Zobrazeno 1 - 10
of 175
pro vyhledávání: '"Storey, J. W. V."'
Autor:
Wang, Songhu, Zhang, Hui, Zhou, Xu, Zhou, Ji-Lin, Fu, Jian-Ning, Yang, Ming, Liu, Huigen, Xie, Jiwei, Wang, Lifan, Wang, Lingzhi, Wittenmyer, R. A., Ashley, M. C. B., Feng, Long-Long, Gong, Xuefei, Lawrence, J. S., Liu, Qiang, Luong-Van, D. M., Ma, Jun, Peng, Xiyan, Storey, J. W. V., Wu, Zhenyu, Yan, Jun, Yang, Huigen, Yang, Ji, Yuan, Xiangyan, Zhang, Tianmeng, Zhang, Xiaojia, Zhu, Zhenxi, Zou, Hu
The Chinese Small Telescope ARray (CSTAR) is the first telescope facility built at Dome A, Antarctica. During the 2008 observing season, the installation provided long-baseline and high-cadence photometric observations in the i-band for 18,145 target
Externí odkaz:
http://arxiv.org/abs/1505.01496
Autor:
Yang, Ming, Zhang, Hui, Wang, Songhu, Zhou, Ji-Lin, Zhou, Xu, Wang, Lingzhi, Wang, Lifan, Wittenmyer, R. A., Liu, Hui-Gen, Meng, Zeyang, Ashley, M. C. B., Storey, J. W. V., Bayliss, D., Tinney, Chris, Wang, Ying, Wu, Donghong, Liang, Ensi, Yu, Zhouyi, Fan, Zhou, Feng, Long-Long, Gong, Xuefei, Lawrence, J. S., Liu, Qiang, Luong-Van, D. M., Ma, Jun, Wu, Zhenyu, Yan, Jun, Yang, Huigen, Yang, Ji, Yuan, Xiangyan, Zhang, Tianmeng, Zhu, Zhenxi, Zou, Hu
Publikováno v:
ApJS,2015,217,28
The Chinese Small Telescope ARray (CSTAR) has observed an area around the Celestial South Pole at Dome A since 2008. About $20,000$ light curves in the i band were obtained lasting from March to July, 2008. The photometric precision achieves about 4
Externí odkaz:
http://arxiv.org/abs/1504.05281
Autor:
Wang, Songhu, Zhang, Hui, Zhou, Ji-Lin, Zhou, Xu, Yang, Ming, Wang, Lifan, Bayliss, D., Zhou, G., Ashley, M. C. B., Fan, Zhou, Feng, Long-Long, Gong, Xuefei, Lawrence, J. S., Liu, Huigen, Liu, Qiang, Luong-Van, D. M., Ma, Jun, Meng, Zeyang, Storey, J. W. V., Wittenmyer, R. A., Wu, Zhenyu, Yan, Jun, Yang, Huigen, Yang, Ji, Yang, Jiayi, Yuan, Xiangyan, Zhang, Tianmeng, Zhu, Zhenxi, Zou, Hu
The Chinese Small Telescope ARray (CSTAR) is a group of four identical, fully automated, static 14.5 cm telescopes. CSTAR is located at Dome A, Antarctica and covers 20 square degree of sky around the South Celestial Pole. The installation is designe
Externí odkaz:
http://arxiv.org/abs/1403.0086
Autor:
Storey, J. W. V.
In the 1970s the microwave spectroscopy group at Monash University became the first in the world to determine the spectral frequencies of urea, glycine, and several other biomolecules. We immediately searched for these at Parkes, using existing centi
Externí odkaz:
http://arxiv.org/abs/1210.0982
Autor:
Tremblin, P., Minier, V., Schneider, N., Durand, G. Al., Ashley, M. C. B., Lawrence, J. S., Luong-Van, D. M., Storey, J. W. V., Durand, G. An., Reinert, Y., Veyssiere, C., Walter, C., Ade, P., Calisse, P. G., Challita, Z., Fossat, E., Sabbatini, L., Pellegrini, A., Ricaud, P., Urban, J.
Over the past few years a major effort has been put into the exploration of potential sites for the deployment of submillimetre astronomical facilities. Amongst the most important sites are Dome C and Dome A on the Antarctic Plateau, and the Chajnant
Externí odkaz:
http://arxiv.org/abs/1110.4311
Autor:
Zhou, Xu, Fan, Zhou, Jiang, Zhaoji, Ashley, M. C. B., Cui, Xiangqun, Feng, Longlong, Gong, Xuefei, Hu, Jingyao, Kulesa, C. A., Lawrence, J. S., Liu, Genrong, Luong-Van, D. M., Ma, Jun, Moore, A. M., Qin, Weijia, Shang, Zhaohui, Storey, J. W. V., Sun, Bo, Travouillon, T., Walker, C. K., Wang, Jiali, Wang, Lifan, Wu, Jianghua, Wu, Zhenyu, Xia, Lirong, Yan, Jun, Yang, Ji, Yang, Huigen, Yuan, Xiangyan, York, D., Zhang, Zhanhai, Zhu, Zhenxi
In 2008 January the 24th Chinese expedition team successfully deployed the Chinese Small Telescope ARray (CSTAR) to DomeA, the highest point on the Antarctic plateau. CSTAR consists of four 14.5cm optical telescopes, each with a different filter (g,
Externí odkaz:
http://arxiv.org/abs/1001.4941
Autor:
Zou, Hu, Zhou, Xu, Jiang, Zhaoji, Ashley, M. C. B., Cui, Xiangqun, Feng, Longlong, Gong, Xuefei, Hu, Jingyao, Kulesa, C. A., Lawrence, J. S., Liu, Genrong, Luong-Van, D. M., Ma, Jun, Moore, A. M., Qin, Weijia, Shang, Zhaohui, Storey, J. W. V., Sun, Bo, Travouillon, T., Walker, C. K., Wang, Jiali, Wang, Lifan, Wu, Jianghua, Wu, Zhenyu, Xia, Lirong, Yan, Jun, Yang, Ji, Yang, Huigen, Yao, Yongqiang, Yuan, Xiangyan, York, D., Zhang, Zhanhai, Zhu, Zhenxi
The i-band observing conditions at Dome A on the Antarctic plateau have been investigated using data acquired during 2008 with the Chinese Small Telescope ARray. The sky brightness, variations in atmospheric transparency, cloud cover, and the presenc
Externí odkaz:
http://arxiv.org/abs/1001.4951
Autor:
Lawrence, J. S., Ashley, M. C. B., Bailey, J., Navascues, D. Barrado y, Bedding, T., Bland-Hawthorn, J., Bond, I., Bruntt, H., Burton, M. G., Cioni, M. -R., Eiroa, C., Epchtein, N., Kiss, L., Lagage, P. O., Minier, V., Mora, A., Olsen, K., Peri, P., Saunders, W., Stello, D., Storey, J. W. V., Tinney, C., Yock, P.
PILOT (the Pathfinder for an International Large Optical Telescope is a proposed 2.5 m optical/infrared telescope to be located at DomeC on the Antarctic plateau. The atmospheric conditions at Dome C deliver a high sensitivity, high photometric preci
Externí odkaz:
http://arxiv.org/abs/0905.4636
Autor:
Lawrence, J. S., Ashley, M. C. B., Bunker, A., Bouwens, R., Burgarella, D., Burton, M. G., Gehrels, N., Glazebrook, K., Pimbblet, K., Quimby, R., Saunders, W., Storey, J. W. V., Wheeler, J. C.
PILOT (the Pathfinder for an International Large Optical Telescope) is a proposed 2.5 m optical/infrared telescope to be located at Dome C on the Antarctic plateau. The atmospheric conditions at Dome C deliver a high sensitivity, high photometric pre
Externí odkaz:
http://arxiv.org/abs/0905.4616
Autor:
Lawrence, J. S., Ashley, M. C. B., Bailey, J., Navascues, D. Barrado y, Bedding, T., Bland-Hawthorn, J., Bond, I., Boulanger, F., Bouwens, R., Bruntt, H., Bunker, A., Burgarella, D., Burton, M. G., Busso, M., Coward, D., Cioni, M. -R., Durand, G., Eiroa, C., Epchtein, N., Gehrels, N., Gillingham, P., Glazebrook, K., Haynes, R., Kiss, L., Lagage, P. O., Bertre, T. Le, Mackay, C., Maillard, J. P., McGrath, A., Minier, V., Mora, A., Olsen, K., Persi, P., Pimbblet, K., Quimby, R., Saunders, W., Schmidt, B., Stello, D., Storey, J. W. V., Tinney, C., Tremblin, P., Wheeler, J. C., Yoc, P.
PILOT (the Pathfinder for an International Large Optical Telescope) is a proposed 2.5 m optical/infrared telescope to be located at Dome C on the Antarctic plateau. Conditions at Dome C are known to be exceptional for astronomy. The seeing (above ~30
Externí odkaz:
http://arxiv.org/abs/0905.4432