Zobrazeno 1 - 10
of 652
pro vyhledávání: '"Taylor, C. J. A."'
Autor:
Cladera, Fernando, Miller, Ian D., Ravichandran, Zachary, Murali, Varun, Hughes, Jason, Hsieh, M. Ani, Taylor, C. J., Kumar, Vijay
One common and desirable application of robots is exploring potentially hazardous and unstructured environments. Air-ground collaboration offers a synergistic approach to addressing such exploration challenges. In this paper, we demonstrate a system
Externí odkaz:
http://arxiv.org/abs/2405.07169
Autor:
Kaul, Prannay, Li, Zhizhong, Yang, Hao, Dukler, Yonatan, Swaminathan, Ashwin, Taylor, C. J., Soatto, Stefano
Mitigating hallucinations in large vision-language models (LVLMs) remains an open problem. Recent benchmarks do not address hallucinations in open-ended free-form responses, which we term "Type I hallucinations". Instead, they focus on hallucinations
Externí odkaz:
http://arxiv.org/abs/2405.05256
Autor:
Cladera, Fernando, Ravichandran, Zachary, Miller, Ian D., Hsieh, M. Ani, Taylor, C. J., Kumar, Vijay
Multi-robot collaboration in large-scale environments with limited-sized teams and without external infrastructure is challenging, since the software framework required to support complex tasks must be robust to unreliable and intermittent communicat
Externí odkaz:
http://arxiv.org/abs/2309.15975
Akademický článek
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Publikováno v:
2017 ApJ 835 16
Measurements of the lithium isotopic ratio in the diffuse interstellar medium from high-resolution spectra of the LiI {\lambda}6708 resonance doublet have now been reported for a number of lines of sight. The majority of the results for the 7Li/6Li r
Externí odkaz:
http://arxiv.org/abs/1704.00357
Akademický článek
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Publikováno v:
Astrophys. J., 750:L15 (6pp), 2012
We present an analysis of 7Li/6Li isotope ratios along four sight lines that probe diffuse molecular gas near the supernova remnant IC 443. Recent gamma-ray observations have revealed the presence of shock-accelerated cosmic rays interacting with the
Externí odkaz:
http://arxiv.org/abs/1203.6057
We present optical spectroscopy of nine cataclysmic binary stars, mostly dwarf novae, obtained primarily to determine orbital periods Porb. The stars and their periods are LX And, 0.1509743(5) d; CZ Aql, 0.2005(6) d; LU Cam, 0.1499686(4) d; GZ Cnc, 0
Externí odkaz:
http://arxiv.org/abs/0704.0948
Autor:
Shemmer, O., Romano, P., Bertram, R., Brinkmann, W., Collier, S., Crowley, K. A., Detsis, E., Filippenko, A. V., Gaskell, C. M., George, T. A., Gliozzi, M., Hiller, M. E., Jewell, T. L., Kaspi, S., Klimek, E. S., Lannon, M. H., Li, W., Martini, P., Mathur, S., Negoro, H., Netzer, H., Papadakis, I., Papamastorakis, I., Peterson, B. M., Peterson, B. W., Pogge, R. W., Pronik, V. I., Rumstay, K. S., Sergeev, S. G., Sergeeva, E. A., Stirpe, G. M., Taylor, C. J., Treffers, R. R., Turner, T. J., Uttley, P., Vestergaard, M., von Braun, K., Wagner, R. M., Zheng, Z.
We present the results of a two-year long optical monitoring program of the narrow-line Seyfert 1 galaxy Akn 564. The majority of this monitoring project was also covered by X-ray observations (RXTE) and for a period of ~50 days, we observed the gala
Externí odkaz:
http://arxiv.org/abs/astro-ph/0107075
Autor:
Thorstensen, J. R., Taylor, C. J.
Publikováno v:
Mon.Not.Roy.Astron.Soc. 326 (2001) 1235
We present spectroscopy and orbital periods Porb of four relatively little-studied cataclysmic variable stars. The stars and their periods are: AF Cam, Porb = 0.324(1) d (the daily cycle count is slightly ambiguous); V2069 Cyg (= RX J2123.7+4217), 0.
Externí odkaz:
http://arxiv.org/abs/astro-ph/0105499