Zobrazeno 1 - 10
of 129
pro vyhledávání: '"Zeng, Lingzhen"'
Autor:
Núñez, Carolina, Appel, John W., Datta, Rahul, Bennett, Charles L., Brewer, Michael K., Bruno, Sarah Marie, Bustos, Ricardo, Chuss, David T., Costen, Nick, Couto, Jullianna Denes, Dahal, Sumit, Denis, Kevin L., Eimer, Joseph R., Essinger-Hileman, Thomas, Iuliano, Jeffrey, Li, Yunyang, Marriage, Tobias A., Mateo, Jennette, Petroff, Matthew A., Shi, Rui, Rostem, Karwan, Valle, Deniz A. N., Watts, Duncan, Wollack, Edward J., Zeng, Lingzhen
We present the in-lab and on-sky performance for the upgraded 90 GHz focal plane of the Cosmology Large Angular Scale Surveyor (CLASS), which had four of its seven detector wafers updated during the austral winter of 2022. The update aimed to improve
Externí odkaz:
http://arxiv.org/abs/2411.12705
Autor:
Giannakopoulos, Christos, Vergès, Clara, Ade, P. A. R., Ahmed, Zeeshan, Amiri, Mandana, Barkats, Denis, Thakur, Ritoban Basu, Bischoff, Colin A., Beck, Dominic, Bock, James J., Boenish, Hans, Buza, Victor, Cheshire IV, James R., Connors, Jake, Cornelison, James, Crumrine, Michael, Cukierman, Ari Jozef, Denison, Edward, Dierickx, Marion, Duband, Lionel, Eiben, Miranda, Elwood, Brodi D., Fatigoni, Sofia, Filippini, Jeff P., Fortes, Antonio, Gao, Min, Goeckner-Wald, Neil, Goldfinger, David C., Grayson, James A., Grimes, Paul K., Hall, Grantland, Halal, George, Halpern, Mark, Hand, Emma, Harrison, Sam A., Henderson, Shawn, Hubmayr, Johannes, Hui, Howard, Irwin, Kent D., Kang, Jae Hwan, Karkare, Kirit S., Kefeli, Sinan, Kovac, J. M., Kuo, Chao-Lin, Lau, King, Lautzenhiser, Margaret, Lennox, Amber, Liu, Tongtian, Megerian, Koko G., Miller, Oliver, Minutolo, Lorenzo, Moncelsi, Lorenzo, Nakato, Yuka, Nguyen, H. T., O'brient, Roger, Patel, Anika, Petroff, Matthew A., Polish, Anna R., Precup, Nathan, Prouve, Thomas, Pryke, Clement, Reintsema, Carl D., Romand, Thibault, Salatino, Maria, Schillaci, Alessandro, Schmitt, Benjamin, Singari, Baibhav, Soliman, Ahmed, Germaine, Tyler St, Steiger, Aaron, Steinbach, Bryan, Sudiwala, Rashmi, Thompson, Keith L., Tsai, Calvin, Tucker, Carole, Turner, Anthony D., Vieregg, Abigail G., Wandui, Albert, Weber, Alexis C., Willmert, Justin, Wu, Wai Ling K., Yang, Hung-I, Yu, Cyndia, Zeng, Lingzhen, Zhang, Cheng, Zhang, Silvia
The BICEP3 and BICEP Array polarimeters are small-aperture refracting telescopes located at the South Pole designed to measure primordial gravitational wave signatures in the Cosmic Microwave Background (CMB) polarization, predicted by inflation. Con
Externí odkaz:
http://arxiv.org/abs/2409.16440
Autor:
Grimes, Paul K., Keating, Garrett K., Blundell, Raymond, Christensen, Robert D., Gurwell, Mark, Kovacs, Attila, Norton, Timothy, Paine, Scott N., Rao, Ramprasad, Tong, Edward C. -Y., Weintroub, Jonathan, Wilner, David, Wilson, Robert W., Zeng, Lingzhen, Zhang, Qizhou
The Submillimeter Array (SMA) is an array of 8 antennas operating at millimeter and submillimeter wavelengths on Maunakea, Hawaii, operated by the Smithsonian Astrophysical Observatory and Academia Sinica Institute of Astronomy and Astrophysics, Taiw
Externí odkaz:
http://arxiv.org/abs/2406.17192
We report the first arcsecond-resolution observations of the magnetic field in the mini starburst complex Sgr B2. SMA polarization observations revealed magnetic field morphology in three dense cores of Sgr B2 N(orth), M(ain), and S(outh). The total
Externí odkaz:
http://arxiv.org/abs/2406.11800
Autor:
Eimer, Joseph R., Li, Yunyang, Brewer, Michael K., Shi, Rui, Ali, Aamir, Appel, John W., Bennett, Charles L., Bruno, Sarah Marie, Bustos, Ricardo, Chuss, David T., Cleary, Joseph, Dahal, Sumit, Datta, Rahul, Couto, Jullianna Denes, Denis, Kevin L., Dünner, Rolando, Essinger-Hileman, Thomas, Fluxá, Pedro, Hubmayer, Johannes, Harrington, Kathleen, Iuliano, Jeffrey, Karakla, John, Marriage, Tobias A., Núñez, Carolina, Parker, Lucas, Petroff, Matthew A., Reeves, Rodrigo A., Rostem, Karwan, Valle, Deniz A. N., Watts, Duncan J., Weiland, Janet L., Wollack, Edward J., Xu, Zhilei, Zeng, Lingzhen
Measurement of the largest angular scale ($\ell < 30$) features of the cosmic microwave background (CMB) polarization is a powerful way to constrain the optical depth to reionization and search for the signature of inflation through the detection of
Externí odkaz:
http://arxiv.org/abs/2309.00675
Autor:
Datta, Rahul, Brewer, Michael K., Couto, Jullianna Denes, Eimer, Joseph, Li, Yunyang, Xu, Zhilei, Ali, Aamir, Appel, John W., Bennett, Charles L., Bustos, Ricardo, Chuss, David T., Cleary, Joseph, Dahal, Sumit, Espinoza, Francisco, Essinger-Hileman, Thomas, Fluxá, Pedro, Harrington, Kathleen, Helson, Kyle, Iuliano, Jeffrey, Karakla, John, Marriage, Tobias A., Novack, Sasha, Núñez, Carolina, Padilla, Ivan L., Parker, Lucas, Petroff, Matthew A., Reeves, Rodrigo, Rostem, Karwan, Shi, Rui, Valle, Deniz A. N., Watts, Duncan J., Weiland, Janet L., Wollack, Edward J., Zeng, Lingzhen
Publikováno v:
The Astrophysical Journal Supplement Series, Volume 273, Number 2 (2024)
The Cosmology Large Angular Scale Surveyor (CLASS) is a telescope array that observes the cosmic microwave background (CMB) over ~75% of the sky from the Atacama Desert, Chile, at frequency bands centered near 40, 90, 150, and 220 GHz. CLASS measures
Externí odkaz:
http://arxiv.org/abs/2308.13309
Autor:
Zeng, Lingzhen, Zhang, Qizhou, Alves, Felipe O., Ching, Tao-Chung, Girart, Josep M., Liu, Junhao
This paper presents the results of full polarization observations of the massive star-forming region W75N, conducted with 3 arcsec spatial resolutions at 345 GHz using the Submillimeter Array (SMA). The magnetic field structures in the dense cores of
Externí odkaz:
http://arxiv.org/abs/2307.06231
Autor:
Li, Yunyang, Eimer, Joseph, Osumi, Keisuke, Appel, John, Brewer, Michael, Ali, Aamir, Bennett, Charles, Bruno, Sarah Marie, Bustos, Ricardo, Chuss, David, Cleary, Joseph, Couto, Jullianna, Dahal, Sumit, Datta, Rahul, Denis, Kevin, Dunner, Rolando, Inostroza, Francisco Raul Espinoza, Essinger-Hileman, Thomas, Fluxa, Pedro, Harrington, Kathleen, Iuliano, Jeffrey, Karakla, John, Marriage, Tobias, Miller, Nathan, Novack, Sasha, Núñez, Carolina, Petroff, Matthew, Reeves, Rodrigo, Rostem, Karwan, Shi, Rui, Valle, Deniz, Watts, Duncan, Weiland, J., Wollack, Edward, Xu, Zhilei, Zeng, Lingzhen
The Cosmology Large Angular Scale Surveyor (CLASS) is a telescope array that observes the cosmic microwave background over 75\% of the sky from the Atacama Desert, Chile, at frequency bands centered near 40, 90, 150, and 220~GHz. This paper describes
Externí odkaz:
http://arxiv.org/abs/2305.01045
Autor:
Dierickx, Marion, Ade, P. A. R., Ahmed, Zeeshan, Amiri, Mandana, Barkats, Denis, Thakur, Ritoban Basu, Bischoff, Colin A., Beck, Dominic, Bock, James J., Buza, Victor, Cheshire IV, James R., Connors, Jake, Cornelison, James, Crumrine, Michael, Cukierman, Ari Jozef, Denison, Edward, Duband, Lionel, Eiben, Miranda, Fatigoni, Sofia, Filippini, Jeff P., Giannakopoulos, Christos, Goeckner-Wald, Neil, Goldfinger, David, Grayson, James A., Grimes, Paul, Hall, Grantland, Halal, George, Halpern, Mark, Hand, Emma, Harrison, Sam A., Henderson, Shawn, Hildebrandt, Sergi, Hilton, Gene C., Hubmayr, Johannes, Hui, Howard, Irwin, Kent D., Kang, Jae Hwan, Karkare, Kirit S., Kefeli, Sinan, Kovac, J. M., Kuo, Chao-Lin, Lau, King, Leitch, Erik M., Lennox, Amber, Megerian, . G., Minutolo, Lorenzo, Moncelsi, Lorenzo, Nakato, Yuka, Namikawa, Toshiya, Nguyen, H. T., O'brient, Roger, Palladino, Steven, Petroff, Matthew, Precup, Nathan, Prouve, Thomas, Pryke, Clement, Racine, Benjamin, Reintsema, Carl D., Santalucia, Destiny, Schillaci, Alessandro, Schmitt, Benjamin, Singari, Baibhav, Soliman, Ahmed, Germaine, Tyler St, Steinbach, Bryan, Sudiwala, Rashmi, Thompson, Keith L., Tucker, Carole, Turner, Anthony D., Umiltà, Caterina, Verges, Clara, Vieregg, Abigail G., Wandui, Albert, Weber, Alexis C., Wiebe, Don, Willmert, Justin, Wu, Wai Ling K., Yang, Hung-I, Yoon, Ki Won, Young, Edward, Yu, Cyndia, Zeng, Lingzhen, Zhang, Cheng, Zhang, Silvia
The BICEP/Keck series of experiments target the Cosmic Microwave Background at degree-scale resolution from the South Pole. Over the next few years, the "Stage-3" BICEP Array (BA) telescope will improve the program's frequency coverage and sensitivit
Externí odkaz:
http://arxiv.org/abs/2111.14751
Autor:
Wang, Maolin, Xu, Yao, Tang, Haoyi, Tian, Shuheng, Zeng, Lingzhen, Li, Haoyu, Wu, Congyi, Hu, Zhibiao, Su, Min, Zheng, Heng, Wang, Meng, Ma, Ding
Publikováno v:
In Chem Catalysis 16 May 2024 4(5)
