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: 197
Backtrace:
File: /var/www/html/application/helpers/my_audit_helper.php
Line: 197
Function: file_get_contents
File: /var/www/html/application/helpers/my_audit_helper.php
Line: 271
Function: simplexml_load_file_from_url
File: /var/www/html/application/helpers/my_audit_helper.php
Line: 1057
Function: getPubMedXML
File: /var/www/html/application/helpers/my_audit_helper.php
Line: 3175
Function: GetPubMedArticleOutput_2016
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
Rovibrational spectra of DO-CS and HDO-CS van der Waals complexes have been measured in the bending region of DO/HDO by direct absorption in a slit supersonic jet expansion. The HO-CS dimer is reinvestigated in the bending region of HO with a higher rotational temperature compared with the previous study [Barclay, A. J. 2024, 26, 23053-23061], namely, ∼10 versus ∼2 K. Only the most stable isomer was observed, and precise molecular constants for these three complexes are determined. The HDO-CS complex in the supersonic jet was relaxed into an equilibrated population. But the line intensities for transitions originating from the = 1 levels in the ground state for both DO-CS and HO-CS are found to be significantly stronger than those predicted with normal nuclear spin statistical weights. This abnormality is likely due to the different yielding rates for the - and - spin species of DO-CS or HO-CS in the supersonic jet expansion.
Download full-text PDF |
Source |
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http://dx.doi.org/10.1021/acs.jpca.5c00087 | DOI Listing |
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