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Article . 2023
License: CC BY
Data sources: Datacite
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Article . 2023
License: CC BY
Data sources: Datacite
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XMM spectra of AT2020ocn

descriptionPublicationkeyboard_double_arrow_right Article 16 Aug 2023Publisher:Zenodo
Authors: Dheeraj Pasham;

doi: 10.5281/zenodo.8252930 , 10.5281/zenodo.8252931

XMM spectra of AT2020ocn

Abstract

Pileup corrected XMM spectra of AT2020ocn from two observation IDs: 0863650101 and 0863650201. The files named PN_Grouped_* can be loaded directly into xspec. They have been grouped using XMMSAS tool specgroup to have at least 1 count per spectral bin. Specifically, "mincounts=1 oversample=3" were used in specgroup. C-statistic should be used while modeling them in XSPEC.

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citations
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
views
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1
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