Zobrazeno 1 - 10
of 1 790
pro vyhledávání: '"Gibson, H"'
Autor:
Proudfoot, Benjamin C. N., Ragozzine, Darin A., Thatcher, Meagan L., Grundy, Will, Spencer, Dallin J., Alailima, Tahina M., Allen, Sawyer, Bowden, Penelope C., Byrd, Susanne, Camacho, Conner D., Campbell, Gibson H., Carlisle, Edison P., Christensen, Jacob A., Christensen, Noah K., Clement, Kaelyn, Derieg, Benjamin J., Dille, Mara K., Dorrett, Cristian, Ellefson, Abigail L., Fleming, Taylor S., Freeman, N. J., Gibson, Ethan J., Giforos, William G., Guerrette, Jacob A., Haddock, Olivia, Hammond, S. Ashton, Hampson, Zachary A., Hancock, Joshua D., Harmer, Madeline S., Henderson, Joseph R., Jensen, Chandler R., Jensen, David, Jensen, Ryleigh E., Jones, Joshua S., Kubal, Cameron C., Lunt, Jacob N., Martins, Stephanie, Matheson, McKenna, Maxwell, Dahlia, Morrell, Timothy D., Myckowiak, McKenna M., Nelsen, Maia A., Neu, Spencer T., Nuccitelli, Giovanna G., Reardon, Kayson M., Reid, Austin S., Richards, Kenneth G., Robertson, Megan R. W., Rydalch, Tanner D., Scoresby, Conner B., Scott, Ryan L., Shakespear, Zacory D., Silveira, Elliot A., Steed, Grace C., Suggs, Christiana Z., Suggs, Garrett D., Tobias, Derek M., Toole, Matthew L., Townsend, McKayla L., Vickers, Kade L., Wagner, Collin R., Wright, Madeline S., Zappala, Emma M. A.
Publikováno v:
AJ 167 144 (2024)
About 40 transneptunian binaries (TNBs) have fully determined orbits with about 10 others being solved except for breaking the mirror ambiguity. Despite decades of study almost all TNBs have only ever been analyzed with a model that assumes perfect K
Externí odkaz:
http://arxiv.org/abs/2403.12783
Publikováno v:
Journal of Intelligent Systems, Vol 15, Iss 1-4, Pp 299-328 (2006)
Externí odkaz:
https://doaj.org/article/ba090aa93d664f30a53b1d2589354940
Autor:
Yagoubov, P., Mroczkowski, T., Belitsky, V., Cuadrado-Calle, D., Cuttaia, F., Fuller, G. A., Gallego, J. -D., Gonzalez, A., Kaneko, K., Mena, P., Molina, R., Nesti, R., Tapia, V., Villa, F., Beltran, M., Cavaliere, F., Ceru, J., Chesmore, G. E., Coughlin, K., De Breuck, C., Fredrixon, M., George, D., Gibson, H., Golec, J., Josaitis, A., Kemper, F., Kotiranta, M., Lapkin, I., Lopez-Fernandez, I., Marconi, G., Mariotti, S., McGenn, W., McMahon, J., Murk, A., Pezzotta, F., Phillips, N., Reyes, N., Ricciardi, S., Sandri, M., Strandberg, M., Terenzi, L., Testi, L., Thomas, B., Uzawa, Y., Vigano, D., Wadefalk, N.
Publikováno v:
A&A 634, A46 (2020)
ALMA has been operating since 2011, but has not yet been populated with the full suite of intended frequency bands. In particular, ALMA Band 2 (67-90 GHz) is the final band in the original ALMA band definition to be approved for production. We aim to
Externí odkaz:
http://arxiv.org/abs/1912.10841
Akademický článek
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