Zobrazeno 1 - 5
of 5
pro vyhledávání: '"Kapur, Agastya"'
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
Autor:
Curyło, Małgorzata, Pennucci, Timothy T., Bailes, Matthew, Bhat, N. D. Ramesh, Cameron, Andrew D., Dai, Shi, Hobbs, George, Kapur, Agastya, Manchester, Richard N., Mandow, Rami, Miles, Matthew T., Russell, Christopher J., Reardon, Daniel J., Shannon, Ryan M., Spiewak, Renée, Zic, Andrew, Zhu, Xing-Jiang
In 2018 an ultra-wide-bandwidth low-frequency (UWL) receiver was installed on the 64-m Parkes Radio Telescope enabling observations with an instantaneous frequency coverage from 704 to 4032 MHz. Here, we present the analysis of a three-year data set
Externí odkaz:
http://arxiv.org/abs/2211.12924
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