ESTIMATION OF TRANSFORMATION COEFFICIENTS OF STANDARD STAR
A magnitude and colour system, such as the UVB system, is defined by a collection of standard stars detected with a certain detector and filter set. To enable observers at different observatories to compare observations, the instrumental system must be turned into a standard system. If Mλ is the standard magnitude, mλ0 is the observed extinction adjusted magnitude, and c is the standard colour index (e.g., MB - MV), they are connected by the equation. (Henden & Kaitchuck 1990)- Mλ = mλ0 + αλ.c + βλ
Authors
- S. K. Tiwari (ORCID: https://orcid.org/0009-0002-4029-8510)
Publication Details
- Journal
- International Journal of Novel Research and Development
- Published
- 2025-01-01
- DOI
- https://doi.org/10.56975/ijnrd.v10i5.306556
- Primary Topic
- Inertial Sensor and Navigation
- Type
- article
- Field-Weighted Citation Impact
- 0.00