Type II supernovae as distance indicators at near-IR wavelengths

Autores
Rodríguez, Ósmar; Pignata, G.; Hamuy, M.; Clocchiatti, Ariel Martin; Phillips, M. M.; Krisciunas, K.; Morrell, Nidia Irene; Folatelli, Gaston; Roth, M.; Castellón, S.; Jang, I. S.; Apostolovski, Y.; López, P.; Marchi, S; Ramírez, R.; Sánchez, P.
Año de publicación
2018
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Motivated by the advantages of observing at near-IR wavelengths, we investigate Type II supernovae (SNe II) as distance indicators at those wavelengths through the Photospheric Magnitude Method (PMM). For the analysis, we use BVIJH photometry and optical spectroscopy of 24 SNe II during the photospheric phase. To correct photometry for extinction and redshift effects, we compute total-to-selective broad-band extinction ratios and K-corrections up to z = 0.032. To estimate host galaxy colour excesses, we use the colour-colour curve method with the V-I versus B-V as colour combination. We calibrate the PMM using four SNe II in galaxies having Tip of the Red Giant Branch distances. Among our 24 SNe II, nine are at cz > 2000 km s -1, which we use to construct Hubble diagrams (HDs). To further explore the PMM distance precision, we include into HDs the four SNe used for calibration and other two in galaxies with Cepheid and SN Ia distances. With a set of 15 SNe II we obtain an HD rms of 0.13 mag for the J-band, which compares to the rms of 0.15-0.26 mag for optical bands. This reflects the benefits of measuring PMM distances with near-IR instead of optical photometry. With the evidence we have, we can set the PMM distance precision with J-band below 10 per cent with a confidence level of 99 per cent.
Fil: Rodríguez, Ósmar. Instituto Milenio de Astrofísica; Chile. Universidad Andrés Bello; Chile
Fil: Pignata, G.. Instituto Milenio de Astrofísica; Chile. Universidad Andrés Bello; Chile
Fil: Hamuy, M.. Universidad de Chile; Chile. Instituto Milenio de Astrofísica; Chile
Fil: Clocchiatti, Ariel Martin. Instituto Milenio de Astrofísica; Chile. Pontificia Universidad Católica de Chile; Chile
Fil: Phillips, M. M.. Carnegie Observatories; Chile
Fil: Krisciunas, K.. Texas A&M University; Estados Unidos
Fil: Morrell, Nidia Irene. Carnegie Observatories; Chile. 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
Fil: Folatelli, Gaston. 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. The University of Tokyo; Japón
Fil: Roth, M.. Carnegie Observatories; Chile. GMTO Corporation; Chile
Fil: Castellón, S.. Carnegie Observatories; Chile
Fil: Jang, I. S.. Leibniz-Institut für Astrophysik Potsdam; Alemania
Fil: Apostolovski, Y.. Instituto Milenio de Astrofísica; Chile. Carnegie Observatories; Chile
Fil: López, P.. Universidad de Chile; Chile
Fil: Marchi, S. Universidad de Chile; Chile
Fil: Ramírez, R.. Universidad de Chile; Chile
Fil: Sánchez, P.. Universidad de Chile; Chile. European Southern Observatory Chile; Chile
Materia
DISTANCE SCALE
GALAXIES: DISTANCES AND REDSHIFTS
SUPERNOVAE: GENERAL
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/125372
Acceder
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network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling Type II supernovae as distance indicators at near-IR wavelengthsRodríguez, ÓsmarPignata, G.Hamuy, M.Clocchiatti, Ariel MartinPhillips, M. M.Krisciunas, K.Morrell, Nidia IreneFolatelli, GastonRoth, M.Castellón, S.Jang, I. S.Apostolovski, Y.López, P.Marchi, SRamírez, R.Sánchez, P.DISTANCE SCALEGALAXIES: DISTANCES AND REDSHIFTSSUPERNOVAE: GENERALhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Motivated by the advantages of observing at near-IR wavelengths, we investigate Type II supernovae (SNe II) as distance indicators at those wavelengths through the Photospheric Magnitude Method (PMM). For the analysis, we use BVIJH photometry and optical spectroscopy of 24 SNe II during the photospheric phase. To correct photometry for extinction and redshift effects, we compute total-to-selective broad-band extinction ratios and K-corrections up to z = 0.032. To estimate host galaxy colour excesses, we use the colour-colour curve method with the V-I versus B-V as colour combination. We calibrate the PMM using four SNe II in galaxies having Tip of the Red Giant Branch distances. Among our 24 SNe II, nine are at cz > 2000 km s -1, which we use to construct Hubble diagrams (HDs). To further explore the PMM distance precision, we include into HDs the four SNe used for calibration and other two in galaxies with Cepheid and SN Ia distances. With a set of 15 SNe II we obtain an HD rms of 0.13 mag for the J-band, which compares to the rms of 0.15-0.26 mag for optical bands. This reflects the benefits of measuring PMM distances with near-IR instead of optical photometry. With the evidence we have, we can set the PMM distance precision with J-band below 10 per cent with a confidence level of 99 per cent.Fil: Rodríguez, Ósmar. Instituto Milenio de Astrofísica; Chile. Universidad Andrés Bello; ChileFil: Pignata, G.. Instituto Milenio de Astrofísica; Chile. Universidad Andrés Bello; ChileFil: Hamuy, M.. Universidad de Chile; Chile. Instituto Milenio de Astrofísica; ChileFil: Clocchiatti, Ariel Martin. Instituto Milenio de Astrofísica; Chile. Pontificia Universidad Católica de Chile; ChileFil: Phillips, M. M.. Carnegie Observatories; ChileFil: Krisciunas, K.. Texas A&M University; Estados UnidosFil: Morrell, Nidia Irene. Carnegie Observatories; Chile. 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; ArgentinaFil: Folatelli, Gaston. 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. The University of Tokyo; JapónFil: Roth, M.. Carnegie Observatories; Chile. GMTO Corporation; ChileFil: Castellón, S.. Carnegie Observatories; ChileFil: Jang, I. S.. Leibniz-Institut für Astrophysik Potsdam; AlemaniaFil: Apostolovski, Y.. Instituto Milenio de Astrofísica; Chile. Carnegie Observatories; ChileFil: López, P.. Universidad de Chile; ChileFil: Marchi, S. Universidad de Chile; ChileFil: Ramírez, R.. Universidad de Chile; ChileFil: Sánchez, P.. Universidad de Chile; Chile. European Southern Observatory Chile; ChileWiley Blackwell Publishing, Inc2018-12-17info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/125372Rodríguez, Ósmar; Pignata, G.; Hamuy, M.; Clocchiatti, Ariel Martin; Phillips, M. M.; et al.; Type II supernovae as distance indicators at near-IR wavelengths; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 483; 4; 17-12-2018; 5459-54790035-8711CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article/483/4/5459/5251835info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/sty3396info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-10T13:17:58Zoai:ri.conicet.gov.ar:11336/125372instacron: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:34982025-09-10 13:17:59.25CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Type II supernovae as distance indicators at near-IR wavelengths
title Type II supernovae as distance indicators at near-IR wavelengths
spellingShingle Type II supernovae as distance indicators at near-IR wavelengths
Rodríguez, Ósmar
DISTANCE SCALE
GALAXIES: DISTANCES AND REDSHIFTS
SUPERNOVAE: GENERAL
title_short Type II supernovae as distance indicators at near-IR wavelengths
title_full Type II supernovae as distance indicators at near-IR wavelengths
title_fullStr Type II supernovae as distance indicators at near-IR wavelengths
title_full_unstemmed Type II supernovae as distance indicators at near-IR wavelengths
title_sort Type II supernovae as distance indicators at near-IR wavelengths
dc.creator.none.fl_str_mv Rodríguez, Ósmar
Pignata, G.
Hamuy, M.
Clocchiatti, Ariel Martin
Phillips, M. M.
Krisciunas, K.
Morrell, Nidia Irene
Folatelli, Gaston
Roth, M.
Castellón, S.
Jang, I. S.
Apostolovski, Y.
López, P.
Marchi, S
Ramírez, R.
Sánchez, P.
author Rodríguez, Ósmar
author_facet Rodríguez, Ósmar
Pignata, G.
Hamuy, M.
Clocchiatti, Ariel Martin
Phillips, M. M.
Krisciunas, K.
Morrell, Nidia Irene
Folatelli, Gaston
Roth, M.
Castellón, S.
Jang, I. S.
Apostolovski, Y.
López, P.
Marchi, S
Ramírez, R.
Sánchez, P.
author_role author
author2 Pignata, G.
Hamuy, M.
Clocchiatti, Ariel Martin
Phillips, M. M.
Krisciunas, K.
Morrell, Nidia Irene
Folatelli, Gaston
Roth, M.
Castellón, S.
Jang, I. S.
Apostolovski, Y.
López, P.
Marchi, S
Ramírez, R.
Sánchez, P.
author2_role author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv DISTANCE SCALE
GALAXIES: DISTANCES AND REDSHIFTS
SUPERNOVAE: GENERAL
topic DISTANCE SCALE
GALAXIES: DISTANCES AND REDSHIFTS
SUPERNOVAE: 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 Motivated by the advantages of observing at near-IR wavelengths, we investigate Type II supernovae (SNe II) as distance indicators at those wavelengths through the Photospheric Magnitude Method (PMM). For the analysis, we use BVIJH photometry and optical spectroscopy of 24 SNe II during the photospheric phase. To correct photometry for extinction and redshift effects, we compute total-to-selective broad-band extinction ratios and K-corrections up to z = 0.032. To estimate host galaxy colour excesses, we use the colour-colour curve method with the V-I versus B-V as colour combination. We calibrate the PMM using four SNe II in galaxies having Tip of the Red Giant Branch distances. Among our 24 SNe II, nine are at cz > 2000 km s -1, which we use to construct Hubble diagrams (HDs). To further explore the PMM distance precision, we include into HDs the four SNe used for calibration and other two in galaxies with Cepheid and SN Ia distances. With a set of 15 SNe II we obtain an HD rms of 0.13 mag for the J-band, which compares to the rms of 0.15-0.26 mag for optical bands. This reflects the benefits of measuring PMM distances with near-IR instead of optical photometry. With the evidence we have, we can set the PMM distance precision with J-band below 10 per cent with a confidence level of 99 per cent.
Fil: Rodríguez, Ósmar. Instituto Milenio de Astrofísica; Chile. Universidad Andrés Bello; Chile
Fil: Pignata, G.. Instituto Milenio de Astrofísica; Chile. Universidad Andrés Bello; Chile
Fil: Hamuy, M.. Universidad de Chile; Chile. Instituto Milenio de Astrofísica; Chile
Fil: Clocchiatti, Ariel Martin. Instituto Milenio de Astrofísica; Chile. Pontificia Universidad Católica de Chile; Chile
Fil: Phillips, M. M.. Carnegie Observatories; Chile
Fil: Krisciunas, K.. Texas A&M University; Estados Unidos
Fil: Morrell, Nidia Irene. Carnegie Observatories; Chile. 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
Fil: Folatelli, Gaston. 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. The University of Tokyo; Japón
Fil: Roth, M.. Carnegie Observatories; Chile. GMTO Corporation; Chile
Fil: Castellón, S.. Carnegie Observatories; Chile
Fil: Jang, I. S.. Leibniz-Institut für Astrophysik Potsdam; Alemania
Fil: Apostolovski, Y.. Instituto Milenio de Astrofísica; Chile. Carnegie Observatories; Chile
Fil: López, P.. Universidad de Chile; Chile
Fil: Marchi, S. Universidad de Chile; Chile
Fil: Ramírez, R.. Universidad de Chile; Chile
Fil: Sánchez, P.. Universidad de Chile; Chile. European Southern Observatory Chile; Chile
description Motivated by the advantages of observing at near-IR wavelengths, we investigate Type II supernovae (SNe II) as distance indicators at those wavelengths through the Photospheric Magnitude Method (PMM). For the analysis, we use BVIJH photometry and optical spectroscopy of 24 SNe II during the photospheric phase. To correct photometry for extinction and redshift effects, we compute total-to-selective broad-band extinction ratios and K-corrections up to z = 0.032. To estimate host galaxy colour excesses, we use the colour-colour curve method with the V-I versus B-V as colour combination. We calibrate the PMM using four SNe II in galaxies having Tip of the Red Giant Branch distances. Among our 24 SNe II, nine are at cz > 2000 km s -1, which we use to construct Hubble diagrams (HDs). To further explore the PMM distance precision, we include into HDs the four SNe used for calibration and other two in galaxies with Cepheid and SN Ia distances. With a set of 15 SNe II we obtain an HD rms of 0.13 mag for the J-band, which compares to the rms of 0.15-0.26 mag for optical bands. This reflects the benefits of measuring PMM distances with near-IR instead of optical photometry. With the evidence we have, we can set the PMM distance precision with J-band below 10 per cent with a confidence level of 99 per cent.
publishDate 2018
dc.date.none.fl_str_mv 2018-12-17
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/11336/125372
Rodríguez, Ósmar; Pignata, G.; Hamuy, M.; Clocchiatti, Ariel Martin; Phillips, M. M.; et al.; Type II supernovae as distance indicators at near-IR wavelengths; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 483; 4; 17-12-2018; 5459-5479
0035-8711
CONICET Digital
CONICET
url http://hdl.handle.net/11336/125372
identifier_str_mv Rodríguez, Ósmar; Pignata, G.; Hamuy, M.; Clocchiatti, Ariel Martin; Phillips, M. M.; et al.; Type II supernovae as distance indicators at near-IR wavelengths; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 483; 4; 17-12-2018; 5459-5479
0035-8711
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article/483/4/5459/5251835
info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/sty3396
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 Wiley Blackwell Publishing, Inc
publisher.none.fl_str_mv Wiley Blackwell Publishing, Inc
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
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score 12.993085

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