Results 181 to 190 of about 24,858 (303)
Ultrahigh-energy gamma-ray emission associated with black hole-jet systems. [PDF]
Natl Sci RevCao Z, Aharonian F, Bai YX, Bao YW, Bastieri D, Bi XJ, Bi YJ, Bian WY, Bukevich AV, Cai C, Cao WY, Cao Z, Chang J, Chang JF, Chen A, Chen ES, Chen G, Chen HX, Chen L, Chen L, Chen MJ, Chen ML, Chen QH, Chen S, Chen SH, Chen SZ, Chen TL, Chen XB, Chen X, Chen Y, Cheng N, Cheng YD, Chu MC, Cui MY, Cui SW, Cui XH, Cui YD, Dai BZ, Dai HL, Dai Z, Luobu D, Diao YX, Dong XQ, Duan KK, Fan JH, Fan YZ, Fang J, Fang JH, Fang K, Feng CF, Feng H, Feng L, Feng S, Feng XT, Feng Y, Feng YL, Gabici S, Gao B, Gao CD, Gao Q, Gao W, Gao WK, Ge M, Ge TT, Geng L, Giacinti G, Gong G, Gou Q, Gu MH, Guo FL, Guo J, Guo XL, Guo YQ, Guo YY, Han YA, Hannuksela OA, Hasan M, He HH, He HN, He JY, He X, He Y, Hernández-Cadena S, Hou BW, Hou C, Hou X, Hu HB, Hu SC, Huang C, Huang DH, Huang J, Huang TQ, Huang WJ, Huang XT, Huang XY, Huang Y, Huang YY, Ji XL, Jia HY, Jia K, Jiang HB, Jiang K, Jiang XW, Jiang ZJ, Jin M, Kaci S, Kang MM, Karpikov I, Khangulyan D, Kuleshov D, Kurinov K, Li BB, Li C, Li C, Li D, Li F, Li H, Li H, Li J, Li J, Li K, Li L, Li RL, Li SD, Li TY, Li WL, Li XR, Li X, Li Y, Li Y, Li Z, Li Z, Liang EW, Liang YF, Lin SJ, Liu B, Liu C, Liu D, Liu DB, Liu H, Liu HD, Liu J, Liu JL, Liu JR, Liu MY, Liu RY, Liu SM, Liu W, Liu X, Liu Y, Liu Y, Liu YN, Lou YQ, Luo Q, Luo Y, Lv HK, Ma BQ, Ma LL, Ma XH, Mao JR, Min Z, Mitthumsiri W, Mou GB, Mu HJ, Neronov A, Ng KCY, Ni MY, Nie L, Ou LJ, Pattarakijwanich P, Pei ZY, Qi JC, Qi MY, Qin JJ, Raza A, Ren CY, Ruffolo D, Sáiz A, Semikoz D, Shao L, Shchegolev O, Shen YZ, Sheng XD, Shi Z, Shu FW, Song HC, Stenkin YV, Stepanov V, Su Y, Sun D, Sun H, Sun Q, Sun X, Sun Z, Tabasam NH, Takata J, Tam PHT, Tan HB, Tang Q, Tang R, Tang Z, Tian W, Tong C, Wan LH, Wang C, Wang G, Wang H, Wang J, Wang K, Wang K, Wang L, Wang L, Wang LY, Wang R, Wang W, Wang X, Wang XJ, Wang XY, Wang Y, Wang YD, Wang ZH, Wang ZX, Wang Z, Wei DM, Wei JJ, Wei YJ, Wen T, Weng SS, Wu CY, Wu HR, Wu QW, Wu S, Wu XF, Wu YS, Xi SQ, Xia J, Xia JJ, Xiang GM, Xiao DX, Xiao G, Xin YL, Xing Y, Xiong DR, Xiong Z, Xu DL, Xu RF, Xu RX, Xu WL, Xue L, Yan DH, Yan JZ, Yan T, Yang CW, Yang CY, Yang FF, Yang LL, Yang MJ, Yang RZ, Yang WX, Yang Z, Yao ZG, Ye XA, Yin LQ, Yin N, You XH, You ZY, Yu YH, Yuan Q, Yue H, Zeng HD, Zeng TX, Zeng W, Zeng X, Zha M, Zhang BB, Zhang BT, Zhang C, Zhang F, Zhang HF, Zhang HM, Zhang HY, Zhang JL, Zhang L, Zhang PF, Zhang PP, Zhang R, Zhang SR, Zhang SS, Zhang W, Zhang X, Zhang XP, Zhang Y, Zhang Y, Zhang ZP, Zhao J, Zhao L, Zhao LZ, Zhao SP, Zhao XH, Zhao Z, Zheng F, Zhong WJ, Zhou B, Zhou H, Zhou JN, Zhou M, Zhou P, Zhou R, Zhou XX, Zhou XX, Zhu BY, Zhu CG, Zhu FR, Zhu H, Zhu KJ, Zou YC, Zuo X. +316 moreeuropepmc +1 more sourceScientist at the Joint Institute for Laboratory Astrophysics
Verso: basic standards. In the early 1960s, with the development of space science brought about by rocket and satellite capabilities and of research in thermonuclear power, interest in the behavior of very hot gases and plasmas had grown substantially ...National Institute of Standards and Technologycore Comparing v11.2 OCO‐2 and v11 OCO‐3 XCO2 ${\mathbf{X}}_{{\text{CO}}_{\mathbf{2}}}$ Retrievals With Ground‐Based COCCON Measurements
Earth and Space Science, Volume 13, Issue 6, June 2026.Abstract
The Orbiting Carbon Observatory‐2 and ‐3 (collectively termed “OCO‐2/3,” hereafter) missions, together, provide precise and accurate global data records that contribute to a better understanding of the variability in atmospheric carbon dioxide (CO2).Saswati Das, Mahesh Kumar Sha, Darko Dubravica, Thomas E. Taylor, Matthäus Kiel, Joshua L. Laughner, Gregory B. Osterman, Christopher W. O’Dell, Brendan Fisher, Robert R. Nelson, Carlos Alberti, Bianca C. Baier, Dimitrios Balis, Hartmut Bösch, Andre Butz, Zhaonan Cai, Jia Chen, Frédéric Chevallier, Alexandru Dandocsi, Nicholas M. Deutscher, Manvendra K. Dubey, Dietrich G. Feist, Lena Feld, Jonathan E. Franklin, Matthias M. Frey, Omaira Garcia, Elaine Gottlieb, Konstantin Gribanov, David W. T. Griffith, Michel Grutter, Frank Hase, Eliezer S. Hernández, Neil Humpage, Laura T. Iraci, Nicole Jacobs, Sujong Jeong, Pascal Jeseck, Tomi Karppinen, Rigel Kivi, Morgan Lopez, Andreas Luther, Maria Makarova, Moritz Makowski, Erin McGee, Marios Mermigkas, Isamu Morino, Justus Notholt, Hirofumi Ohyama, Thomas Panou, Hayoung Park, Robert Parker, David F. Pollard, Markus Rettinger, Sébastien Roche, Coleen M. Roehl, Constantina Rousogenous, Kei Shiomi, William R. Simpson, Wolfgang Stremme, Kimberly Strong, Ralf Sussmann, Noemie L. Taquet, Yao Té, Chrysanthi Topaloglou, Geoffrey Toon, Qiansi Tu, Mihalis Vrekoussis, Pucai Wang, Thorsten Warneke, Steven C. Wofsy, Debra Wunch, Minqiang Zhou, Elizabeth Spicer, Annmarie Eldering, Susan Kulawik, Abhishek Chatterjee, Vivienne H. Payne +76 morewiley +1 more sourceReview of Astrophysics Experiments on Intense Lasers
, 2000 Astrophysics has traditionally been pursued at astronomical observatories and on theorists' computers. Observations record images from space, and theoretical models are developed to explain the observations. A component often missing has been the ability Takabe, H., Drake, R. P., Arnett, D., Remington, B. A. +3 morecore Tests of HgCdTe Photodetectors Performances for Implementation on the MIST-A Instrument. [PDF]
Sensors (Basel)Cencia C, La Francesca E, Ciarniello M, Raponi A, Capaccioni F, De Sanctis MC, De Angelis S, Formisano M, Ferrari M, Biondi D, Boccaccini A, Stefani S, Piccioni G, Mura A, Galiano A, Tommasi L, Bartolo C, Iuzzolino M, Bucciantini L, Dami M, Cossu G, Nencioni S, Olivieri A, Ammannito E, Tiberia A, Filacchione G. +25 moreeuropepmc +1 more sourceJoint Institute for Laboratory Astrophysics, negative sheet 1
In the early 1960s, with the development of space science brought about by rocket and satellite capabilities and of research in thermonuclear power, interest in the behavior of very hot gases and plasmas had grown substantially.National Institute of Standards and Technologycore