Zobrazeno 1 - 10
of 28
pro vyhledávání: '"Hundertmark, M. P. G."'
Autor:
Street, R. A., Bachelet, E., Tsapras, Y., Hundertmark, M. P. G., Bozza, V., Bramich, D. M., Cassan, A., Dominik, M., Jaimes, R. Figuera, Horne, K., Mao, S., Saha, A., Wambsganss, J., Zang, Weicheng
The ROME/REA (Robotic Observations of Microlensing Events/Reactive Event Assessment) Survey was a Key Project at Las Cumbres Observatory (hereafter LCO) which continuously monitored 20 selected fields (3.76 sq.deg.) in the Galactic Bulge throughout t
Externí odkaz:
http://arxiv.org/abs/2403.05987
Autor:
Street, R. A., Gough-Kelly, S., Lam, C., Varela, A., Makler, M., Bachelet, E., Lu, J. R., Abrams, N., Pusack, A., Terry, S., Di~Stefano, R., Tsapras, Y., Hundertmark, M. P. G., Grand, R. J. J., Daylan, T., Sobeck, J.
[Abridged] The Nancy Grace Roman Space Telescope will be one of several flagship survey facilities operating over the next decade starting $\sim$2025. The deep near-IR imaging that Roman will deliver will be highly complementary to the capabilities o
Externí odkaz:
http://arxiv.org/abs/2306.13792
Autor:
Street, R. A., Li, X., Khakpash, S., Bellm, E., Girardi, L., Jones, L., Abrams, N. S., Tsapras, Y., Hundertmark, M. P. G., Bachelet, E., Gandhi, P., Szkody, P., Clarkson, W. I., Szabo, R., Prisinzano, L., Bonito, R., Buckley, D. A. H., Marais, J. P., Di Stefano, R.
Galactic science encompasses a wide range of subjects in the study of the Milky Way and Magellanic Clouds, from Young Stellar Objects to X-ray Binaries. Mapping these populations, and exploring transient phenomena within them, are among the primary s
Externí odkaz:
http://arxiv.org/abs/2305.11988
Autor:
Bachelet, E., Tsapras, Y., Gould, Andrew, Street, R. A., Bennett, David P., Hundertmark, M. P. G., Bozza, V., Bramich, D. M., Cassan, A., Dominik, M., Horne, K., Mao, S., Saha, A., Wambsganss, J., Zang, Weicheng, Abe, Fumio, Barry, Richard, Bhattacharya, Aparna, Bond, Ian A., Fukui, Akihiko, Fujii, Hirosane, Hirao, Yuki, Itow, Yoshitaka, Kirikawa, Rintaro, Koshimoto, Naoki, Matsubara, Yutaka, Matsumoto, Sho, Miyazaki, Shota, Muraki, Yasushi, Olmschenk, Greg, Ranc, Clément, Okamura, Arisa, Rattenbury, Nicholas J., Satoh, Yuki, Sumi, Takahiro, Suzuki, Daisuke, Silva, Stela Ishitani, Toda, Taiga, Tristram, Paul . J., Vandorou, Aikaterini, Yama, Hibiki, Albrow, Michael D., Chung, Sun-Ju, Han, Cheongho, Hwang, Kyu-Ha, Jung, Youn Kil, Ryu, Yoon-Hyun, Shin, In-Gu, Shvartzvald, Yossi, Yee, Jennifer C., Cha, Sang-Mok, Kim, Dong-Jin, Kim, Seung-Lee, Lee, Chung-Uk, Lee, Dong-Joo, Lee, Yongseok, Park, Byeong-Gon, Pogge, Richard W., Udalski, Andrzej, Mróz, Przemek, Poleski, Rados law, Skowron, Jan, Szymański, Micha l K., Soszyński, Igor, Pietrukowicz, Pawe l, Kozlowski, Szymon, Ulaczyk, Krzysztof, Rybicki, Krzysztof A., Iwanek, Patryk, Wrona, Marcin, Gromadzki, Mariusz
We report on the observations, analysis and interpretation of the microlensing event MOA-2019- BLG-008. The observed anomaly in the photometric light curve is best described through a binary lens model. In this model, the source did not cross caustic
Externí odkaz:
http://arxiv.org/abs/2205.07522
Autor:
Miyazaki, Shota, Sumi, Takahiro, Bennett, David P., Udalski, Andrzej, Shvartzvald, Yossi, Street, Rachel, Bozza, Valerio, Yee, Jennifer C., Bond, Ian A., Rattenbury, Nicholas, Koshimoto, Naoki, Suzuki, Daisuke, Fukui, Akihiko, Abe, F., Bhattacharya, A., Barry, R., Donachie, M., Fujii, H., Hirao, Y., Itow, Y., Kamei, Y., Kondo, I., Li, M. C. A., Ling, C. H., Matsubara, Y., Matsuo, T., Muraki, Y., Nagakane, M., Ohnishi, K., Ranc, C., Saito, T., Sharan, A., Shibai, H., Suematsu, H., Sullivan, D. J., Tristram, P. J., Yamakawa, T., Yonehara, A., Skowron, J., Poleski, R., Mr'oz, P., Szyma'nski, M. K., Soszy'nski, I., Pietrukowicz, P., KozLowski, S., Ulaczyk, K., Wyrzykowski, L., Friedmann, Matan, Kaspi, Shai, Maoz, Dan, Albrow, M., Christie, G., DePoy, D. L., Gal-Yam, A., Gould, A., Lee, C. -U., Manulis, I., McCormick, J., Natusch, T., Ngan, H., Pogge, R. W., Porritt, I., Tsapras, Y., Bachelet, E., Hundertmark, M. P. G., Dominik, M., Bramich, D. M., Cassan, A., Jaimes, R. Figuera, Horne, K., Schmidt, R., Snodgrass, C., Wambsganss, J., Steele, I. A., Menzies, J., Mao, S., Jorgensen, U. G., Burgdorf, M. J., Ciceri, S., Novati, S. Calchi, D'Ago, G., Evans, D. F., Hinse, T. C., Kains, N., Kerins, E., Korhonen, H., Mancini, L., Popovas, A., Rabus, M., Rahvar, S., Scarpetta, G., Skottfelt, J., Southworth, J., Peixinho, N., Verma, P.
We present the analysis of the binary-lens microlensing event OGLE-2013-BLG-0911. The best-fit solutions indicate the binary mass ratio of q~0.03 which differs from that reported in Shvartzvald+2016. The event suffers from the well-known close/wide d
Externí odkaz:
http://arxiv.org/abs/1912.09613
Autor:
Street, R. A., Bachelet, E., Tsapras, Y., Hundertmark, M. P. G., Bozza, V., Dominik, M., Bramich, D. M., Cassan, A., Horne, K., Mao, S., Saha, A., Wambsganss, J., Zang, Weicheng, Jorgensen, U. G., Longa-Pena, P., Peixinho, N., Sajadian, S., Burgdorf, M. J., Campbell-White, J., Dib, S., Evans, D. F., Fujii, Y. I., Hinse, T. C., Khalouei, E., Lowry, S., Rahvar, S., Rabus, M., Skottfelt, J., Snodgrass, C., Southworth, J., Tregloan-Reed, J.
We report observations of the binary microlensing event OGLE-2018-BLG-0022, provided by the ROME/REA Survey, which indicate that the lens is a low-mass binary star consisting of M3 (0.375+/-0.020 Msun) and M7 (0.098+/-0.005 Msun) components. The lens
Externí odkaz:
http://arxiv.org/abs/1903.08733
Autor:
Street, R. A., Lund, M. B., Donachie, M., Khakpash, S., Golovich, N., Penny, M., Bennett, D., Dawson, W. A., Pepper, J., Rabus, M., Szkody, P., Clarkson, W. I., Di Stefano, R., Rattenbury, N., Hundertmark, M. P. G., Tsapras, Y., Ridgway, S., Stassun, K., Bozza, V., Bhattacharya, A., Novati, S. Calchi, Shvartzvald, Y.
NASA's WFIRST mission will perform a wide-field, NIR survey of the Galactic Bulge to search for exoplanets via the microlensing techniques. As the mission is due to launch in the mid-2020s, around half-way through the LSST Main Survey, we have a uniq
Externí odkaz:
http://arxiv.org/abs/1812.04445
Autor:
Street, R. A., Lund, M. B., Khakpash, S., Donachie, M., Dawson, W. A., Golovich, N., Wyrzykowski, L., Szkody, P., Naylor, T., Penny, M., Rattenbury, N., Dall'Ora, M., Clarkson, W. I., Bennett, D., Pepper, J., Rabus, M., Hundertmark, M. P. G., Tsapras, Y., Di Stefano, R., Ridgway, S., Liu, M., Lin, E.
The overwhelming majority of objects visible to LSST lie within the Galactic Plane. Though many previous surveys have avoided this region for fear of stellar crowding, LSST's spatial resolution combined with its state-of-the-art Difference Image Anal
Externí odkaz:
http://arxiv.org/abs/1812.03137
Spitzer Microlensing Program as a Probe for Globular Cluster Planets. Analysis of OGLE-2015-BLG-0448
Autor:
Poleski, Radosław, Zhu, Wei, Christie, Grant W., Udalski, Andrzej, Gould, Andrew, Bachelet, Etienne, Skottfelt, Jesper, Novati, Sebastiano Calchi, Szymański, M. K., Soszyński, I., Pietrzyński, G., Wyrzykowski, Ł., Ulaczyk, K., Pietrukowicz, P., Kozłowski, Szymon, Skowron, J., Mróz, P., Pawlak, M., Beichman, C., Bryden, G., Carey, S., Fausnaugh, M., Gaudi, B. S., Henderson, C. B., Pogge, R. W., Shvartzvald, Y., Wibking, B., Yee, J. C., Beatty, T. G., Eastman, J. D., Drummond, J., Friedmann, M., Henderson, M., Johnson, J. A., Kaspi, S., Maoz, D., McCormick, J., McCrady, N., Natusch, T., Ngan, H., Porritt, I., Relles, H. M., Sliski, D. H., Tan, T. -G., Wittenmyer, R. A., Wright, J. T., Street, R. A., Tsapras, Y., Bramich, D. M., Horne, K., Snodgrass, C., Steele, I. A., Menzies, J., Jaimes, R. Figuera, Wambsganss, J., Schmidt, R., Cassan, A., Ranc, C., Mao, S., Bozza, V., Dominik, M., Hundertmark, M. P. G., Jørgensen, U. G., Andersen, M. I., Burgdorf, M. J., Ciceri, S., D'Ago, G., Evans, D. F., Gu, S. -H., Hinse, T. C., Kains, N., Kerins, E., Korhonen, H., Kuffmeier, M., Mancini, L., Popovas, A., Rabus, M., Rahvar, S., Rasmussen, R. T., Southworth, G. Scarpetta J., Surdej, J., Unda-Sanzana, E., Verma, P., von Essen, C., Wang, Y. -B., Wertz, O.
The microlensing event OGLE-2015-BLG-0448 was observed by Spitzer and lay within the tidal radius of the globular cluster NGC 6558. The event had moderate magnification and was intensively observed, hence it had the potential to probe the distributio
Externí odkaz:
http://arxiv.org/abs/1512.08520
Autor:
Street, R. A., Udalski, A., Novati, S. Calchi, Hundertmark, M. P. G., Zhu, W., Gould, A., Yee, J., Tsapras, Y., Bennett, D. P., Project, The RoboNet, Consortium, MiNDSTEp, Jorgensen, U. G., Dominik, M., Andersen, M. I., Bachelet, E., Bozza, V., Bramich, D. M., Burgdorf, M. J., Cassan, A., Ciceri, S., D'Ago, G., Dong, Subo, Evans, D. F., Gu, Sheng-hong, Harkonnen, H., Hinse, T. C., Horne, Keith, Jaimes, R. Figuera, Kains, N., Kerins, E., Korhonen, H., Kuffmeier, M., Mancini, L., Menzies, J., Mao, S., Peixinho, N., Popovas, A., Rabus, M., Rahvar, S., Ranc, C., Rasmussen, R. Tronsgaard, Scarpetta, G., Schmidt, R., Skottfelt, J., Snodgrass, C., Southworth, J., Steele, I. A., Surdej, J., Unda-Sanzana, E., Verma, P., von Essen, C., Wambsganss, J., Wang, Yi-Bo., Wertz, O., Project, The OGLE, Poleski, R., Pawlak, M., Szymanski, M. K., Skowron, J., Mroz, P., Kozlowski, S., Wyrzykowski, L., Pietrukowicz, P., Pietrzynski, G., Soszynski, I., Ulaczyk, K., Beichman, The Spitzer Team C., Bryden, G., Carey, S., Gaudi, B. S., Henderson, C., Pogge, R. W., Shvartzvald, Y., Collaboration, The MOA, Abe, F., Asakura, Y., Bhattacharya, A., Bond, I. A., Donachie, M., Freeman, M., Fukui, A., Hirao, Y., Inayama, K., Itow, Y., Koshimoto, N., Li, M. C. A., Ling, C. H., Masuda, K., Matsubara, Y., Muraki, Y., Nagakane, M., Nishioka, T., Ohnishi, K., Oyokawa, H., Rattenbury, N., Saito, To., Sharan, A., Sullivan, D. J., Sumi, T., Suzuki, D., Tristram, J., Wakiyama, Y., Yonehara, A., Han, KMTNet Modeling Team C., Choi, J. -Y., Park, H., Jung, Y. K., Shin, I. -G.
We report the detection of a Cold Neptune m_planet=21+/-2MEarth orbiting a 0.38MSol M dwarf lying 2.5-3.3 kpc toward the Galactic center as part of a campaign combining ground-based and Spitzer observations to measure the Galactic distribution of pla
Externí odkaz:
http://arxiv.org/abs/1508.07027