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
Conference object . 2021
License: CC BY
Data sources: Datacite
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
Other literature type . 2021
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/
ZENODO
Conference object . 2021
License: CC BY
Data sources: Datacite
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
Conference object . 2019
License: CC BY
Data sources: Datacite
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
Other literature type . 2019
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/
ZENODO
Conference object . 2019
License: CC BY
Data sources: Datacite
versions View all 4 versions
addClaim

PySME - Spectroscopy Made Easier

Authors: Wehrhahn, Ansgar;

PySME - Spectroscopy Made Easier

Abstract

{"references": ["Asplund, Martin, Nicolas Grevesse, A. Jacques Sauval, and Pat Scott. 2009. \"The Chemical Composition of the Sun.\" Annual Review of Astronomy and Astrophysics 47 (1): 481\u2013522. https://doi.org/10.1146/annurev.astro.46.060407.145222", "Buder, Sven, Martin Asplund, Ly Duong, Janez Kos, Karin Lind, Melissa K. Ness, Sanjib Sharma, et al. 2018. \"The GALAH Survey: second data release.\" Monthly Notices of the RAS 478 (4): 4513\u201352. https://doi.org/10.1093/mnras/sty1281", "Gustafsson, B., B. Edvardsson, K. Eriksson, U. G. J\u00f8rgensen,. Nordlund, and B. Plez. 2008. \"A grid of MARCS model atmospheres for late-type stars. I. Methods and general properties.\" Astronomy and Astrophysics 486 (3): 951\u201370. https://doi.org/10.1051/0004-6361:200809724", "Kupka, F. G., T. A. Ryabchikova, N. E. Piskunov, H. C. Stempels, and W. W. Weiss. 2000. \"VALD-2 \u2013 the New Vienna Atomic Line Database.\" Baltic Astronomy 9 (January): 590\u201394. https://doi.org/10.1515/astro-2000-0420", "Kupka, F., N. Piskunov, T. A. Ryabchikova, H. C. Stempels, and W. W. Weiss. 1999. \"VALD-2: Progress of the Vienna Atomic Line Data Base.\" Astronomy and Astrophysics, Supplement 138 (July): 119\u201333. https://doi.org/10.1051/aas:1999267", "Loss, RD. 2003. \"Atomic Weights of the Elements 2001 (Iupac Technical Report).\" Pure and Applied Chemistry 75 (8). De Gruyter: 1107\u201322", "Piskunov, N. E., F. Kupka, T. A. Ryabchikova, W. W. Weiss, and C. S. Jeffery. 1995. \"VALD: The Vienna Atomic Line Data Base.\" Astronomy and Astrophysics, Supplement 112 (September): 525", "Piskunov, Nikolai, and Jeff A. Valenti. 2017. \"Spectroscopy Made Easy: Evolution.\" Astronomy and Astrophysics 597 (January): A16. https://doi.org/10.1051/0004-6361/201629124", "Ryabchikova, T. A., N. E. Piskunov, F. Kupka, and W. W. Weiss. 1997. \"The Vienna Atomic Line Database : Present State and Future Development.\" Baltic Astronomy 6 (March): 244\u201347. https://doi.org/10.1515/astro-1997-0216", "Ryabchikova, T., N. Piskunov, R. L. Kurucz, H. C. Stempels, U. Heiter, Yu Pakhomov, and P. S. Barklem. 2015. \"A major upgrade of the VALD database.\" Physica Scripta 90 (5): 054005. https://doi.org/10.1088/0031-8949/90/5/054005", "Valenti, J. A., and N. Piskunov. 1996. \"Spectroscopy made easy: A new tool for fitting observations with synthetic spectra.\" Astronomy and Astrophysics, Supplement 118 (September): 595\u2013603"]}

Over 20 years ago Valenti & Piskuonov developed the stellar spectral synthesis library Spectroscopy Made Easy (SME) to simplify stellar spectral analysis, and it has been used in hundreds of works since. PySME is a new Python frontend to the same library, developed with the same goal in mind: Making spectroscopy easier for everyone. PySME creates accurate, high-resolution synthetic spectra, based on a range of stellar parameters, a linelist and a model atmosphere. It can also be used the other way around. Give PySME an observation and it will determine the best fit stellar parameters for that spectrum. This is also useful for Exoplanet research. It is important to understand the host star, to properly understand the workings of the orbiting planet.

An interactive version of this poster is available at http://sme.astro.uu.se/poster.html

Related Organizations
Keywords

Astronomy, Cool Stars on the main sequence, Astronomdagarna 2019, Software, Spectroscopy, Python

  • 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).
    1
    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
    OpenAIRE UsageCounts
    Usage byUsageCounts
    visibility views 17
    download downloads 19
  • 17
    views
    19
    downloads
    Powered byOpenAIRE UsageCounts
Powered by OpenAIRE graph
Found an issue? Give us feedback
visibility
download
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!
views
OpenAIRE UsageCountsViews provided by UsageCounts
downloads
OpenAIRE UsageCountsDownloads provided by UsageCounts
1
Average
Average
Average
17
19
Green
Related to Research communities