Year |
Citation |
Score |
2023 |
Richardson ND, Pavao CM, Eldridge JJ, Pablo H, Chené AN, Wysocki P, Gies DR, Younes G, Hare J. A high-mass X-ray binary descended from an ultra-stripped supernova. Nature. 614: 45-47. PMID 36725992 DOI: 10.1038/s41586-022-05618-9 |
0.443 |
|
2020 |
Jones D, Conroy KE, Horvat M, Giammarco J, Kochoska A, Pablo H, Brown AJ, Sowicka P, Prša A. Physics of Eclipsing Binaries. IV. The Impact of Interstellar Extinction on the Light Curves of Eclipsing Binaries Astrophysical Journal Supplement Series. 247: 63. DOI: 10.3847/1538-4365/Ab7927 |
0.448 |
|
2019 |
Walczak P, Daszyńska-Daszkiewicz J, Pigulski A, Pamyatnykh A, Moffat AFJ, Handler G, Pablo H, Popowicz A, Wade G, Weiss WW, Zwintz K. Seismic modelling of early B-type pulsators observed by BRITE – I. θ Ophiuchi Monthly Notices of the Royal Astronomical Society. 485: 3544-3557. DOI: 10.1093/Mnras/Stz639 |
0.511 |
|
2018 |
Richardson ND, Pablo H, Sterken C, Pigulski A, Koenigsberger G, Moffat AFJ, Madura TI, Hamaguchi K, Corcoran MF, Damineli A, Gull TR, Hillier DJ, Weigelt G, Handler G, Popowicz A, et al. BRITE-Constellation reveals evidence for pulsations in the enigmatic binary η Carinae Monthly Notices of the Royal Astronomical Society. 475: 5417-5423. DOI: 10.1093/Mnras/Sty157 |
0.44 |
|
2012 |
Pablo H, Kawaler SD, Reed MD, Bloemen S, Charpinet S, Hu H, Telting J, Østensen RH, Baran AS, Green EM, Hermes JJ, Barclay T, O'Toole SJ, Mullally F, Kurtz DW, et al. Seismic evidence for non-synchronization in two close sdb+dM binaries from Kepler photometry Monthly Notices of the Royal Astronomical Society. 422: 1343-1351. DOI: 10.1111/J.1365-2966.2012.20707.X |
0.54 |
|
2012 |
Pablo H, Kawaler SD, Green EM. ERRATUM: “EXPLORING B4: A PULSATING sdB STAR, IN A BINARY, IN THE OPEN CLUSTER NGC 6791” (2011, ApJ, 740, L47) The Astrophysical Journal. 750: L26. DOI: 10.1088/2041-8205/750/1/L26 |
0.516 |
|
2011 |
Pablo H, Kawaler SD, Green EM. Exploring B4: A pulsating sdB star, in a binary, in the open cluster NGC 6791 Astrophysical Journal Letters. 740. DOI: 10.1088/2041-8205/740/2/L47 |
0.586 |
|
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