Zobrazeno 1 - 10
of 56
pro vyhledávání: '"P. C. M. Yock"'
Autor:
Tsapras, Y., Choi, J. -Y., Street, R. A., Han, C., Bozza, V., Gould, A., Dominik, M., Beaulieu, J. -P., Udalski, A., Jørgensen, U. G., Sumi, T., Bramich, D. M., Browne, P., Horne, K., Hundertmark, M., Ipatov, S., Kains, N., Snodgrass, C., Steele, I. A., Alsubai, K. A., Andersen, J. M., Novati, S. Calchi, Damerdji, Y., Diehl, C., Elyiv, A., Giannini, E., Hardis, S., Harpsøe, K., Hinse, T. C., Juncher, D., Kerins, E., Korhonen, H., Liebig, C., Mancini, L., Mathiasen, M., Penny, M. T., Rabus, M., Rahvar, S., Scarpetta, G., Skottfelt, J., Southworth, J., Surdej, J., Tregloan-Reed, J., Vilela, C., Wambsganss, J., Skowron, J., Poleski, R., Kozłowski, S., Wyrzykowski, Łukasz, Szymański, M. K., Kubiak, M., Pietrukowicz, P., Pietrzyński, G., Soszyński, I., Ulaczyk, K., Albrow, M. D., Bachelet, E., Barry, R., Batista, V., Bhattacharya, A., Brillant, S., Caldwell, J. A. R., Cassan, A., Cole, A., Corrales, E., Coutures, Ch., Dieters, S., Prester, D. Dominis, Donatowicz, J., Fouqué, P., Greenhill, J., Kane, S. R., Kubas, D., Marquette, J. -B., Menzies, J., P`ere, C., Pollard, K. R., Wouters, D., Christie, G., DePoy, D. L., Dong, S., Drummond, J., Gaudi, B. S., Henderson, C. B., Hwang, K. H., Jung, Y. K., Kavka, A., Koo, J. -R., Lee, C. -U., Maoz, D., Monard, L. A. G., Natusch, T., Ngan, H., Park, H., Pogge, R. W., Porritt, I., Shin, I. -G., Shvartzvald, Y., Tan, T. G., Yee, J. C., Abe, F., Bennett, D. P., Bond, I. A., Botzler, C. S., Freeman, M., Fukui, A., Fukunaga, D., Itow, Y., Koshimoto, N., Ling, C. H., Masuda, K., Matsubara, Y., Muraki, Y., Namba, S., Ohnishi, K., Rattenbury, N. J., Saito, To., Sullivan, D. J., Sweatman, W. L., Suzuki, D., Tristram, P. J., Tsurumi, N., Wada, K., Yamai, N., Yonehara, P. C. M. Yock A.
We present a detailed analysis of survey and follow-up observations of microlensing event OGLE-2012-BLG-0406 based on data obtained from 10 different observatories. Intensive coverage of the lightcurve, especially the perturbation part, allowed us to
Externí odkaz:
http://arxiv.org/abs/1310.2428
Autor:
Hwang, K. -H., Han, C., Bond, I. A., Miyake, N., Abe, F., Bennett, D. P., Botzler, C. S., Fukui, A., Furusawa, K., 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., Nishimoto, K., Ohnishi, K., Perrott, Y. C., Rattenbury, N., Saito, To., Sako, T., Skuljan, L., Sullivan, D. J., Sumi, T., Suzuki, D., Sweatman, W. L., Tristram, J., Wada, K., L., P. C. M. Yock D., Depoy, Gaudi, B. S., Gould, A., Lee, C. -U., Pogge, R. W.
We report the result of the analysis of the light curve of the microlensing event MOA-2009-BLG-016. The light curve is characterized by a short-duration anomaly near the peak and an overall asymmetry. We find that the peak anomaly is due to a binary
Externí odkaz:
http://arxiv.org/abs/1006.1396
Autor:
I.-G. Shin, Andrew Gould, P. Pietrukowicz, Naoki Koshimoto, Darren L. DePoy, Igor Soszyński, K. Wada, S. Kozlowski, Lydia C. Philpott, Michael D. Albrow, Łukasz Wyrzykowski, C. H. Ling, Denis J. Sullivan, Yasushi Muraki, Ian A. Bond, Jack D. Drummond, Paul J. Tristram, Atsunori Yonehara, Jennifer C. Yee, Nicholas J. Rattenbury, Jan Skowron, C.-U. Lee, R. W. Pogge, D. Maoz, S. Namba, Tim Natusch, K. Ohnishi, C. Han, To. Saito, N. Tsurumi, G. Pietrzynski, P. Mróz, Yutaka Matsubara, M. Friedmann, J.-Y. Choi, A. Fukui, Krzysztof Ulaczyk, Daisuke Suzuki, Radek Poleski, K.-H. Hwang, D. Fukunaga, M. Kubiak, Shai Kaspi, Yossi Shvartzvald, H. Ngan, C. S. Botzler, G. W. Christie, Thiam-Guan Tan, Takahiro Sumi, Kimiaki Masuda, B. S. Gaudi, Fumio Abe, Jennie McCormick, I. Porritt, David P. Bennett, Yoshitaka Itow, Youn Kil Jung, P. C. M. Yock, H. Park, Andrzej Udalski, Michał K. Szymański, P. Larsen, N. Yamai, M. Freeman
Publikováno v:
Science. 345:46-49
We detect a cold, terrestrial planet in a binary-star system using gravitational microlensing. The planet has low mass (2 Earth masses) and lies projected at $a_{\perp,ph}$ ~ 0.8 astronomical units (AU) from its host star, similar to the Earth-Sun di
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d45170a54db29d5292cf50e8d28609a9
https://doi.org/10.1126/science.1251527
https://doi.org/10.1126/science.1251527
Autor:
A. de Ugarte Postigo, P. C. M. Yock, Ian A. Bond, T. de J. Mateo Sanguino, O. Rabaza-Castillo, S. Guziy, Rafael Fernández-Muñoz, G. W. Christie, Stanislav Vítek, Chenzhou Cui, L. Sabau-Graziati, Yi-Zhong Fan, O. Lara-Gil, S. Castillo-Carrión, I. Kheyfets, William H. Allen, J. C. Tello, A. J. Castro-Tirado, R. Sanchez-Ramirez, D. Pérez-Ramírez, Petr Kubánek, J. Gorosabel, B. A. de la Morena Carretero, Il Han Park, Martin Jelínek, René Hudec, J. A. Díaz Andreu, J. M. Castro Cerón, Ronan Cunniffe, C. Perez del Pulgar
Publikováno v:
EAS Publications Series. 61:251-254
The Burst Observer and Optical Transient Exploring System (BOOTES), is a global robotic observatory network, which started in 1998 with Spanish leadership devoted to study optical emissions from gamma ray bursts (GRBs) that occur in the Universe. We
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1979be883886484ab6ef7d156d8be39b
https://doi.org/10.1051/eas/1361038
https://doi.org/10.1051/eas/1361038
Autor:
M. Nagaya, Denis J. Sullivan, Ian A. Bond, Kisaku Kamiya, J. B. Hearnshow, P. M. Kilmartin, Paul J. Tristram, K. Ohnishi, Susumu Sato, Kimiaki Masuda, T. K. Sako, K. Furusawa, Yoshimi Matsubara, Yasushi Muraki, Takahiro Sumi, P. C. M. Yock, Toshifumi Yanagisawa, S. Noda, Fumio Abe, N. Miyake, Yoshitaka Itow, Akihiko Fukui, T. Saito
Publikováno v:
Proceedings of the International Astronomical Union. 4:366-369
The Microlensing Observations in Astrophysics (MOA) is a microlensing survey conducted at Mt. John Observatory in New Zealand. We searched transiting planet candidates from the MOA-I Galactic bulge data, which have been obtained with a 61cm B&C teles
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::645b7cfd8d3cc0c809058358633c0eff
https://doi.org/10.1017/s1743921308026665
https://doi.org/10.1017/s1743921308026665
Autor:
David P. Bennett, Yoshitaka Itow, Kimiaki Masuda, V. Batista, Arnaud Cassan, Chang S. Han, J. W. Menzies, M. Zub, P. Fouqué, Kailash C. Sahu, P. C. M. Yock, Michael D. Albrow, Andrew Williams, S. Dieters, J. Donatowicz, Yasushi Muraki, M. Hundertmark, J.-P. Beaulieu, J.-B. Marquette, N. Kains, D. Dominis Prester, Atsunori Yonehara, Ch. Coutures, Yutaka Matsubara, Martin Dominik, Winston L. Sweatman, Keith Horne, K. R. Pollard, Joachim Wambsganss, Kouji Ohnishi, B. S. Gaudi, Byeong-Gon Park, J. G. Greenhill, Subo Dong, S. R. Kane, Nicholas J. Rattenbury, Andrew Gould, U. G. Jørgensen, Clément Ranc, Yiannis Tsapras, Paul J. Tristram, Ian A. Bond, Denis J. Sullivan, Takahiro Sumi, D. Kubas, Rachel Street, Fumio Abe, To. Saito, Akihiko Fukui, C.-U. Lee, Etienne Bachelet
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2015, 580, ⟨10.1051/0004-6361/201525791⟩
Astronomy and Astrophysics-A&A, 2015, 580, ⟨10.1051/0004-6361/201525791⟩
We present the analysis of MOA-2007-BLG-197Lb, the first brown dwarf companion to a Sun-like star detected through gravitational microlensing. The event was alerted and followed-up photometrically by a network of telescopes from the PLANET, MOA, and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::24f56eaec55e53d823244be5b276365a
https://hal-insu.archives-ouvertes.fr/insu-03644894/file/aa25791-15.pdf
https://hal-insu.archives-ouvertes.fr/insu-03644894/file/aa25791-15.pdf
Autor:
Joseph M. Anderson, Jennie McCormick, Darren L. DePoy, Igor Soszyński, Krzysztof Z. Stanek, Richard W. Pogge, Ian A. Bond, Shude Mao, G. W. Christie, Andrzej Udalski, O. Szewczyk, Michał K. Szymański, P. C. M. Yock, C. Han, M. Kubiak, Bohdan Paczynski, L. Wyrzykowski, David P. Bennett, Iain A. Steele, M. F. Bode, Martin Burgdorf, K. Ulaczyk, Subo Dong, C. S. Botzler, Deokkeun An, Shawn Poindexter, Grzegorz Pietrzyński, Keith Horne, D. M. Bramich, S. C. Swaving, N. J. Rattenbury, B. S. Gaudi, Colin Snodgrass, Byeong-Gon Park, A. Y. Zhou, Andrew Gould
Publikováno v:
The Astrophysical Journal. 644:L37-L40
We detect a Neptune mass-ratio (q~8e-5) planetary companion to the lens star in the extremely high-magnification (A~800) microlensing event OGLE-2005-BLG-169. If the parent is a main-sequence star, it has mass M~0.5 M_sun implying a planet mass of ~1
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::13d34e98af7db3ba598fd26ef5249413
https://doi.org/10.1086/505421
https://doi.org/10.1086/505421
Autor:
Matthew Whiting, Wilfred M. Walsh, Peter G. Tuthill, Michael C. B. Ashley, Jon Lawrence, Joss Bland-Hawthorn, Rob Sharp, Sarah T. Maddison, P. C. M. Yock, Geraint F. Lewis, Michael G. Burton, C. H. Smith, Ian A. Bond, Timothy R. Bedding, Jeremy Bailey, C. G. Tinney, Chris Blake, M. G. Hidas, Andrew Walsh, Vincent Minier, Karl Glazebrook, Seppo Mattila, John W. V. Storey, Stuart D. Ryder, Steven N. Longmore, David D. Woods, Tony Wong
Publikováno v:
Publications of the Astronomical Society of Australia. 22:199-235
The cold, dry and stable air above the summits of the Antarctic plateau provides the best ground-based observing conditions from optical to sub-mm wavelengths to be found on the Earth. PILOT is a proposed 2 m telescope, to be built at Dome C in Antar
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f1bdd4d6db4f4596209afa5db8254739
https://doi.org/10.1071/as04077
https://doi.org/10.1071/as04077
Autor:
Y. Kato, S. Noda, To. Saito, Takahiro Sumi, R. J. Dodd, Mareki Honma, Masaki Sekiguchi, Nicholas J. Rattenbury, Fumio Abe, John B. Hearnshaw, Yukitoshi Kan-ya, Hiroshi Sato, M. Yoshizawa, Kimiaki Masuda, Yasushi Muraki, Morihiro Honda, M. Reid, J. Skuljan, Ian A. Bond, P. M. Kilmartin, R. Yamada, M. Takeuti, P. C. M. Yock, Y. Saito, Toshifumi Yanagisawa, Yoshimi Matsubara, Denis J. Sullivan, T. Nakamura, Jun Jugaku, K. Ohnishi
Publikováno v:
International Astronomical Union Colloquium. 193:332-335
More than 4000 stars observed in both MOA and DENIS projects showing periodic or quasi-periodic light curves are studied. Almost all Mira stars are located on the classical period-luminosity relation, and the multiplicity of the period-luminosity rel
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::6169ac9bdd84db0def16743c91d6d6f2
https://doi.org/10.1017/s0252921100010885
https://doi.org/10.1017/s0252921100010885
Autor:
M. Reid, Y. Matsubara, Kimiaki Masuda, Ian A. Bond, Takahiro Sumi, O. K. L. Petterson, P. M. Kilmartin, Ryoichi Nishi, P. J. Tristram, S. Noda, Yoshihiko Saito, Yukitoshi Kan-ya, Toshifumi Yanagisawa, Y. Muraki, S. Wilkinson, Denis J. Sullivan, Mareki Honma, Fumio Abe, R. J. Dodd, K. Ohnishi, John B. Hearnshaw, N. J. Rattenbury, Hiroshi Sato, P. C. M. Yock, To. Saito, Morihiro Honda, J. Skuljan, Masaki Sekiguchi, M. Takeuti, T. Nakamura
Publikováno v:
The Astrophysical Journal. 591:204-227
We analyze the data of the gravitational microlensing survey carried out by by the MOA group during 2000 towards the Galactic Bulge (GB). Our observations are designed to detect efficiently high magnification events with faint source stars and short
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::802c0846786e2aa9f54c27da9a023978
https://doi.org/10.1086/375212
https://doi.org/10.1086/375212