International audienceWe report an erratum in Morabito et al. (2019, A&A, 622, A15). When calculating radio powers from observed flux densities, the wrong sign convention was used. This resulted in an underestimation of the radio powers by a median value of 0.6 dex and a maximum of 1 dex. The conclusions of the paper are unchanged
International audienceIn our recent Letter (A. Vourlidas et al. [ApJ, 656, L105 [2007]], hereafter P...
This is a correction to the paper’Galaxy source counts at 7.7 μm, 10 μm and 15 μm with the James Web...
International audienceIn our recent Letter (A. Vourlidas et al. [ApJ, 656, L105 [2007]], hereafter P...
International audienceWe report an erratum in Morabito et al. (2019, A&A, 622, A15). When calculatin...
International audienceWe report an erratum in Morabito et al. (2019, A&A, 622, A15). When calculatin...
We report an erratum in Morabito et al. (2019, A&A, 622, A15). When calculating radio powers from ob...
We report an erratum in Morabito et al. (2019, A&A, 622, A15). When calculating radio powers from ob...
In this Letter, we omitted to cite preliminary results from the low-energy extension of the Pierre A...
In this Letter, we omitted to cite preliminary results from the low-energy extension of the Pierre A...
In this Letter, we omitted to cite preliminary results from the low-energy extension of the Pierre A...
Corrects an error in van Straten, W. (2009) The statistics of radio astronomical polarimetry: bright...
© 2017 The Authors. This is an erratum to the paper 'Galactic synchrotron emissivity measurements be...
This is a correction to: Monthly Notices of the Royal Astronomical Society, Volume 496, Issue 1, Jul...
In the paper "Quasar X-Ray Spectra Revisited " by P. Shastri, B. J. Wilkes, M. Elvis, and J. McDowel...
International audienceIn our recent Letter (A. Vourlidas et al. [ApJ, 656, L105 [2007]], hereafter P...
International audienceIn our recent Letter (A. Vourlidas et al. [ApJ, 656, L105 [2007]], hereafter P...
This is a correction to the paper’Galaxy source counts at 7.7 μm, 10 μm and 15 μm with the James Web...
International audienceIn our recent Letter (A. Vourlidas et al. [ApJ, 656, L105 [2007]], hereafter P...
International audienceWe report an erratum in Morabito et al. (2019, A&A, 622, A15). When calculatin...
International audienceWe report an erratum in Morabito et al. (2019, A&A, 622, A15). When calculatin...
We report an erratum in Morabito et al. (2019, A&A, 622, A15). When calculating radio powers from ob...
We report an erratum in Morabito et al. (2019, A&A, 622, A15). When calculating radio powers from ob...
In this Letter, we omitted to cite preliminary results from the low-energy extension of the Pierre A...
In this Letter, we omitted to cite preliminary results from the low-energy extension of the Pierre A...
In this Letter, we omitted to cite preliminary results from the low-energy extension of the Pierre A...
Corrects an error in van Straten, W. (2009) The statistics of radio astronomical polarimetry: bright...
© 2017 The Authors. This is an erratum to the paper 'Galactic synchrotron emissivity measurements be...
This is a correction to: Monthly Notices of the Royal Astronomical Society, Volume 496, Issue 1, Jul...
In the paper "Quasar X-Ray Spectra Revisited " by P. Shastri, B. J. Wilkes, M. Elvis, and J. McDowel...
International audienceIn our recent Letter (A. Vourlidas et al. [ApJ, 656, L105 [2007]], hereafter P...
International audienceIn our recent Letter (A. Vourlidas et al. [ApJ, 656, L105 [2007]], hereafter P...
This is a correction to the paper’Galaxy source counts at 7.7 μm, 10 μm and 15 μm with the James Web...
International audienceIn our recent Letter (A. Vourlidas et al. [ApJ, 656, L105 [2007]], hereafter P...