The photometry and flare analysis of Kepler flare candidate 2MASS J22285440- 1325178 has been presented. The light curve shows the amplitude distributions for the 2MASS J22285440-1325178. From the light curve, the shorter amplitude represents the short duration of the flares while the larger amplitude show the highest peak of the flares, with amplitude range duration from 7457.70-15482.7700 (e-/sec). The magnitude of the flares varies with times (days) and the light curve, the plot of the light curve demonstrates the frequency of the flares and the range of the magnitude. The amplitude represents the flux peak of each flare, which indicates that flare stars have larger amplitudes and hence larger star spots than normal stars. Our data was obtained from the Milkulski Archive for Space Telescope (MAST). The instrument used for data analysis of 2MASS J22285440-1325178 candidate are python Jupiter notebook software package. In addition, aperture photometric reduction of 2MASS J22285440-1325178 at EPIC 206050032 have been carried out to obtain the light curve. Furthermore, flare amplitude was analyzed as well as the flare rise time and equivalent duration.
| Published in | American Journal of Astronomy and Astrophysics (Volume 10, Issue 2) |
| DOI | 10.11648/j.ajaa.20231002.11 |
| Page(s) | 14-22 |
| Creative Commons |
This is an Open Access article, distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution and reproduction in any medium or format, provided the original work is properly cited. |
| Copyright |
Copyright © The Author(s), 2023. Published by Science Publishing Group |
Flares, Photometry, Amplitudes, Flux
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APA Style
Muallim Yakubu, Chima Abraham Iheanyichukwu, Kassimu Abdullahi Anderson. (2023). The Study of the Photometry and Flare Analysis of Kepler Flare Candidate 2MASS J22285440-1325178. American Journal of Astronomy and Astrophysics, 10(2), 14-22. https://doi.org/10.11648/j.ajaa.20231002.11
ACS Style
Muallim Yakubu; Chima Abraham Iheanyichukwu; Kassimu Abdullahi Anderson. The Study of the Photometry and Flare Analysis of Kepler Flare Candidate 2MASS J22285440-1325178. Am. J. Astron. Astrophys. 2023, 10(2), 14-22. doi: 10.11648/j.ajaa.20231002.11
AMA Style
Muallim Yakubu, Chima Abraham Iheanyichukwu, Kassimu Abdullahi Anderson. The Study of the Photometry and Flare Analysis of Kepler Flare Candidate 2MASS J22285440-1325178. Am J Astron Astrophys. 2023;10(2):14-22. doi: 10.11648/j.ajaa.20231002.11
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Download@article{10.11648/j.ajaa.20231002.11,
author = {Muallim Yakubu and Chima Abraham Iheanyichukwu and Kassimu Abdullahi Anderson},
title = {The Study of the Photometry and Flare Analysis of Kepler Flare Candidate 2MASS J22285440-1325178},
journal = {American Journal of Astronomy and Astrophysics},
volume = {10},
number = {2},
pages = {14-22},
doi = {10.11648/j.ajaa.20231002.11},
url = {https://doi.org/10.11648/j.ajaa.20231002.11},
eprint = {https://article.sciencepublishinggroup.com/pdf/10.11648.j.ajaa.20231002.11},
abstract = {The photometry and flare analysis of Kepler flare candidate 2MASS J22285440- 1325178 has been presented. The light curve shows the amplitude distributions for the 2MASS J22285440-1325178. From the light curve, the shorter amplitude represents the short duration of the flares while the larger amplitude show the highest peak of the flares, with amplitude range duration from 7457.70-15482.7700 (e-/sec). The magnitude of the flares varies with times (days) and the light curve, the plot of the light curve demonstrates the frequency of the flares and the range of the magnitude. The amplitude represents the flux peak of each flare, which indicates that flare stars have larger amplitudes and hence larger star spots than normal stars. Our data was obtained from the Milkulski Archive for Space Telescope (MAST). The instrument used for data analysis of 2MASS J22285440-1325178 candidate are python Jupiter notebook software package. In addition, aperture photometric reduction of 2MASS J22285440-1325178 at EPIC 206050032 have been carried out to obtain the light curve. Furthermore, flare amplitude was analyzed as well as the flare rise time and equivalent duration.},
year = {2023}
}
TY - JOUR T1 - The Study of the Photometry and Flare Analysis of Kepler Flare Candidate 2MASS J22285440-1325178 AU - Muallim Yakubu AU - Chima Abraham Iheanyichukwu AU - Kassimu Abdullahi Anderson Y1 - 2023/09/18 PY - 2023 N1 - https://doi.org/10.11648/j.ajaa.20231002.11 DO - 10.11648/j.ajaa.20231002.11 T2 - American Journal of Astronomy and Astrophysics JF - American Journal of Astronomy and Astrophysics JO - American Journal of Astronomy and Astrophysics SP - 14 EP - 22 PB - Science Publishing Group SN - 2376-4686 UR - https://doi.org/10.11648/j.ajaa.20231002.11 AB - The photometry and flare analysis of Kepler flare candidate 2MASS J22285440- 1325178 has been presented. The light curve shows the amplitude distributions for the 2MASS J22285440-1325178. From the light curve, the shorter amplitude represents the short duration of the flares while the larger amplitude show the highest peak of the flares, with amplitude range duration from 7457.70-15482.7700 (e-/sec). The magnitude of the flares varies with times (days) and the light curve, the plot of the light curve demonstrates the frequency of the flares and the range of the magnitude. The amplitude represents the flux peak of each flare, which indicates that flare stars have larger amplitudes and hence larger star spots than normal stars. Our data was obtained from the Milkulski Archive for Space Telescope (MAST). The instrument used for data analysis of 2MASS J22285440-1325178 candidate are python Jupiter notebook software package. In addition, aperture photometric reduction of 2MASS J22285440-1325178 at EPIC 206050032 have been carried out to obtain the light curve. Furthermore, flare amplitude was analyzed as well as the flare rise time and equivalent duration. VL - 10 IS - 2 ER -
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