The Early Detection and Follow-up of the Highly Obscured Type II Supernova 2016ija/DLT16am

L. Tartaglia; D. J. Sand; S. Valenti; S. Wyatt; J. P. Anderson; I. Arcavi; C. Ashall; M. T. Botticella; R. Cartier; T. W. Chen; A. Cikota; D. Coulter; M. Della Valle; R. J. Foley; A. Gal-Yam; L. Galbany; C. Gall; J. B. Haislip; J. Harmanen; G. Hosseinzadeh; D. A. Howell; E. Y. Hsiao; C. Inserra; S. W. Jha; E. Kankare; C. D. Kilpatrick; V. V. Kouprianov; H. Kuncarayakti; T. J. Maccarone; K. Maguire; S. Mattila; P. A. Mazzali; C. McCully; A. Melandri; N. Morrell; M. M. Phillips; G. Pignata; A. L. Piro; S. Prentice; D. E. Reichart; C. Rojas-Bravo; S. J. Smartt; K. W. Smith; J. Sollerman; M. D. Stritzinger; M. Sullivan; F. Taddia; D. R. Young; D. J. Sands

doi:10.3847/1538-4357/aaa014

The Early Detection and Follow-up of the Highly Obscured Type II Supernova 2016ija/DLT16am

L. Tartaglia, D. J. Sand, S. Valenti, S. Wyatt, J. P. Anderson, I. Arcavi, C. Ashall, M. T. Botticella, R. Cartier, T. W. Chen, A. Cikota, D. Coulter, M. Della Valle, R. J. Foley, A. Gal-Yam, L. Galbany, C. Gall, J. B. Haislip, J. Harmanen, G. HosseinzadehD. A. Howell, E. Y. Hsiao, C. Inserra, S. W. Jha, E. Kankare, C. D. Kilpatrick, V. V. Kouprianov, H. Kuncarayakti, T. J. Maccarone, K. Maguire, S. Mattila, P. A. Mazzali, C. McCully, A. Melandri, N. Morrell, M. M. Phillips, G. Pignata, A. L. Piro, S. Prentice, D. E. Reichart, C. Rojas-Bravo, S. J. Smartt, K. W. Smith, J. Sollerman, M. D. Stritzinger, M. Sullivan, F. Taddia, D. R. Young, D. J. Sands

Department of Particle Physics and Astrophysics

Weizmann Institute of Science

Research output: Contribution to journal › Article › peer-review

Abstract

We present our analysis of the Type II supernova DLT16am (SN 2016ija). The object was discovered during theongoing D < 40 Mpc (DLT40) one-day cadence supernova search at r ∼ 20.1 mag in the edge-on nearby(D = 20.0 ± 4.0 Mpc) galaxy NGC 1532. The subsequent prompt and high-cadenced spectroscopic andphotometric follow-up revealed a highly extinguished transient, with E(B - V) = 1.95 ±0.15 mag, consistentwith a standard extinction law with RV=3.1 and a bright (MV = -18.48 ±0.77 mag) absolute peak magnitude. Acomparison of the photometric features with those of large samples of SNe II reveals a fast rise for the derivedluminosity and a relatively short plateau phase, with a slope of S50V = 0.84 ±0.04 mag 50 days, consistent withthe photometric properties typical of those of fast-declining SNe II. Despite the large uncertainties on the distance andthe extinction in the direction of DLT16am, the measured photospheric expansion velocity and the derived absoluteV-band magnitude at ~50 days after the explosion match the existing luminosity-velocity relation for SNe II.

Original language	English
Article number	62
Number of pages	16
Journal	Astrophysical Journal
Volume	853
Issue number	1
DOIs	https://doi.org/10.3847/1538-4357/aaa014
State	Published - 20 Jan 2018

Keywords

galaxies: individual (NGC 1532)
supernovae: general
supernovae: individual (SN 2016ija, DLT16am)

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

Access to Document

10.3847/1538-4357/aaa014

Cite this

Tartaglia, L., Sand, D. J., Valenti, S., Wyatt, S., Anderson, J. P., Arcavi, I., Ashall, C., Botticella, M. T., Cartier, R., Chen, T. W., Cikota, A., Coulter, D., Valle, M. D., Foley, R. J., Gal-Yam, A., Galbany, L., Gall, C., Haislip, J. B., Harmanen, J., ... Sands, D. J. (2018). The Early Detection and Follow-up of the Highly Obscured Type II Supernova 2016ija/DLT16am. Astrophysical Journal, 853(1), Article 62. https://doi.org/10.3847/1538-4357/aaa014

@article{fe80bd4172c44b34b063373bc6ace1a6,

title = "The Early Detection and Follow-up of the Highly Obscured Type II Supernova 2016ija/DLT16am",

abstract = "We present our analysis of the Type II supernova DLT16am (SN 2016ija). The object was discovered during theongoing D < 40 Mpc (DLT40) one-day cadence supernova search at r ∼ 20.1 mag in the edge-on nearby(D = 20.0 ± 4.0 Mpc) galaxy NGC 1532. The subsequent prompt and high-cadenced spectroscopic andphotometric follow-up revealed a highly extinguished transient, with E(B - V) = 1.95 ±0.15 mag, consistentwith a standard extinction law with RV=3.1 and a bright (MV = -18.48 ±0.77 mag) absolute peak magnitude. Acomparison of the photometric features with those of large samples of SNe II reveals a fast rise for the derivedluminosity and a relatively short plateau phase, with a slope of S50V = 0.84 ±0.04 mag 50 days, consistent withthe photometric properties typical of those of fast-declining SNe II. Despite the large uncertainties on the distance andthe extinction in the direction of DLT16am, the measured photospheric expansion velocity and the derived absoluteV-band magnitude at \textasciitilde{}50 days after the explosion match the existing luminosity-velocity relation for SNe II.",

keywords = "galaxies: individual (NGC 1532), supernovae: general, supernovae: individual (SN 2016ija, DLT16am)",

author = "L. Tartaglia and Sand, \{D. J.\} and S. Valenti and S. Wyatt and Anderson, \{J. P.\} and I. Arcavi and C. Ashall and Botticella, \{M. T.\} and R. Cartier and Chen, \{T. W.\} and A. Cikota and D. Coulter and Valle, \{M. Della\} and Foley, \{R. J.\} and A. Gal-Yam and L. Galbany and C. Gall and Haislip, \{J. B.\} and J. Harmanen and G. Hosseinzadeh and Howell, \{D. A.\} and Hsiao, \{E. Y.\} and C. Inserra and Jha, \{S. W.\} and E. Kankare and Kilpatrick, \{C. D.\} and Kouprianov, \{V. V.\} and H. Kuncarayakti and Maccarone, \{T. J.\} and K. Maguire and S. Mattila and Mazzali, \{P. A.\} and C. McCully and A. Melandri and N. Morrell and Phillips, \{M. M.\} and G. Pignata and Piro, \{A. L.\} and S. Prentice and Reichart, \{D. E.\} and C. Rojas-Bravo and Smartt, \{S. J.\} and Smith, \{K. W.\} and J. Sollerman and Stritzinger, \{M. D.\} and M. Sullivan and F. Taddia and Young, \{D. R.\} and Sands, \{D. J.\}",

note = "Funding Information: D.A.H., C.M., and G.H. are supported by NSF grant 1313484. Funding Information: Research by D.J.S. and L.T.L. is supported by NSF grants AST-1412504 and AST-1517649. Funding Information: This work is based on observations collected at: the Very Large Telescope operated by the European Organisation for Astronomical Research in the Southern hemisphere, Chile as part of the ESO large programme 198.A-0915; ESOO La Silla Observatory as part of PESSTO (197.D-1075.191.D-0935); the Gemini Observatory, under program GN-2016B-Q-57, which is operated by the Association of Universities for Research in Astronomy, Inc., under a cooperative agreement with the NSF on behalf of the Gemini partnership: the National Science Foundation (United States), the National Research Council (Canada), CONICYT (Chile), Ministerio de Ciencia, Tecnolo-g{\'i}a e Innovaci{\'o}n Productiva (Argentina), and Minist{\'e}rio da Ci{\^e}ncia, Tecnologia e Inova{\c c}{\~a}o (Brazil). Funding Information: Part of the funding for GROND (both hardware as well as personnel) was generously granted from the Leibniz-Prize to Prof. G. Hasinger (DFG grant HA 1850/28-1). Funding Information: L.G. was supported in part by the US National Science Foundation under grant AST-1311862. Funding Information: M.D.S. acknowledges support by a research grant (13261) from the VILLUM FONDEN and for financial support of NUTS by the Instrument Center for Danish Astrophysics (IDA). Funding Information: C.G. acknowledges support from the Carlsberg Foundation. Funding Information: R.C. and M.S. acknowledge support from STFC grant ST/ L000679/1 and EU/FP7-ERC grant No. 615929. T.W.C. acknowledges the support through the Sofia Kovalevskaja Award to P. Schady from the Alexander von Humboldt Foundation of Germany. Funding Information: The UCSC group is supported in part by NSF grant AST-1518052, the Gordon \& Betty Moore Foundation, and from fellowships from the Alfred P. Sloan Foundation and the David and Lucile Packard Foundation to R.J.F. Funding Information: J.H. acknowledges financial support from the Finnish Cultural Foundation and the Vilho, Yrj{\"o}, and Kalle V{\"a}is{\"a}l{\"a} Foundation of the Finnish Academy of Science and Letters. Funding Information: A.G.-Y. is supported by the EU via ERC grant No. 725161, the Quantum Universe I-Core program, the ISF, the BSF Transformative program and by a Kimmel award. Funding Information: M.M.P., N.M., and E.Y.H. acknowledge the support provided by the National Science Foundation under grant No. AST-1008343, AST-1613472, and AST-1613426. Funding Information: Support for G.P. is provided by the Ministry of Economy, Development, and Tourism{\textquoteright}s Millennium Science Initiative through grant IC120009, awarded to The Millennium Institute of Astrophysics, MAS.",

year = "2018",

month = jan,

day = "20",

doi = "10.3847/1538-4357/aaa014",

language = "الإنجليزيّة",

volume = "853",

journal = "Astrophysical Journal",

issn = "0004-637X",

publisher = "IOP Publishing Ltd.",

number = "1",

}

Tartaglia, L, Sand, DJ, Valenti, S, Wyatt, S, Anderson, JP, Arcavi, I, Ashall, C, Botticella, MT, Cartier, R, Chen, TW, Cikota, A, Coulter, D, Valle, MD, Foley, RJ, Gal-Yam, A, Galbany, L, Gall, C, Haislip, JB, Harmanen, J, Hosseinzadeh, G, Howell, DA, Hsiao, EY, Inserra, C, Jha, SW, Kankare, E, Kilpatrick, CD, Kouprianov, VV, Kuncarayakti, H, Maccarone, TJ, Maguire, K, Mattila, S, Mazzali, PA, McCully, C, Melandri, A, Morrell, N, Phillips, MM, Pignata, G, Piro, AL, Prentice, S, Reichart, DE, Rojas-Bravo, C, Smartt, SJ, Smith, KW, Sollerman, J, Stritzinger, MD, Sullivan, M, Taddia, F, Young, DR & Sands, DJ 2018, 'The Early Detection and Follow-up of the Highly Obscured Type II Supernova 2016ija/DLT16am', Astrophysical Journal, vol. 853, no. 1, 62. https://doi.org/10.3847/1538-4357/aaa014

TY - JOUR

T1 - The Early Detection and Follow-up of the Highly Obscured Type II Supernova 2016ija/DLT16am

AU - Tartaglia, L.

AU - Sand, D. J.

AU - Valenti, S.

AU - Wyatt, S.

AU - Anderson, J. P.

AU - Arcavi, I.

AU - Ashall, C.

AU - Botticella, M. T.

AU - Cartier, R.

AU - Chen, T. W.

AU - Cikota, A.

AU - Coulter, D.

AU - Valle, M. Della

AU - Foley, R. J.

AU - Gal-Yam, A.

AU - Galbany, L.

AU - Gall, C.

AU - Haislip, J. B.

AU - Harmanen, J.

AU - Hosseinzadeh, G.

AU - Howell, D. A.

AU - Hsiao, E. Y.

AU - Inserra, C.

AU - Jha, S. W.

AU - Kankare, E.

AU - Kilpatrick, C. D.

AU - Kouprianov, V. V.

AU - Kuncarayakti, H.

AU - Maccarone, T. J.

AU - Maguire, K.

AU - Mattila, S.

AU - Mazzali, P. A.

AU - McCully, C.

AU - Melandri, A.

AU - Morrell, N.

AU - Phillips, M. M.

AU - Pignata, G.

AU - Piro, A. L.

AU - Prentice, S.

AU - Reichart, D. E.

AU - Rojas-Bravo, C.

AU - Smartt, S. J.

AU - Smith, K. W.

AU - Sollerman, J.

AU - Stritzinger, M. D.

AU - Sullivan, M.

AU - Taddia, F.

AU - Young, D. R.

AU - Sands, D. J.

N1 - Funding Information: D.A.H., C.M., and G.H. are supported by NSF grant 1313484. Funding Information: Research by D.J.S. and L.T.L. is supported by NSF grants AST-1412504 and AST-1517649. Funding Information: This work is based on observations collected at: the Very Large Telescope operated by the European Organisation for Astronomical Research in the Southern hemisphere, Chile as part of the ESO large programme 198.A-0915; ESOO La Silla Observatory as part of PESSTO (197.D-1075.191.D-0935); the Gemini Observatory, under program GN-2016B-Q-57, which is operated by the Association of Universities for Research in Astronomy, Inc., under a cooperative agreement with the NSF on behalf of the Gemini partnership: the National Science Foundation (United States), the National Research Council (Canada), CONICYT (Chile), Ministerio de Ciencia, Tecnolo-gía e Innovación Productiva (Argentina), and Ministério da Ciência, Tecnologia e Inovação (Brazil). Funding Information: Part of the funding for GROND (both hardware as well as personnel) was generously granted from the Leibniz-Prize to Prof. G. Hasinger (DFG grant HA 1850/28-1). Funding Information: L.G. was supported in part by the US National Science Foundation under grant AST-1311862. Funding Information: M.D.S. acknowledges support by a research grant (13261) from the VILLUM FONDEN and for financial support of NUTS by the Instrument Center for Danish Astrophysics (IDA). Funding Information: C.G. acknowledges support from the Carlsberg Foundation. Funding Information: R.C. and M.S. acknowledge support from STFC grant ST/ L000679/1 and EU/FP7-ERC grant No. 615929. T.W.C. acknowledges the support through the Sofia Kovalevskaja Award to P. Schady from the Alexander von Humboldt Foundation of Germany. Funding Information: The UCSC group is supported in part by NSF grant AST-1518052, the Gordon & Betty Moore Foundation, and from fellowships from the Alfred P. Sloan Foundation and the David and Lucile Packard Foundation to R.J.F. Funding Information: J.H. acknowledges financial support from the Finnish Cultural Foundation and the Vilho, Yrjö, and Kalle Väisälä Foundation of the Finnish Academy of Science and Letters. Funding Information: A.G.-Y. is supported by the EU via ERC grant No. 725161, the Quantum Universe I-Core program, the ISF, the BSF Transformative program and by a Kimmel award. Funding Information: M.M.P., N.M., and E.Y.H. acknowledge the support provided by the National Science Foundation under grant No. AST-1008343, AST-1613472, and AST-1613426. Funding Information: Support for G.P. is provided by the Ministry of Economy, Development, and Tourism’s Millennium Science Initiative through grant IC120009, awarded to The Millennium Institute of Astrophysics, MAS.

PY - 2018/1/20

Y1 - 2018/1/20

N2 - We present our analysis of the Type II supernova DLT16am (SN 2016ija). The object was discovered during theongoing D < 40 Mpc (DLT40) one-day cadence supernova search at r ∼ 20.1 mag in the edge-on nearby(D = 20.0 ± 4.0 Mpc) galaxy NGC 1532. The subsequent prompt and high-cadenced spectroscopic andphotometric follow-up revealed a highly extinguished transient, with E(B - V) = 1.95 ±0.15 mag, consistentwith a standard extinction law with RV=3.1 and a bright (MV = -18.48 ±0.77 mag) absolute peak magnitude. Acomparison of the photometric features with those of large samples of SNe II reveals a fast rise for the derivedluminosity and a relatively short plateau phase, with a slope of S50V = 0.84 ±0.04 mag 50 days, consistent withthe photometric properties typical of those of fast-declining SNe II. Despite the large uncertainties on the distance andthe extinction in the direction of DLT16am, the measured photospheric expansion velocity and the derived absoluteV-band magnitude at ~50 days after the explosion match the existing luminosity-velocity relation for SNe II.

AB - We present our analysis of the Type II supernova DLT16am (SN 2016ija). The object was discovered during theongoing D < 40 Mpc (DLT40) one-day cadence supernova search at r ∼ 20.1 mag in the edge-on nearby(D = 20.0 ± 4.0 Mpc) galaxy NGC 1532. The subsequent prompt and high-cadenced spectroscopic andphotometric follow-up revealed a highly extinguished transient, with E(B - V) = 1.95 ±0.15 mag, consistentwith a standard extinction law with RV=3.1 and a bright (MV = -18.48 ±0.77 mag) absolute peak magnitude. Acomparison of the photometric features with those of large samples of SNe II reveals a fast rise for the derivedluminosity and a relatively short plateau phase, with a slope of S50V = 0.84 ±0.04 mag 50 days, consistent withthe photometric properties typical of those of fast-declining SNe II. Despite the large uncertainties on the distance andthe extinction in the direction of DLT16am, the measured photospheric expansion velocity and the derived absoluteV-band magnitude at ~50 days after the explosion match the existing luminosity-velocity relation for SNe II.

KW - galaxies: individual (NGC 1532)

KW - supernovae: general

KW - supernovae: individual (SN 2016ija, DLT16am)

UR - http://www.scopus.com/inward/record.url?scp=85041124321&partnerID=8YFLogxK

U2 - 10.3847/1538-4357/aaa014

DO - 10.3847/1538-4357/aaa014

M3 - مقالة

SN - 0004-637X

VL - 853

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 1

M1 - 62

ER -

The Early Detection and Follow-up of the Highly Obscured Type II Supernova 2016ija/DLT16am

Abstract

Keywords

All Science Journal Classification (ASJC) codes

Access to Document

Other files and links

Fingerprint

Cite this