Search Results - "Warner, B.D."

Spin states of asteroids in the Eos collisional family by Hanuš, J., Delbo’, M., Alí-Lagoa, V., Bolin, B., Jedicke, R., Ďurech, J., Cibulková, H., Pravec, P., Kušnirák, P., Behrend, R., Marchis, F., Antonini, P., Arnold, L., Audejean, M., Bachschmidt, M., Bernasconi, L., Brunetto, L., Casulli, S., Dymock, R., Esseiva, N., Esteban, M., Gerteis, O., de Groot, H., Gully, H., Hamanowa, Hiroko, Hamanowa, Hiromi, Krafft, P., Lehký, M., Manzini, F., Michelet, J., Morelle, E., Oey, J., Pilcher, F., Reignier, F., Roy, R., Salom, P.A., Warner, B.D.

“…•We present updated and new shape model determinations for 31 asteroids from the Eos collisional family.•We compiled a sample of shapes and rotation state…”
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On the maximum amplitude of harmonics of an asteroid lightcurve by Harris, A.W., Pravec, P., Galád, A., Skiff, B.A., Warner, B.D., Világi, J., Gajdoš, Š., Carbognani, A., Hornoch, K., Kušnirák, P., Cooney, W.R., Gross, J., Terrell, D., Higgins, D., Bowell, E., Koehn, B.W.

“…•Only the second harmonic of a lightcurve due to shape can exceed a peak-to-peak amplitude of ∼0.3 magnitude.•Lightcurves of lower amplitude are formally…”
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Construction and evaluation of an instrument for the automated synthesis of oligodeoxyribonucleotides by Warner, B D, Warner, M E, Karns, G A, Ku, L, Brown-Shimer, S, Urdea, M S

“…The details for constructing an easily used and maintained laboratory instrument capable of routine oligodeoxyribonucleotide synthesis are presented. The…”
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