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Related Article: H.C. Neal, V.V. Nesterov, B.W. Smucker|2022|IUCrData|7|x220525|doi:10.1107/S2414314622005259

An entry from the Cambridge Structural Database, the world’s repository for small molecule crystal structures. The entry contains experimental data from a crystal diffraction study. The deposited dataset for this entry is freely available from the CCDC and typically includes 3D coordinates, cell parameters, space group, experimental conditions and quality measures. Related Article: Eser S. Akturk, Glenn P. A. Yap, Klaus H. Theopold|2015|Chem.Commun.|51|15402|doi:10.1039/C5CC05993C

An entry from the Cambridge Structural Database, the world’s repository for small molecule crystal structures. The entry contains experimental data from a crystal diffraction study. The deposited dataset for this entry is freely available from the CCDC and typically includes 3D coordinates, cell parameters, space group, experimental conditions and quality measures. Related Article: Jade Pratt, Aimee M. Bryan, Michelle Faust, Jessica N. Boynton, Petra Vasko, Brian D. Rekken, Akseli Mansikkamäki, James C. Fettinger, Heikki M. Tuononen, Philip P. Power|2018|Inorg.Chem.|57|6491|doi:10.1021/acs.inorgchem.8b00551

NCBI accession numbers for prokaryotic host and viral genomes used in the training and evaluation of VirFinder. (XLSX 2752 kb)

Related Article: Cayley R. Harding, Jonathan Cann, Audrey Laventure, Mozhgan Sadeghianlemraski, Marwa Abd-Ellah, Keerthan R. Rao, Benjamin Sidney Gelfand, Hany Aziz, Loren Kaake, Chad Risko, Gregory C. Welch|2020|Materials Horizons|7|2959|doi:10.1039/D0MH00785D

An entry from the Cambridge Structural Database, the world’s repository for small molecule crystal structures. The entry contains experimental data from a crystal diffraction study. The deposited dataset for this entry is freely available from the CCDC and typically includes 3D coordinates, cell parameters, space group, experimental conditions and quality measures. Related Article: Qiong Yu, Jatinder Singh, Richard J. Staples, Jean'ne M. Shreeve|2022|Chem.Eng.Journal|431|133235|doi:10.1016/j.cej.2021.133235 Related Article: Qiong Yu, Jean'ne M. Shreeve|2022|CSD Communication|||

We present multiwavelength observations of the afterglow of GRB130427A, the brightest (in total fluence) Gamma-Ray Burst (GRB) of the past 29yr. Optical spectroscopy from Gemini-North reveals the redshift of the GRB to be z=0.340, indicating that its unprecedented brightness is primarily the result of its relatively close proximity to Earth; the intrinsic luminosities of both the GRB and its afterglow are not extreme in comparison to other bright GRBs. We present a large suite of multiwavelength observations spanning from 300s to 130days after the burst and demonstrate that the afterglow shows relatively simple, smooth evolution at all frequencies, with no significant late-time flaring or rebrightening activity. The entire data set from 1GHz to 10GeV can be modeled as synchrotron emission from a combination of reverse and forward shocks in good agreement with the standard afterglow model, providing strong support to the applicability of the underlying theory and clarifying the nature of the GeV emission observed to last for minutes to hours following other very bright GRBs. A tenuous, wind-stratified circumburst density profile is required by the observations, suggesting a massive-star progenitor with a low mass-loss rate, perhaps due to low metallicity. GRBs similar in nature to GRB 130427A, inhabiting low-density media and exhibiting strong reverse shocks, are probably not uncommon but may have been difficult to recognize in the past owing to their relatively faint late-time radio emission; more such events should be found in abundance by the new generation of sensitive radio and millimeter instruments.

Figure S1

An entry from the Cambridge Structural Database, the world’s repository for small molecule crystal structures. The entry contains experimental data from a crystal diffraction study. The deposited dataset for this entry is freely available from the CCDC and typically includes 3D coordinates, cell parameters, space group, experimental conditions and quality measures. Related Article: Juneyoung Lee, Jessica M. Grandner, Keary M. Engle, K. N. Houk, and Robert H. Grubbs|2016|J.Am.Chem.Soc.|138|7171|doi:10.1021/jacs.6b03767

A FASTA amino acid alignment used to generate the gene tree.