Zobrazeno 1 - 2
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pro vyhledávání: '"Li, Megan G."'
Autor:
Li, Megan G., Sheikh, Sofia Z., Gilbertson, Christian, He, Matthias Y., Isaacson, Howard, Croft, Steve, Sneed, Evan L.
Publikováno v:
The Astronomical Journal 166.5 (2023): 182
A stable-frequency transmitter with relative radial acceleration to a receiver will show a change in received frequency over time, known as a "drift rate''. For a transmission from an exoplanet, we must account for multiple components of drift rate:
Externí odkaz:
http://arxiv.org/abs/2311.01427
Autor:
Margot, Jean-Luc, Li, Megan G., Pinchuk, Pavlo, Myhrvold, Nathan, Lesyna, Larry, Alcantara, Lea E., Andrakin, Megan T., Arunseangroj, Jeth, Baclet, Damien S., Belk, Madison H., Bhadha, Zerxes R., Brandis, Nicholas W., Carey, Robert E., Cassar, Harrison P., Chava, Sai S., Chen, Calvin, Chen, James, Cheng, Kellen T., Cimbri, Alessia, Cloutier, Benjamin, Combitsis, Jordan A., Couvrette, Kelly L., Coy, Brandon P., Davis, Kyle W., Delcayre, Antoine F., Du, Michelle R., Feil, Sarah E., Fu, Danning, Gilmore, Travis J., Grahill-Bland, Emery, Iglesias, Laura M., Juneau, Zoe, Karapetian, Anthony G., Karfakis, George, Lambert, Christopher T., Lazbin, Eric A., Li, Jian H., Zhuofu, Li, Liskij, Nicholas M., Lopilato, Anthony V., Lu, Darren J., Ma, Detao, Mathur, Vedant, Minasyan, Mary H., Muller, Maxwell K., Nasielski, Mark T., Nguyen, Janice T., Nicholson, Lorraine M., Niemoeller, Samantha, Ohri, Divij, Padhye, Atharva U., Penmetcha, Supreethi V., Prakash, Yugantar, Xinyi, Qi, Rindt, Liam, Sahu, Vedant, Scally, Joshua A., Scott, Zefyr, Seddon, Trevor J., Shohet, Lara-Lynn V., Sinha, Anchal, Sinigiani, Anthony E., Song, Jiuxu, Stice, Spencer M., Uplisashvili, Andria, Vanga, Krishna, Vazquez, Amaury G., Vetushko, George, Villa, Valeria, Vincent, Maria, Waasdorp, Ian J., Wagaman, Ian B., Wang, Amanda, Wight, Jade C., Wong, Ella, Yamaguchi, Natsuko, Zhang, Zijin, Zhao, Junyang, Lynch, Ryan S.
Publikováno v:
AJ 166 206 (2023)
We conducted a search for narrowband radio signals over four observing sessions in 2020-2023 with the L-band receiver (1.15-1.73 GHz) of the 100 m diameter Green Bank Telescope. We pointed the telescope in the directions of 62 TESS Objects of Interes
Externí odkaz:
http://arxiv.org/abs/2308.02712