Zobrazeno 1 - 10
of 2 299
pro vyhledávání: '"BUTLER, B. P."'
Subsurface Thermophysical Properties of Europa's Leading and Trailing Hemispheres as Revealed by ALM
We present best-fit values of porosity -- and the corresponding effective thermal inertiae -- determined from three different depths in Europa's near-subsurface (~1-20 cm). The porosity of the upper ~20 cm of Europa's subsurface varies between 75-50%
Externí odkaz:
http://arxiv.org/abs/2402.01952
Akademický článek
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Autor:
Lellouch, E., Butler, B., Moreno, R., Gurwell, M., Lavvas, P., Bertrand, T., Fouchet, T., Strobel, D. F., Moullet, A.
Following the detection of CO and HCN in Pluto's atmosphere, we report on new ALMA observations of Pluto with two main goals: (i) obtaining spatially-resolved measurements (~0.06'' on the ~0.15'' disk subtended by Pluto and its atmosphere) of CO(3-2)
Externí odkaz:
http://arxiv.org/abs/2109.12866
Akademický článek
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Akademický článek
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Autor:
Law, C. J., Butler, B. J., Prochaska, J. X., Zackay, B., Burke-Spolaor, S., Mannings, A., Tejos, N., Josephy, A., Andersen, B., Chawla, P., Heintz, K. E., Aggarwal, K., Bower, G. C., Demorest, P. B., Kilpatrick, C. D., Lazio, T. J. W., Linford, J., Mckinven, R., Tendulkar, S., Simha, S.
We present the discovery and subarcsecond localization of a new Fast Radio Burst with the Karl G. Jansky Very Large Array and realfast search system. The FRB was discovered on 2019 June 14 with a dispersion measure of 959 pc/cm3. This is the highest
Externí odkaz:
http://arxiv.org/abs/2007.02155
Autor:
Carilli, C. L., Murphy, E., Rosero, V., Mooley, K., Jimenez-Andrade, E., Golap, K., Butler, B.
We investigate the imaging performance of an interferometric array in the case of wide field, high resolution, narrow band, snapshot imaging. We find that, when uv-cell sizes are sufficiently small (ie. image sizes are sufficiently large), each insta
Externí odkaz:
http://arxiv.org/abs/2007.00712
Autor:
Marcote, B., Nimmo, K., Hessels, J. W. T., Tendulkar, S. P., Bassa, C. G., Paragi, Z., Keimpema, A., Bhardwaj, M., Karuppusamy, R., Kaspi, V. M., Law, C. J., Michilli, D., Aggarwal, K., Andersen, B., Archibald, A. M., Bandura, K., Bower, G. C., Boyle, P. J., Brar, C., Burke-Spolaor, S., Butler, B. J., Cassanelli, T., Chawla, P., Demorest, P., Dobbs, M., Fonseca, E., Giri, U., Good, D. C., Gourdji, K., Josephy, A., Kirichenko, A. Yu., Kirsten, F., Landecker, T. L., Lang, D., Lazio, T. J. W., Li, D. Z., Lin, H. -H., Linford, J. D., Masui, K., Mena-Parra, J., Naidu, A., Ng, C., Patel, C., Pen, U. -L., Pleunis, Z., Rafiei-Ravandi, M., Rahman, M., Renard, A., Scholz, P., Siegel, S. R., Smith, K. M., Stairs, I. H., Vanderlinde, K., Zwaniga, A. V.
Fast radio bursts (FRBs) are brief, bright, extragalactic radio flashes. Their physical origin remains unknown, but dozens of possible models have been postulated. Some FRB sources exhibit repeat bursts. Though over a hundred FRB sources have been di
Externí odkaz:
http://arxiv.org/abs/2001.02222
Autor:
Law, C. J., Omand, C. M. B., Kashiyama, K., Murase, K., Bower, G. C., Aggarwal, K., Burke-Spolaor, S., Butler, B. J., Demorest, P., Lazio, T. J. W., Linford, J., Tendulkar, S. P., Rupen, M. P.
We present results of a search for late-time radio emission and Fast Radio Bursts (FRBs) from a sample of type-I superluminous supernovae (SLSNe-I). We used the Karl G. Jansky Very Large Array to observe ten SLSN-I more than 5 years old at a frequenc
Externí odkaz:
http://arxiv.org/abs/1910.02036
Autor:
Lacy, M., Baum, S. A., Chandler, C. J., Chatterjee, S., Clarke, T. E., Deustua, S., English, J., Farnes, J., Gaensler, B. M., Gugliucci, N., Hallinan, G., Kent, B. R., Kimball, A., Law, C. J., Lazio, T. J. W., Marvil, J., Mao, S. A., Medlin, D., Mooley, K., Murphy, E. J., Myers, S., Osten, R., Richards, G. T., Rosolowsky, E., Rudnick, L., Schinzel, F., Sivakoff, G. R., Sjouwerman, L. O., Taylor, R., White, R. L., Wrobel, J., Andernach, H., Beasley, A. J., Berger, E., Bhatnagar, S., Birkinshaw, M., Bower, G. C., Brandt, W. N., Brown, S., Burke-Spolaor, S., Butler, B. J., Comerford, J., Demorest, P. B., Fu, H., Giacintucci, S., Golap, K., Guth, T., Hales, C. A., Hiriart, R., Hodge, J., Horesh, A., Ivezic, Z., Jarvis, M. J., Kamble, A., Kassim, N., Liu, X., Loinard, L., Lyons, D. K., Masters, J., Mezcua, M., Moellenbrock, G. A., Mroczkowski, T., Nyland, K., O'Dea, C. P., O'Sullivan, S. P., Peters, W. M., Radford, K., Rao, U., Robnett, J., Salcido, J., Shen, Y., Sobotka, A., Witz, S., Vaccari, M., van Weeren, R. J., Vargas, A., Williams, P. K. G., Yoon, I.
The Very Large Array Sky Survey (VLASS) is a synoptic, all-sky radio sky survey with a unique combination of high angular resolution ($\approx$2.5"), sensitivity (a 1$\sigma$ goal of 70 $\mu$Jy/beam in the coadded data), full linear Stokes polarimetr
Externí odkaz:
http://arxiv.org/abs/1907.01981