Abstract
A model-independent method for detection of transit borders, using the polynomial approximation of the light-curve parts, is proposed. The trial processing of long-cadence light-curves of 183 Kepler's exoplanets reveals for some objects a variability of transit's start/end- times and asymmetry. The diagnostic diagram was constructed for preliminary classification and interpretation of such results.
| Original language | English |
|---|---|
| Title of host publication | EPSC-DPS Joint Meeting 2019 |
| Volume | 13 |
| Publication status | Published - Sept 2019 |
Austrian Fields of Science 2012
- 103003 Astronomy
- 103004 Astrophysics
Fingerprint
Dive into the research topics of 'Border variability of transit light-curves'. Together they form a unique fingerprint.Cite this
- APA
- Author
- BIBTEX
- Harvard
- Standard
- RIS
- Vancouver