The Effect of Photometric Errors on the Measured Width of the Main Sequence in Star Clusters
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arXiv
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| Natura: | Preprint |
| Pubblicazione: |
2025
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| _version_ | 1866915348484194304 |
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| author | Spangler, Steven R. |
| author_facet | Spangler, Steven R. |
| contents | This paper deals with the effect of errors in the B and V magnitudes, or measurements in any other color system, on the width of the main sequence in a color-magnitude (Hertzsprung-Russell) diagram. The width is defined as the dispersion in apparent (or absolute) magnitude at a fixed, measured photometric color. I find that the dispersion is larger than might be thought, a priori. A statistical analysis is presented which demonstrates that the error in the magnitude residual from a linear approximation to the main sequence is Gaussian, but with a standard deviation which is much larger, in general, than the errors in the individual B and V magnitudes. This result is confirmed by a Monte Carlo simulation of a main sequence population with specified errors in B and V magnitudes, and can be explained on the basis of simple algebraic arguments. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2506_14585 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | The Effect of Photometric Errors on the Measured Width of the Main Sequence in Star Clusters Spangler, Steven R. Solar and Stellar Astrophysics This paper deals with the effect of errors in the B and V magnitudes, or measurements in any other color system, on the width of the main sequence in a color-magnitude (Hertzsprung-Russell) diagram. The width is defined as the dispersion in apparent (or absolute) magnitude at a fixed, measured photometric color. I find that the dispersion is larger than might be thought, a priori. A statistical analysis is presented which demonstrates that the error in the magnitude residual from a linear approximation to the main sequence is Gaussian, but with a standard deviation which is much larger, in general, than the errors in the individual B and V magnitudes. This result is confirmed by a Monte Carlo simulation of a main sequence population with specified errors in B and V magnitudes, and can be explained on the basis of simple algebraic arguments. |
| title | The Effect of Photometric Errors on the Measured Width of the Main Sequence in Star Clusters |
| topic | Solar and Stellar Astrophysics |
| url | https://arxiv.org/abs/2506.14585 |