New GTC spectroscopic data and a statistical study to better constrain the redshift of the BL Lac RGB J2243 + 203
We present new spectroscopic data of the BL Lac RGB 2243 + 203, and its surroundings, obtained with the OSIRIS Multi Object Spectrograph (MOS) mounted in the Gran Telescopio Canarias (GTC). The spectra of neither the BL Lac nor its host galaxy show any spectral feature, thus hindering direct determi...
Guardado en:
Publicado: |
2019
|
---|---|
Materias: | |
Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00358711_v482_n4_p5422_RosaGonzalez http://hdl.handle.net/20.500.12110/paper_00358711_v482_n4_p5422_RosaGonzalez |
Aporte de: |
id |
paper:paper_00358711_v482_n4_p5422_RosaGonzalez |
---|---|
record_format |
dspace |
spelling |
paper:paper_00358711_v482_n4_p5422_RosaGonzalez2023-06-08T15:01:51Z New GTC spectroscopic data and a statistical study to better constrain the redshift of the BL Lac RGB J2243 + 203 BL lacertae objects: individual: RGB 2243 + 203 Galaxies: distances Redshifts We present new spectroscopic data of the BL Lac RGB 2243 + 203, and its surroundings, obtained with the OSIRIS Multi Object Spectrograph (MOS) mounted in the Gran Telescopio Canarias (GTC). The spectra of neither the BL Lac nor its host galaxy show any spectral feature, thus hindering direct determination of its redshift. The spectroscopic redshift distribution of objects in the MOS field of view shows four galaxies with redshift between 0.5258 and 0.5288. We make use of a statistical analysis to test the possibility that the targeted BL Lac may be a member of that group. By using the spectroscopic redshifts obtained with our GTC observations, we found that this probability is between 86 and 93 per cent. © 2018 The Author(s). 2019 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00358711_v482_n4_p5422_RosaGonzalez http://hdl.handle.net/20.500.12110/paper_00358711_v482_n4_p5422_RosaGonzalez |
institution |
Universidad de Buenos Aires |
institution_str |
I-28 |
repository_str |
R-134 |
collection |
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
topic |
BL lacertae objects: individual: RGB 2243 + 203 Galaxies: distances Redshifts |
spellingShingle |
BL lacertae objects: individual: RGB 2243 + 203 Galaxies: distances Redshifts New GTC spectroscopic data and a statistical study to better constrain the redshift of the BL Lac RGB J2243 + 203 |
topic_facet |
BL lacertae objects: individual: RGB 2243 + 203 Galaxies: distances Redshifts |
description |
We present new spectroscopic data of the BL Lac RGB 2243 + 203, and its surroundings, obtained with the OSIRIS Multi Object Spectrograph (MOS) mounted in the Gran Telescopio Canarias (GTC). The spectra of neither the BL Lac nor its host galaxy show any spectral feature, thus hindering direct determination of its redshift. The spectroscopic redshift distribution of objects in the MOS field of view shows four galaxies with redshift between 0.5258 and 0.5288. We make use of a statistical analysis to test the possibility that the targeted BL Lac may be a member of that group. By using the spectroscopic redshifts obtained with our GTC observations, we found that this probability is between 86 and 93 per cent. © 2018 The Author(s). |
title |
New GTC spectroscopic data and a statistical study to better constrain the redshift of the BL Lac RGB J2243 + 203 |
title_short |
New GTC spectroscopic data and a statistical study to better constrain the redshift of the BL Lac RGB J2243 + 203 |
title_full |
New GTC spectroscopic data and a statistical study to better constrain the redshift of the BL Lac RGB J2243 + 203 |
title_fullStr |
New GTC spectroscopic data and a statistical study to better constrain the redshift of the BL Lac RGB J2243 + 203 |
title_full_unstemmed |
New GTC spectroscopic data and a statistical study to better constrain the redshift of the BL Lac RGB J2243 + 203 |
title_sort |
new gtc spectroscopic data and a statistical study to better constrain the redshift of the bl lac rgb j2243 + 203 |
publishDate |
2019 |
url |
https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00358711_v482_n4_p5422_RosaGonzalez http://hdl.handle.net/20.500.12110/paper_00358711_v482_n4_p5422_RosaGonzalez |
_version_ |
1768544030801526784 |