Variability of the fine-structure constant

DOI

We have previously presented evidence for a varying fine-structure constant, {alpha}, in two independent samples of Keck/HIRES quasi-stellar object (QSO) absorption spectra. Here we present a detailed many-multiplet analysis of a third Keck/HIRES sample containing 78 absorption systems. We also re-analyse the previous samples, providing a total of 128 absorption systems over the redshift range 0.2<zabs<3.7.

Cone search capability for table J/MNRAS/345/609/table3 (The raw results from the {Chi}^2^ minimization procedure)

Identifier
DOI http://doi.org/10.26093/cds/vizier.73450609
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/MNRAS/345/609
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/345/609
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/345/609
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/MNRAS/345/609
Provenance
Creator Murphy M.T.; Webb J.K.; Flambaum V.V.
Publisher CDS
Publication Year 2004
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Galactic and extragalactic Astronomy; High Energy Astrophysics; Interdisciplinary Astronomy; Natural Sciences; Physics; Stellar Astronomy