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Technical comment on the paper of Dessert et al. "The dark matter interpretation of the 3.5 keV line is inconsistent with blank-sky observations"
by Alexey Boyarsky, Denys Malyshev, Oleg Ruchayskiy, Denys Savchenko
This Submission thread is now published as
|Authors (as Contributors):||Denys Savchenko|
|Arxiv Link:||https://arxiv.org/abs/2004.06601v2 (pdf)|
|Date submitted:||2021-02-25 08:53|
|Submitted by:||Savchenko, Denys|
|Submitted to:||SciPost Astronomy Core|
An unidentified line at energy around 3.5 keV was detected in the spectra of dark matter-dominated objects. Recent work of Dessert et al. [1812.06976] used 30 Msec of XMM-Newton blank-sky observations to constrain the admissible line flux, challenging its dark matter decay origin. We demonstrate that these bounds are overestimated by more than an order of magnitude due to improper background modeling. Therefore the dark matter interpretation of the 3.5 keV signal remains viable.
Published as SciPost Astro. Core 1, 001 (2021)
Author comments upon resubmission
We are submitting the revised version of the Technical comment with changes suggested by the Referee.
These changes aimed at visual clarification for the readers of the points in the article.
It took more time than expected for a minor revision due to COVID-related disruptions.
List of changes
1. Fig. 2 added, which shows the actual spectra together with models under consideration.
2. Additional paragraph referencing Fig. 2 added.
3. Typesetting changed to match SciPost style.
Submission & Refereeing History
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Reports on this Submission
Report 1 by Dominique Eckert on 2021-4-12 (Invited Report)
Thanks for addressing my previous points, I think the new figure showing the actual spectrum is very nice and it convincingly makes the case for including the various lines. I am happy to recommend acceptance of the paper.