Article (Scientific journals)
Correction to: Redshift drift and strong gravitational lensing
Helbig, Phillip
2024In Monthly Notices of the Royal Astronomical Society, 528 (2), p. 1582-1582
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Keywords :
Space and Planetary Science; Astronomy and Astrophysics; gravitational lensing: strong; galaxies:clusters:general; galaxies: distances and redshifts; dark matter; cosmology: miscellaneous; cosmology: theory; errata; addenda
Abstract :
[en] As a correction, there is no abstract. Here is a summary: Unfortunately, my paper contains a mistake. I wrote that "[b]y measuring the difference in redshift between two images, one effectively measures the time delay". However, the difference in redshift is proportional to the to the time delay and to the Hubble constant (my equation 5), thus one cannot use the measured difference in redshift between images of a gravitational-lens system in order to measure the Hubble constant. All other aspects of my paper are unaffected: consistency check on standard cosmology, using an Einstein ring to correct for the change in redshift due to the moving-lens effect, effectively measuring time delays (for a given Hubble constant!) on much longer timescales and/or for non-variable sources, measuring the transverse velocity of the lens, and determing which images in a complex gravitational-lens system correspond to the same source.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Helbig, Phillip  ;  Université de Liège - ULiège > Unités de recherche interfacultaires > Space sciences, Technologies and Astrophysics Research (STAR) ; Thomas-Mann-Str. 9 , D-63477 Maintal , Germany
Language :
English
Title :
Correction to: Redshift drift and strong gravitational lensing
Publication date :
23 January 2024
Journal title :
Monthly Notices of the Royal Astronomical Society
ISSN :
0035-8711
eISSN :
1365-2966
Publisher :
Oxford University Press (OUP)
Volume :
528
Issue :
2
Pages :
1582-1582
Peer reviewed :
Peer Reviewed verified by ORBi
Commentary :
Correction to. https://orbi.uliege.be/handle/2268/298190
Available on ORBi :
since 29 January 2024

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