Search Results - "dwarf planet"

Studying the Solar system with the International Pulsar Timing Array by Caballero, R., Guo, Y., Lee, K., Lazarus, P., Champion, D., Desvignes, G., Kramer, M., Plant, K., Arzoumanian, Z., Bailes, M., Bassa, C., Bhat, Ramesh, Brazier, A., Burgay, M., Burke-Spolaor, S., Chamberlin, S., Chatterjee, S., Cognard, I., Cordes, J., Dai, S., Demorest, P., Dolch, T., Ferdman, R., Fonseca, E., Gair, J., Garver-Daniels, N., Gentile, P., Gonzalez, M., Graikou, E., Guillemot, L., Hobbs, G., Janssen, G., Karuppusamy, R., Keith, M., Kerr, M., Lam, M., Lasky, P., Lazio, T., Levin, L., Liu, K., Lommen, A., Lorimer, D., Lynch, R., Madison, D., Manchester, R., McKee, J., McLaughlin, M., McWilliams, S., Mingarelli, C., Nice, D., Osiowski, S., Palliyaguru, N., Pennucci, T., Perera, B., Perrodin, D., Possenti, A., Ransom, S., Reardon, D., Sanidas, S., Sesana, A., Shaifullah, G., Shannon, Ryan, Siemens, X., Simon, J., Spiewak, R., Stairs, I., Stappers, B., Stinebring, D., Stovall, K., Swiggum, J., Taylor, S., Theureau, G., Tiburzi, C.

“…Constraints on planetary-system masses have been improved by factors of up to 20 from the previous relevant study using the same assumptions, with the mass of the Jovian system measured at 9.5479189(3) × 10-4M?. The mass of the dwarf planet Ceres is measured at 4.7(4) × 10-10M?. We also present the first sensitivity curves using real data that place generic limits on the masses of UMOs, which can also be used as upper limits on the mass of putative exotic objects. …”
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Moa-2010-BLG-073L: An m-dwarf with a substellar companion at the planet/brown dwarf boundary by Street, R., Choi, J., Tsapras, Y., Han, C., Furusawa, K., Hundertmark, M., Gould, A., Sumi, T., Bond, I., Wouters, D., Zellem, R., Udalski, A., Snodgrass, C., Horne, K., Dominik, M., Browne, P., Kains, N., Bramich, D., Bajek, D., Steele, I., Ipatov, S., Abe, F., Bennett, D., Botzler, C., Chote, P., Freeman, M., Fukui, A., Harris, P., Itow, Y., Ling, C., Masuda, K., Matsubara, Y., Miyake, N., Muraki, Y., Nagayama, T., Nishimaya, S., Ohnishi, K., Rattenbury, N., Saito, T., Sullivan, D., Suzuki, D., Sweatman, W., Tristram, P., Wada, K., Yock, P., Szymanski, M., Kubiak, M., Pietrzynski, G., Soszynski, I., Poleski, R., Ulaczyk, K., Wyrzykowski, L., Yee, J., Dong, S., Shin, I., Lee, C., Skowron, J., Andrade de Almeida, L., DePoy, D., Gaudi, B., Hung, L., Jablonski, F., Kaspi, S., Klein, N., Hwang, K., Koo, J., Maoz, D., Munoz, J., Pogge, R., Polishhook, D., Shporer, A., McCormick, J., Christie, G., Natusch, T., Allen, B., Drummond, J., Moorhouse, D., Thornley, G., Knowler, M., Bos, M., Bolt, G., Beaulieu, J., Albrow, M., Batista, V., Brillant, S., Caldwell, J., Cassan, A., Cole, A., Corrales, E., Coutures, C., Dieters, S., Dominis Prester, D., Donatowicz, J., Fouque, P., Bachelet, E., Greenhill, J., Kane, S., Kubas, D., Marquette, J., Martin, R., Menzies, J., Pollard, K., Sahu, K., Wambsganss, J., Williams, Andrew, Zub, M., Alsubai, K., Bozza, V., Burgdorf, M., Calchi Novati, S., Dodds, P., Dreizler, S., Finet, F., Gerner, T., Hardis, S., Harpsoe, K., Hessman, F., Hinse, T., Jorgensen, U., Kerins, E., Liebig, C., Mancini, L., Mathiasen, M., Penny, M., Proft, S., Rahvar, S., Ricci, D., Scarpetta, G., Schafer, S., Schonebeck, F., Southworth, J., Surdej, J.

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