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ZENODO
Dataset . 2025
License: CC BY
Data sources: ZENODO
ZENODO
Dataset . 2025
License: CC BY
Data sources: Datacite
ZENODO
Dataset . 2025
License: CC BY
Data sources: Datacite
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SED fitting results for "The initial-to-final mass relation of white dwarfs in intermediate-separation binaries"

Authors: Hallakoun, Na'ama; Shahaf, Sahar; Ben-Ami, Sagi;

SED fitting results for "The initial-to-final mass relation of white dwarfs in intermediate-separation binaries"

Abstract

SED Fitting Results. Both $\chi^2_\text{IR}$ and $\chi^2_\text{opt}$ are calculated using both optical and IR data, and normalized by the number of degrees of freedom ($N_\text{IR}+N_\text{opt} - 2$). However, $\chi^2_\text{opt}$ is calculated using the model fit to optical data only. Candidates 101, 140, 160, 192, 194, 282 are suspected of showing IR excess, and therefore are not given a full optical+IR fit. $T_\text{eff,2}$ values are obtained from the full binary fit for candidates with UV excess. \label{tab:sed_results}

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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