Results 11 to 20 of about 41,592 (205)

The very red afterglow of GRB 000418 - further evidence for dust extinction in a GRB host galaxy [PDF]

, 2000
We report near-infrared and optical follow-up observations of the afterglow of the Gamma-Ray Burst 000418 starting 2.5 days after the occurrence of the burst and extending over nearly seven weeks.
A. A. Henden, A. Castro‐Tirado, A. Guarnieri, A. Magazzu, A. Oscoz, A. Piccioni, Aptekar R., B. Stecklum, Beuermann K., C. Bartolini, C. Sanchez‐Fernandez, Chi X., D. Butler, D. H. Hartmann, Dal Fiume D., E. Mazets, E. Palazzi, E. Pian, F. Ghinassi, Goldsten J., Hurley K., Israel G. L., J. A. Munoz, J. Goldsten, J. Gorosabel, J. Greiner, J. M. Castro Ceron, J. Trombka, K. Hurley, K. Noeske, M. Kasper, Masetti N., Meszaros P., N. Masetti, N. Tanvir, O. Fischer, P. M. Vreeswijk, P. Papaderos, Palazzi E., R. Gold, R. Starr, R. Weiss, S. Benetti, S. Golenetskii, S. Hippler, S. Klose, Sdzius J., T. Cline, T. McClanahan, Th. Ott, Wijers R. A. M. J., Zharikov S. V.   +51 more
core   +11 more sources

(INVITED) On the mechanism leading to afterglow in Gd2O2S:Pr

Optical Materials: X, 2021
The performance of scintillator materials and phosphors for x-ray imaging is adversely affected by afterglow, giving rise to ghost images and thus compromising image quality.
Cees Ronda, Andries Meijerink
doaj   +1 more source

Afterglow and thermoluminescence of ZrO2 nanopowders [PDF]

Open Physics, 2014
Puust Laurits, Kiisk Valter, Utt Kathriin, Mändar Hugo, Sildos Ilmo   +4 more
doaj   +2 more sources

Temporal dusty plasma afterglow: A review

Frontiers in Physics, 2022
In complex plasmas, dust particles are charged through their interactions with the electrons and ions of the surrounding plasma. In low-temperature laboratory plasmas, dust particles most commonly acquire a negative charge. In particular, in a laboratory
Lénaïc Couëdel, Lénaïc Couëdel
doaj   +1 more source

Green Afterglow of Undoped SrAl₂O₄

Nanomaterials, 2021
Undoped SrAl2O4 nanocrystals were obtained via solution combustion using urea as fuel. The afterglow properties of undoped SrAl2O4 were investigated. Green afterglow from undoped SrAl2O4 is visible to the human eye when the 325 nm irradiation of a helium–
Bao-Gai Zhai, Yuan-Ming Huang
doaj   +1 more source

Luminescent properties of Mg1.99SnO4:0.01Mn2+ phosphors doped with Zn2+

Journal of Materiomics, 2023
In this work, a series of ZnxMg1.99-xSnO4:0.01Mn2+ (x = 0, 0.01, 0.02, 0.03, 0.04) green long afterglow phosphors are prepared by high-temperature solid-phase reaction. The photoluminescence and long afterglow performance of host material doped with Zn2+
Ge Gao, Qiang Li, Pengxiao Hao, Xiao Huang, Hongjie Luo   +4 more
doaj   +1 more source

Butterfly-Shaped Guest Molecules Enable Tunable Room-Temperature Phosphorescence in Host-Guest Doped Systems. [PDF]

Adv Sci (Weinh)
Butterfly‐shaped triphenylamine‐based guest molecules (DBDBD) doped into rigid host matrices (TPP, CA) achieve efficient, multicolor‐tunable room‐temperature phosphorescence (RTP). The host‐guest synergy enables ultralong afterglow (up to 4 s) and quantum yields (Φp = 3.42%), with applications in dynamic anti‐counterfeiting and information encryption ...
Lou Z, Feng W, Wang K, Gong K, Wen G, Ji D.   +5 more
europepmc   +2 more sources

Inclination Estimates from Off-Axis GRB Afterglow Modelling

Universe, 2021
For gravitational wave (GW) detected neutron star mergers, one of the leading candidates for electromagnetic (EM) counterparts is the afterglow from an ultra-relativistic jet.
Gavin P. Lamb, Joseph J. Fernández, Fergus Hayes, Albert K. H. Kong, En-Tzu Lin, Nial R. Tanvir, Martin Hendry, Ik Siong Heng, Surojit Saha, John Veitch   +9 more
doaj   +1 more source

Gamma Ray Bursts vs. Afterglows [PDF]

, 1998
When does a GRB stop and its afterglow begin? A GRB may be defined as emission by internal shocks and its afterglow as emission by an external shock, but it is necessary to distinguish them observationally.
Katz, J. I.
core   +2 more sources

Afterglow Carbon Dots: From Fundamentals to Applications

Research, 2021
The ability of carbon dots (CDs) to emit afterglow emission in addition to fluorescence in response to UV-to-visible excitation allows them to be a new class of luminescent materials.
Chenxi Peng, Xue Chen, Meiling Chen, Shenci Lu, Yu Wang, Suli Wu, Xiaowang Liu, Wei Huang   +7 more
doaj   +1 more source