A JWST Near- and Mid-infrared Nebular Spectrum of the Type Ia Supernova 2021aefx
暂无分享,去创建一个
W. E. Kerzendorf | K. Maguire | J. Maund | O. Graur | S. Jha | C. McCully | A. Rest | R. Foley | G. Hosseinzadeh | D. Howell | L. Galbany | M. Graham | D. Sand | N. Morrell | L. Strolger | P. Garnavich | Lifan Wang | B. Shappee | N. Suntzeff | E. Hsiao | O. Fox | J. Johansson | C. Ashall | K. Krisciunas | E. Baron | K. Bostroem | M. Stritzinger | J. Hughes | S. Kendrew | T. D. Jaeger | E. Karamehmetoglu | C. Badenes | T. Temim | K. Maeda | C. Telesco | C. Burns | T. Szalai | A. Fisher | M. Tucker | Sahana Kumar | J. M. DerKacy | J. Andrews | M. Shahbandeh | M. Deckers | Jing Lu | J. O’Brien | B. Barna | Y. Camacho-Neves | L. Kwok | J. Pierel | M. Phillips | P. Mazzali | P. Hoeflich | A. Flors | C. Larison | Max J. B. Newman | Tyco Mera Evans | Kyle Medler | M. Phillips | J. Hughes | J. DerKacy | T. M. Evans | K. Medler
[1] P. Ferruit,et al. The in-flight noise performance of the JWST/NIRSpec detector system , 2022, Astronomical Telescopes + Instrumentation.
[2] J. Maund,et al. Spectropolarimetry of the Thermonuclear Supernova SN 2021rhu: High Calcium Polarization 79 Days after Peak Luminosity , 2022, The Astrophysical Journal.
[3] S. Jha,et al. Constraining the Progenitor System of the Type Ia Supernova 2021aefx , 2022, The Astrophysical Journal Letters.
[4] P. Brown,et al. A Speed Bump: SN 2021aefx Shows that Doppler Shift Alone Can Explain Early Excess Blue Flux in Some Type Ia Supernovae , 2022, The Astrophysical Journal Letters.
[5] H. Rix,et al. The Near-Infrared Spectrograph (NIRSpec) on the James Webb Space Telescope. I. Overview of the instrument and its capabilities , 2022, Astronomy & Astrophysics.
[6] C. McCully,et al. Nebular-Phase Spectra of Type Ia Supernovae from the Las Cumbres Observatory Global Supernova Project , 2022, 2201.07864.
[7] C. Kochanek,et al. A Rapid Ionization Change in the Nebular-phase Spectra of the Type Ia SN 2011fe , 2021, The Astrophysical Journal Letters.
[8] F. Timmes,et al. Stable nickel production in Type Ia supernovae: A smoking gun for the progenitor mass? , 2021, Astronomy & Astrophysics.
[9] L. Galbany,et al. Measuring an Off-center Detonation through Infrared Line Profiles: The Peculiar Type Ia Supernova SN 2020qxp/ASASSN-20jq , 2021, The Astrophysical Journal.
[10] G. Rieke,et al. Milky Way Mid-Infrared Spitzer Spectroscopic Extinction Curves: Continuum and Silicate Features , 2021, The Astrophysical Journal.
[11] J. Buchner. UltraNest - a robust, general purpose Bayesian inference engine , 2021, J. Open Source Softw..
[12] Jaime Fern'andez del R'io,et al. Array programming with NumPy , 2020, Nature.
[13] L. Dessart,et al. Understanding nebular spectra of Type Ia supernovae , 2019, Monthly Notices of the Royal Astronomical Society.
[14] K. Gordon,et al. An Analysis of the Shapes of Interstellar Extinction Curves. VII. Milky Way Spectrophotometric Optical-through-ultraviolet Extinction and Its R-dependence , 2019, The Astrophysical Journal.
[15] K. Maguire,et al. A year-long plateau in the late-time near-infrared light curves of type Ia supernovae , 2019, Nature Astronomy.
[16] W. Hillebrandt,et al. Sub-Chandrasekhar progenitors favoured for type Ia supernovae: Evidence from late-time spectroscopy★. , 2019, Monthly Notices of the Royal Astronomical Society.
[17] W. E. Kerzendorf,et al. Limits on stable iron in Type Ia supernovae from near-infrared spectroscopy , 2018, Astronomy & Astrophysics.
[18] M. Stritzinger,et al. Near-infrared Spectral Evolution of the Type Ia Supernova 2014J in the Nebular Phase: Implications for the Progenitor System , 2018, The Astrophysical Journal.
[19] W. E. Kerzendorf,et al. Nebular spectroscopy of SN 2014J: Detection of stable nickel in near-infrared spectra , 2018, Astronomy & Astrophysics.
[20] Adrian M. Price-Whelan,et al. Binary Companions of Evolved Stars in APOGEE DR14: Search Method and Catalog of ∼5000 Companions , 2018, The Astronomical Journal.
[21] K. Maguire,et al. Using late-time optical and near-infrared spectra to constrain Type Ia supernova explosion properties , 2018, 1803.10252.
[22] J. Prieto,et al. The Resolved Stellar Populations in the LEGUS Galaxies1 , 2018, 1801.05467.
[23] M. Phillips,et al. The Early Detection and Follow-up of the Highly Obscured Type II Supernova 2016ija/DLT16am , 2017, 1711.03940.
[24] M. Kasliwal,et al. Spitzer observations of SN 2014J and properties of mid-IR emission in Type Ia Supernovae , 2014, 1411.3332.
[25] Pierre-Olivier Lagage,et al. The mid-infrared instrument for the James Webb Space Telescope: performance and operation of the Low-Resolution Spectrometer , 2016, Astronomical Telescopes + Instrumentation.
[26] J. Parrent,et al. Progressive redshifts in the late-time spectra of Type Ia supernovae , 2016, 1604.01044.
[27] Davis,et al. The diversity of Type II supernova versus the similarity in their progenitors , 2016, 1603.08953.
[28] Bruce Swinyard,et al. The Mid-Infrared Instrument for JWST, II: Design and Build , 2015, 1508.02333.
[29] K. Maguire,et al. Measuring nickel masses in Type Ia supernovae using cobalt emission in nebular phase spectra , 2015, 1507.02501.
[30] Ipmu,et al. Nebular spectra and abundance tomography of the Type Ia supernova SN 2011fe: a normal SN Ia with a stable Fe core , 2015, 1504.04857.
[31] Adam A. Miller,et al. TYPE Ia SUPERNOVAE STRONGLY INTERACTING WITH THEIR CIRCUMSTELLAR MEDIUM , 2013, Proceedings of the International Astronomical Union.
[32] J. Muzerolle,et al. The JWST Calibration Pipeline , 2015 .
[33] J. Amiaux,et al. The Mid-Infrared Instrument for the James Webb Space Telescope, IV: The Low-Resolution Spectrometer , 2015 .
[34] L. Bergeron,et al. The Mid-Infrared Instrument for the James Webb Space Telescope, VII: The MIRI Detectors , 2015 .
[35] W. Hillebrandt,et al. Extensive HST ultraviolet spectra and multiwavelength observations of SN 2014J in M82 indicate reddening and circumstellar scattering by typical dust , 2014, 1405.3677.
[36] ARC Centre of Excellence for All-sky Astrophysics,et al. A search for H i absorption in nearby radio galaxies using HIPASS , 2014, 1402.3530.
[37] C. Evans,et al. The VLT-FLAMES Tarantula Survey. XV. VFTS 822: A candidate Herbig B[e] star at low metallicity , 2014, 1401.3149.
[38] D. Dragomir,et al. Las Cumbres Observatory Global Telescope Network , 2013, 1305.2437.
[39] Stuart A. Sim,et al. Three-dimensional delayed-detonation models with nucleosynthesis for Type Ia supernovae , 2012, 1211.3015.
[40] A. Riess,et al. THE SPECTROSCOPIC DIVERSITY OF TYPE Ia SUPERNOVAE , 2000, The Astronomical Journal.
[41] J. Bernard-Salas,et al. CASSIS: THE CORNELL ATLAS OF SPITZER/INFRARED SPECTROGRAPH SOURCES. II. HIGH-RESOLUTION OBSERVATIONS , 2011, 1108.3507.
[42] Steven M. Crawford,et al. PySALT: the SALT science pipeline , 2010, Astronomical Telescopes + Instrumentation.
[43] W. Hillebrandt,et al. Double-detonation sub-Chandrasekhar supernovae: can minimum helium shell masses detonate the core? , 2010, 1002.2173.
[44] Lifan Wang,et al. Spectropolarimetry of Supernovae , 2008, 0811.1054.
[45] L. Girardi,et al. THE ACS NEARBY GALAXY SURVEY TREASURY , 2007, 0905.3737.
[46] W. Hillebrandt,et al. Double-detonation supernovae of sub-Chandrasekhar mass white dwarfs , 2007, 0710.5486.
[47] J. Rho,et al. Freshly Formed Dust in the Cassiopeia A Supernova Remnant as Revealed by the Spitzer Space Telescope , 2007, 0709.2880.
[48] R. Kotak,et al. Signatures of Delayed Detonation, Asymmetry, and Electron Capture in the Mid-Infrared Spectra of Supernovae 2003hv and 2005df , 2007, astro-ph/0702117.
[49] Bernadette Rodgers,et al. Performance of the Gemini near-infrared spectrograph , 2006, SPIE Astronomical Telescopes + Instrumentation.
[50] Gary Muller,et al. Design of the Gemini near-infrared spectrograph , 2006, SPIE Astronomical Telescopes + Instrumentation.
[51] Michael P. Smith,et al. The prime focus imaging spectrograph for the Southern African Large Telescope: structural and mechanical design and commissioning , 2001, SPIE Astronomical Telescopes + Instrumentation.
[52] Lifan Wang. Dust around Type Ia Supernovae , 2005, astro-ph/0511003.
[53] Walter Seifert,et al. LUCIFER: a Multi-Mode NIR Instrument for the LBT , 2003, SPIE Astronomical Telescopes + Instrumentation.
[54] A. Moorwood,et al. Instrument Design and Performance for Optical/Infrared Ground-based Telescopes, , 2003 .
[55] Koichi Iwamoto,et al. Nucleosynthesis in Chandrasekhar Mass Models for Type Ia Supernovae and Constraints on Progenitor Systems and Burning-Front Propagation , 1999 .
[56] G. Sharpe,et al. Double detonations at the core–envelope boundary in Type Ia supernovae , 1998 .
[57] W. Meikle,et al. Infrared and optical spectroscopy of type Ia supernovae in the nebular phase , 1997, astro-ph/9707119.
[58] J. Wheeler,et al. Maximum Brightness and Postmaximum Decline of Light Curves of Type Supernovae Ia: A Comparison of Theory and Observations , 1996, astro-ph/9609070.
[59] J. Wheeler,et al. Delayed detonation models for normal and subluminous type Ia sueprnovae: Absolute brightness, light curves, and molecule formation , 1995 .
[60] S. Woosley,et al. Sub-Chandrasekhar mass models for Type IA supernovae , 1994 .
[61] J. Wheeler,et al. Explosive nucleosynthesis and type I supernovae , 1984 .