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
ZENODO
Dataset . 2025
License: CC BY
Data sources: Datacite
ZENODO
Dataset . 2025
License: CC BY
Data sources: Datacite
versions View all 2 versions
addClaim

VLT/UVES Deep Spectroscopy of Galactic High-ADF PNe

Authors: Huang, Haomiao; Fang, Xuan; García-Rojas, Jorge; Tu, Zhijun; Liu, Jifeng; Liu, Xiaowei;

VLT/UVES Deep Spectroscopy of Galactic High-ADF PNe

Abstract

This repository contains the data products from our VLT/UVES deep spectroscopy of Galactic planetary nebulae, Hf 2-2, M 1-42 and NGC 6153, which exhibit high values of abundance discrepancy factor (ADF). The uploaded files include:- Three PDF files ("Hf2-2_1d.pdf", "M1-42_1d.pdf", "NGC6153_1d.pdf") showing the extracted 1D UVES spectra of each nebula. Wavelengths are given in Å, and fluxes are normalized so that F(Hβ) = 100. - A compressed archive "2D.zip" containing the fully calibrated 2D spectra in standard FITS format, organized by object and exposure time (long and short exposures). These FITS files can be read and analysed with common astronomy tools such as Astropy, IRAF/PyRAF, SAOImage DS9, etc.- A compressed archive "NGC6153_PV_diagram.zip" containing PDF figures of position–velocity (PV) diagrams in various nebular lines and related diagnostic maps for NGC 6153. These figures show, for example, line emission, electron temperature and density diagnostics, recombination and charge-exchange corrections, and ADF maps, corresponding to the figures discussed in our paper (Huang et al. 2025, ApJS, in press). The 2D FITS spectra are the primary data products that can be used to reproduce and extend the emission-line measurements and spatially-resolved diagnostic results presented in our paper. The PDF files of the 1D spectra and PV-diagrams provide visual demonstrations for convenience, and are direct links between the UVES data files and the figures in the associated article. 

Related Organizations
  • 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