Zum Hauptinhalt springen

The study of the stars in the Big Data era ; El estudio de las estrellas en la era del big data

Klapp, Jaime ; Fierro-Santillán, Celia Rosa ; et al.
In: CIENCIA ergo-sum; Vol. 31 (2024): CIENCIA ergo-sum, 2023
academicJournal

Titel:
The study of the stars in the Big Data era ; El estudio de las estrellas en la era del big data
Autor/in / Beteiligte Person: Klapp, Jaime ; Fierro-Santillán, Celia Rosa ; Sigalotti, Leonardo Di G.
Link:
Zeitschrift: CIENCIA ergo-sum; Vol. 31 (2024): CIENCIA ergo-sum, 2023
Veröffentlichung: Universidad Autónoma del Estado de México, 2023
Medientyp: academicJournal
DOI: 10.30878/ces.v31n0a36
Sonstiges:
  • Nachgewiesen in: BASE
  • Sprachen: Spanish; Castilian
  • Document Type: article in journal/newspaper
  • File Description: application/pdf
  • Language: Spanish; Castilian
  • Relation: https://cienciaergosum.uaemex.mx/article/view/18108/15682; Bayo, A., Rodrigo, C., Barrado y Navascués, D., Solano, E., Gutiérrez, R., Morales-Calderón, M., & Allard, F. (2008). VOSA: virtual observatory SED analyzer, Astronomy & Astrophysics, 492, 277-287. https://doi.org/10.1051/0004-6361:200810395; Cheng, L., Zhang, F., Kang X., & Wang, L. (2018). A new stellar spectrum interpolation algorithm and its application to Yunnan-III evolutionary population synthesis models. Monthly Notices of the Royal Astronomical Society, 476, 4071-4084. https://doi.org/10.1093/mnras/sty373; Dafonte, C., Fustes, D., Manteiga, M., Garabato, D., Álvarez, M. A., Ulla, A., & Allende Prieto, C. (2016). On the estimation of stellar parameters with uncertainty prediction from Generative Artificial Neural Networks: application to Gaia RVS simulated spectra. Astronomy & Astrophysics, 594, A68, 1-10. https://doi.org/10.1051/0004-6361/201527045; Fierro, C. R., Borissova, J., Zsargó, J., Díaz-Azuara, A., Kurtev, R., Georgiev, L., Ramírez Alegría, S., & Peñaloza, F. (2015). Atlas of CMFGEN Models for OB Massive Stars, Publications of the Astronomical Society of the Pacific, 127, 428-436. https://iopscience.iop.org/article/10.1086/681703; Fierro-Santillán, C. R., Zsargó, J., Klapp, J., Díaz-Azuara, S. A., Arrieta, A., Arias, L., & Sigalotti, L. Di G. (2018). FITspec: A New Algorithm for the Automated Fit of Synthetic Stellar Spectra for OB Stars. The Astrophysical Journal Supplement, 236, 38-53. https://iopscience.iop.org/article/10.3847/1538-4365/aabd3a; Gräfener, G., Koesterke, L., & Hamann, W. -R. (2002). Line-blanketed model atmospheres for WR stars. Astronomy & Astrophysics, 387, 244-257. https://doi.org/10.1051/0004-6361:20020269; Hamann, W. -R., & Gräfener, G. (2003). A temperature correction method for expanding atmospheres. Astronomy & Astrophysics, 410, 993-1000. https://doi.org/10.1051/0004-6361:20031308; Hamann, W.-R., & Gräfener, G. (2004). Grids of model spectra for WN stars, ready for use. Astronomy & Astrophysics, 427, 697-704. https://doi.org/10.1051/0004-6361:20040506; Hamann D. M., & Hamann W.-R. (2004). University of Postdam, PoWR - The Potsdam Wolf-Rayet Models. https://www.astro.physik.uni-potsdam.de/~wrh/PoWR/powrgrid1.php#obgridstart.; Hillier, D. J., & Miller, D. L. (1998). The Treatment of Non-LTE Line Blanketing in Spherically Expanding Outflows. The Astrophysical Journal Supplement, 496, 407-427. https://iopscience.iop.org/article/ 10.1086/305350; Hubeny, I., & Lanz, T. (1995), Non-LTE Line-Blanketed Model Atmospheres of Hot Stars. I. Hybrid Complete Linearization/Accelerated Lambda Iteration Method. The Astrophysical Journal, 439, 875-904. https:// articles.adsabs.harvard.edu/full/1995ApJ.439.875H; Palacios, A., Gebran, M., Josselin, E., Martins, F., Plez, B., Belmas, M., & Lèbre A. (2010). POLLUX: a database of synthetic stellar spectra. Astronomy & Astrophysics, 516, A13, 1-8. https://doi.org/10.1051/0004- 6361/200913932; Puls, J., Urbaneja, M.A., Venero, R., et al. (2005). Astronomy & Astrophysics, 465, 669-698. https://ui.adsabs. harvard.edu/link_gateway/2005A%26A.435.669P/PUB_PDF; Sander, A., Shenar, T., Hainich, R., Gimenez-García A., Todt H., & Hamman, W. -R. (2015). On the consistent treatment of the quasi-hydrostatic layers in hot star atmospheres. Astronomy & Astrophysics, 577, A13, 1-13. https://doi.org/10.1051/0004-6361/201425356; Santolaya-Rey, A. E., Puls, J., & Herrero, A. (1997). Atmospheric NLTE-models for the spectroscopic analysis of luminous blue stars with winds. Astronomy & Astrophysics, 323, 488-512. https://articles.adsabs.harvard.edu/full/1997A%26A.323.488S; Sharma, K., Kembhavi, A., Kembhavi, A., Sivarani, T., Abraham, S., & Vaghmare, K. (2019). Detecting Outliers in SDSS using Convolutional Neural Network. Bulletin de la Société Royale des Sciences de Liège, 88, 174- 181. https://popups.uliege.be/0037-9565/index.php?id=8811; Sharma, K., Singth, H. P., Gupta, R., Kembhavi, A., Vaghmare, K., Shi, J., Zhao, Y., Zhang, J., & Wu, Y. (2020). Detecting Outliers in SDSS using Convolutional Neural Network. Bulletin de la Société Royale des Sciences de Liège, 88, 174-181. https://doi.org/10.25518/0037-9565.8811; Ting, Y. -S., Conroy, C., Rix, H. -W., & Cargile P. (2019). The Payne: Self-consistent ab initio Fitting of Stellar Spectra. The Astrophysical Journal Supplement, 879(2). https://iopscience.iop.org/article/10.3847/1538-4357/ab2331; UNAM (Universidad Nacional Autónoma de México). (2015). Atlas of CMFGEN Models for OB Massive Stars. http://www.astroscu.unam.mx/atlas/index.html; Zsargó, J., Fierro-Santillán, C. R., Klapp, J., Arrieta, A., Arias, L., Valencia, J. M. , Sigalotti, L. Di G., Hareter, M., & Puebla, R. E. (2020). Creating and using large grids of precalculated model atmospheres for a rapid analysis of stellar spectra. Astronomy & Astrophysics, 643, A88, 1-20. https://doi.org/10.1051/0004- 6361/202038066; https://cienciaergosum.uaemex.mx/article/view/18108
  • Rights: Derechos de autor 2023 CIENCIA ergo-sum ; http://creativecommons.org/licenses/by-nc-nd/4.0

Klicken Sie ein Format an und speichern Sie dann die Daten oder geben Sie eine Empfänger-Adresse ein und lassen Sie sich per Email zusenden.

oder
oder

Wählen Sie das für Sie passende Zitationsformat und kopieren Sie es dann in die Zwischenablage, lassen es sich per Mail zusenden oder speichern es als PDF-Datei.

oder
oder

Bitte prüfen Sie, ob die Zitation formal korrekt ist, bevor Sie sie in einer Arbeit verwenden. Benutzen Sie gegebenenfalls den "Exportieren"-Dialog, wenn Sie ein Literaturverwaltungsprogramm verwenden und die Zitat-Angaben selbst formatieren wollen.

xs 0 - 576
sm 576 - 768
md 768 - 992
lg 992 - 1200
xl 1200 - 1366
xxl 1366 -