Zobrazeno 1 - 10
of 3 803
pro vyhledávání: '"Tan, C. P."'
Autor:
Cerny, W., Chiti, A., Geha, M., Mutlu-Pakdil, B., Drlica-Wagner, A., Tan, C. Y., Adamów, M., Pace, A. B., Simon, J. D., Sand, D. J., Ji, A. P., Li, T. S., Vivas, A. K., Bell, E. F., Carlin, J. L., Carballo-Bello, J. A., Chaturvedi, A., Choi, Y., Doliva-Dolinsky, A., Gnedin, O. Y., Limberg, G., Martínez-Vázquez, C. E., Mau, S., Medina, G. E., Navabi, M., Noël, N. E. D., Placco, V. M., Riley, A. H., Roederer, I. U., Stringfellow, G. S., Bom, C. R., Ferguson, P. S., James, D. J., Martínez-Delgado, D., Massana, P., Nidever, D. L., Sakowska, J. D., Santana-Silva, L., Sherman, N. F., Tollerud, E. J.
We present the discovery of Aquarius III, an ultra-faint Milky Way satellite galaxy identified in the second data release of the DECam Local Volume Exploration (DELVE) survey. Based on deeper follow-up imaging with DECam, we find that Aquarius III is
Externí odkaz:
http://arxiv.org/abs/2410.00981
Autor:
Tan, C. Y., Cerny, W., Drlica-Wagner, A., Pace, A. B., Geha, M., Ji, A. P., Li, T. S., Adamów, M., Anbajagane, D., Bom, C. R., Carballo-Bello, J. A., Carlin, J. L., Chang, C., Choi, Y., Collins, M. L. M., Doliva-Dolinsky, A., Ferguson, P. S., Gruendl, R. A., James, D. J., Limberg, G., Navabi, M., Martínez-Delgado, D., Martínez-Vázquez, C. E., Medina, G. E., Mutlu-Pakdil, B., Nidever, D. L., Noël, N. E. D., Riley, A. H., Sakowska, J. D., Sand, D. J., Sharp, J., Stringfellow, G. S., Tolley, C., Vivas, A. K.
We report the discovery and spectroscopic confirmation of an ultra-faint Milky Way (MW) satellite in the constellation of Leo. This system was discovered as a spatial overdensity of resolved stars observed with Dark Energy Camera (DECam) data from an
Externí odkaz:
http://arxiv.org/abs/2408.00865
Autor:
Tan, C. Y., Balcewicz, M.
The measurement of beam emittances by extracting the quadrupole mode signal from a 4 plate beam position monitor (BPM) was published at least 40 years ago. Unfortunately, in practice, this method suffers from poor signal to noise ratio and requires a
Externí odkaz:
http://arxiv.org/abs/2406.15238
Autor:
Grover, G., Bhat, N. D. R., McSweeney, S., Lee, C. P., Meyers, B. W., Tan, C. M., Kudale, S. S.
The phenomenon of pulsar nulling, where pulsars temporarily and stochastically cease their radio emission, is thought to be indicative of a `dying' pulsar, where radio emission ceases entirely. Here we report the discovery of a long-period pulsar, PS
Externí odkaz:
http://arxiv.org/abs/2405.16725
Autor:
McEwen, A. E., Swiggum, J. K., Kaplan, D. L., Tan, C. M., Meyers, B. W., Fonseca, E., Agazie, G. Y., Chawla, P., Crowter, K., DeCesar, M. E., Dolch, T., Dong, F. A., Fiore, W., Good, D. C., Istrate, A. G., Kaspi, V. M., Kondratiev, V. I., van Leeuwen, J., Levin, L., Lewis, E. F., Lynch, R. S., Masui, K. W., McKee, J. W., McLaughlin, M. A., Noori, H. Al, Parent, E., Ransom, S. M., Siemens, X., Spiewak, R., Stairs, I. H.
Publikováno v:
journal = {\apj}, year = 2024, month = feb, volume = {962}, number = {2}, pages = {167}
The Green Bank North Celestial Cap survey is one of the largest and most sensitive searches for pulsars and transient radio objects. Observations for the survey have finished; priorities have shifted toward long-term monitoring of its discoveries. In
Externí odkaz:
http://arxiv.org/abs/2312.07471
Autor:
van der Wateren, E., Bassa, C. G., Janssen, G. H., Yanes-Rizo, I. V., Casares, J., Nelemans, G., Stappers, B. W., Tan, C. M.
We report on radio timing observations of PSR J0210+5845 which reveal large deviations from typical pulsar spin-down behaviour. We interpret these deviations as being due to binary motion around the $V=13.5$ star 2MASS J02105640$+$5845176, which is c
Externí odkaz:
http://arxiv.org/abs/2312.01892
Autor:
Aguilar-Arevalo, A. A., Barrow, J. L., Bhat, C., Bogenschuetz, J., Bonifazi, C., Bross, A., Cervantes, B., D'Olivo, J., De Roeck, A., Dutta, B., Eads, M., Eldred, J., Estrada, J., Fava, A., Vilela, C. Fernandes, Moroni, G. Fernandez, Flaugher, B., Gardiner, S., Gurung, G., Gutierrez, P., Jang, W. Y., Kelly, K. J., Kim, D., Kobilarcik, T., Liu, Z., Lyu, K. F., Machado, P., Mahapatra, R., Marjanovic, M., Mastbaum, A., Pandey, V., Pellico, W., Perez, S., Reichenbacher, J., Rodrigues, D., Sousa, A., Simons, B., Snowden-Ifft, D., Tan, C. -Y., Toups, M., Tran, N., Tsai, Y. -T., Van de Water, R. G., Vilar, R., Westerdale, S., Yu, J., Zettlemoyer, J., Zwaska, R.
The Fermilab Proton-Improvement-Plan-II (PIP-II) is being implemented in order to support the precision neutrino oscillation measurements at the Deep Underground Neutrino Experiment, the U.S. flagship neutrino experiment. The PIP-II LINAC is presentl
Externí odkaz:
http://arxiv.org/abs/2311.09915
Publikováno v:
Risk Management and Healthcare Policy, Vol Volume 17, Pp 2829-2837 (2024)
Lidan Yi,1,* Qiao Liu,1,* Chongqing Tan,1 Xiaomin Wan,1 Xia Luo,1 Yinbo Li,2 Haiying Li,3 Xiaohui Zeng3 1Department of Pharmacy, The Second Xiangya Hospital of Central South University, Changsha, People’s Republic of China; 2Hunan Center fo
Externí odkaz:
https://doaj.org/article/187498f177ec4067b7d5c0dbd382a2a0
Autor:
Wijethunga, S. A. K., Eddy, N., Eldred, J., Tan, C. Y., Fellenz, B., Pozdeyev, E., Sharankova, R. V.
Fermilab Booster synchrotron requires an intensity upgrade from 4.5x1012 to 6.5x1012 protons per pulse as a part of Fermilab's Proton Improvement Plan-II (PIP-II). One of the factors which may limit the high-intensity performance is the fast transver
Externí odkaz:
http://arxiv.org/abs/2307.10450
Publikováno v:
Breast Cancer: Targets and Therapy, Vol Volume 16, Pp 705-723 (2024)
Chunlei Tan,1 Jinling Xu,2 Shiyuan Zhang,1 Shuqiang Liu,1 Xiaotian Yang,1 Danping Wu,1 Boqian Yu,1 Yuanxi Huang1 1Department of Breast Surgery, Harbin Medical University Cancer Hospital, Harbin, Heilongjiang, 150081, People’s Republic of China; 2En
Externí odkaz:
https://doaj.org/article/3f97c95570ab47faba480a288558d2db