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21by Nakamura, M., Algaba, J. -C., Asada, K., Chen, B., Chen, M. -T., Han, J., Ho, P. H. P., Hsieh, S. -N., Huang, T., Inoue, M., Koch, P., Kuo, C. -Y., Martin-Cocher, P., Matsushita, S., Meyer-Zhao, Z., Nishioka, H., Nystom, G., Pradel, N., Pu, H. -Y., Raffin, P., Shen, H. -Y., Tseng, C. -Y., Team, the Greenland Telescope Project“... network will achieve a superior angular resolution of about 20 $μ$as at 350 GHz, corresponding to $\sim2...”
Published 2013
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22by Panov, A. D., Astapov, I. I., Awad, A. K., Beskin, G. M., Bezyazeekov, P. A., Blank, M., Bonvech, E. A., Borodin, A. N., Bruckner, M., Budnev, N. M., Bulan, A. V., Chernov, D. V., Chiavassa, A., Dyachok, A. N., Gafarov, A. R., Garmash, A. Yu., Grebenyuk, V. M., Gress, O. A., Gress, T. I., Grinyuk, A. A., Grishin, O. G., Horns, D., Ivanova, A. L., Kalmykov, N. N., Kindin, V. V., Kiryuhin, S. N., Kokoulin, R. P., Kompaniets, K. G., Korosteleva, E. E., Kozhin, V. A., Kravchenko, E. A., Krivopalova, A. A., Kuzmichev, L. A., Kryukov, A. P., Lagutin, A. A., Lavrova, M. V., Lemeshev, Yu., Lubsandorzhiev, B. K., Lubsandorzhiev, N. B., Lukanov, A. D., Mirgazov, R. R., Mirzoyan, R., Monkhoev, R. D., Osipova, E. A., Pakhorukov, A. L., Pan, A., Pankov, L. V., Petrukhin, A. A., Podgrudkov, D. A., Poleschuk, V. A., Popova, E. G., Porelli, A., Postnikov, E. B., Prosin, V. V., Ptuskin, V. S., Pushnin, A. A., Raikin, R. I., Razumov, A., Rjabov, E., Rubtsov, G. I., Sagan, Y. I., Samoliga, V. S., Sidorenkov, A. Yu., Silaev, A. A., Silaev, A. A., Skurikhin, A. V., Satyshev, I., Sokolov, A. V., Suvorkin, Y., Sveshnikova, L. G., Tabolenko, V. A., Tanaev, A. B., Tarashansky, B. A., Ternovoy, M., Tkachev, L. G., Tluczykont, M., Ushakov, N., Vaidyanathan, A., Volchugov, P. A., Volkov, N. V., Voronin, D., Wischnewski, R., Yashin, I. I., Zagorodnikov, A. V., Zhurov, D. P.“...\,ns is established as $\sim 2 \times 10^{-3}$ events/sr/hour. : 15 pages, 6 figures, reported...”
Published in Forests (2021)
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23by Abarr, Q., Awaki, H., Baring, M. G., Bose, R., De Geronimo, G., Dowkontt, P., Errando, M., Guarino, V., Hattori, K., Hayashida, K., Imazato, F., Ishida, M., Iyer, N. K., Kislat, F., Kiss, M., Kitaguchi, T., Krawczynski, H., Lisalda, L., Matake, H., Maeda, Y., Matsumoto, H., Mineta, T., Miyazawa, T., Mizuno, T., Okajima, T., Pearce, M., Rauch, B. F., Ryde, F., Shreves, C., Spooner, S., Stana, T. -A., Takahashi, H., Takeo, M., Tamagawa, T., Tamura, K., Tsunemi, H., Uchida, N., Uchida, Y., West, A. T., Wulf, E. A., Yamamoto, R.“... source for $t_{\rm day}$ days, the Minimum Detectable Polarisation (at 99% confidence level) is $\sim$2...”
Published 2020
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24by Abarr, Q., Awaki, H., Baring, M. G., Bose, R., De Geronimo, G., Dowkontt, P., Errando, M., Guarino, V., Hattori, K., Hayashida, K., Imazato, F., Ishida, M., Iyer, N. K., Kislat, F., Kiss, M., Kitaguchi, T., Krawczynski, H., Lisalda, L., Matake, H., Maeda, Y., Matsumoto, H., Mineta, T., Miyazawa, T., Mizuno, T., Okajima, T., Pearce, M., Rauch, B. F., Ryde, F., Shreves, C., Spooner, S., Stana, T. -A., Takahashi, H., Takeo, M., Tamagawa, T., Tamura, K., Tsunemi, H., Uchida, N., Uchida, Y., West, A. T., Wulf, E. A., Yamamoto, R.“... source for $t_{\rm day}$ days, the Minimum Detectable Polarisation (at 99% confidence level) is $\sim$2...”
Published in Astroparticle Physics (2020)
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25by Nakamura, M., Algaba, J. -C., Asada, K., Chen, B., Chen, M. -T., Han, J., Ho, P. H. P., Hsieh, S. -N., Huang, T., Inoue, M., Koch, P., Kuo, C. -Y., Martin-Cocher, P., Matsushita, S., Meyer-Zhao, Z., Nishioka, H., Nystom, G., Pradel, N., Pu, H. -Y., Raffin, P., Shen, H. -Y., Tseng, C. -Y., Team, the Greenland Telescope Project“... network will achieve a superior angular resolution of about 20 $\mu$as at 350 GHz, corresponding to $\sim...”
Published in EPJ Web of Conferences (2013)
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26by Panov, A. D., Astapov, I. I., Awad, A. K., Beskin, G. M., Bezyazeekov, P. A., Blank, M., Bonvech, E. A., Borodin, A. N., Bruckner, M., Budnev, N. M., Bulan, A. V., Chernov, D. V., Chiavassa, A., Dyachok, A. N., Gafarov, A. R., Garmash, A. Yu., Grebenyuk, V. M., Gress, O. A., Gress, T. I., Grinyuk, A. A., Grishin, O. G., Horns, D., Ivanova, A. L., Kalmykov, N. N., Kindin, V. V., Kiryuhin, S. N., Kokoulin, R. P., Kompaniets, K. G., Korosteleva, E. E., Kozhin, V. A., Kravchenko, E. A., Krivopalova, A. A., Kuzmichev, L. A., Kryukov, A. P., Lagutin, A. A., Lavrova, M. V., Lemeshev, Yu., Lubsandorzhiev, B. K., Lubsandorzhiev, N. B., Lukanov, A. D., Mirgazov, R. R., Mirzoyan, R., Monkhoev, R. D., Osipova, E. A., Pakhorukov, A. L., Pan, A., Pankov, L. V., Petrukhin, A. A., Podgrudkov, D. A., Poleschuk, V. A., Popova, E. G., Porelli, A., Postnikov, E. B., Prosin, V. V., Ptuskin, V. S., Pushnin, A. A., Raikin, R. I., Razumov, A., Rjabov, E., Rubtsov, G. I., Sagan, Y. I., Samoliga, V. S., Sidorenkov, A. Yu., Silaev, A. A., Skurikhin, A. V., Satyshev, I., Sokolov, A. V., Suvorkin, Y., Sveshnikova, L. G., Tabolenko, V. A., Tanaev, A. B., Tarashansky, B. A., Ternovoy, M., Tkachev, L. G., Tluczykont, M., Ushakov, N., Vaidyanathan, A., Volchugov, P. A., Volkov, N. V., Voronin, D., Wischnewski, R., Yashin, I. I., Zagorodnikov, A. V., Zhurov, D. P.“...\,ns is established as $\sim 2 \times 10^{-3}$ events/sr/hour. Comment: 15 pages, 6 figures, reported...”
Published in Physics of Atomic Nuclei (2021)
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27by Harker, Alexander A., Schindelegger, Michael, Ponte, Rui M., Salstein, David A.“... of less than $$\sim $$ ∼ 2 weeks. Accounting for OAM in rotation budgets from other models typically...”
Published in Journal of Geodesy (2021)
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28by Mantz, Adam B., Allen, Steven W., Morris, R. Glenn, Canning, Rebecca E. A., Bayliss, Matthew, Bleem, Lindsey E., Floyd, Benjamin T., McDonald, Michael“...}$; cluster emission is detected above the background to a radius of $\sim 2.2 r_{500}$, or approximately...”
Published 2020
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29ANTARES and IceCube combined search for neutrino point-like and extended sources in the Southern Skyby Illuminati, Giulia“.... The sensitivity to neutrino sources located in the Southern Sky is improved by a factor of $\sim$2 compared...”
Published 2019
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30by Mantz, Adam B., Allen, Steven W., Morris, R. Glenn, Canning, Rebecca A., Bayliss, Matthew, Bleem, Lindsey E., Floyd, Benjamin T., McDonald, Michael“...^{14}\, {\rm M}_{\odot }$; cluster emission is detected above the background to a radius of $\sim \!2...”
Published in Monthly Notices of the Royal Astronomical Society (2022)
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31ANTARES and IceCube combined search for neutrino point-like and extended sources in the Southern Skyby Illuminati, Giulia“.... The sensitivity to neutrino sources located in the Southern Sky is improved by a factor of $\sim$2 compared...”
Published 2019
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32by Mantz, Adam B., Allen, Steven W., Morris, R. Glenn, Canning, Rebecca E. A., Bayliss, Matthew, Bleem, Lindsey E., Floyd, Benjamin T., McDonald, Michael“...}$; cluster emission is detected above the background to a radius of $\sim 2.2 r_{500}$, or approximately...”
Published in Monthly Notices of the Royal Astronomical Society (2020)
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33by Wu, Sirui, Napolitano, Nicola R., Tortora, Crescenzo, von Marttens, Rodrigo, Casarini, Luciano, Li, Rui, Lin, Weipeng“... dynamical methods based on Jeans equations. Dynamical masses are reproduced within 0.30 dex ($\sim2\sigma...”
Published 2023
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34by Mantz, Adam B, Allen, Steven W, Morris, R Glenn, Canning, Rebecca E A, Bayliss, Matthew, Bleem, Lindsey E, Floyd, Benjamin T, McDonald, Michael“...^{14}\, {\rm M}_{\odot }$; cluster emission is detected above the background to a radius of $\sim \!2...”
Published in Monthly Notices of the Royal Astronomical Society (2020)
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35by Cecil, G., Fogarty, L. M. R., Richards, S., Bland-Hawthorn, J., Lange, R., Moffett, A., Catinella, B., Cortese, L., Ho, I. -T., Taylor, E. N., Bryant, J. J., Allen, J. T., Sweet, S. M., Croom, S. M., Driver, S. P., Goodwin, M., Kelvin, L., Green, A. W., Konstantopoulos, I. S., Owers, M. S., Lawrence, J. S., Lorente, N. P. F.“... and stars from non-parametric Diskfit fits out to $r\sim2r_e$. For 12/14 with measured H I profiles, ionized...”
Published 2015
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36by Johnson, Kenneth Alan“... (pH 6.7) were collected to $\sim$2.2A. In $\alpha$ subunits, the alkyl moieties of the ligands lay...”
Published 1993
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37by Shin, T., Adhikari, S., Baxter, E. J., Chang, C., Jain, B., Battaglia, N., Bleem, L., Bocquet, S., DeRose, J., Gruen, D., Hilton, M., Kravtsov, A., McClintock, T., Rozo, E., Rykoff, E. S., Varga, T. N., Wechsler, R. H., Wu, H., Zhang, Z., Aiola, S., Allam, S., Bechtol, K., Benson, B. A., Bertin, E., Bond, J. R., Brodwin, M., Brooks, D., Buckley-Geer, E., Burke, D. L., Carlstrom, J. E., Carnero Rosell, A., Carrasco Kind, M., Carretero, J., Castander, F. J., Choi, S. K., Cunha, C. E., Crawford, T. M., da Costa, L. N., De Vicente, J., Desai, S., Devlin, M. J., Dietrich, J. P., Doel, P., Dunkley, J., Eifler, T. F., Evrard, A. E., Flaugher, B., Fosalba, P., Gallardo, P. A., García-Bellido, J., Gaztanaga, E., Gerdes, D. W., Gralla, M., Gruendl, R. A., Gschwend, J., Gupta, N., Gutierrez, G., Hartley, W. G., Hill, J. C., Ho, S. P., Hollowood, D. L., Honscheid, K., Hoyle, B., Huffenberger, K., Hughes, J. P., James, D. J., Jeltema, T., Kim, A. G., Krause, E., Kuehn, K., Lahav, O., Lima, M., Madhavacheril, M. S., Maia, M. A. G., Marshall, J. L., Maurin, L., McMahon, J., Menanteau, F., Miller, C. J., Miquel, R., Mohr, J. J., Naess, S., Nati, F., Newburgh, L., Niemack, M. D., Ogando, R. L. C., Page, L. A., Partridge, B., Patil, S., Plazas, A. A., Rapetti, D., Reichardt, C. L., Romer, A. K., Sanchez, E., Scarpine, V., Schindler, R., Serrano, S., Smith, M., Smith, R. C., Soares-Santos, M., Sobreira, F., Staggs, S. T., Stark, A., Stein, G., Suchyta, E., Swanson, M. E. C., Tarle, G., Thomas, D., van Engelen, A., Wollack, E. J., Xu, Z.“... selected redMaPPer clusters, $r_{\rm sp}$ is $\sim$ $2\sigma$ smaller than in the simulations...”
Published in Monthly Notices of the Royal Astronomical Society (2022)
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38by Mantz, Adam B, Allen, Steven W, Morris, R Glenn, Canning, Rebecca EA, Bayliss, Matthew, Bleem, Lindsey E, Floyd, Benjamin T, McDonald, Michael“... the background to a radius of $\sim \!2.2\, r_{500}$, or approximately the virial radius. The intracluster gas...”
Published 2020
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39by Mantz, Adam B, Allen, Steven W, Morris, R Glenn, Canning, Rebecca EA, Bayliss, Matthew, Bleem, Lindsey E, Floyd, Benjamin T, McDonald, Michael A.“... the background to a radius of $\sim \!2.2\, r_{500}$, or approximately the virial radius. The intracluster gas...”
Published 2020
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40by Couchot, F., Henrot-Versillé, S., Perdereau, O., Plaszczynski, S., d'Orfeuil, B. Rouillé, Spinelli, M., Tristram, M.“... optical depth $\tau$ and the primordial perturbation amplitude $A_s$, a $\sim2\sigma$ tension on $\tau...”
Published in Astronomy & Astrophysics (2015)
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