label] => Availability [Group] => URL [Data] => https://doi.org/10.1051/0004-6361/202347779<br />https://doi.org/10.1051/0004-6361/202347779/pdf<br />https://orbi.uliege.be/handle/2268/310094<br />https://orbi.uliege.be/bitstream/2268/310094/1/2310.10332.pdf ) Array ( [Name] => Copyright [Label] => Rights [Group] => Cpyrght [Data] => open access ; http://purl.org/coar/access_right/c_abf2 ; info:eu-repo/semantics/openAccess ) Array ( [Name] => AN [Label] => Accession Number [Group] => ID [Data] => edsbas.CDD6F2C9 ) |
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