File Download
  Links for fulltext
     (May Require Subscription)
Supplementary

Conference Paper: Transformations From Standard Photometric Systems To The Gaia Passbands

TitleTransformations From Standard Photometric Systems To The Gaia Passbands
Authors
Ritter, AHuang, C
Issue Date2020
PublisherInstitute of Physics Publishing. The Journal's web site is located at https://iopscience.iop.org/journal/1742-6596
Citation
10th International Conference on Applied Physics and Mathematics (ICAPM 2020), Tokyo, Japan, 10-12 January 2020. In Journal of Physics: Conference Series, 2020, v. 1593, p. 012039:1-9 How to Cite?
DOI: http://dx.doi.org/10.1088/1742-6596/1593/1/012039
AbstractAims. Provide a transformation from the standard photometric filters to Gaia G, GBP and GRP passbands. Methods. The relations between the standard photometric filters in the Johnson-Cousins UBV RC IC photometric system, the SDSS ugriz system, and the Gaia passbands were fitted with up to third order polynomials for dwarfs and giants individually. Results. At least for the Gaia GBP passband the Johnson-Cousins filter are better suited for a reliable prediction. No improvement is seen for higher than third order polynomial fits for any of the performed transformations. Conclusions. The provided dependencies amongst colours can be used to transform the apparent magnitudes in the B, V, RC, and SDSS griz passbands to Gaia G, GBP, and GBR photometry, allowing for a comparison of the Gaia survey to models of the Galaxy and to previous large surveys.
Persistent Identifierhttp://hdl.handle.net/10722/284703
ISSN
1742-6596
2020 SCImago Journal Rankings: 0.210

 

DC FieldValueLanguage
dc.contributor.authorRitter, A-
dc.contributor.authorHuang, C-
dc.date.accessioned2020-08-07T09:01:31Z-
dc.date.available2020-08-07T09:01:31Z-
dc.date.issued2020-
dc.identifier.citation10th International Conference on Applied Physics and Mathematics (ICAPM 2020), Tokyo, Japan, 10-12 January 2020. In Journal of Physics: Conference Series, 2020, v. 1593, p. 012039:1-9-
dc.identifier.issn1742-6596-
dc.identifier.urihttp://hdl.handle.net/10722/284703-
dc.description.abstractAims. Provide a transformation from the standard photometric filters to Gaia G, GBP and GRP passbands. Methods. The relations between the standard photometric filters in the Johnson-Cousins UBV RC IC photometric system, the SDSS ugriz system, and the Gaia passbands were fitted with up to third order polynomials for dwarfs and giants individually. Results. At least for the Gaia GBP passband the Johnson-Cousins filter are better suited for a reliable prediction. No improvement is seen for higher than third order polynomial fits for any of the performed transformations. Conclusions. The provided dependencies amongst colours can be used to transform the apparent magnitudes in the B, V, RC, and SDSS griz passbands to Gaia G, GBP, and GBR photometry, allowing for a comparison of the Gaia survey to models of the Galaxy and to previous large surveys.-
dc.languageeng-
dc.publisherInstitute of Physics Publishing. The Journal's web site is located at https://iopscience.iop.org/journal/1742-6596-
dc.relation.ispartofJournal of Physics: Conference Series-
dc.relation.ispartof10th International Conference on Applied Physics and Mathematics (ICAPM 2020)-
dc.rightsJournal of Physics: Conference Series. Copyright © Institute of Physics Publishing.-
dc.rightsThis work is licensed under a Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.-
dc.titleTransformations From Standard Photometric Systems To The Gaia Passbands-
dc.typeConference_Paper-
dc.identifier.emailRitter, A: aritter@hku.hk-
dc.description.naturepublished_or_final_version-
dc.identifier.doi10.1088/1742-6596/1593/1/012039-
dc.identifier.scopuseid_2-s2.0-85092587440-
dc.identifier.hkuros312554-
dc.identifier.volume1593-
dc.identifier.spage012039:1-
dc.identifier.epage012039:9-
dc.publisher.placeUnited Kingdom-
dc.identifier.issnl1742-6588-

Export via OAI-PMH Interface in XML Formats

OR

Export to Other Non-XML Formats