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Akademický článek
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Autor:
Eisner, N. L., Barragán, O., Aigrain, S., Lintott, C., Miller, G., Zicher, N., Boyajian, T. S., Briceño, C., Bryant, E. M., Christiansen, J. L., Feinstein, A. D., Flor-Torres, L. M., Fridlund, M., Gandolfi, D., Gilbert, J., Guerrero, N., Jenkins, J. M., Jones, K., Kristiansen, M. H., Vanderburg, A., Law, N., López-Sánchez, A. R., Mann, A. W., Safron, E. J., Schwamb, M. E., Stassun, K. G., Osborn, H. P., Wang, J., Zic, A., Ziegler, C., Barnet, F., Bean, S. J., Bundy, D. M., Chetnik, Z., Dawson, J. L., Garstone, J., Stenner, A. G., Huten, M., Larish, S., Melanson, L. D., Mitchell, T., Moore, C., Peltsch, K., Rogers, D. J., Schuster, C., Smith, D. S., Simister, D. J., Tanner, C., Terentev, I., Tsymbal, A.
We report on the discovery and validation of TOI 813b (TIC 55525572 b), a transiting exoplanet identified by citizen scientists in data from NASA's Transiting Exoplanet Survey Satellite (TESS) and the first planet discovered by the Planet Hunters TES
Externí odkaz:
http://arxiv.org/abs/1909.09094
Autor:
Milam, S. N., Hammel, H. B., Bauer, J., Brozovic, M., Grav, T., Holler, B. J., Lisse, C., Mainzer, A., Reddy, V., Schwamb, M. E., Spahr, T., Thomas, C. A., Woods, D.
Assess the joint capabilities of emerging telescopes for near-Earth objects (NEOs) survey and characterization, and what they will add to the current capabilities or replace. NASA telescopes in prime mission, in development, or under study, and reque
Externí odkaz:
http://arxiv.org/abs/1907.08972
Autor:
Blakeslee, J. P., Rodney, S. A., Lotz, J. M., Sivo, G., Sivanandam, S., Andersen, M., Carrasco, R., Ferrarese, L., Foley, R. J., Goodsell, S., Hirst, P., Jensen, J. B., Kelly, P. L., Kaurov, A. A., Lemoine-Busserolle, M., Miller, B. W., O'Meara, J., Roe, H., Schwamb, M. E., Scharwächter, J.
Two groundbreaking new facilities will commence operations early in the 2020s and thereafter define much of the broad landscape of US optical-infrared astronomy in the remaining decade. The Large Synoptic Survey Telescope (LSST), perched atop Cerro P
Externí odkaz:
http://arxiv.org/abs/1903.08184
Autor:
Gueye, P., Glister, A. A. Kabir J., Lee, B. W., Gilman, R., Higinbotham, D. W., Piasetzky, E., Ron, G., Sarty, A. J., Strauch, S., Adeyemi, A., Allada, K., Armstrong, W., Arrington, J., Arenhovel, H., Beck, A., Benmokhtar, F., Berman, B. L., Boeglin, W., Brash, E., Camsonne, A., Calarco, J., Chen, J. P., Choi, S., Chudakov, E., Coman, L., Craver, B., Cusanno, F., Dumas, J., Dutta, C., Feuerbach, R., Freyberger, A., Frullani, S., Garibaldi, F., Hansen, J. -O., Holmstrom, T., Hyde, C. E., Ibrahim, H., Ilieva, Y., Jiang, X., Jones, M. K., Katramatou, A. T., Kelleher, A., Khrosinkova, E., Kuchina, E., Kumbartzki, G., LeRose, J. J., Lindgren, R., Markowitz, P., Beck, S. May-Tal, McCullough, E., Meekins, D., Meziane, M., Meziani, Z. -E., Michaels, R., Moffit, B., Norum, B. E., Petratos, G. G., Oh, Y., Olson, M., Paolone, M., Paschke, K., Perdrisat, C. F., Potokar, M., Pomatsalyuk, R., Pomerantz, I., Puckett, A., Punjabi, V., Qian, X., Qiang, Y., Ransome, R. D., Reyhan, M., Roche, J., Rousseau, Y., Sawatzky, B., Schulte, E., Schwamb, M., Shabestari, M., Shahinyan, A., Shneor, R., Sirca, S., Slifer, K., Solvignon, P., Song, J., Sparks, R., Subedi, R., Urciuoli, G. M., Wang, K., Wojtsekhowski, B., Yan, X., Yao, H., Zhan, X., Zhu, X.
Publikováno v:
Eur. Phys. J. A 56 (2020) 126
Measurements of elastic electron scattering data within the past decade have highlighted two-photon exchange contributions as a necessary ingredient in theoretical calculations to precisely evaluate hydrogen elastic scattering cross sections. This co
Externí odkaz:
http://arxiv.org/abs/1805.12441
Autor:
Brasser, R., Schwamb, M. E.
The detached object Sedna is likely at the inner edge of the Oort cloud, more precisely the inner Oort cloud (IOC). Until recently it was the sole member of this population. The recent discovery of the detached object 2012 VP113 has confirmed that th
Externí odkaz:
http://arxiv.org/abs/1411.1844
Autor:
Zhang, Z. -W., Lehner, M. J., Wang, J. -H., Wen, C. -Y., Wang, S. -Y., King, S. -K., Granados, Á. P., Alcock, C., Axelrod, T., Bianco, F. B., Byun, Y. -I., Chen, W. P., Coehlo, N. K., Cook, K. H., de Pater, I., Kim, D. -W., Lee, T., Lissauer, J. J., Marshall, S. L., Protopapas, P., Rice, J. A., Schwamb, M. E.
The Taiwanese-American Occultation Survey (TAOS) aims to detect serendipitous occultations of stars by small (about 1 km diameter) objects in the Kuiper Belt and beyond. Such events are very rare (<0.001 events per star per year) and short in duratio
Externí odkaz:
http://arxiv.org/abs/1301.6182
Autor:
Matheson, T., Joyce, R. R., Allen, L. E., Saha, A., Silva, D. R., Wood-Vasey, W. M., Adams, J. J., Anderson, R. E., Beck, T. L., Bentz, M. C., Bershady, M. A., Binkert, W. S., Butler, K., Camarata, M. A., Eigenbrot, A., Everett, M., Gallagher, J. S., Glikman, P. M. Garnavich E., Harbeck, D., Hargis, J. R., Herbst, H., Horch, E. P., Howell, S. B., Jha, S., Kaczmarek, J. F., Knezek, P., Manne-Nicholas, E., Mathieu, R. D., Meixner, M., Milliman, K., Power, J., Rajagopal, J., Reetz, K., Rhode, K. L., Schechtman-Rook, A., Schwamb, M. E., Schweiker, H., Simmons, B., Simon, J. D., Summers, D., Young, M. D., Weyant, A., Wilcots, E. M., Will, G., Williams, D.
We present near infra-red light curves of supernova (SN) 2011fe in M101, including 34 epochs in H band starting fourteen days before maximum brightness in the B-band. The light curve data were obtained with the WIYN High-Resolution Infrared Camera (W
Externí odkaz:
http://arxiv.org/abs/1205.3828
Autor:
Huang, K. Y., Urata, Y., Tung, Y. H., Lin, H. M., Xin, L. P., Yoshida, M., Zheng, W., Akerlof, C., Wang, S. Y., Ip, W. H., Lehner, M. J., Bianco, F. B., Kawai, N., Kuroda, D., Marshall, S. L., Schwamb, M. E., Qiu, Y., Wang, J. H., Wen, C. Y., Wei, J., Yanagisawa, K., Zhang, Z. W.
We present the study on GRB 071112C X-ray and optical light curves. In these two wavelength ranges, we have found different temporal properties. The R-band light curve showed an initial rise followed by a single power-law decay, while the X-ray light
Externí odkaz:
http://arxiv.org/abs/1202.1356
We analyse the origin of three Centaurs with perihelia in the range 15 AU to 30 AU, inclinations above 70 deg and semi-major axes shorter than 100 AU. Based on long-term numerical simulations we conclude that these objects most likely originate from
Externí odkaz:
http://arxiv.org/abs/1111.7037