| |
Kanbur, S. M. |
| Volume |
Paper Title |
Page Number |
Authors |
| 83 |
The Use of Maximum Light in Cepheid Distance Estimators |
359 |
Kanbur, S. M.; Hendry, M. A. |
| 94 |
Cepheids. Supernovae and the Value of H0 |
357 |
Hendry, M. A.; Kanbur, S. M. |
| 135 |
PL Relations at Maximum Light for Mira Variables |
111 |
Kanbur, S. M.; Hendry, M. A.; Clarke, D. |
| 167 |
Reconstructing Cepheid Light Curves |
192 |
Hendry, M. A.; Tanvir, N. R.; Kanbur, S. M. |
| 203 |
The Use of Principal Components Analysis in Analysing Variable Star Data |
56 |
Kanbur, S. M.; Iono, D.; Tanvir, N. A.; Hendry, M. A. |
| 451 |
Multiphase Comparison of Period-Luminosity Relations for Magellanic Cloud Cepheids |
311 |
Bellinger, E. P.; Kanbur, S. M.; Ngeow, C. |
| 514 |
Large Magellanic Cloud Near-Infrared Synoptic Survey (LMCNISS): Overview and Science Highlights for Classical and Type-II Cepheids |
31 |
Ngeow, C.; Bhardwaj, A.; Macri, L. M.; Kanbur, S. M. |
| 515 |
The Role of Opacities in Stellar Pulsation |
189 |
Kanbur, S. M.; Marconi, M.; Bhardwaj, A.; Kundu, R.; Singh, H. P. |
| 529 |
A Study of the Stellar Photosphere-Hydrogen Ionisation Front Interaction in Pulsating Variables Using Period-Colour Relations |
98 |
Das, S.; Kanbur, S. M.; Bellinger, E. P.; Bhardwaj, A.; Singh, H. P. |
| 529 |
Light Curve Structure Reveals Fundamental Parameters of Cepheid and RR Lyrae Stars |
104 |
Kanbur, S. M.; Bellinger, E. P.; Bhardwaj, A.; Marconi, M. |
|
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