Zobrazeno 1 - 10
of 869
pro vyhledávání: '"Doherty, J A"'
Autor:
Barnes, J. R., Standing, M. R., Haswell, C. A., Staab, D., Doherty, J. P. J., Waller-Bridge, M., Fossati, L., Soto, M., Anglada-Escudé, G., Llama, J., McCune, C., Lewis, F. W.
We present radial velocity measurements of the very bright ($V\sim5.7$) nearby F star, DMPP-4 (HD 184960). The anomalously low Ca II H&K emission suggests mass loss from planets orbiting a low activity host star. Periodic radial velocity variability
Externí odkaz:
http://arxiv.org/abs/2307.07530
Autor:
Staab, D., Haswell, C. A., Barnes, J. R., Anglada-Escudé, G., Fossati, L., Doherty, J. P. J., Cooper, J., Jenkins, J. S., Díaz, M. R., Soto, M. G.
The Dispersed Matter Planet Project targets stars with anomalously low Ca II H&K chromospheric emission. High precision, high cadence radial velocity measurements of the F8V star HD 38677 / DMPP-1 reveal four short period planets. DMPP-1 has log(R'HK
Externí odkaz:
http://arxiv.org/abs/1912.10792
Autor:
O'Neill, M.P., Osuchowski, A.L., Cai, Y., Bransby, M.F., Watson, P.G., Gaudin, C., Doherty, J., Dalgaard, E., Ross, R.
Publikováno v:
In Ocean Engineering 15 September 2023 284
Publikováno v:
In Applied Ergonomics July 2023 110
Autor:
Cecchi, M., Adachi, M., Basile, A., Buhl, D.L., Chadchankar, H., Christensen, S., Christian, E., Doherty, J., Fadem, K.C., Farley, B., Forman, M.S., Honda, S., Johannesen, J., Kinon, B.J., Klamer, D., Marino, M.J., Missling, C., O'Donnell, P., Piser, T., Puryear, C.B., Quirk, M.C., Rotte, M., Sanchez, C., Smith, D.G., Uslaner, J.M., Javitt, D.C., Keefe, R.S.E., Mathalon, D., Potter, W.Z., Walling, D.P., Ereshefsky, L.
Publikováno v:
In Schizophrenia Research April 2023 254:178-189
Akademický článek
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Publikováno v:
In Journal of Hydrology October 2019 577
Publikováno v:
Journal of Applied Physics; 7/21/2022, Vol. 132 Issue 3, p1-6, 6p
Publikováno v:
Journal of Applied Physics. 7/21/2022, Vol. 132 Issue 3, p1-6. 6p.
We generalize the KPZ equation to an O(3) $N=2j+1$ component model. In the limit $N \to \infty$ we show that the mode coupling equations become exact. Solving these approximately we find that the dynamic exponent $z$ increases from $3/2$ for $d=1$ to
Externí odkaz:
http://arxiv.org/abs/cond-mat/9307053