Zobrazeno 1 - 10
of 966
pro vyhledávání: '"Rogers, P F"'
Autor:
Kuchera, A. N., Shahid, R., Zhao, J., Edmondson, A., DeYoung, P. A., Frank, N., McDonaugh, J., Peterson-Veatch, O., Rogers, W. F., Redpath, T., Thoennessen, M.
Background: $^{15}$Be is an unbound nuclide that has been observed to decay by one-neutron emission. Shell model calculations predict two low-lying states in its energy spectrum, however, only a single resonance has been observed from coincident meas
Externí odkaz:
http://arxiv.org/abs/2411.04927
Autor:
Anderson, Seamus L., Benedix, Gretchen K., Godel, Belinda, Alosius, Romain M. L., Krietsch, Daniela, Busemann, Henner, Maden, Colin, Friedrich, Jon M., McMonigal, Lara R., Welten, Kees C., Caffee, Marc W., Macke, Robert J., Cadogan, Seán, Ryan, Dominic H., Jourdan, Fred, Mayers, Celia, Laubenstein, Matthias, Greenwood, Richard C., Roberts, Malcom P., Devillepoix, Hadrien A. R., Sansom, Eleanor K., Towner, Martin C., Cupák, Martin, Bland, Philip A., Forman, Lucy V., Fairweather, John H., Rogers, Ashley F., Timms, Nicholas E.
Over the Nullarbor Plain in South Australia, the Desert Fireball Network detected a fireball on the night of 1 June 2019 (7:30 pm local time), and six weeks later recovered a single meteorite (42 g) named Arpu Kuilpu. This meteorite was then distribu
Externí odkaz:
http://arxiv.org/abs/2409.10382
Autor:
Rogers, Axl F., van Straten, Willem, Gulyaev, Sergei, Parthasarathy, Aditya, Hobbs, George, Chen, Zu-Cheng, Feng, Yi, Goncharov, Boris, Kapur, Agastya, Liu, Xiaojin, Reardon, Daniel, Russell, Christopher J., Zic, Andrew
This paper demonstrates the impact of state-of-the-art instrumental calibration techniques on the precision of arrival times obtained from 9.6 years of observations of millisecond pulsars using the Murriyang 64-m CSIRO Parkes Radio Telescope. Our stu
Externí odkaz:
http://arxiv.org/abs/2407.20015
Autor:
The International Pulsar Timing Array Collaboration, Agazie, G., Antoniadis, J., Anumarlapudi, A., Archibald, A. M., Arumugam, P., Arumugam, S., Arzoumanian, Z., Askew, J., Babak, S., Bagchi, M., Bailes, M., Nielsen, A. -S. Bak, Baker, P. T., Bassa, C. G., Bathula, A., Bécsy, B., Berthereau, A., Bhat, N. D. R., Blecha, L., Bonetti, M., Bortolas, E., Brazier, A., Brook, P. R., Burgay, M., Burke-Spolaor, S., Burnette, R., Caballero, R. N., Cameron, A., Case, R., Chalumeau, A., Champion, D. J., Chanlaridis, S., Charisi, M., Chatterjee, S., Chatziioannou, K., Cheeseboro, B. D., Chen, S., Chen, Z. -C., Cognard, I., Cohen, T., Coles, W. A., Cordes, J. M., Cornish, N. J., Crawford, F., Cromartie, H. T., Crowter, K., Curyło, M., Cutler, C. J., Dai, S., Dandapat, S., Deb, D., DeCesar, M. E., DeGan, D., Demorest, P. B., Deng, H., Desai, S., Desvignes, G., Dey, L., Dhanda-Batra, N., Di Marco, V., Dolch, T., Drachler, B., Dwivedi, C., Ellis, J. A., Falxa, M., Feng, Y., Ferdman, R. D., Ferrara, E. C., Fiore, W., Fonseca, E., Franchini, A., Freedman, G. E., Gair, J. R., Garver-Daniels, N., Gentile, P. A., Gersbach, K. A., Glaser, J., Good, D. C., Goncharov, B., Gopakumar, A., Graikou, E., Grießmeier, J. -M., Guillemot, L., Gültekin, K., Guo, Y. J., Gupta, Y., Grunthal, K., Hazboun, J. S., Hisano, S., Hobbs, G. B., Hourihane, S., Hu, H., Iraci, F., Islo, K., Izquierdo-Villalba, D., Jang, J., Jawor, J., Janssen, G. H., Jennings, R. J., Jessner, A., Johnson, A. D., Jones, M. L., Joshi, B. C., Kaiser, A. R., Kaplan, D. L., Kapur, A., Kareem, F., Karuppusamy, R., Keane, E. F., Keith, M. J., Kelley, L. Z., Kerr, M., Key, J. S., Kharbanda, D., Kikunaga, T., Klein, T. C., Kolhe, N., Kramer, M., Krishnakumar, M. A., Kulkarni, A., Laal, N., Lackeos, K., Lam, M. T., Lamb, W. G., Larsen, B. B., Lazio, T. J. W., Lee, K. J., Levin, Y., Lewandowska, N., Littenberg, T. B., Liu, K., Liu, T., Liu, Y., Lommen, A., Lorimer, D. R., Lower, M. E., Luo, J., Luo, R., Lynch, R. S., Lyne, A. G., Ma, C. -P., Maan, Y., Madison, D. R., Main, R. A., Manchester, R. N., Mandow, R., Mattson, M. A., McEwen, A., McKee, J. W., McLaughlin, M. A., McMann, N., Meyers, B. W., Meyers, P. M., Mickaliger, M. B., Miles, M., Mingarelli, C. M. F., Mitridate, A., Natarajan, P., Nathan, R. S., Ng, C., Nice, D. J., Niţu, I. C., Nobleson, K., Ocker, S. K., Olum, K. D., Osłowski, S., Paladi, A. K., Parthasarathy, A., Pennucci, T. T., Perera, B. B. P., Perrodin, D., Petiteau, A., Petrov, P., Pol, N. S., Porayko, N. K., Possenti, A., Prabu, T., Leclere, H. Quelquejay, Radovan, H. A., Rana, P., Ransom, S. M., Ray, P. S., Reardon, D. J., Rogers, A. F., Romano, J. D., Russell, C. J., Samajdar, A., Sanidas, S. A., Sardesai, S. C., Schmiedekamp, A., Schmiedekamp, C., Schmitz, K., Schult, L., Sesana, A., Shaifullah, G., Shannon, R. M., Shapiro-Albert, B. J., Siemens, X., Simon, J., Singha, J., Siwek, M. S., Speri, L., Spiewak, R., Srivastava, A., Stairs, I. H., Stappers, B. W., Stinebring, D. R., Stovall, K., Sun, J. P., Surnis, M., Susarla, S. C., Susobhanan, A., Swiggum, J. K., Takahashi, K., Tarafdar, P., Taylor, J., Taylor, S. R., Theureau, G., Thrane, E., Thyagarajan, N., Tiburzi, C., Toomey, L., Turner, J. E., Unal, C., Vallisneri, M., van der Wateren, E., van Haasteren, R., Vecchio, A., Krishnan, V. Venkatraman, Verbiest, J. P. W., Vigeland, S. J., Wahl, H. M., Wang, S., Wang, Q., Witt, C. A., Wang, J., Wang, L., Wayt, K. E., Wu, Z., Young, O., Zhang, L., Zhang, S., Zhu, X. -J., Zic, A.
The Australian, Chinese, European, Indian, and North American pulsar timing array (PTA) collaborations recently reported, at varying levels, evidence for the presence of a nanohertz gravitational wave background (GWB). Given that each PTA made differ
Externí odkaz:
http://arxiv.org/abs/2309.00693
Autor:
Reardon, Daniel J., Zic, Andrew, Shannon, Ryan M., Di Marco, Valentina, Hobbs, George B., Kapur, Agastya, Lower, Marcus E., Mandow, Rami, Middleton, Hannah, Miles, Matthew T., Rogers, Axl F., Askew, Jacob, Bailes, Matthew, Bhat, N. D. Ramesh, Cameron, Andrew, Kerr, Matthew, Kulkarni, Atharva, Manchester, Richard N., Nathan, Rowina S., Russell, Christopher J., Osłowski, Stefan, Zhu, Xing-Jiang
The noise in millisecond pulsar (MSP) timing data can include contributions from observing instruments, the interstellar medium, the solar wind, solar system ephemeris errors, and the pulsars themselves. The noise environment must be accurately chara
Externí odkaz:
http://arxiv.org/abs/2306.16229
Autor:
Zic, Andrew, Reardon, Daniel J., Kapur, Agastya, Hobbs, George, Mandow, Rami, Curyło, Małgorzata, Shannon, Ryan M., Askew, Jacob, Bailes, Matthew, Bhat, N. D. Ramesh, Cameron, Andrew, Chen, Zu-Cheng, Dai, Shi, Di Marco, Valentina, Feng, Yi, Kerr, Matthew, Kulkarni, Atharva, Lower, Marcus E., Luo, Rui, Manchester, Richard N., Miles, Matthew T., Nathan, Rowina S., Osłowski, Stefan, Rogers, Axl F., Russell, Christopher J., Sarkissian, John M., Shamohammadi, Mohsen, Spiewak, Renée, Thyagarajan, Nithyanandan, Toomey, Lawrence, Wang, Shuangqiang, Zhang, Lei, Zhang, Songbo, Zhu, Xing-Jiang
We present the third data release from the Parkes Pulsar Timing Array (PPTA) project. The release contains observations of 32 pulsars obtained using the 64-m Parkes "Murriyang" radio telescope. The data span is up to 18 years with a typical cadence o
Externí odkaz:
http://arxiv.org/abs/2306.16230
Autor:
Reardon, Daniel J., Zic, Andrew, Shannon, Ryan M., Hobbs, George B., Bailes, Matthew, Di Marco, Valentina, Kapur, Agastya, Rogers, Axl F., Thrane, Eric, Askew, Jacob, Bhat, N. D. Ramesh, Cameron, Andrew, Curyło, Małgorzata, Coles, William A., Dai, Shi, Goncharov, Boris, Kerr, Matthew, Kulkarni, Atharva, Levin, Yuri, Lower, Marcus E., Manchester, Richard N., Mandow, Rami, Miles, Matthew T., Nathan, Rowina S., Osłowski, Stefan, Russell, Christopher J., Spiewak, Renée, Zhang, Songbo, Zhu, Xing-Jiang
Pulsar timing arrays aim to detect nanohertz-frequency gravitational waves (GWs). A background of GWs modulates pulsar arrival times and manifests as a stochastic process, common to all pulsars, with a signature spatial correlation. Here we describe
Externí odkaz:
http://arxiv.org/abs/2306.16215
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