International audienceFigure 1 as originally published did not match its corresponding caption; although the image was meant to be updated, it was unintentionally left unchanged. The correct Figure 1 with its corresponding caption is shown below
Due to an error at the publisher, in the published article the number of pulsars presented in the pa...
Table 1 contained one error. The time of ascending node T asc was incorrect due to a numerical conve...
In this article the wrong figure appeared as Fig. 38; the Fig. 38 should have appeared as shown belo...
International audienceFigure 1 as originally published did not match its corresponding caption; alth...
Figure 1 as originally published did not match its corresponding caption; although the image was mea...
The paper ‘Asteroseismology of KIC 11754974: a high-amplitude SX Phe pulsator in a 343-d binary syst...
International audienceThe paper ‘Evidence for an intermediate-mass black hole in the globular cluste...
Here we correct a factor of 2 missed in one of figures and the corresponding sentence in the text. I...
Corrects an error in Corongiu, A. et. al. (2012). A Shapiro delay detection in the binary system hos...
Due to an oversight of ours in proofreading and a communication problem with the publisher, the figu...
International audienceAfter publication of this article (Nishitani et al. 2019), it was brought to o...
International audienceNot Available Herschel is an ESA space observatory with science instruments pr...
Due to an error at the publisher, in the published article the number of pulsars presented in the pa...
This is an erratum to the paper ‘Testing gravity with wide binary stars like α Centauri’, published ...
International audienceBecause of an error in entering proof corrections, the term log((g)ϑ) in § 4.1...
Due to an error at the publisher, in the published article the number of pulsars presented in the pa...
Table 1 contained one error. The time of ascending node T asc was incorrect due to a numerical conve...
In this article the wrong figure appeared as Fig. 38; the Fig. 38 should have appeared as shown belo...
International audienceFigure 1 as originally published did not match its corresponding caption; alth...
Figure 1 as originally published did not match its corresponding caption; although the image was mea...
The paper ‘Asteroseismology of KIC 11754974: a high-amplitude SX Phe pulsator in a 343-d binary syst...
International audienceThe paper ‘Evidence for an intermediate-mass black hole in the globular cluste...
Here we correct a factor of 2 missed in one of figures and the corresponding sentence in the text. I...
Corrects an error in Corongiu, A. et. al. (2012). A Shapiro delay detection in the binary system hos...
Due to an oversight of ours in proofreading and a communication problem with the publisher, the figu...
International audienceAfter publication of this article (Nishitani et al. 2019), it was brought to o...
International audienceNot Available Herschel is an ESA space observatory with science instruments pr...
Due to an error at the publisher, in the published article the number of pulsars presented in the pa...
This is an erratum to the paper ‘Testing gravity with wide binary stars like α Centauri’, published ...
International audienceBecause of an error in entering proof corrections, the term log((g)ϑ) in § 4.1...
Due to an error at the publisher, in the published article the number of pulsars presented in the pa...
Table 1 contained one error. The time of ascending node T asc was incorrect due to a numerical conve...
In this article the wrong figure appeared as Fig. 38; the Fig. 38 should have appeared as shown belo...