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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/
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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/
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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/
Software Heritage
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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/
GitHub
Software
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Software Heritage
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/
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pessto software on GitHub
pessto software on GitHub in support of 'The broad-lined Type-Ic supernova SN 2022xxf and its extraordinary two-humped light curves I. Signatures of H/He-free interaction in the first four months'
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Related research
(32)
Abstract
pessto pipeline
32
Research products, page
1
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4
Eruptive mass loss less than a year before the explosion of superluminous supernovae
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SN 2023tsz: a helium-interaction-driven supernova in a very low-mass galaxy
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SN 2021zny: an early flux excess combined with late-time oxygen emission suggests a double white dwarf merger event
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Transient fading X-ray emission detected during the optical rise of a tidal disruption event
2024
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SN 2018agk: A Prototypical Type Ia Supernova with a Smooth Power-law Rise in Kepler (K2)
2021
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SN 2018gjx reveals that some SNe Ibn are SNe IIb exploding in dense circumstellar material
2020
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Eruptive mass loss less than a year before the explosion of superluminous supernovae
2025
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1100 days in the life of the supernova 2018ibb The best pair-instability supernova candidate, to date
2024
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1100 days in the life of the supernova 2018ibb
2024
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The broad-lined Type-Ic supernova SN 2022xxf and its extraordinary two-humped light curves
2023
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