Optical spectroscopic observations of gamma-ray blazar candidates. VII. Follow-up campaign in the southern hemisphere
- Autores
- Peña-Herazo, H.A.; Marchesini, Ezequiel Joaquín; Álvarez Crespo, N.; Ricci, F.; Massaro, F.; Chavushyan, V.; Landoni, M.; Strader, J.; Chomiuk, L.; Cheung, C.C.; Masetti, N.; Jiménez Bailón, E.; DAbrusco, R.; Paggi, A.; Milisavljevic, D.; La Franca, F.; Smith, H.A.; Tosti, G.
- Año de publicación
- 2017
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- Searching for low energy counterparts of γ-rays sources is one of the major challenges in modern γ-ray astronomy. In the third Fermi source catalog about 30% of detected sources are unidentified/unassociated Gamma-ray Sources (UGSs). We recently started an optical spectroscopic follow up campaign to confirm the blazar-like nature of candidates counterparts of UGSs. Here we report the spectra of 61 targets collected with the Southern Astrophysical Research Telescope (SOAR) between 2014 and the 2017. Our sample includes 33 potential counterparts of UGSs, selected on the basis of WISE colors, and 27 blazar candidates of uncertain type associated with gamma-ray sources of the last release of the Fermi catalog. We confirm the BZB nature of 20 sources lying within the positional uncertainty region of the UGSs. All the observed BCUs show blazar-like spectra, classified as 2 BZQs and 25 BZBs, for which we obtained 6 redshift estimates. Within the BCUs observations we report the redshift estimate for the BZB associated with, 3FGL J1106.4-3643 that is the second most distant BL Lac known to date, at z≥ 1.084.
Fil: Peña-Herazo, H.A.. Università degli Studi di Torino; Italia. Sezione di Torino; Italia. Instituto Nacional de Astrofísica, Óptica y Electrónica; México
Fil: Marchesini, Ezequiel Joaquín. Università degli Studi di Torino; Italia. Sezione di Torino; Italia. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina. Istituto di Astrofisica Spaziale e Fisica Cosmica di Bologna; Italia
Fil: Álvarez Crespo, N.. Università degli Studi di Torino; Italia. Sezione di Torino; Italia
Fil: Ricci, F.. Università Roma Tre; Italia
Fil: Massaro, F.. Università degli Studi di Torino; Italia. Sezione di Torino; Italia
Fil: Chavushyan, V.. Instituto Nacional de Astrofísica, Óptica y Electrónica; México
Fil: Landoni, M.. Osservatorio Astronomico di Brera; Italia
Fil: Strader, J.. Michigan State University; Estados Unidos
Fil: Chomiuk, L.. Michigan State University; Estados Unidos
Fil: Cheung, C.C.. Spece Sciences División. Naval Research Laboratory; Estados Unidos
Fil: Masetti, N.. Universidad Andrés Bello; Chile. Istituto di Astrofisica Spaziale e Fisica Cosmica di Bologna; Italia
Fil: Jiménez Bailón, E.. Universidad Nacional Autónoma de México; México
Fil: DAbrusco, R.. Università degli Studi di Napoli Federico II; Italia
Fil: Paggi, A.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Fil: Milisavljevic, D.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Fil: La Franca, F.. Università Roma Tre; Italia
Fil: Smith, H.A.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Fil: Tosti, G.. Università degli Studi di Perugia; Italia - Materia
-
Galaxies: Active
Galaxies: Bl Lacertae Objects
Quasars: General - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/49985
Ver los metadatos del registro completo
id |
CONICETDig_71a0f6c86806ae0dcf5bfeb522120b21 |
---|---|
oai_identifier_str |
oai:ri.conicet.gov.ar:11336/49985 |
network_acronym_str |
CONICETDig |
repository_id_str |
3498 |
network_name_str |
CONICET Digital (CONICET) |
spelling |
Optical spectroscopic observations of gamma-ray blazar candidates. VII. Follow-up campaign in the southern hemispherePeña-Herazo, H.A.Marchesini, Ezequiel JoaquínÁlvarez Crespo, N.Ricci, F.Massaro, F.Chavushyan, V.Landoni, M.Strader, J.Chomiuk, L.Cheung, C.C.Masetti, N.Jiménez Bailón, E.DAbrusco, R.Paggi, A.Milisavljevic, D.La Franca, F.Smith, H.A.Tosti, G.Galaxies: ActiveGalaxies: Bl Lacertae ObjectsQuasars: Generalhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Searching for low energy counterparts of γ-rays sources is one of the major challenges in modern γ-ray astronomy. In the third Fermi source catalog about 30% of detected sources are unidentified/unassociated Gamma-ray Sources (UGSs). We recently started an optical spectroscopic follow up campaign to confirm the blazar-like nature of candidates counterparts of UGSs. Here we report the spectra of 61 targets collected with the Southern Astrophysical Research Telescope (SOAR) between 2014 and the 2017. Our sample includes 33 potential counterparts of UGSs, selected on the basis of WISE colors, and 27 blazar candidates of uncertain type associated with gamma-ray sources of the last release of the Fermi catalog. We confirm the BZB nature of 20 sources lying within the positional uncertainty region of the UGSs. All the observed BCUs show blazar-like spectra, classified as 2 BZQs and 25 BZBs, for which we obtained 6 redshift estimates. Within the BCUs observations we report the redshift estimate for the BZB associated with, 3FGL J1106.4-3643 that is the second most distant BL Lac known to date, at z≥ 1.084.Fil: Peña-Herazo, H.A.. Università degli Studi di Torino; Italia. Sezione di Torino; Italia. Instituto Nacional de Astrofísica, Óptica y Electrónica; MéxicoFil: Marchesini, Ezequiel Joaquín. Università degli Studi di Torino; Italia. Sezione di Torino; Italia. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina. Istituto di Astrofisica Spaziale e Fisica Cosmica di Bologna; ItaliaFil: Álvarez Crespo, N.. Università degli Studi di Torino; Italia. Sezione di Torino; ItaliaFil: Ricci, F.. Università Roma Tre; ItaliaFil: Massaro, F.. Università degli Studi di Torino; Italia. Sezione di Torino; ItaliaFil: Chavushyan, V.. Instituto Nacional de Astrofísica, Óptica y Electrónica; MéxicoFil: Landoni, M.. Osservatorio Astronomico di Brera; ItaliaFil: Strader, J.. Michigan State University; Estados UnidosFil: Chomiuk, L.. Michigan State University; Estados UnidosFil: Cheung, C.C.. Spece Sciences División. Naval Research Laboratory; Estados UnidosFil: Masetti, N.. Universidad Andrés Bello; Chile. Istituto di Astrofisica Spaziale e Fisica Cosmica di Bologna; ItaliaFil: Jiménez Bailón, E.. Universidad Nacional Autónoma de México; MéxicoFil: DAbrusco, R.. Università degli Studi di Napoli Federico II; ItaliaFil: Paggi, A.. Harvard-Smithsonian Center for Astrophysics; Estados UnidosFil: Milisavljevic, D.. Harvard-Smithsonian Center for Astrophysics; Estados UnidosFil: La Franca, F.. Università Roma Tre; ItaliaFil: Smith, H.A.. Harvard-Smithsonian Center for Astrophysics; Estados UnidosFil: Tosti, G.. Università degli Studi di Perugia; ItaliaSpringer2017-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/49985Peña-Herazo, H.A.; Marchesini, Ezequiel Joaquín; Álvarez Crespo, N.; Ricci, F.; Massaro, F.; et al.; Optical spectroscopic observations of gamma-ray blazar candidates. VII. Follow-up campaign in the southern hemisphere; Springer; Astrophysics And Space Science; 362; 12; 12-20170004-640XCONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1007/s10509-017-3208-7info:eu-repo/semantics/altIdentifier/url/ps://link.springer.com/article/10.1007%2Fs10509-017-3208-7info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T12:08:08Zoai:ri.conicet.gov.ar:11336/49985instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-10-22 12:08:08.403CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Optical spectroscopic observations of gamma-ray blazar candidates. VII. Follow-up campaign in the southern hemisphere |
title |
Optical spectroscopic observations of gamma-ray blazar candidates. VII. Follow-up campaign in the southern hemisphere |
spellingShingle |
Optical spectroscopic observations of gamma-ray blazar candidates. VII. Follow-up campaign in the southern hemisphere Peña-Herazo, H.A. Galaxies: Active Galaxies: Bl Lacertae Objects Quasars: General |
title_short |
Optical spectroscopic observations of gamma-ray blazar candidates. VII. Follow-up campaign in the southern hemisphere |
title_full |
Optical spectroscopic observations of gamma-ray blazar candidates. VII. Follow-up campaign in the southern hemisphere |
title_fullStr |
Optical spectroscopic observations of gamma-ray blazar candidates. VII. Follow-up campaign in the southern hemisphere |
title_full_unstemmed |
Optical spectroscopic observations of gamma-ray blazar candidates. VII. Follow-up campaign in the southern hemisphere |
title_sort |
Optical spectroscopic observations of gamma-ray blazar candidates. VII. Follow-up campaign in the southern hemisphere |
dc.creator.none.fl_str_mv |
Peña-Herazo, H.A. Marchesini, Ezequiel Joaquín Álvarez Crespo, N. Ricci, F. Massaro, F. Chavushyan, V. Landoni, M. Strader, J. Chomiuk, L. Cheung, C.C. Masetti, N. Jiménez Bailón, E. DAbrusco, R. Paggi, A. Milisavljevic, D. La Franca, F. Smith, H.A. Tosti, G. |
author |
Peña-Herazo, H.A. |
author_facet |
Peña-Herazo, H.A. Marchesini, Ezequiel Joaquín Álvarez Crespo, N. Ricci, F. Massaro, F. Chavushyan, V. Landoni, M. Strader, J. Chomiuk, L. Cheung, C.C. Masetti, N. Jiménez Bailón, E. DAbrusco, R. Paggi, A. Milisavljevic, D. La Franca, F. Smith, H.A. Tosti, G. |
author_role |
author |
author2 |
Marchesini, Ezequiel Joaquín Álvarez Crespo, N. Ricci, F. Massaro, F. Chavushyan, V. Landoni, M. Strader, J. Chomiuk, L. Cheung, C.C. Masetti, N. Jiménez Bailón, E. DAbrusco, R. Paggi, A. Milisavljevic, D. La Franca, F. Smith, H.A. Tosti, G. |
author2_role |
author author author author author author author author author author author author author author author author author |
dc.subject.none.fl_str_mv |
Galaxies: Active Galaxies: Bl Lacertae Objects Quasars: General |
topic |
Galaxies: Active Galaxies: Bl Lacertae Objects Quasars: General |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
Searching for low energy counterparts of γ-rays sources is one of the major challenges in modern γ-ray astronomy. In the third Fermi source catalog about 30% of detected sources are unidentified/unassociated Gamma-ray Sources (UGSs). We recently started an optical spectroscopic follow up campaign to confirm the blazar-like nature of candidates counterparts of UGSs. Here we report the spectra of 61 targets collected with the Southern Astrophysical Research Telescope (SOAR) between 2014 and the 2017. Our sample includes 33 potential counterparts of UGSs, selected on the basis of WISE colors, and 27 blazar candidates of uncertain type associated with gamma-ray sources of the last release of the Fermi catalog. We confirm the BZB nature of 20 sources lying within the positional uncertainty region of the UGSs. All the observed BCUs show blazar-like spectra, classified as 2 BZQs and 25 BZBs, for which we obtained 6 redshift estimates. Within the BCUs observations we report the redshift estimate for the BZB associated with, 3FGL J1106.4-3643 that is the second most distant BL Lac known to date, at z≥ 1.084. Fil: Peña-Herazo, H.A.. Università degli Studi di Torino; Italia. Sezione di Torino; Italia. Instituto Nacional de Astrofísica, Óptica y Electrónica; México Fil: Marchesini, Ezequiel Joaquín. Università degli Studi di Torino; Italia. Sezione di Torino; Italia. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina. Istituto di Astrofisica Spaziale e Fisica Cosmica di Bologna; Italia Fil: Álvarez Crespo, N.. Università degli Studi di Torino; Italia. Sezione di Torino; Italia Fil: Ricci, F.. Università Roma Tre; Italia Fil: Massaro, F.. Università degli Studi di Torino; Italia. Sezione di Torino; Italia Fil: Chavushyan, V.. Instituto Nacional de Astrofísica, Óptica y Electrónica; México Fil: Landoni, M.. Osservatorio Astronomico di Brera; Italia Fil: Strader, J.. Michigan State University; Estados Unidos Fil: Chomiuk, L.. Michigan State University; Estados Unidos Fil: Cheung, C.C.. Spece Sciences División. Naval Research Laboratory; Estados Unidos Fil: Masetti, N.. Universidad Andrés Bello; Chile. Istituto di Astrofisica Spaziale e Fisica Cosmica di Bologna; Italia Fil: Jiménez Bailón, E.. Universidad Nacional Autónoma de México; México Fil: DAbrusco, R.. Università degli Studi di Napoli Federico II; Italia Fil: Paggi, A.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos Fil: Milisavljevic, D.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos Fil: La Franca, F.. Università Roma Tre; Italia Fil: Smith, H.A.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos Fil: Tosti, G.. Università degli Studi di Perugia; Italia |
description |
Searching for low energy counterparts of γ-rays sources is one of the major challenges in modern γ-ray astronomy. In the third Fermi source catalog about 30% of detected sources are unidentified/unassociated Gamma-ray Sources (UGSs). We recently started an optical spectroscopic follow up campaign to confirm the blazar-like nature of candidates counterparts of UGSs. Here we report the spectra of 61 targets collected with the Southern Astrophysical Research Telescope (SOAR) between 2014 and the 2017. Our sample includes 33 potential counterparts of UGSs, selected on the basis of WISE colors, and 27 blazar candidates of uncertain type associated with gamma-ray sources of the last release of the Fermi catalog. We confirm the BZB nature of 20 sources lying within the positional uncertainty region of the UGSs. All the observed BCUs show blazar-like spectra, classified as 2 BZQs and 25 BZBs, for which we obtained 6 redshift estimates. Within the BCUs observations we report the redshift estimate for the BZB associated with, 3FGL J1106.4-3643 that is the second most distant BL Lac known to date, at z≥ 1.084. |
publishDate |
2017 |
dc.date.none.fl_str_mv |
2017-12 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
format |
article |
status_str |
publishedVersion |
dc.identifier.none.fl_str_mv |
http://hdl.handle.net/11336/49985 Peña-Herazo, H.A.; Marchesini, Ezequiel Joaquín; Álvarez Crespo, N.; Ricci, F.; Massaro, F.; et al.; Optical spectroscopic observations of gamma-ray blazar candidates. VII. Follow-up campaign in the southern hemisphere; Springer; Astrophysics And Space Science; 362; 12; 12-2017 0004-640X CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/49985 |
identifier_str_mv |
Peña-Herazo, H.A.; Marchesini, Ezequiel Joaquín; Álvarez Crespo, N.; Ricci, F.; Massaro, F.; et al.; Optical spectroscopic observations of gamma-ray blazar candidates. VII. Follow-up campaign in the southern hemisphere; Springer; Astrophysics And Space Science; 362; 12; 12-2017 0004-640X CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/doi/10.1007/s10509-017-3208-7 info:eu-repo/semantics/altIdentifier/url/ps://link.springer.com/article/10.1007%2Fs10509-017-3208-7 |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
dc.format.none.fl_str_mv |
application/pdf application/pdf |
dc.publisher.none.fl_str_mv |
Springer |
publisher.none.fl_str_mv |
Springer |
dc.source.none.fl_str_mv |
reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
reponame_str |
CONICET Digital (CONICET) |
collection |
CONICET Digital (CONICET) |
instname_str |
Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.name.fl_str_mv |
CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.mail.fl_str_mv |
dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
_version_ |
1846782450164826112 |
score |
12.982451 |