Zobrazeno 1 - 10
of 2 305
pro vyhledávání: '"Lan, Ting"'
Autor:
Chang, Yu-Ling, Lan, Ting-Wen, Prochaska, J. Xavier, Napolitano, Lucas, Anand, Abhijeet, Aguilar, J., Ahlen, S., Brooks, D., Claybaugh, T., de la Macorra, A., Dey, Arjun, Doel, P., Gontcho, S. Gontcho A, Guy, J., Juneau, S., Kisner, T., Lambert, A., Landriau, M., Guillou, L. Le, Manera, M., Martini, P., Meisner, A., Miquel, R., Moustakas, J., Myers, A. D., Nie, J., Poppett, C., Rezaie, M., Rossi, G., Sanchez, E., Schubnell, M., Seo, H., Sprayberry, D., Tarle, G., Weaver, B. A., Zou, H.
We explore the influence of radio-mode feedback on the properties of the cool circumgalactic medium (CGM). To this end, we assemble a statistical sample of approximately 30,000 radio galaxies with background quasars by combining optical spectroscopic
Externí odkaz:
http://arxiv.org/abs/2405.08314
Autor:
Liang, Akun, Gonzalez-Platas, Javier, Turnbull, Robin, Popescu, Catalin, Fernandez-Guillen, Ismael, Abargues, Rafael, Boix, Pablo P., Shi, Lan-Ting, Errandonea, Daniel
Publikováno v:
J. Am. Chem. Soc. 2022, 144, 20099-20108
The high-pressure crystal structure evolution of CH3NH3PbBr3 (MAPbBr3) perovskite has been investigated by single-crystal X-ray diffraction and synchrotron-based powder X-ray diffraction. Single-crystal X-ray diffraction reveals that the crystal stru
Externí odkaz:
http://arxiv.org/abs/2401.13468
Autor:
Han, Jiwon Jesse, Dey, Arjun, Price-Whelan, Adrian M., Najita, Joan, Schlafly, Edward F., Saydjari, Andrew, Wechsler, Risa H., Bonaca, Ana, Schlegel, David J, Conroy, Charlie, Raichoor, Anand, Drlica-Wagner, Alex, Kollmeier, Juna A., Koposov, Sergey E., Besla, Gurtina, Rix, Hans-Walter, Goodman, Alyssa, Finkbeiner, Douglas, Anand, Abhijeet, Ashby, Matthew, Bahr-Kalus, Benedict, Beaton, Rachel, Behera, Jayashree, Bell, Eric F., Bellm, Eric C, BenZvi, Segev, Silva, Leandro Beraldo e, Birrer, Simon, Blanton, Michael R., Bock, Jamie, Broekgaarden, Floor, Brout, Dillon, Brown, Warren, Brown, Anthony G. A., Bulbul, Esra, Calderon, Rodrigo, Carlin, Jeffrey L, Carrillo, Andreia, Castander, Francisco Javier, Chakraborty, Priyanka, Chandra, Vedant, Chiang, Yi-Kuan, Choi, Yumi, Clark, Susan E., Clarkson, William I., Cooper, Andrew, Crill, Brendan, Cunha, Katia, Cunningham, Emily, Dalcanton, Julianne, Danieli, Shany, Daylan, Tansu, de Jong, Roelof S., DeRose, Joseph, Dey, Biprateep, Dickinson, Mark, Dominguez, Mariano, Dong, Dillon, Eifler, Tim, El-Badry, Kareem, Erkal, Denis, Escala, Ivanna, Fazio, Giovanni, Ferguson, Annette M. N., Ferraro, Simone, Filion, Carrie, Forero-Romero, Jaime E., Fu, Shenming, Galbany, Lluís, Garavito-Camargo, Nicolas, Gawiser, Eric, Geha, Marla, Gnedin, Oleg Y., Gomez, Sebastian, Greene, Jenny, Guy, Julien, Hadzhiyska, Boryana, Hawkins, Keith, Heinrich, Chen, Hernquist, Lars, Hirata, Christopher, Hora, Joseph, Horowitz, Benjamin, Horta, Danny, Huang, Caroline, Huang, Xiaosheng, Huanyuan, Shan, Hunt, Jason A. S., Ibata, Rodrigo, Jannuzi, Buell, Johnston, Kathryn V., Jones, Michael G., Juneau, Stephanie, Kado-Fong, Erin, Kalari, Venu, Kallivayalil, Nitya, Karim, Tanveer, Keeley, Ryan, Khoperskov, Sergey, Kim, Bokyoung, Kovács, András, Krause, Elisabeth, Kremer, Kyle, Kremin, Anthony, Krolewski, Alex, Kulkarni, S. R., Kuna, Marine, L'Huillier, Benjamin, Lacy, Mark, Lan, Ting-Wen, Lang, Dustin, Leahy, Denis, Li, Jiaxuan, Lim, Seunghwan, López-Morales, Mercedes, Macri, Lucas, Marc, Manera, Mau, Sidney, McCarthy, Patrick J, McDonald, Eithne, McQuinn, Kristen, Meisner, Aaron, Melnick, Gary, Merloni, Andrea, Millard, Cléa, Millon, Martin, Minchev, Ivan, Montero-Camacho, Paulo, Morales-Gutierrez, Catalina, Morrell, Nidia, Moustakas, John, Moustakas, Leonidas, Murray, Zachary, Mutlu-Pakdil, Burcin, Myeong, GyuChul, Myers, Adam D., Nadler, Ethan, Navarete, Felipe, Ness, Melissa, Nidever, David L., Nikutta, Robert, Nushkia, Chamba, Olsen, Knut, Pace, Andrew B., Pacucci, Fabio, Padmanabhan, Nikhil, Parkinson, David, Pearson, Sarah, Peng, Eric W., Petric, Andreea O., Petric, Andreea, Ratcliffe, Bridget, Razieh, Emami, Reiprich, Thomas, Rezaie, Mehdi, Ricci, Marina, Rich, R. Michael, Richstein, Hannah, Riley, Alexander H., Rockosi, Constance, Rossi, Graziano, Salvato, Mara, Samushia, Lado, Sanchez, Javier, Sand, David J, Sanderson, Robyn E, Šarčević, Nikolina, Sarkar, Arnab, Savino, Alessandro, Schweizer, Francois, Shafieloo, Arman, Shengqi, Yang, Shields, Joseph, Shipp, Nora, Simon, Josh, Siudek, Malgorzata, Siwei, Zou, Slepian, Zachary, Smith, Verne, Sobeck, Jennifer, Sohn, Sangmo Tony, Som, Debopam, Speagle, Joshua S., Spergel, David, Szabo, Robert, Tan, Ting, Theissen, Christopher, Tollerud, Erik, Tolls, Volker, Tran, Kim-Vy, Tsiane, Kabelo, Vacca, William D., Valluri, Monica, Verberi, TonyLouis, Warfield, Jack, Weaverdyck, Noah, Weiner, Benjamin, Weisz, Daniel, Wetzel, Andrew, White, Martin, Williams, Christina C., Wolk, Scott, Wu, John F., Wyse, Rosemary, Yang, Justina R., Zaritsky, Dennis, Zelko, Ioana A., Zhimin, Zhou, Zucker, Catherine
The Nancy Grace Roman Space Telescope is capable of delivering an unprecedented all-sky, high-spatial resolution, multi-epoch infrared map to the astronomical community. This opportunity arises in the midst of numerous ground- and space-based surveys
Externí odkaz:
http://arxiv.org/abs/2306.11784
Autor:
Napolitano, Lucas, Pandey, Agnesh, Myers, Adam D., Lan, Ting-Wen, Anand, Abhijeet, Aguilar, Jessica, Ahlen, Steven, Alexander, David M., Brooks, David, Canning, Rebecca, Circosta, Chiara, De La Macorra, Axel, Doel, Peter, Eftekharzadeh, Sarah, Fawcett, Victoria A., Font-Ribera, Andreu, Garcia-Bellido, Juan, Gontcho, Satya Gontcho A, Guillou, L. Le, Guy, Julien, Honscheid, Klaus, Juneau, Stephanie, Kisner, T., Landriau, Martin, Meisner, Aaron M., Miquel, Ramon, Moustakas, J., Percival, Will J., Prochaska, J. Xavier, Schubnell, Michael, Tarle, Gregory, Weaver, B. A., Weiner, Benjamin, Zhou, Zhimin, Zou, Hu, Zou, Siwei
Publikováno v:
2023AJ....166...99N
We present findings of the detection of Magnesium II (Mg II, {\lambda} = 2796, 2803 {\AA}) absorbers from the early data release of the Dark Energy Spectroscopic Instrument (DESI). DESI is projected to obtain spectroscopy of approximately 3 million q
Externí odkaz:
http://arxiv.org/abs/2305.20016
Autor:
Brodzeller, Allyson, Dawson, Kyle, Bailey, Stephen, Yu, Jiaxi, Ross, A. J., Bault, A., Filbert, S., Aguilar, J., Ahlen, S., Alexander, David M., Armengaud, E., Berti, A., Brooks, D., Chaussidon, E., de la Macorra, A., Doel, P., Fanning, K., Fawcett, V. A., Font-Ribera, A., Gontcho, S. Gontcho A, Guy, J., Honscheid, K., Juneau, S., Kehoe, R., Kisner, T., Kremin, Anthony, Lan, Ting-Wen, Landriau, M., Levi, Michael E., Magneville, C., Martini, Paul, Meisner, Aaron M., Miquel, R., Moustakas, J., Palanque-Delabrouille, N., Percival, W. J., Prada, F., Ravoux, C., Rossi, Graziano, Saulder, C., Siudek, M., Tarlé, Gregory, Weaver, B. A., Youles, S., Zheng, Zheng, Zhou, Rongpu, Zhou, Zhimin
Millions of quasar spectra will be collected by the Dark Energy Spectroscopic Instrument (DESI), leading to a four-fold increase in the number of known quasars. High accuracy quasar classification is essential to tighten constraints on cosmological p
Externí odkaz:
http://arxiv.org/abs/2305.10426
Let $\mathcal{D}$ be a non-trivial $G$-block-transitive $3$-$(v,k,1)$ design, where $T\leq G \leq \mathrm{Aut}(T)$ for some finite non-abelian simple group $T$. It is proved that if $T$ is a simple exceptional group of Lie type, then $T$ is either th
Externí odkaz:
http://arxiv.org/abs/2305.08052
Autor:
Guy, J., Bailey, S., Kremin, A., Alam, Shadab, Alexander, D. M., Prieto, C. Allende, BenZvi, S., Bolton, A. S., Brooks, D., Chaussidon, E., Cooper, A. P., Dawson, K., de la Macorra, A., Dey, A., Dey, Biprateep, Dhungana, G., Eisenstein, D. J., Font-Ribera, A., Forero-Romero, J. E., Gaztañaga, E., Gontcho, S. Gontcho A, Green, D., Honscheid, K., Ishak, M., Kehoe, R., Kirkby, D., Kisner, T., Koposov, Sergey E., Lan, Ting-Wen, Landriau, M., Guillou, L. Le, Levi, Michael E., Magneville, C., Manser, Christopher J., Martini, P., Meisner, Aaron M., Miquel, R., Moustakas, J., Myers, Adam D., Newman, Jeffrey A., Nie, Jundan, Palanque-Delabrouille, N., Percival, W. J., Poppett, C., Prada, F., Raichoor, A., Ravoux, C., Ross, A. J., Schlafly, E. F., Schlegel, D., Schubnell, M., Sharples, Ray M., Tarlé, Gregory, Weaver, B. A., Yèche, Christophe, Zhou, Rongpu, Zhou, Zhimin, Zou, H.
We describe the spectroscopic data processing pipeline of the Dark Energy Spectroscopic Instrument (DESI), which is conducting a redshift survey of about 40 million galaxies and quasars using a purpose-built instrument on the 4-m Mayall Telescope at
Externí odkaz:
http://arxiv.org/abs/2209.14482
Autor:
Lan, Ting, Lü, Huazhong
The balanced hypercube $BH_{n}$, a variant of the hypercube, is a novel interconnection network for massive parallel systems. It is known that the balanced hypercube remains Hamiltonian after deleting at most $4n-5$ faulty edges if each vertex is inc
Externí odkaz:
http://arxiv.org/abs/2208.08601
Autor:
Myers, Adam D., Moustakas, John, Bailey, Stephen, Weaver, Benjamin A., Cooper, Andrew P., Forero-Romero, Jaime E., Abolfathi, Bela, Alexander, David M., Brooks, David, Chaussidon, Edmond, Chuang, Chia-Hsun, Dawson, Kyle, Dey, Arjun, Dey, Biprateep, Dhungana, Govinda, Doel, Peter, Fanning, Kevin, Gaztañaga, Enrique, Gontcho, Satya Gontcho A, Gonzalez-Morales, Alma X., Hahn, ChangHoon, Herrera-Alcantar, Hiram K., Honscheid, Klaus, Ishak, Mustapha, Karim, Tanveer, Kirkby, David, Kisner, Theodore, Koposov, Sergey E., Kremin, Anthony, Lan, Ting-Wen, Landriau, Martin, Lang, Dustin, Levi, Michael E., Magneville, Christophe, Napolitano, Lucas, Martini, Paul, Meisner, Aaron, Newman, Jeffrey A., Palanque-Delabrouille, Nathalie, Percival, Will, Poppett, Claire, Prada, Francisco, Raichoor, Anand, Ross, Ashley J., Schlafly, Edward F., Schlegel, David, Schubnell, Michael, Tan, Ting, Tarle, Gregory, Wilson, Michael J., Yèche, Christophe, Zhou, Rongpu, Zhou, Zhimin, Zou, Hu
Publikováno v:
2023, AJ, 165, 50
In 2021 May, the Dark Energy Spectroscopic Instrument (DESI) began a 5 yr survey of approximately 50 million total extragalactic and Galactic targets. The primary DESI dark-time targets are emission line galaxies (ELGs), luminous red galaxies (LRGs)
Externí odkaz:
http://arxiv.org/abs/2208.08518
Autor:
Alexander, David M., Davis, Tamara M., Chaussidon, E., Fawcett, V. A., Gonzalez-Morales, Alma X., Lan, Ting-Wen, Yeche, Christophe, Ahlen, S., Aguilar, J. N., Armengaud, E., Bailey, S., Brooks, D., Cai, Z., Canning, R., Carr, A., Chabanier, S., Cousinou, Marie-Claude, Dawson, K., de la Macorra, A., Dey, A., Dey, Biprateep, Dhungana, G., Edge, A. C., Eftekharzadeh, S., Fanning, K., Farr, James, Font-Ribera, A., Garcia-Bellido, J., Garrison, Lehman, Gaztanaga, E., Gontcho, Satya Gontcho A, Gordon, C., Gonzalez, Stefany Guadalupe Medellin, Guy, J., Herrera-Alcantar, Hiram K., Jiang, L., Juneau, S., Karacayli, Naim, Kehoe, R., Kisner, T., Kovacs, A., Landriau, M., Levi, Michael E., Magneville, C., Martini, P., Meisner, Aaron M., Mezcua, M., Miquel, R., Camacho, P. Montero, Moustakas, J., Munoz-Gutierrez, Andrea, Myers, Adam D., Nadathur, S., Napolitano, L., Nie, J. D., Palanque-Delabrouille, N., Pan, Z., Percival, W. J., Perez-Rafols, I., Poppett, C., Prada, F., Ramirez-Perez, Cesar, Ravoux, C., Rosario, D. J., Schubnell, M., Tarle, Gregory, Walther, M., Weiner, B., Youles, S., Zhou, Zhimin, Zou, H., Zou, Siwei
A key component of the Dark Energy Spectroscopic Instrument (DESI) survey validation (SV) is a detailed visual inspection (VI) of the optical spectroscopic data to quantify key survey metrics. In this paper we present results from VI of the quasar su
Externí odkaz:
http://arxiv.org/abs/2208.08517