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5by Desai, S., Armstrong, R., Mohr, J. J., Semler, D. R., Liu, J., Bertin, E., Alam, S. S., Barkhouse, W. A., Bazin, G., Buckley-Geer, E. J., Cooper, M. C., Hansen, S. M., High, F. W., Lin, H., Lin, Y. T., Ngeow, C. -C., Rest, A., Song, J., Tucker, D., Zenteno, A.“...MASS which has $\sim2$% accuracy. The scatter of stars about the stellar locus indicates a systematics...”
Published 2012
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6by Desai, S., Armstrong, R., Mohr, J. J., Semler, D. R., Liu, J., Bertin, E., Alam, S. S., Barkhouse, W. A., Bazin, G., Buckley-Geer, E. J., Cooper, M. C., Hansen, S. M., High, F. W., Lin, H., Lin, Y. T., Ngeow, C. -C., Rest, A., Song, J., Tucker, D., Zenteno, A.“... derives from 2MASS which has $\sim2$% accuracy. The scatter of stars about the stellar locus indicates a...”
Published in The Astrophysical Journal (2012)
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7by Fripiat, François, André, Luc, Cardinal, Damien, Cavagna, Anne-Julie, Savoye, Nicolas, Dehairs, Frank“... supplies summer mixed layer with 4.0±0.7molSim-2yr-1. This supply must be equivalent to the net annual bSiO...”
Published 2011
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8by Mai, Yifan, Vaughan, Sam P., Croom, Scott M., van de Sande, Jesse, Barsanti, Stefania, Bland-Hawthorn, Joss, Brough, Sarah, Bryant, Julia J., Colless, Matthew, Goodwin, Michael, Groves, Brent, Konstantopoulos, Iraklis S., Lawrence, Jon S., Lorente, Nuria P. F., Richards, Samuel N.“... 3 Mpc. The negative signals for neighbours at distance around 10 Mpc are also significant at $\sim 2...”
Published in Monthly Notices of the Royal Astronomical Society (2022)
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9“... WimpSim [2]. In Table 4 of Ref. [1], the labels and units of columns 7 and 8 suggest that the muon flux...”
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10“... registered at Yakutsk array with energy $\sim$2$\cdot$10$^{20}$ eV. : 6 pages, 3 figures...”
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11“... registered at Yakutsk array with energy $\sim$2$\cdot$10$^{20}$ eV. Comment: 6 pages, 3 figures...”
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12by Fripiat, F., Cavagna, A. -j., Dehairs, F., Speich, Sabrina, Andre, L., Cardinal, D.“... +/- 1.3 and 1.1 +/- 0.3 mol Sim(-2) for the Antarctic Zone and Polar Front Zone, respectively...”
Published in Ocean Science (2011)
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13“... to an accuracy of $\sim 2%$, in turn fixing the ratio of the pressure of the dark energy to its density ($w...”
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14by Ave, M., Boyle, P. J., Gahbauer, F., Hoppner, C., Horandel, J. R., Ichimura, M., Muller, D., Romero-Wolf, A.“... to the individual energy spectra above 20 GeV per amu exhibits nearly the same spectral index ($\sim$ 2.65 $\pm...”
Published 2008
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15by Ave, M., Boyle, P. J., Gahbauer, F., Hoppner, C., Horandel, J. R., Ichimura, M., Muller, D., Romero-Wolf, A.“... to the individual energy spectra above 20 GeV per amu exhibits nearly the same spectral index ($\sim$ 2.65 $\pm...”
Published in The Astrophysical Journal (2008)
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16“... to an accuracy of $\sim 2%$, in turn fixing the ratio of the pressure of the dark energy to its density ($w...”
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17by Angulo, R., Baugh, C. M., Frenk, C. S., Bower, R. G., Jenkins, A., Morris, S. L.“... to an accuracy of $\sim 2%$, in turn fixing the ratio of the pressure of the dark energy to its density ($w...”
Published in Monthly Notices of the Royal Astronomical Society: Letters (2005)
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18by Konstantopoulos, Bryant, Kelvin, Cecil, Ho, Fogarty, Sweet, Green, Owers, Lorente, Moffett, Goodwin, Lawrence, Lange, Cortese, Richards, Allen, Taylor, Bland-Hawthorn, Catinella, Croom, Driver“... and stars from non-parametric Diskfit fits out to $r\sim2r_e$. For 12/14 with measured H I profiles, ionized...”
Published 2016
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19“... $\sim$2 $\cdot$ 10$^{20}$ eV. : 11 pages, 20 figures, 2 tables, accepted for publication in NIM A. arXiv...”
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20by Knurenko, S. P., Petrov, Z. E., Petrov, I. S.“... $\sim$2 $\cdot$ 10$^{20}$ eV. Comment: 11 pages, 20 figures, 2 tables, accepted for publication in NIM A...”
Published in Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment (2017)
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