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...

Descripción completa

Guardado en:
Detalles Bibliográficos
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