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Baran, A. |
Volume |
Paper Title |
Page Number |
Authors |
372 |
HS 2231+2441: A New Eclipsing sdB Binary of the HW Vir Type |
483 |
Ostensen, R.; Oreiro, R.; Drechsel, H.; Heber, U.; Baran, A.; Pigulski, A. |
372 |
BUL-SC16 335: A New Eclipsing Pre-Cataclysmic Binary with a Very Short Orbital Period |
487 |
Polubek, G.; Pigulski, A.; Baran, A.; Udalski, A. |
372 |
Change of Splittings in the Pulsating Subdwarf Balloon 090100001 |
607 |
Baran, A.; Oreiro, R.; Pigulski, A.; Perez, F.; Ulla, A.; Garrido, R.; Rodriguez, C.; Monserrat, T.; Fox Machado, L.; Gonzales, J.M.; Reed, M.; Zhou, A.Y.; Harms, S.; Eggen, J.R.; Kim, S.-L.; Crowe, R.; Choo, K.-J.; Chen, W.-P.; Lee, H.-T.; Huan, F.-Y.; Siwak, M.; Koziel, D.; Zola, S. |
392 |
Results for Three-Season Photometry of Balloon 090100001 |
273 |
Baran, A.; Oreiro, R.; Pigulski, A.; Pérez Hernández, F.; Ulla, A.; Reed, M.D. |
392 |
Comparing the Observed Frequencies of Balloon 09010001 with Theoretical Modes of Oscillation |
277 |
Oreiro, R.; Baran, A.; Pérez Hernández, F.; Ulla, A.; Pigulski, A. |
435 |
Comparison of the B and V Colors as Calculated at Maximum from Physical Parameters of W UMa Stars Observed by the Tycho Mission |
91 |
Pokrzywka, B.; Zakrzewski, B.; Stachowski, G.; Baran, A.; Kreiner, J. M. |
438 |
Measuring the Diffuse Polarized Foreground of the ELAIS-N1 Deep Field |
303 |
Baran, A.; Fiege, J.; Taylor, A. R.; Foster, T.; Landecker, T. L. |
481 |
A Search for High-Degree Modes in Two Pulsating sdB Stars |
169 |
Baran, A.; Reed, M.; Jeffery, C.; Telting, J.; Farris, L.; Shadwick, M.; Kiaeerad, F. |
481 |
Low-Resolution Radial-Velocity Monitoring of Pulsating sdBs in the Kepler Field |
287 |
Telting, J.; Østensen, R.; Reed, M.; Kiæerad, F.; Farris, L.; Baran, A.; Oreiro, R.; O'Toole, S. |
496 |
Observational Verification of the Limb-Darkening Law Based on Kepler Data |
217 |
Zola, S.; Baran, A.; Debski, B.; Jableka, D. |
496 |
Light Curve Morphology: The Evolution of the O‘Connell Effect and the Maxima Separation |
293 |
Debski, B.; Zola, S.; Baran, A. |
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