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Araucaria Project (English Wikipedia)

Analysis of information sources in references of the Wikipedia article "Araucaria Project" in English language version.

refsWebsite
Global rank English rank
4arxiv.org
69th place
59th place
4doi.org
2nd place
2nd place
4nih.gov
4th place
4th place
3harvard.edu
18th place
17th place
1worldcat.org
5th place
5th place

arxiv.org

  • Pietrzyński; et al. (2010). "The dynamical mass of a classical Cepheid variable star in an eclipsing binary system". Nature. 468 (7323): 542–544. arXiv:1012.0231. Bibcode:2010Natur.468..542P. doi:10.1038/nature09598. PMID 21107425.
  • Pietrzyński; et al. (2012). "RR-Lyrae-type pulsations from a 0.26-solar-mass star in a binary system". Nature. 484 (7392): 75–77. arXiv:1204.1872. Bibcode:2012Natur.484...75P. doi:10.1038/nature10966. PMID 22481359.
  • Pietrzyński; et al. (2013). "An eclipsing binary distance to the Large Magellanic Cloud accurate to 2 per cent". Nature. 495 (7439): 76–79. arXiv:1303.2063. Bibcode:2013Natur.495...76P. doi:10.1038/nature11878. PMID 23467166.
  • Pietrzyński, G.; Graczyk, D.; Gallenne, A.; Gieren, W.; Thompson, I. B.; Pilecki, B.; Karczmarek, P.; Górski, M.; Suchomska, K.; Taormina, M.; Zgirski, B. (2019). "A distance to the Large Magellanic Cloud that is precise to one per cent". Nature. 567 (7747): 200–203. arXiv:1903.08096. doi:10.1038/s41586-019-0999-4. ISSN 0028-0836. PMID 30867610.

doi.org

  • Pietrzyński; et al. (2010). "The dynamical mass of a classical Cepheid variable star in an eclipsing binary system". Nature. 468 (7323): 542–544. arXiv:1012.0231. Bibcode:2010Natur.468..542P. doi:10.1038/nature09598. PMID 21107425.
  • Pietrzyński; et al. (2012). "RR-Lyrae-type pulsations from a 0.26-solar-mass star in a binary system". Nature. 484 (7392): 75–77. arXiv:1204.1872. Bibcode:2012Natur.484...75P. doi:10.1038/nature10966. PMID 22481359.
  • Pietrzyński; et al. (2013). "An eclipsing binary distance to the Large Magellanic Cloud accurate to 2 per cent". Nature. 495 (7439): 76–79. arXiv:1303.2063. Bibcode:2013Natur.495...76P. doi:10.1038/nature11878. PMID 23467166.
  • Pietrzyński, G.; Graczyk, D.; Gallenne, A.; Gieren, W.; Thompson, I. B.; Pilecki, B.; Karczmarek, P.; Górski, M.; Suchomska, K.; Taormina, M.; Zgirski, B. (2019). "A distance to the Large Magellanic Cloud that is precise to one per cent". Nature. 567 (7747): 200–203. arXiv:1903.08096. doi:10.1038/s41586-019-0999-4. ISSN 0028-0836. PMID 30867610.

harvard.edu

ui.adsabs.harvard.edu

  • Pietrzyński; et al. (2010). "The dynamical mass of a classical Cepheid variable star in an eclipsing binary system". Nature. 468 (7323): 542–544. arXiv:1012.0231. Bibcode:2010Natur.468..542P. doi:10.1038/nature09598. PMID 21107425.
  • Pietrzyński; et al. (2012). "RR-Lyrae-type pulsations from a 0.26-solar-mass star in a binary system". Nature. 484 (7392): 75–77. arXiv:1204.1872. Bibcode:2012Natur.484...75P. doi:10.1038/nature10966. PMID 22481359.
  • Pietrzyński; et al. (2013). "An eclipsing binary distance to the Large Magellanic Cloud accurate to 2 per cent". Nature. 495 (7439): 76–79. arXiv:1303.2063. Bibcode:2013Natur.495...76P. doi:10.1038/nature11878. PMID 23467166.

nih.gov

pubmed.ncbi.nlm.nih.gov

  • Pietrzyński; et al. (2010). "The dynamical mass of a classical Cepheid variable star in an eclipsing binary system". Nature. 468 (7323): 542–544. arXiv:1012.0231. Bibcode:2010Natur.468..542P. doi:10.1038/nature09598. PMID 21107425.
  • Pietrzyński; et al. (2012). "RR-Lyrae-type pulsations from a 0.26-solar-mass star in a binary system". Nature. 484 (7392): 75–77. arXiv:1204.1872. Bibcode:2012Natur.484...75P. doi:10.1038/nature10966. PMID 22481359.
  • Pietrzyński; et al. (2013). "An eclipsing binary distance to the Large Magellanic Cloud accurate to 2 per cent". Nature. 495 (7439): 76–79. arXiv:1303.2063. Bibcode:2013Natur.495...76P. doi:10.1038/nature11878. PMID 23467166.
  • Pietrzyński, G.; Graczyk, D.; Gallenne, A.; Gieren, W.; Thompson, I. B.; Pilecki, B.; Karczmarek, P.; Górski, M.; Suchomska, K.; Taormina, M.; Zgirski, B. (2019). "A distance to the Large Magellanic Cloud that is precise to one per cent". Nature. 567 (7747): 200–203. arXiv:1903.08096. doi:10.1038/s41586-019-0999-4. ISSN 0028-0836. PMID 30867610.

worldcat.org

search.worldcat.org

  • Pietrzyński, G.; Graczyk, D.; Gallenne, A.; Gieren, W.; Thompson, I. B.; Pilecki, B.; Karczmarek, P.; Górski, M.; Suchomska, K.; Taormina, M.; Zgirski, B. (2019). "A distance to the Large Magellanic Cloud that is precise to one per cent". Nature. 567 (7747): 200–203. arXiv:1903.08096. doi:10.1038/s41586-019-0999-4. ISSN 0028-0836. PMID 30867610.