Severity: Warning
Message: file_get_contents(https://...@pubfacts.com&api_key=b8daa3ad693db53b1410957c26c9a51b4908&a=1): Failed to open stream: HTTP request failed! HTTP/1.1 429 Too Many Requests
Filename: helpers/my_audit_helper.php
Line Number: 176
Backtrace:
File: /var/www/html/application/helpers/my_audit_helper.php
Line: 176
Function: file_get_contents
File: /var/www/html/application/helpers/my_audit_helper.php
Line: 250
Function: simplexml_load_file_from_url
File: /var/www/html/application/helpers/my_audit_helper.php
Line: 3122
Function: getPubMedXML
File: /var/www/html/application/controllers/Detail.php
Line: 575
Function: pubMedSearch_Global
File: /var/www/html/application/controllers/Detail.php
Line: 489
Function: pubMedGetRelatedKeyword
File: /var/www/html/index.php
Line: 316
Function: require_once
The ternary rare-earth-metal nickel indides RENiIn (RE = Gd, Tb, Dy) were prepared by arc-melting mixtures of the elements followed by annealing at 870 K. They adopt the YbCuMg-type structure (space group 6/, Pearson symbol 68, = 2), as determined by laboratory and synchrotron powder diffraction methods for RE = Gd ( = 9.6435(10) Å, = 22.118(3) Å) and Tb ( = 9.5695(8) Å, = 21.983(3) Å), and single-crystal X-ray diffraction methods for RE = Dy ( = 9.533(5) Å, = 21.890(13) Å). The centrosymmetric YbCuMg-type structure is closely related to the noncentrosymmetric PrIrMg-type structure. Triangular In clusters within RENiIn represent a rare type of cluster found among metal-rich indides; the reasons for their formation were investigated by density functional theory methods.
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Source |
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http://dx.doi.org/10.1021/acs.inorgchem.1c02486 | DOI Listing |
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