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| BD+36 488 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.20CEST04:39:02 |
Sort references on where and how often the object is cited
trying to find the most relevant references on this object.
More on score
| Bibcode/DOI | Score |
in Title|Abstract| Keywords |
in a table | in teXt, Caption, ... | Nb occurence | Nb objects in ref |
Citations (from ADS) |
Title | First 3 Authors |
|---|---|---|---|---|---|---|---|---|---|
1997KFNT...13e..70R 
|
49739 | 3 | GPM - compiled catalogue of absolute proper motions of stars in selected areas of sky with galaxies. | RYBKA S.P. and YATSENKO A.I. | |||||
| 2012ApJ...754..106D | 16 | D | 1 | 10 | 29 | Infrared eclipses of the strongly irradiated planet WASP-33b, and oscillations of its host star. | DEMING D., FRAINE J.D., SADA P.V., et al. | ||
|
2013A&A...553A..44K
|
39 | X | 1 | 23 | 19 | Comprehensive time series analysis of the transiting extrasolar planet WASP-33b. | KOVACS G., KOVACS T., HARTMAN J.D., et al. | ||
| 2014A&A...561A..48V | 80 | X | 2 | 6 | 22 | Pulsation analysis and its impact on primary transit modeling in WASP-33. | VON ESSEN C., CZESLA S., WOLTER U., et al. | ||
| 2015A&A...584A..75V | 40 | X | 1 | 7 | 9 | A temperature inversion in WASP-33b? . Large Binocular Telescope occultation data confirm significant thermal flux at short wavelengths. | VON ESSEN C., MALLONN M., ALBRECHT S., et al. | ||
|
2016AJ....152..181H
|
16 | D | 1 | 9279 | 22 | SETI observations of exoplanets with the Allen Telescope Array. | HARP G.R., RICHARDS J., TARTER J.C., et al. | ||
| 2019A&A...622A..71V | 168 | X C | 3 | 8 | 11 | An optical transmission spectrum of the ultra-hot Jupiter WASP-33 b. First indication of aluminum oxide in an exoplanet. | VON ESSEN C., MALLONN M., WELBANKS L., et al. | ||
|
2019MNRAS.490.3158C
|
17 | D | 1 | 465834 | 28 | A catalogue of stellar diameters and fluxes for mid-infrared interferometry. | CRUZALEBES P., PETROV R.G., ROBBE-DUBOIS S., et al. | ||
| 2022MNRAS.512.4404W | 45 | X | 1 | 14 | 3 | Nodal precession of WASP-33b for 11 yr by Doppler tomographic and transit photometric observations. | WATANABE N., NARITA N., PALLE E., et al. |
