Zobrazeno 1 - 10
of 111
pro vyhledávání: '"collaboration, the PLANET"'
Autor:
Batista, Virginie, Gould, A., Dieters, S., Dong, Subo, Bond, I., Beaulieu, J. P., Maoz, D., Monard, B., Christie, G. W., McCormick, J., Albrow, M. D., Horne, K., Tsapras, Y., Burgdorf, M. J., Novati, S. Calchi, Skottfelt, J., Caldwell, J., Kozlowski, S., Kubas, D., Gaudi, B. S., Han, C., Bennett, D. P., An, J., Collaboration, the MOA, Collaboration, the PLANET, Collaboration, the MicroFUN, Consortium, the MiNDSTEp, Collaboration, the RoboNet
We report the discovery of a planet with a high planet-to-star mass ratio in the microlensing event MOA-2009-BLG-387, which exhibited pronounced deviations over a 12-day interval, one of the longest for any planetary event. The host is an M dwarf, wi
Externí odkaz:
http://arxiv.org/abs/1102.0558
Autor:
Miyake, N., Sumi, T., Dong, Subo, Street, R., Mancini, L., Gould, A., Bennett, D. P., Tsapras, Y., Yee, J. C., Albrow, M. D., Bond, I. A., Fouque, P., Browne, P., Han, C., Snodgrass, C., Finet, F., Furusawa, K., Harpsoe, K., Allen, W., Hundertmark, M., Freeman, M., Suzuki, D., Abe, F., Botzler, C. S., Douchin, D., Fukui, A., Hayashi, F., Hearnshaw, J. B., Hosaka, S., Itow, Y., Kamiya, K., Kilmartin, P. M., Korpela, A., Lin, W., Ling, C. H., Makita, S., Masuda, K., Matsubara, Y., Muraki, Y., Nagayama, T., Nishimoto, K., Ohnishi, K., Perrott, Y. C., Rattenbury, N., Saito, To., Skuljan, L., Sullivan, D. J., Sweatman, W. L., Tristram, P. J., Wada, K., Yock, P. C. M., Collaboration, The MOA, Bolt, G., Bos, M., Christie, G. W., DePoy, D. L., Drummond, J., Gal-Yam, A., Gaudi, B. S., Gorbikov, E., Higgins, D., Janczak, K. -H. Hwang J., Kaspi, S., Lee, C. -U., Koo, J. -R., lowski, S. Koz, Lee, Y., Mallia, F., Maury, A., Maoz, D., McCormick, J., Monard, L. A. G., Moorhouse, D., Mu~noz, J. A., Natusch, T., Ofek, E. O., Pogge, R. W., Polishook, D., Santallo, R., Shporer, A., Spector, O., Thornley, G., Collaboration, The Micro FUN, Allan, A., Bramich, D. M., Horne, K., Kains, N., Steele, I., Collaboration, The RoboNet, Bozza, V., Burgdorf, M. J., Novati, S. Calchi, Dominik, M., Dreizler, S., Glitrup, M., Hessman, F. V., Hinse, T. C., Jorgensen, U. G., Liebig, C., Maier, G., Mathiasen, M., Rahvar, S., Ricci, D., Scarpetta, G., Skottfelt, J., Southworth, J., Surdej, J., Wambsganss, J., Zimmer, F., Consortium, The MiNDSTEp, Batista, V., Beaulieu, J. P., Brillant, S., Cassan, A., Cole, A., Corrales, E., Coutures, Ch., Dieters, S., Greenhill, J., Kubas, D., Menzies, J., Collaboration, The PLANET
We report the gravitational microlensing discovery of a sub-Saturn mass planet, MOA-2009-BLG-319Lb, orbiting a K or M-dwarf star in the inner Galactic disk or Galactic bulge. The high cadence observations of the MOA-II survey discovered this microlen
Externí odkaz:
http://arxiv.org/abs/1010.1809
Autor:
Sumi, T., Bennett, D. P., Bond, I. A., Udalski, A., Batista, V., Dominik, M., Fouqué, P., Kubas, D., Gould, A., Macintosh, B., Cook, K., Dong, S., Skuljan, L., Cassan, A., Collaboration, The MOA, Abe, F., Botzler, C. S., Fukui, A., Furusawa, K., Hearnshaw, J. B., Itow, Y., Kamiya, K., Kilmartin, P. M., Korpela, A., Lin, W., Ling, C. H., Masuda, K., Matsubara, Y., Miyake, N., Muraki, Y., Nagaya, M., Nagayama, T., Ohnishi, K., Okumura, T., Perrott, Y. C., Rattenbury, N., Saito, To., Sako, T., Sullivan, D. J., Sweatman, W. L., Yock, P. C. M., Collaboration, The PLANET, Beaulieu, J. P., Cole, A., Coutures, Ch., Duran, M. F., Greenhill, J., Jablonski, F., Marboeuf, U., Martioli, E., Pedretti, E., Pejcha, O., Rojo, P., Albrow, M. D., Brillant, S., Bode, M., Bramich, D. M., Burgdorf, M. J., Caldwell, J. A. R., Calitz, H., Corrales, E., Dieters, S., Prester, D. Dominis, Donatowicz, J., Hill, K., Hoffman, M., Horne, K., J, U. G., Kains, N., Kane, S., Marquette, J. B., Martin, R., Meintjes, P., Menzies, J., Pollard, K. R., Sahu, K. C., Snodgrass, C., Steele, I., Street, R., Tsapras, Y., Wambsganss, J., Williams, A., Zub, M., Collaboration, The OGLE, Szyma, M. K., Kubiak, M., Pietrzy, G., Soszy, I., Szewczyk, O., Ulaczyk, K., Collaboration, The microFUN, Allen, W., Christie, G. W., DePoy, D. L., Gaudi, B. S., Han, C., Janczak, J., Lee, C. -U., McCormick, J., Mallia, F., Monard, B., Natusch, T., Park, B. -G., Pogge, R. W., Santallo, R.
Publikováno v:
Astrophys.J.710:1641-1653,2010
We present the discovery of a Neptune-mass planet OGLE-2007-BLG-368Lb with a planet-star mass ratio of q=[9.5 +/- 2.1] x 10^{-5} via gravitational microlensing. The planetary deviation was detected in real-time thanks to the high cadence of the MOA s
Externí odkaz:
http://arxiv.org/abs/0912.1171
Autor:
Janczak, Julia, Fukui, A., Dong, Subo, Monard, B., Kozlowski, Szymon, Gould, A., Beaulieu, J. P., Kubas, Daniel, Marquette, J. B., Sumi, T., Bond, I. A., Bennett, D. P., collaboration, the MOA, collaboration, the MicroFUN, collaboration, the MiNDSTEp, collaboration, the PLANET
Publikováno v:
Astrophys.J.711:731-743,2010
We report the detection of sub-Saturn-mass planet MOA-2008-BLG-310Lb and argue that it is the strongest candidate yet for a bulge planet. Deviations from the single-lens fit are smoothed out by finite-source effects and so are not immediately apparen
Externí odkaz:
http://arxiv.org/abs/0908.0529
Autor:
Yee, J. C., Udalski, A., Sumi, T., Dong, Subo, Kozłowski, S., Bird, J. C., Cole, A., Higgins, D., McCormick, J., Monard, B., Polishook, D., Shporer, A., Spector, O., OGLE, the, microFUN, the, MOA, the, Collaboration, the PLANET
We analyze the extreme high-magnification microlensing event OGLE-2008-BLG-279, which peaked at a maximum magnification of A ~ 1600 on 30 May 2008. The peak of this event exhibits both finite-source effects and terrestrial parallax, from which we det
Externí odkaz:
http://arxiv.org/abs/0907.5411
Autor:
Gaudi, B. S., Albrow, M. D., An, J., Beaulieu, J. -P., Caldwell, J. A. R., DePoy, D. L., Dominik, M., Gould, A., Greenhill, J., Hill, K., Kane, S., Martin, R., Menzies, J., Naber, R. M., Pel, J. -W., Pogge, R. W., Pollard, K. R., Sackett, P. D., Sahu, K. C., Vermaak, P., Vreeswijk, P. M., Watson, R., Williams, A., Collaboration, The PLANET
We analyze five years of PLANET photometry of microlensing events toward the Galactic bulge to search for the short-duration deviations from single lens light curves that are indicative of the presence of planetary companions to the primary microlens
Externí odkaz:
http://arxiv.org/abs/astro-ph/0104100
Autor:
Albrow, M. D., An, J., Beaulieu, J. -P., Caldwell, J. A. R., DePoy, D. L., Dominik, M., Gaudi, B. S., Gould, A., Greenhill, J., Hill, K., Kane, S., Martin, R., Menzies, J., Naber, R. M., Pel, J. -W., Pogge, R. W., Pollard, K. R., Sackett, P. D., Sahu, K. C., Vermaak, P., Vreeswijk, P. M., Watson, R., Williams, A., Collaboration, The PLANET
We search for signatures of planets in 43 intensively monitored microlensing events that were observed between 1995 and 1999. Planets would be expected to cause a short duration (~1 day) deviation on the smooth, symmetric light curve produced by a si
Externí odkaz:
http://arxiv.org/abs/astro-ph/0008078
Autor:
Dominik, M., Albrow, M. D., Beaulieu, J. -P., Caldwell, J. A. R., DePoy, D. L., Gaudi, B. S., Gould, A., Greenhill, J., Hill, K., Kane, S., Martin, R., Menzies, J., Naber, R. M., Pel, J. -W., Pogge, R. W., Pollard, K. R., Sackett, P. D., Sahu, K. C., Vermaak, P., Watson, R., Williams, A., collaboration, The PLANET
Among various techniques to search for extra-solar planets, microlensing has some unique characteristics. Contrary to all other methods which favour nearby objects, microlensing is sensitive to planets around stars at distances of several kpc. These
Externí odkaz:
http://arxiv.org/abs/astro-ph/9910465
Autor:
BURR, JENNI
Publikováno v:
Legacy (National Association for Interpretation); May/Jun2013, Vol. 24 Issue 3, p28-29, 2p
Autor:
Janczak, Julia, Fukui, A., Dong, Subo, Monard, B., Kozlowski, Szymon, Gould, A., Beaulieu, J. P., Kubas, Daniel, Marquette, J. B., Sumi, T., Bond, I. A., Bennett, D. P., collaboration, the MOA, collaboration, the MicroFUN, collaboration, the MiNDSTEp, collaboration, the PLANET
Publikováno v:
The Astrophysical Journal. 711:731-743
We report the detection of sub-Saturn-mass planet MOA-2008-BLG-310Lb and argue that it is the strongest candidate yet for a bulge planet. Deviations from the single-lens fit are smoothed out by finite-source effects and so are not immediately apparen
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::085cf973096d5636b90fd14ef409bb75
https://doi.org/10.1088/0004-637x/711/2/731
https://doi.org/10.1088/0004-637x/711/2/731