Mass Production 2021 KMTNet Microlensing Planets. III Virtual Observatory Resource

Authors
  1. Shin I.-G.
  2. Yee J.C.
  3. Gould A.
  4. Hwang K.-H.
  5. Yang H.
  6. Bond I.A.,(the Leading Authors)
  7. Albrow M.D.
  8. Chung S.-J.
  9. Han C.
  10. Jung Y.K.,Ryu Y.-H.
  11. Shvartzvald Y.
  12. Zang W.
  13. Cha S.-M.
  14. Kim D.-J.
  15. Kim S.-L.,Lee C.-U.
  16. Lee D.-J.
  17. Lee Y.
  18. Park B.-G.
  19. Pogge R.W.,(the Kmtnet Collaboration)
  20. Abe F.
  21. Barry R.
  22. Bennett D.P.,Bhattacharya A.
  23. Fujii H.
  24. Fukui A.
  25. Hirao Y.
  26. Silva S.I.
  27. Itow Y.,Kirikawa R.
  28. Kondo I.
  29. Koshimoto N.
  30. Matsubara Y.
  31. Matsumoto S.,Miyazaki S.
  32. Muraki Y.
  33. Okamura A.
  34. Olmschenk G.
  35. Ranc C.
  36. Rattenbury N.J.,Satoh Y.
  37. Sumi T.
  38. Suzuki D.
  39. Toda T.
  40. Tristram P.J.
  41. Vandorou A.
  42. Yama H.,(the Moa Collaboration)
  43. Published by
    CDS
Abstract

We present the analysis of three more planets from the KMTNet 2021 microlensing season. KMT-2021-BLG-0119Lb is a ~6M_Jup_ planet orbiting an early M-dwarf or a K-dwarf, KMT-2021-BLG-0192Lb is a ~2M_Nep_ planet orbiting an M-dwarf, and KMT-2021-BLG-2294Lb is a ~1.25M_Nep_ planet orbiting a very-low-mass M-dwarf or a brown dwarf. These by-eye planet detections provide an important comparison sample to the sample selected with the AnomalyFinder algorithm, and in particular, KMT-2021-BLG-2294 is a case of a planet detected by eye but not by algorithm. KMT-2021-BLG-2294Lb is part of a population of microlensing planets around very-low-mass host stars that spans the full range of planet masses, in contrast to the planet population at <~0.1au, which shows a strong preference for small planets.

Keywords
  1. exoplanets
  2. dwarf-stars
  3. infrared-photometry
  4. visible-astronomy
  5. photometry
Bibliographic source Bibcode
2023AJ....165....8S
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/165/8
IVOA Identifier IVOID
ivo://CDS.VizieR/J/AJ/165/8
Document Object Identifer DOI
doi:10.26093/cds/vizier.51650008

Access

Web browser access HTML
https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AJ/165/8
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/165/8
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/165/8
IVOA Table Access TAP
https://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).
IVOA Cone Search SCS
For use with a cone search client (e.g., TOPCAT).
https://vizier.cds.unistra.fr/viz-bin/conesearch/J/AJ/165/8/table1?
https://vizier.iucaa.in/viz-bin/conesearch/J/AJ/165/8/table1?
http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AJ/165/8/table1?

History

2023-06-07T06:30:57Z
Resource record created
2023-06-07T06:30:57Z
Created
2023-10-03T12:58:59Z
Updated

Contact

Name
CDS support team
Postal Address
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
E-Mail
cds-question@unistra.fr