Systematic KMTNet Planetary Anomaly Search. VIII. Complete Sample of 2019 Subprime Field Planets

Simple item page
aut.relation.endpage226
aut.relation.issue6
aut.relation.journalAstronomical Journal
aut.relation.startpage226
aut.relation.volume165
dc.contributor.authorJung, YK
dc.contributor.authorZang, W
dc.contributor.authorWang, H
dc.contributor.authorHan, C
dc.contributor.authorGould, A
dc.contributor.authorUdalski, A
dc.contributor.authorZhu, W
dc.contributor.authorAlbrow, MD
dc.contributor.authorChung, SJ
dc.contributor.authorHwang, KH
dc.contributor.authorRyu, YH
dc.contributor.authorShin, IG
dc.contributor.authorShvartzvald, Y
dc.contributor.authorYang, H
dc.contributor.authorYee, JC
dc.contributor.authorCha, SM
dc.contributor.authorKim, DJ
dc.contributor.authorKim, SL
dc.contributor.authorLee, CU
dc.contributor.authorLee, DJ
dc.contributor.authorLee, Y
dc.contributor.authorPark, BG
dc.contributor.authorPogge, RW
dc.contributor.authorMaoz, D
dc.contributor.authorSzymański, MK
dc.contributor.authorSkowron, J
dc.contributor.authorPoleski, R
dc.contributor.authorSoszyński, I
dc.contributor.authorPietrukowicz, P
dc.contributor.authorKozłowski, S
dc.contributor.authorUlaczyk, K
dc.contributor.authorRybicki, KA
dc.contributor.authorIwanek, P
dc.contributor.authorWrona, M
dc.contributor.authorPorritt, I
dc.contributor.authorGreen, J
dc.contributor.authorHennerley, S
dc.contributor.authorMarmont, A
dc.contributor.authorMao, S
dc.contributor.authorNatusch, T
dc.contributor.authorPenny, MT
dc.contributor.authorNatusch, T
dc.date.accessioned2023-05-30T02:37:13Z
dc.date.available2023-05-30T02:37:13Z
dc.date.issued2023-05-04
dc.description.abstractWe complete the publication of all microlensing planets (and “possible planets”) identified by the uniform approach of the KMT AnomalyFinder system in the 21 KMT subprime fields during the 2019 observing season, namely, KMT-2019-BLG-0298, KMT-2019-BLG-1216, KMT-2019-BLG-2783, OGLE-2019-BLG-0249, and OGLE-2019-BLG-0679 (planets), as well as OGLE-2019-BLG-0344 and KMT-2019-BLG-0304 (possible planets). The five planets have mean log mass ratio measurements of (−2.6, −3.6, −2.5, −2.2, −2.3), median mass estimates of (1.81, 0.094, 1.16, 7.12, 3.34) M Jup, and median distance estimates of (6.7, 2.7, 5.9, 6.4, 5.6) kpc, respectively. The main scientific interest of these planets is that they complete the AnomalyFinder sample for 2019, which has a total of 25 planets that are likely to enter the statistical sample. We find statistical consistency with the previously published 33 planets from the 2018 AnomalyFinder analysis according to an ensemble of five tests. Of the 58 planets from 2018-2019, 23 were newly discovered by AnomalyFinder. Within statistical precision, half of the planets have caustic crossings, while half do not; an equal number of detected planets result from major- and minor-image light-curve perturbations; and an equal number come from KMT prime fields versus subprime fields.
dc.identifier.citationAstronomical Journal, ISSN: 0004-6256 (Print); 1538-3881 (Online), American Astronomical Society, 165(6), 226-226. doi: 10.3847/1538-3881/accb8f
dc.identifier.doi10.3847/1538-3881/accb8f
dc.identifier.issn0004-6256
dc.identifier.issn1538-3881
dc.identifier.urihttps://hdl.handle.net/10292/16201
dc.publisherAmerican Astronomical Society
dc.relation.urihttps://iopscience.iop.org/article/10.3847/1538-3881/accb8f
dc.rights.accessrightsOpenAccess
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/
dc.subject5109 Space Sciences
dc.subject51 Physical Sciences
dc.subject0201 Astronomical and Space Sciences
dc.subjectAstronomy & Astrophysics
dc.subject5101 Astronomical sciences
dc.subject5107 Particle and high energy physics
dc.titleSystematic KMTNet Planetary Anomaly Search. VIII. Complete Sample of 2019 Subprime Field Planets
dc.typeJournal Article
pubs.elements-id507061
Files
Original bundle
Now showing 1 - 1 of 1
Thumbnail Image
Name:
Jung_2023_AJ_165_226.pdf
Size:
5.21 MB
Format:
Adobe Portable Document Format
Description:
Journal article
Download
Collections
School of Engineering, Computer and Mathematical Sciences - Te Kura Mātai Pūhanga, Rorohiko, Pāngarau