Medium-resolution Isaac Newton Telescope library of empirical spectra

Clicks: 4
ID: 294601
2006
Article Quality & Performance Metrics
Overall Quality
Not rated
Combines reader engagement with the AI quality analysis. This article has not been analysed, so there is no overall score — reader engagement is measured and shown alongside.
AI Quality Assessment
Not analyzed
Readership in this journal
Steady

Ranked #182 of 913 articles by views in monthly notices of the royal astronomical society

Most read Least read

Bar heights use a square-root scale. Only the 120 most-read articles are drawn; the journal has 913 in total.

Mint this article as an NFT
Not yet minted

Create a permanent, verifiable on-chain record of this article on the Scimatic Network. The NFT is held in your Journament account, and you can withdraw it to your own wallet at any time.

5 SUSD one-off · no wallet required
Abstract
A new stellar library developed for stellar population synthesis modelling is presented. The library consists of 985 stars spanning a large range in atmospheric parameters. The spectra were obtained at the 2.5-m Isaac Newton Telescope and cover the range λλ 3525–7500 Å at 2.3 Å (full width at half-maximum) spectral resolution. The spectral resolution, spectral-type coverage, flux-calibration accuracy and number of stars represent a substantial improvement over previous libraries used in population-synthesis models.
Reference Key
openalex_W2163117531 Use this key to autocite in the manuscript while using SciMatic Manuscript Manager or Thesis Manager
Authors P. Sánchez–Blázquez, R. F. Peletier, J. Jiménez-Vicente, N. Cardiel, A. J. Cenarro, J. Falcón‐Barroso, J. Gorgas, S. O. Selam, A. Vazdekis
Journal monthly notices of the royal astronomical society
Year 2006
DOI
10.1111/j.1365-2966.2006.10699.x
URL
Keywords Keywords not found

Citations

No citations found. To add a citation, contact the admin at info@scimatic.org

No comments yet. Be the first to comment on this article.