Observations of the planetary nebula SMP LMC 058 with the JWST MIRI medium resolution spectrometer

O. C. Jones; J. Álvarez-Márquez; G. C. Sloan; P. J. Kavanagh; I. Argyriou; D. R. Law; A. Labiano; P. Patapis; Michael Mueller; Kirsten L. Larson; Stacey N. Bright; P. D. Klaassen; O. D. Fox; Danny Gasman; V. C. Geers; Adrian M. Glauser; Pierre Guillard; Omnarayani Nayak; A. Noriega-Crespo; Michael E. Ressler; B. Sargent; T. Temim; B. Vandenbussche; Macarena García Marín

doi:10.1093/mnras/stad1609

Observations of the planetary nebula SMP LMC 058 with the JWST MIRI medium resolution spectrometer

O. C. Jones
, J. Álvarez-Márquez
, G. C. Sloan
, P. J. Kavanagh
, I. Argyriou
, D. R. Law
, A. Labiano
, P. Patapis
, Michael Mueller
, Kirsten L. Larson
, Stacey N. Bright
, P. D. Klaassen
, O. D. Fox
, Danny Gasman
, V. C. Geers
, Adrian M. Glauser
, Pierre Guillard
, Omnarayani Nayak
, A. Noriega-Crespo
, Michael E. Ressler

B. Sargent, T. Temim, B. Vandenbussche, Macarena García Marín

Astrophysical Sciences

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

47 Scopus citations

Abstract

During the commissioning of JWST, the medium-resolution spectrometer (MRS) on the mid-infrared instrument (MIRI) observed the planetary nebula SMP LMC 058 in the Large Magellanic Cloud. The MRS was designed to provide medium resolution (R = λ/Δλ) 3D spectroscopy in the whole MIRI range. SMP LMC 058 is the only source observed in JWST commissioning that is both spatially and spectrally unresolved by the MRS and is a good test of JWST's capabilities. The new MRS spectra reveal a wealth of emission lines not previously detected in this planetary nebula. From these lines, the spectral resolving power (λ/Δλ) of the MRS is confirmed to be in the range R = 4000-1500, depending on the MRS spectral sub-band. In addition, the spectra confirm that the carbon-rich dust emission is from complex hydrocarbons and SiC grains and that there is little to no time evolution of the SiC dust and emission line strengths over a 17-yr epoch. These commissioning data reveal the great potential of the MIRI MRS for the study of circumstellar and interstellar material.

Original language	English (US)
Pages (from-to)	2519-2529
Number of pages	11
Journal	Monthly Notices of the Royal Astronomical Society
Volume	523
Issue number	2
DOIs	https://doi.org/10.1093/mnras/stad1609
State	Published - Aug 1 2023

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

Keywords

infrared: general
instrumentation: spectrographs
planetary nebulae: individual: SMP LMC 058

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10.1093/mnras/stad1609

Cite this

Jones, O. C., Álvarez-Márquez, J., Sloan, G. C., Kavanagh, P. J., Argyriou, I., Law, D. R., Labiano, A., Patapis, P., Mueller, M., Larson, K. L., Bright, S. N., Klaassen, P. D., Fox, O. D., Gasman, D., Geers, V. C., Glauser, A. M., Guillard, P., Nayak, O., Noriega-Crespo, A., ... García Marín, M. (2023). Observations of the planetary nebula SMP LMC 058 with the JWST MIRI medium resolution spectrometer. Monthly Notices of the Royal Astronomical Society, 523(2), 2519-2529. https://doi.org/10.1093/mnras/stad1609

@article{340ae3d1aa12401eb7297b14410f25ce,

title = "Observations of the planetary nebula SMP LMC 058 with the JWST MIRI medium resolution spectrometer",

abstract = "During the commissioning of JWST, the medium-resolution spectrometer (MRS) on the mid-infrared instrument (MIRI) observed the planetary nebula SMP LMC 058 in the Large Magellanic Cloud. The MRS was designed to provide medium resolution (R = λ/Δλ) 3D spectroscopy in the whole MIRI range. SMP LMC 058 is the only source observed in JWST commissioning that is both spatially and spectrally unresolved by the MRS and is a good test of JWST's capabilities. The new MRS spectra reveal a wealth of emission lines not previously detected in this planetary nebula. From these lines, the spectral resolving power (λ/Δλ) of the MRS is confirmed to be in the range R = 4000-1500, depending on the MRS spectral sub-band. In addition, the spectra confirm that the carbon-rich dust emission is from complex hydrocarbons and SiC grains and that there is little to no time evolution of the SiC dust and emission line strengths over a 17-yr epoch. These commissioning data reveal the great potential of the MIRI MRS for the study of circumstellar and interstellar material.",

keywords = "infrared: general, instrumentation: spectrographs, planetary nebulae: individual: SMP LMC 058",

author = "Jones, \{O. C.\} and J. {\'A}lvarez-M{\'a}rquez and Sloan, \{G. C.\} and Kavanagh, \{P. J.\} and I. Argyriou and Law, \{D. R.\} and A. Labiano and P. Patapis and Michael Mueller and Larson, \{Kirsten L.\} and Bright, \{Stacey N.\} and Klaassen, \{P. D.\} and Fox, \{O. D.\} and Danny Gasman and Geers, \{V. C.\} and Glauser, \{Adrian M.\} and Pierre Guillard and Omnarayani Nayak and A. Noriega-Crespo and Ressler, \{Michael E.\} and B. Sargent and T. Temim and B. Vandenbussche and \{Garc{\'i}a Mar{\'i}n\}, Macarena",

note = "Publisher Copyright: {\textcopyright} 2023 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society.",

year = "2023",

month = aug,

day = "1",

doi = "10.1093/mnras/stad1609",

language = "English (US)",

volume = "523",

pages = "2519--2529",

journal = "Monthly Notices of the Royal Astronomical Society",

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Jones, OC, Álvarez-Márquez, J, Sloan, GC, Kavanagh, PJ, Argyriou, I, Law, DR, Labiano, A, Patapis, P, Mueller, M, Larson, KL, Bright, SN, Klaassen, PD, Fox, OD, Gasman, D, Geers, VC, Glauser, AM, Guillard, P, Nayak, O, Noriega-Crespo, A, Ressler, ME, Sargent, B, Temim, T, Vandenbussche, B & García Marín, M 2023, 'Observations of the planetary nebula SMP LMC 058 with the JWST MIRI medium resolution spectrometer', Monthly Notices of the Royal Astronomical Society, vol. 523, no. 2, pp. 2519-2529. https://doi.org/10.1093/mnras/stad1609

TY - JOUR

T1 - Observations of the planetary nebula SMP LMC 058 with the JWST MIRI medium resolution spectrometer

AU - Jones, O. C.

AU - Álvarez-Márquez, J.

AU - Sloan, G. C.

AU - Kavanagh, P. J.

AU - Argyriou, I.

AU - Law, D. R.

AU - Labiano, A.

AU - Patapis, P.

AU - Mueller, Michael

AU - Larson, Kirsten L.

AU - Bright, Stacey N.

AU - Klaassen, P. D.

AU - Fox, O. D.

AU - Gasman, Danny

AU - Geers, V. C.

AU - Glauser, Adrian M.

AU - Guillard, Pierre

AU - Nayak, Omnarayani

AU - Noriega-Crespo, A.

AU - Ressler, Michael E.

AU - Sargent, B.

AU - Temim, T.

AU - Vandenbussche, B.

AU - García Marín, Macarena

PY - 2023/8/1

Y1 - 2023/8/1

N2 - During the commissioning of JWST, the medium-resolution spectrometer (MRS) on the mid-infrared instrument (MIRI) observed the planetary nebula SMP LMC 058 in the Large Magellanic Cloud. The MRS was designed to provide medium resolution (R = λ/Δλ) 3D spectroscopy in the whole MIRI range. SMP LMC 058 is the only source observed in JWST commissioning that is both spatially and spectrally unresolved by the MRS and is a good test of JWST's capabilities. The new MRS spectra reveal a wealth of emission lines not previously detected in this planetary nebula. From these lines, the spectral resolving power (λ/Δλ) of the MRS is confirmed to be in the range R = 4000-1500, depending on the MRS spectral sub-band. In addition, the spectra confirm that the carbon-rich dust emission is from complex hydrocarbons and SiC grains and that there is little to no time evolution of the SiC dust and emission line strengths over a 17-yr epoch. These commissioning data reveal the great potential of the MIRI MRS for the study of circumstellar and interstellar material.

AB - During the commissioning of JWST, the medium-resolution spectrometer (MRS) on the mid-infrared instrument (MIRI) observed the planetary nebula SMP LMC 058 in the Large Magellanic Cloud. The MRS was designed to provide medium resolution (R = λ/Δλ) 3D spectroscopy in the whole MIRI range. SMP LMC 058 is the only source observed in JWST commissioning that is both spatially and spectrally unresolved by the MRS and is a good test of JWST's capabilities. The new MRS spectra reveal a wealth of emission lines not previously detected in this planetary nebula. From these lines, the spectral resolving power (λ/Δλ) of the MRS is confirmed to be in the range R = 4000-1500, depending on the MRS spectral sub-band. In addition, the spectra confirm that the carbon-rich dust emission is from complex hydrocarbons and SiC grains and that there is little to no time evolution of the SiC dust and emission line strengths over a 17-yr epoch. These commissioning data reveal the great potential of the MIRI MRS for the study of circumstellar and interstellar material.

KW - infrared: general

KW - instrumentation: spectrographs

KW - planetary nebulae: individual: SMP LMC 058

UR - https://www.scopus.com/pages/publications/85162794735

UR - https://www.scopus.com/pages/publications/85162794735#tab=citedBy

U2 - 10.1093/mnras/stad1609

DO - 10.1093/mnras/stad1609

M3 - Article

AN - SCOPUS:85162794735

SN - 0035-8711

VL - 523

SP - 2519

EP - 2529

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

IS - 2

ER -

Observations of the planetary nebula SMP LMC 058 with the JWST MIRI medium resolution spectrometer

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