1 - 20 toradh á dtaispeáint as 2,402 toradh san iomlán ar an gcuardach 'M.', am iarratais: 0.19s Beachtaigh na torthaí
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    de réir CMS Collaboration, Abercrombie, Daniel Robert, Allen, Brandon Leigh, Apyan, Aram, Azzolini, Virginia, Barbieri, Richard Alexander, Baty, Austin Alan, Bi, Ran, Bierwagen, Katharina, Brandt, Stephanie Akemi, Busza, Wit, Cali, Ivan Amos, D'Alfonso, Mariarosaria, Demiragli, Zeynep, Gomez-Ceballos, Guillelmo, Goncharov, Maxim, Hsu, Dylan George, Iiyama, Yutaro, Innocenti, Gian Michele, Klute, Markus, Kovalskyi, Dmytro, Krajczar, Krisztian F., Lai, Yue Shi, Lee, Yen-Jie, Levin, Andrew Michael, Luckey Jr, P David, Maier, Benedikt, Marini, Andrea Carlo, McGinn, Christopher Francis, Mironov, Camelia Maria, Narayanan, Siddharth Madhavan, Niu, Xinmei, Paus, Christoph M. E., Roland, Christof E, Roland, Gunther M, Salfeld-Nebgen, Jakob Maxillian Henry, Stephans, George S. F., Tatar, Kaya, Velicanu, Dragos Alexandru, Wang, Jing, Wang, Ta-Wei, Wyslouch, Boleslaw
    Foilsithe / Cruthaithe 2017
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    ...We present the generation and detection of squeezed light in the 2  μm wavelength region...
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    ... of M31 in generating the high angular momentum orbit of the Clouds, a puzzle that has only been...
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    ... M dwarfs) are fully convective, and are expected to have a different type of dynamo mechanism than...
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    ...We present the analysis of two observations of M92 taken with the Chandra X-Ray Observatory. We...
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  8. 8
    de réir Conrad, Janet, Louis, William C., Shaevitz, Michael H.
    Foilsithe / Cruthaithe 2014
    ... with Δm[superscript 2]≈1 eV[superscript 2]. The two experiments are complementary, so comparing...
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    ...We present an analysis of 15 Chandra observations of the nearby spiral galaxy M81 taken over...
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    ...We study a Chandra X-ray Observatory ACIS-S observation of the Galactic globular cluster M12...
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    ... Telescope Multiband Imaging Photometer 24 μm observations of the previously used X-ray sample, and we find...
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    ... to orbit the latest-type M stars. Using TESS photometry, we report the discovery of two planets transiting...
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    ... period of 0.52 days around an M3-type star (0.381 ± 0.019 M, 0.391 ± 0.020 R) located 20.385 ± 0.019 pc...
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    de réir Arenz, M., Baek, W.-J., Beck, M., Beglarian, A., Behrens, J., Bergmann, T., Berlev, A., Besserer, U., Blaum, K., Bode, T., Bornschein, B., Bornschein, L., Brunst, T., Chilingaryan, S., Choi, W. Q, Deffert, M., Doe, P. J, Dragoun, O., Drexlin, G., Dyba, S., Edzards, F., Eitel, K., Ellinger, E., Engel, R., Enomoto, S., Erhard, M., Eversheim, D., Fedkevych, M., Fischer, S., Fränkle, F. M, Franklin, G. B, Friedel, F., Fulst, A., Gil, W., Glück, F., Ureña, A. G, Grohmann, S., Grössle, R., Gumbsheimer, R., Hackenjos, M., Hannen, V., Harms, F., Haußmann, N., Heizmann, F., Helbing, K., Herz, W., Hickford, S., Hilk, D., Hillesheimer, D., Howe, M. A, Huber, A., Jansen, A., Kellerer, J., Kernert, N., Kippenbrock, L., Kleesiek, M., Klein, M., Kopmann, A., Korzeczek, M., Kovalík, A., Krasch, B., Kraus, M., Kuckert, L., Lasserre, T., Lebeda, O., Letnev, J., Lokhov, A., Machatschek, M., Marsteller, A., Martin, E. L, Mertens, S., Mirz, S., Monreal, B., Neumann, H., Niemes, S., Off, A., Osipowicz, A., Otten, E., Parno, D. S, Pollithy, A., Poon, A. W P, Priester, F., Ranitzsch, P. C, Rest, O., Robertson, R. G H, Roccati, F., Rodenbeck, C., Röllig, M., Röttele, C., Ryšavý, M., Sack, R., Saenz, A., Schimpf, L., Schlösser, K., Schlösser, M., Schönung, K., Schrank, M., Seitz-Moskaliuk, H., Sentkerestiová, J., Slezák, M., Steidl, M., Steinbrink, N., Sturm, M., Suchopar, M., Suesser, M., Telle, H. H, Thorne, L. A, Thümmler, T., Titov, N., Tkachev, I., Trost, N., Valerius, K., Vénos, D., Vianden, R., Hernández, A. P V, Weber, M., Weinheimer, C., Weiss, C., Welte, S., Wendel, J., Wilkerson, J. F, Wolf, J., Wüstling, S., Zadoroghny, S., Buzinsky, Nicholas Gregory, Formaggio, Joseph A, Sibille, Valerian
    Foilsithe / Cruthaithe 2018
    ... on measuring the energy difference of two [superscript 83m]Kr conversion electron lines with the KATRIN setup...
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