Year |
Citation |
Score |
2019 |
Quarles B, Barnes JW, Lissauer JJ, Chambers J. Obliquity Evolution of the Potentially Habitable Exoplanet Kepler-62f. Astrobiology. PMID 31613645 DOI: 10.1089/Ast.2018.1932 |
0.325 |
|
2019 |
Quarles B, Kaib N. Instabilities in the Early Solar System due to a Self-gravitating Disk. The Astronomical Journal. 157. PMID 31534266 DOI: 10.3847/1538-3881/Aafa71 |
0.491 |
|
2019 |
Orosz JA, Welsh WF, Haghighipour N, Quarles B, Short DR, Mills SM, Satyal S, Torres G, Agol E, Fabrycky DC, Jontof-Hutter D, Windmiller G, Müller TWA, Hinse TC, Cochran WD, et al. Discovery of a Third Transiting Planet in the Kepler-47 Circumbinary System The Astronomical Journal. 157: 174. DOI: 10.3847/1538-3881/Ab0Ca0 |
0.711 |
|
2018 |
Quarles B, Satyal S, Kostov V, Kaib N, Haghighipour N. Stability Limits of Circumbinary Planets: Is There a Pile-up in theKeplerCBPs? The Astrophysical Journal. 856: 150. DOI: 10.3847/1538-4357/Aab264 |
0.714 |
|
2017 |
Quarles B, Quintana EV, Lopez E, Schlieder JE, Barclay T. Plausible Compositions of the Seven TRAPPIST-1 Planets Using Long-term Dynamical Simulations The Astrophysical Journal. 842: L5. DOI: 10.3847/2041-8213/Aa74Bf |
0.506 |
|
2016 |
Barnes JW, Quarles B, Lissauer JJ, Chambers J, Hedman MM. Obliquity Variability of a Potentially Habitable Early Venus. Astrobiology. PMID 27328026 DOI: 10.1089/Ast.2015.1427 |
0.383 |
|
2016 |
Coughlin JL, Mullally F, Thompson SE, Rowe JF, Burke CJ, Latham DW, Batalha NM, Ofir A, Quarles BL, Henze CE, Wolfgang A, Caldwell DA, Bryson ST, Shporer A, Catanzarite J, et al. PLANETARY CANDIDATES OBSERVED by KEPLER. VII. the FIRST FULLY UNIFORM CATALOG BASED on the ENTIRE 48-MONTH DATA SET (Q1-Q17 DR24) Astrophysical Journal, Supplement Series. 224. DOI: 10.3847/0067-0049/224/1/12 |
0.356 |
|
2016 |
Kostov VB, Orosz JA, Welsh WF, Doyle LR, Fabrycky DC, Haghighipour N, Quarles B, Short DR, Cochran WD, Endl M, Ford EB, Gregorio J, Hinse TC, Isaacson H, Jenkins JM, et al. KEPLER-1647B: The LARGEST and LONGEST-PERIOD KEPLER TRANSITING CIRCUMBINARY PLANET Astrophysical Journal. 827. DOI: 10.3847/0004-637X/827/1/86 |
0.516 |
|
2016 |
Quarles B, Lissauer JJ. LONG-TERM STABILITY of PLANETS in the α CENTAURI SYSTEM Astronomical Journal. 151. DOI: 10.3847/0004-6256/151/5/111 |
0.489 |
|
2016 |
Kirk B, Conroy K, Prša A, Abdul-Masih M, Kochoska A, Matijevič G, Hambleton K, Barclay T, Bloemen S, Boyajian T, Doyle LR, Fulton BJ, Hoekstra AJ, Jek K, Kane SR, ... ... Quarles B, et al. KEPLER ECLIPSING BINARY STARS. VII. the CATALOG of ECLIPSING BINARIES FOUND in the ENTIRE KEPLER DATA SET Astronomical Journal. 151. DOI: 10.3847/0004-6256/151/3/68 |
0.394 |
|
2015 |
Mullally F, Coughlin JL, Thompson SE, Rowe J, Burke C, Latham DW, Batalha NM, Bryson ST, Christiansen J, Henze CE, Ofir A, Quarles B, Shporer A, Eylen VV, Laerhoven CV, et al. Planetary candidates observed by kepler. VI. planet sample from Q1-Q16 (47 months) Astrophysical Journal, Supplement Series. 217. DOI: 10.1088/0067-0049/217/2/31 |
0.331 |
|
2015 |
Welsh WF, Orosz JA, Short DR, Cochran WD, Endl M, Brugamyer E, Haghighipour N, Buchhave LA, Doyle LR, Fabrycky DC, Hinse TC, Kane SR, Kostov V, Mazeh T, Mills SM, ... ... Quarles B, et al. KEPLER 453 b - THE 10th KEPLER TRANSITING CIRCUMBINARY PLANET Astrophysical Journal. 809. DOI: 10.1088/0004-637X/809/1/26 |
0.535 |
|
2015 |
Quarles BL, Lissauer JJ. Dynamical evolution of the Earth-Moon progenitors - Whence Theia? Icarus. 248: 318-339. DOI: 10.1016/J.Icarus.2014.10.044 |
0.508 |
|
2014 |
Musielak ZE, Quarles B. The three-body problem. Reports On Progress in Physics. Physical Society (Great Britain). 77: 065901. PMID 24913140 DOI: 10.1088/0034-4885/77/6/065901 |
0.551 |
|
2014 |
Quintana EV, Barclay T, Raymond SN, Rowe JF, Bolmont E, Caldwell DA, Howell SB, Kane SR, Huber D, Crepp JR, Lissauer JJ, Ciardi DR, Coughlin JL, Everett ME, Henze CE, ... ... Quarles B, et al. An Earth-sized planet in the habitable zone of a cool star. Science (New York, N.Y.). 344: 277-80. PMID 24744370 DOI: 10.1126/Science.1249403 |
0.401 |
|
2014 |
Satyal S, Hinse TC, Quarles B, Noyola JP. Chaotic dynamics of the planet in HD 196885 AB Monthly Notices of the Royal Astronomical Society. 443: 1310-1318. DOI: 10.1093/Mnras/Stu1221 |
0.715 |
|
2014 |
Conroy KE, Prša A, Stassun KG, Bloemen S, Parvizi M, Quarles B, Boyajian T, Barclay T, Shporer A, Latham DW, Abdul-Masih M. Kepler eclipsing binary stars. V. Identification of 31 candidate eclipsing binaries in the K2 engineering dataset Publications of the Astronomical Society of the Pacific. 126: 914-922. DOI: 10.1086/678953 |
0.32 |
|
2013 |
Satyal S, Quarles B, Hinse TC. Application of chaos indicators in the study of dynamics of S-type extrasolar planets in stellar binaries Monthly Notices of the Royal Astronomical Society. 433: 2215-2225. DOI: 10.1093/Mnras/Stt888 |
0.709 |
|
2013 |
Cuntz M, Quarles B, Eberle J, Shukayr A. On the possibility of habitable moons in the system of HD 23079: Results from orbital stability studies Publications of the Astronomical Society of Australia. 30. DOI: 10.1017/Pas.2013.011 |
0.525 |
|
2012 |
Quarles B, Cuntz M, Musielak ZE. The stability of the suggested planet in the νOctantis system: A numerical and statistical study Monthly Notices of the Royal Astronomical Society. 421: 2930-2939. DOI: 10.1111/J.1365-2966.2012.20568.X |
0.513 |
|
2012 |
Quarles B, Musielak ZE, Cuntz M. Habitability of earth-mass planets and moons in the Kepler-16 system Astrophysical Journal. 750. DOI: 10.1088/0004-637X/750/1/14 |
0.531 |
|
2012 |
Quarles B, Musielak ZE, Cuntz M. Study of resonances for the restricted 3-body problem Astronomische Nachrichten. 333: 551-560. DOI: 10.1002/Asna.201111704 |
0.371 |
|
2011 |
Quarles B, Eberle J, Musielak ZE, Cuntz M. The instability transition for the restricted 3-body problem: III. the Lyapunov exponent criterion Astronomy and Astrophysics. 533. DOI: 10.1051/0004-6361/201016199 |
0.539 |
|
2011 |
Eberle J, Cuntz M, Quarles B, Musielak ZE. Case studies of habitable Trojan planets in the system of HD 23079 International Journal of Astrobiology. 10: 325-334. DOI: 10.1017/S1473550411000176 |
0.538 |
|
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