Powered by OpenAIRE graph
Found an issue? Give us feedback
image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/ ZENODOarrow_drop_down
image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/
ZENODO
Dataset . 2025
License: CC BY
Data sources: ZENODO
image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/
Universiteit van Amsterdam (UvA) Institutional Repository UvA-DARE
Dataset
License: CC BY
Data sources: Universiteit van Amsterdam (UvA) Institutional Repository UvA-DARE
ZENODO
Dataset . 2025
License: CC BY
Data sources: Datacite
ZENODO
Dataset . 2025
License: CC BY
Data sources: Datacite
 View all 3 versions
Claim

X-ray investigation of the remarkable galaxy group Nest200047

Research datakeyboard_double_arrow_right Dataset 12 Jun 2025 Netherlands Publisher:Zenodo
Authors: Majumder, Anwesh; Simionescu, Aurora; Plšek, Tomáš; Brienza, Marisa; Churazov, Eugene; Khabibullin, Ildar; Gastaldello, Fabio; +7 Authors

doi: 10.5281/zenodo.15650741 , 10.5281/zenodo.15650740

X-ray investigation of the remarkable galaxy group Nest200047

Abstract

Data reproduction package for the paper "X-ray investigation of the remarkable galaxy group Nest200047" by Anwesh Majumder, M.W. Wise, A. Simionescu, M.N. de Vries (accepted in MNRAS). Raw data: The Chandra and XMM data can be downloaded from https://cda.harvard.edu/chaser/ and http://nxsa.esac.esa.int/nxsa-web/#search using the observation IDs. See the 'Data' section of the paper to know what to download. Any additional data source has been mentioned in the paper as footnotes. Software required: CIAO (https://cxc.cfa.harvard.edu/ciao/) XMM-SAS (https://www.cosmos.esa.int/web/xmm-newton/download-and-install-sas) Jupyter Notebook and Python-3.9 or higher (https://jupyter.org) SPEX (https://spex-xray.github.io/spex-help/index.html) PyProffit (https://pyproffit.readthedocs.io/en/latest/index.html) CXBups (https://zenodo.org/records/2575495) There are README files inside directories. 

Country
Netherlands
Related Organizations
View all View all
Keywords

Shock waves, Methods: data analysis, Galaxies: active, Galaxies: groups: individual: Nest200047

  • BIP!
    Impact byBIP!
    selected citations
    These citations are derived from selected sources.
    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).
    		 0
    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.
    		 Average
    influence
    This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
    		 Average
    impulse
    This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
    		 Average
Powered by OpenAIRE graph
Found an issue? Give us feedback
selected citations
These citations are derived from selected sources.
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!
0
Average
Average
Average
Related to Research communities
Netherlands Research Portal