Multifrequency Study of the Blazar 3C 454.3
This work is devoted to multi-frequency studying of the blazar 3C 454.3. The study includes spectroscopic and photometric observations in the optical, IR, and gamma-ray bands. We investigate whether a correlation exists in the light curves at different wavelengths. We have carried out observations o...
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MDPI AG
2016-12-01
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Online Access: | http://www.mdpi.com/2075-4434/5/1/3 |
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author | Ilhuiyolitzin Villicaña-Pedraza Francisco Carreto-Parra Alberto Carramiñana Julio Saucedo-Morales |
author_facet | Ilhuiyolitzin Villicaña-Pedraza Francisco Carreto-Parra Alberto Carramiñana Julio Saucedo-Morales |
author_sort | Ilhuiyolitzin Villicaña-Pedraza |
collection | DOAJ |
description | This work is devoted to multi-frequency studying of the blazar 3C 454.3. The study includes spectroscopic and photometric observations in the optical, IR, and gamma-ray bands. We investigate whether a correlation exists in the light curves at different wavelengths. We have carried out observations of the optical spectrum (from 4000 to 7000 Angstroms) between 2007 and 2009, and identified MgII [2800 Angstroms] and FeII emission line features. We have obtained optical magnitudes and color indices of the quasar and performed a correlation between the optical, IR, and gamma-ray light curves. We have found statistically significant correlations between the light curves at different wavelengths. |
first_indexed | 2024-12-21T13:38:25Z |
format | Article |
id | doaj.art-99bf117d013740debb45c8189de8191a |
institution | Directory Open Access Journal |
issn | 2075-4434 |
language | English |
last_indexed | 2024-12-21T13:38:25Z |
publishDate | 2016-12-01 |
publisher | MDPI AG |
record_format | Article |
series | Galaxies |
spelling | doaj.art-99bf117d013740debb45c8189de8191a2022-12-21T19:02:06ZengMDPI AGGalaxies2075-44342016-12-0151310.3390/galaxies5010003galaxies5010003Multifrequency Study of the Blazar 3C 454.3Ilhuiyolitzin Villicaña-Pedraza0Francisco Carreto-Parra1Alberto Carramiñana2Julio Saucedo-Morales3Departamento de Física Teórica, Universidad Autónoma de Madrid, Madrid 28049, SpainScience Department, New Mexico State University, Las cruces, NM 88003, USACoordinación de Astrofísica, Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla 72840, MéxicoDepartamento de Investigación en Física, Universidad de Sonora, Hermosillo Sonora 83000, MéxicoThis work is devoted to multi-frequency studying of the blazar 3C 454.3. The study includes spectroscopic and photometric observations in the optical, IR, and gamma-ray bands. We investigate whether a correlation exists in the light curves at different wavelengths. We have carried out observations of the optical spectrum (from 4000 to 7000 Angstroms) between 2007 and 2009, and identified MgII [2800 Angstroms] and FeII emission line features. We have obtained optical magnitudes and color indices of the quasar and performed a correlation between the optical, IR, and gamma-ray light curves. We have found statistically significant correlations between the light curves at different wavelengths.http://www.mdpi.com/2075-4434/5/1/3blazarAGN3C 454.3Multifrequency |
spellingShingle | Ilhuiyolitzin Villicaña-Pedraza Francisco Carreto-Parra Alberto Carramiñana Julio Saucedo-Morales Multifrequency Study of the Blazar 3C 454.3 Galaxies blazar AGN 3C 454.3 Multifrequency |
title | Multifrequency Study of the Blazar 3C 454.3 |
title_full | Multifrequency Study of the Blazar 3C 454.3 |
title_fullStr | Multifrequency Study of the Blazar 3C 454.3 |
title_full_unstemmed | Multifrequency Study of the Blazar 3C 454.3 |
title_short | Multifrequency Study of the Blazar 3C 454.3 |
title_sort | multifrequency study of the blazar 3c 454 3 |
topic | blazar AGN 3C 454.3 Multifrequency |
url | http://www.mdpi.com/2075-4434/5/1/3 |
work_keys_str_mv | AT ilhuiyolitzinvillicanapedraza multifrequencystudyoftheblazar3c4543 AT franciscocarretoparra multifrequencystudyoftheblazar3c4543 AT albertocarraminana multifrequencystudyoftheblazar3c4543 AT juliosaucedomorales multifrequencystudyoftheblazar3c4543 |