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Erratum to: Search for new physics in dijet angular distributions using proton-proton collisions at s=13TeV and constraints on dark matter and other models.

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Title: Erratum to: Search for new physics in dijet angular distributions using proton-proton collisions at s=13TeV and constraints on dark matter and other models.
Authors: Sirunyan, A. M.1 (AUTHOR), Tumasyan, A.1 (AUTHOR), Adam, W.2 (AUTHOR), Ambrogi, F.2 (AUTHOR), Asilar, E.2 (AUTHOR), Bergauer, T.2 (AUTHOR), Brandstetter, J.2 (AUTHOR), Brondolin, E.2 (AUTHOR), Dragicevic, M.2 (AUTHOR), Erö, J.2 (AUTHOR), Valle, A. Escalante Del2 (AUTHOR), Flechl, M.2 (AUTHOR), Friedl, M.2 (AUTHOR), Frühwirth, R.2,3 (AUTHOR), Ghete, V. M.2 (AUTHOR), Grossmann, J.2 (AUTHOR), Hrubec, J.2 (AUTHOR), Jeitler, M.2,3 (AUTHOR), König, A.2 (AUTHOR), Krammer, N.2 (AUTHOR)
Source: European Physical Journal C -- Particles & Fields. Apr2022, Vol. 82 Issue 4, p1-15. 15p.
Subjects: Angular distribution (Nuclear physics), Dark matter, Physics, Proton-proton interactions
Abstract: The original article can be found online at https://doi.org/10.1140/epjc/s10052-018-6242-x. J. C (2018) 78:789 https://doi.org/10.1140/epjc/s10052-018-6242-x In this article the author name Luigi Calligaris was incorrectly written as A. Calligaris. [Extracted from the article]
Copyright of European Physical Journal C -- Particles & Fields is the property of Springer Nature and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.)
Database: Engineering Source
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  Data: Erratum to: Search for new physics in dijet angular distributions using proton-proton collisions at s=13TeV and constraints on dark matter and other models.
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  Data: <searchLink fieldCode="AR" term="%22Sirunyan%2C+A%2E+M%2E%22">Sirunyan, A. M.</searchLink><relatesTo>1</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Tumasyan%2C+A%2E%22">Tumasyan, A.</searchLink><relatesTo>1</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Adam%2C+W%2E%22">Adam, W.</searchLink><relatesTo>2</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Ambrogi%2C+F%2E%22">Ambrogi, F.</searchLink><relatesTo>2</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Asilar%2C+E%2E%22">Asilar, E.</searchLink><relatesTo>2</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Bergauer%2C+T%2E%22">Bergauer, T.</searchLink><relatesTo>2</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Brandstetter%2C+J%2E%22">Brandstetter, J.</searchLink><relatesTo>2</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Brondolin%2C+E%2E%22">Brondolin, E.</searchLink><relatesTo>2</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Dragicevic%2C+M%2E%22">Dragicevic, M.</searchLink><relatesTo>2</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Erö%2C+J%2E%22">Erö, J.</searchLink><relatesTo>2</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Valle%2C+A%2E+Escalante+Del%22">Valle, A. Escalante Del</searchLink><relatesTo>2</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Flechl%2C+M%2E%22">Flechl, M.</searchLink><relatesTo>2</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Friedl%2C+M%2E%22">Friedl, M.</searchLink><relatesTo>2</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Frühwirth%2C+R%2E%22">Frühwirth, R.</searchLink><relatesTo>2,3</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Ghete%2C+V%2E+M%2E%22">Ghete, V. M.</searchLink><relatesTo>2</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Grossmann%2C+J%2E%22">Grossmann, J.</searchLink><relatesTo>2</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Hrubec%2C+J%2E%22">Hrubec, J.</searchLink><relatesTo>2</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Jeitler%2C+M%2E%22">Jeitler, M.</searchLink><relatesTo>2,3</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22König%2C+A%2E%22">König, A.</searchLink><relatesTo>2</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Krammer%2C+N%2E%22">Krammer, N.</searchLink><relatesTo>2</relatesTo> (AUTHOR)
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  Data: <searchLink fieldCode="JN" term="%22European+Physical+Journal+C+--+Particles+%26+Fields%22">European Physical Journal C -- Particles & Fields</searchLink>. Apr2022, Vol. 82 Issue 4, p1-15. 15p.
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  Data: <searchLink fieldCode="DE" term="%22Angular+distribution+%28Nuclear+physics%29%22">Angular distribution (Nuclear physics)</searchLink><br /><searchLink fieldCode="DE" term="%22Dark+matter%22">Dark matter</searchLink><br /><searchLink fieldCode="DE" term="%22Physics%22">Physics</searchLink><br /><searchLink fieldCode="DE" term="%22Proton-proton+interactions%22">Proton-proton interactions</searchLink>
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  Data: The original article can be found online at https://doi.org/10.1140/epjc/s10052-018-6242-x. J. C (2018) 78:789 https://doi.org/10.1140/epjc/s10052-018-6242-x In this article the author name Luigi Calligaris was incorrectly written as A. Calligaris. [Extracted from the article]
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  Data: <i>Copyright of European Physical Journal C -- Particles & Fields is the property of Springer Nature and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract.</i> (Copyright applies to all Abstracts.)
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