Magnitude And Color Transformations Between Sirius And 2Mass Photometric Systems
(2008) In Baltic Astronomy 17(3-4). p.283-292- Abstract
- We provide magnitude and color transformations between two near-infrared photometric systems, 2MASS and SIRIUS, the latter currently implemented with the three-Channel SIRIUS camera on 1.4 m Infrared Survey Facility telescope at the South African Astronomical Observatory. The transformation equations are derived using a carefully selected sample of 32 770 stars in the. Large and Small Magellanic Clouds that have high quality observations available in both photometric systems. The derived transformations are valid in the color range -0.1 < (J - H)(SIRIUS) < 1.15, -0.05 < (H - K-s)(SIRIUS) < 0.7 and -0.1 < (J - K-s)(SIRIUS) < 1.7.
Please use this url to cite or link to this publication:
https://lup.lub.lu.se/record/1375191
- author
- Kucinskas, A. ; Dobrovolskas, V. ; Lazauskaite, R. ; Lindegren, Lennart LU and Tanabe, T.
- organization
- publishing date
- 2008
- type
- Contribution to journal
- publication status
- published
- subject
- keywords
- methods: data analysis, infrared: stars, techniques: photometric, catalogs surveys
- in
- Baltic Astronomy
- volume
- 17
- issue
- 3-4
- pages
- 283 - 292
- publisher
- Institute of Theoretical Physics and Astronomy, Vilnius University
- external identifiers
-
- wos:000263863100003
- scopus:62249219723
- ISSN
- 1392-0049
- language
- English
- LU publication?
- yes
- id
- f7443d96-5f2c-4caf-8a79-fee56ea79a08 (old id 1375191)
- date added to LUP
- 2016-04-01 13:35:40
- date last changed
- 2024-01-09 15:49:43
@article{f7443d96-5f2c-4caf-8a79-fee56ea79a08, abstract = {{We provide magnitude and color transformations between two near-infrared photometric systems, 2MASS and SIRIUS, the latter currently implemented with the three-Channel SIRIUS camera on 1.4 m Infrared Survey Facility telescope at the South African Astronomical Observatory. The transformation equations are derived using a carefully selected sample of 32 770 stars in the. Large and Small Magellanic Clouds that have high quality observations available in both photometric systems. The derived transformations are valid in the color range -0.1 < (J - H)(SIRIUS) < 1.15, -0.05 < (H - K-s)(SIRIUS) < 0.7 and -0.1 < (J - K-s)(SIRIUS) < 1.7.}}, author = {{Kucinskas, A. and Dobrovolskas, V. and Lazauskaite, R. and Lindegren, Lennart and Tanabe, T.}}, issn = {{1392-0049}}, keywords = {{methods: data analysis; infrared: stars; techniques: photometric; catalogs surveys}}, language = {{eng}}, number = {{3-4}}, pages = {{283--292}}, publisher = {{Institute of Theoretical Physics and Astronomy, Vilnius University}}, series = {{Baltic Astronomy}}, title = {{Magnitude And Color Transformations Between Sirius And 2Mass Photometric Systems}}, volume = {{17}}, year = {{2008}}, }