The JWST Discovery of the Triply Imaged Type Ia “Supernova H0pe” and Observations of the Galaxy Cluster PLCK G165.7+67.0

A Type Ia supernova (SN) at z = 1.78 was discovered in James Webb Space Telescope Near Infrared Camera imaging of the galaxy cluster PLCK G165.7+67.0 (G165; z = 0.35). The SN is situated 1.5–2 kpc from the host-galaxy nucleus and appears in three different locations as a result of gravitational lens...
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Autor*in:	Brenda L. Frye [verfasserIn] Massimo Pascale [verfasserIn] Justin Pierel [verfasserIn] Wenlei Chen [verfasserIn] Nicholas Foo [verfasserIn] Reagen Leimbach [verfasserIn] Nikhil Garuda [verfasserIn] Seth H. Cohen [verfasserIn] Patrick S. Kamieneski [verfasserIn] Rogier A. Windhorst [verfasserIn] Anton M. Koekemoer [verfasserIn] Pat Kelly [verfasserIn] Jake Summers [verfasserIn] Michael Engesser [verfasserIn] Daizhong Liu [verfasserIn] Lukas J. Furtak [verfasserIn] Maria del Carmen Polletta [verfasserIn] Kevin C. Harrington [verfasserIn] S. P. Willner [verfasserIn] Jose M. Diego [verfasserIn] Rolf A. Jansen [verfasserIn] Dan Coe [verfasserIn] Christopher J. Conselice [verfasserIn] Liang Dai [verfasserIn] Hervé Dole [verfasserIn] Jordan C. J. D’Silva [verfasserIn] Simon P. Driver [verfasserIn] Norman A. Grogin [verfasserIn] Madeline A. Marshall [verfasserIn] Ashish K. Meena [verfasserIn] Mario Nonino [verfasserIn] Rafael Ortiz III [verfasserIn] Nor Pirzkal [verfasserIn] Aaron Robotham [verfasserIn] Russell E. Ryan Jr. [verfasserIn] Lou Strolger [verfasserIn] Scott Tompkins [verfasserIn] Christopher N. A. Willmer [verfasserIn] Haojing Yan [verfasserIn] Min S. Yun [verfasserIn] Adi Zitrin [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2024

Schlagwörter:	Strong gravitational lensing Rich galaxy clusters High-redshift galaxy clusters Galaxy cluster counts Galaxy spectroscopy

Übergeordnetes Werk:	In: The Astrophysical Journal - IOP Publishing, 2022, 961(2024), 2, p 171
Übergeordnetes Werk:	volume:961 ; year:2024 ; number:2, p 171

Links:	Link aufrufen Link aufrufen Link aufrufen Journal toc

DOI / URN:	10.3847/1538-4357/ad1034

Katalog-ID:	DOAJ096516925

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520			\|a A Type Ia supernova (SN) at z = 1.78 was discovered in James Webb Space Telescope Near Infrared Camera imaging of the galaxy cluster PLCK G165.7+67.0 (G165; z = 0.35). The SN is situated 1.5–2 kpc from the host-galaxy nucleus and appears in three different locations as a result of gravitational lensing by G165. These data can yield a value for Hubble’s constant using time delays from this multiply imaged SN Ia that we call “SN H0pe.” Over the cluster, we identified 21 image multiplicities, confirmed five of them using the Near-Infrared Spectrograph, and constructed a new lens model that gives a total mass within 600 kpc of (2.6 ± 0.3) × 10 ^14 M _⊙ . The photometry uncovered a galaxy overdensity coincident with the SN host galaxy. NIRSpec confirmed six member galaxies, four of which surround the SN host galaxy with relative velocity ≲900 km s ^−1 and projected physical extent ≲33 kpc. This compact galaxy group is dominated by the SN host galaxy, which has a stellar mass of (5.0 ± 0.1) × 10 ^11 M _⊙ . The group members have specific star formation rates of 2–260 Gyr ^−1 derived from the H α -line fluxes corrected for stellar absorption, dust extinction, and slit losses. Another group centered on a strongly lensed dusty star-forming galaxy is at z = 2.24. The total (unobscured and obscured) SFR of this second galaxy group is estimated to be (≳ 100 M _⊙ yr ^−1 ), which translates to a supernova rate of ∼1 SNe yr ^−1 , suggesting that regular monitoring of this cluster may yield additional SNe.
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700	0		\|a Anton M. Koekemoer \|e verfasserin \|4 aut
700	0		\|a Pat Kelly \|e verfasserin \|4 aut
700	0		\|a Jake Summers \|e verfasserin \|4 aut
700	0		\|a Michael Engesser \|e verfasserin \|4 aut
700	0		\|a Daizhong Liu \|e verfasserin \|4 aut
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700	0		\|a Maria del Carmen Polletta \|e verfasserin \|4 aut
700	0		\|a Kevin C. Harrington \|e verfasserin \|4 aut
700	0		\|a S. P. Willner \|e verfasserin \|4 aut
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700	0		\|a Norman A. Grogin \|e verfasserin \|4 aut
700	0		\|a Madeline A. Marshall \|e verfasserin \|4 aut
700	0		\|a Ashish K. Meena \|e verfasserin \|4 aut
700	0		\|a Mario Nonino \|e verfasserin \|4 aut
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700	0		\|a Lou Strolger \|e verfasserin \|4 aut
700	0		\|a Scott Tompkins \|e verfasserin \|4 aut
700	0		\|a Christopher N. A. Willmer \|e verfasserin \|4 aut
700	0		\|a Haojing Yan \|e verfasserin \|4 aut
700	0		\|a Min S. Yun \|e verfasserin \|4 aut
700	0		\|a Adi Zitrin \|e verfasserin \|4 aut
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allfields	10.3847/1538-4357/ad1034 doi (DE-627)DOAJ096516925 (DE-599)DOAJ6cc49a5947ac4a70931e819d2c75b613 DE-627 ger DE-627 rakwb eng QB460-466 Brenda L. Frye verfasserin aut The JWST Discovery of the Triply Imaged Type Ia “Supernova H0pe” and Observations of the Galaxy Cluster PLCK G165.7+67.0 2024 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier A Type Ia supernova (SN) at z = 1.78 was discovered in James Webb Space Telescope Near Infrared Camera imaging of the galaxy cluster PLCK G165.7+67.0 (G165; z = 0.35). The SN is situated 1.5–2 kpc from the host-galaxy nucleus and appears in three different locations as a result of gravitational lensing by G165. These data can yield a value for Hubble’s constant using time delays from this multiply imaged SN Ia that we call “SN H0pe.” Over the cluster, we identified 21 image multiplicities, confirmed five of them using the Near-Infrared Spectrograph, and constructed a new lens model that gives a total mass within 600 kpc of (2.6 ± 0.3) × 10 ^14 M _⊙ . The photometry uncovered a galaxy overdensity coincident with the SN host galaxy. NIRSpec confirmed six member galaxies, four of which surround the SN host galaxy with relative velocity ≲900 km s ^−1 and projected physical extent ≲33 kpc. This compact galaxy group is dominated by the SN host galaxy, which has a stellar mass of (5.0 ± 0.1) × 10 ^11 M _⊙ . The group members have specific star formation rates of 2–260 Gyr ^−1 derived from the H α -line fluxes corrected for stellar absorption, dust extinction, and slit losses. Another group centered on a strongly lensed dusty star-forming galaxy is at z = 2.24. The total (unobscured and obscured) SFR of this second galaxy group is estimated to be (≳ 100 M _⊙ yr ^−1 ), which translates to a supernova rate of ∼1 SNe yr ^−1 , suggesting that regular monitoring of this cluster may yield additional SNe. Strong gravitational lensing Rich galaxy clusters High-redshift galaxy clusters Galaxy cluster counts Galaxy spectroscopy Astrophysics Massimo Pascale verfasserin aut Justin Pierel verfasserin aut Wenlei Chen verfasserin aut Nicholas Foo verfasserin aut Reagen Leimbach verfasserin aut Nikhil Garuda verfasserin aut Seth H. Cohen verfasserin aut Patrick S. Kamieneski verfasserin aut Rogier A. Windhorst verfasserin aut Anton M. Koekemoer verfasserin aut Pat Kelly verfasserin aut Jake Summers verfasserin aut Michael Engesser verfasserin aut Daizhong Liu verfasserin aut Lukas J. Furtak verfasserin aut Maria del Carmen Polletta verfasserin aut Kevin C. Harrington verfasserin aut S. P. Willner verfasserin aut Jose M. Diego verfasserin aut Rolf A. Jansen verfasserin aut Dan Coe verfasserin aut Christopher J. Conselice verfasserin aut Liang Dai verfasserin aut Hervé Dole verfasserin aut Jordan C. J. D’Silva verfasserin aut Simon P. Driver verfasserin aut Norman A. Grogin verfasserin aut Madeline A. Marshall verfasserin aut Ashish K. Meena verfasserin aut Mario Nonino verfasserin aut Rafael Ortiz III verfasserin aut Nor Pirzkal verfasserin aut Aaron Robotham verfasserin aut Russell E. Ryan Jr. verfasserin aut Lou Strolger verfasserin aut Scott Tompkins verfasserin aut Christopher N. A. Willmer verfasserin aut Haojing Yan verfasserin aut Min S. Yun verfasserin aut Adi Zitrin verfasserin aut In The Astrophysical Journal IOP Publishing, 2022 961(2024), 2, p 171 (DE-627)269019219 (DE-600)1473835-1 15384357 nnns volume:961 year:2024 number:2, p 171 https://doi.org/10.3847/1538-4357/ad1034 kostenfrei https://doaj.org/article/6cc49a5947ac4a70931e819d2c75b613 kostenfrei https://doi.org/10.3847/1538-4357/ad1034 kostenfrei https://doaj.org/toc/1538-4357 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 961 2024 2, p 171
spelling	10.3847/1538-4357/ad1034 doi (DE-627)DOAJ096516925 (DE-599)DOAJ6cc49a5947ac4a70931e819d2c75b613 DE-627 ger DE-627 rakwb eng QB460-466 Brenda L. Frye verfasserin aut The JWST Discovery of the Triply Imaged Type Ia “Supernova H0pe” and Observations of the Galaxy Cluster PLCK G165.7+67.0 2024 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier A Type Ia supernova (SN) at z = 1.78 was discovered in James Webb Space Telescope Near Infrared Camera imaging of the galaxy cluster PLCK G165.7+67.0 (G165; z = 0.35). The SN is situated 1.5–2 kpc from the host-galaxy nucleus and appears in three different locations as a result of gravitational lensing by G165. These data can yield a value for Hubble’s constant using time delays from this multiply imaged SN Ia that we call “SN H0pe.” Over the cluster, we identified 21 image multiplicities, confirmed five of them using the Near-Infrared Spectrograph, and constructed a new lens model that gives a total mass within 600 kpc of (2.6 ± 0.3) × 10 ^14 M _⊙ . The photometry uncovered a galaxy overdensity coincident with the SN host galaxy. NIRSpec confirmed six member galaxies, four of which surround the SN host galaxy with relative velocity ≲900 km s ^−1 and projected physical extent ≲33 kpc. This compact galaxy group is dominated by the SN host galaxy, which has a stellar mass of (5.0 ± 0.1) × 10 ^11 M _⊙ . The group members have specific star formation rates of 2–260 Gyr ^−1 derived from the H α -line fluxes corrected for stellar absorption, dust extinction, and slit losses. Another group centered on a strongly lensed dusty star-forming galaxy is at z = 2.24. The total (unobscured and obscured) SFR of this second galaxy group is estimated to be (≳ 100 M _⊙ yr ^−1 ), which translates to a supernova rate of ∼1 SNe yr ^−1 , suggesting that regular monitoring of this cluster may yield additional SNe. Strong gravitational lensing Rich galaxy clusters High-redshift galaxy clusters Galaxy cluster counts Galaxy spectroscopy Astrophysics Massimo Pascale verfasserin aut Justin Pierel verfasserin aut Wenlei Chen verfasserin aut Nicholas Foo verfasserin aut Reagen Leimbach verfasserin aut Nikhil Garuda verfasserin aut Seth H. Cohen verfasserin aut Patrick S. Kamieneski verfasserin aut Rogier A. Windhorst verfasserin aut Anton M. Koekemoer verfasserin aut Pat Kelly verfasserin aut Jake Summers verfasserin aut Michael Engesser verfasserin aut Daizhong Liu verfasserin aut Lukas J. Furtak verfasserin aut Maria del Carmen Polletta verfasserin aut Kevin C. Harrington verfasserin aut S. P. Willner verfasserin aut Jose M. Diego verfasserin aut Rolf A. Jansen verfasserin aut Dan Coe verfasserin aut Christopher J. Conselice verfasserin aut Liang Dai verfasserin aut Hervé Dole verfasserin aut Jordan C. J. D’Silva verfasserin aut Simon P. Driver verfasserin aut Norman A. Grogin verfasserin aut Madeline A. Marshall verfasserin aut Ashish K. Meena verfasserin aut Mario Nonino verfasserin aut Rafael Ortiz III verfasserin aut Nor Pirzkal verfasserin aut Aaron Robotham verfasserin aut Russell E. Ryan Jr. verfasserin aut Lou Strolger verfasserin aut Scott Tompkins verfasserin aut Christopher N. A. Willmer verfasserin aut Haojing Yan verfasserin aut Min S. Yun verfasserin aut Adi Zitrin verfasserin aut In The Astrophysical Journal IOP Publishing, 2022 961(2024), 2, p 171 (DE-627)269019219 (DE-600)1473835-1 15384357 nnns volume:961 year:2024 number:2, p 171 https://doi.org/10.3847/1538-4357/ad1034 kostenfrei https://doaj.org/article/6cc49a5947ac4a70931e819d2c75b613 kostenfrei https://doi.org/10.3847/1538-4357/ad1034 kostenfrei https://doaj.org/toc/1538-4357 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 961 2024 2, p 171
allfields_unstemmed	10.3847/1538-4357/ad1034 doi (DE-627)DOAJ096516925 (DE-599)DOAJ6cc49a5947ac4a70931e819d2c75b613 DE-627 ger DE-627 rakwb eng QB460-466 Brenda L. Frye verfasserin aut The JWST Discovery of the Triply Imaged Type Ia “Supernova H0pe” and Observations of the Galaxy Cluster PLCK G165.7+67.0 2024 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier A Type Ia supernova (SN) at z = 1.78 was discovered in James Webb Space Telescope Near Infrared Camera imaging of the galaxy cluster PLCK G165.7+67.0 (G165; z = 0.35). The SN is situated 1.5–2 kpc from the host-galaxy nucleus and appears in three different locations as a result of gravitational lensing by G165. These data can yield a value for Hubble’s constant using time delays from this multiply imaged SN Ia that we call “SN H0pe.” Over the cluster, we identified 21 image multiplicities, confirmed five of them using the Near-Infrared Spectrograph, and constructed a new lens model that gives a total mass within 600 kpc of (2.6 ± 0.3) × 10 ^14 M _⊙ . The photometry uncovered a galaxy overdensity coincident with the SN host galaxy. NIRSpec confirmed six member galaxies, four of which surround the SN host galaxy with relative velocity ≲900 km s ^−1 and projected physical extent ≲33 kpc. This compact galaxy group is dominated by the SN host galaxy, which has a stellar mass of (5.0 ± 0.1) × 10 ^11 M _⊙ . The group members have specific star formation rates of 2–260 Gyr ^−1 derived from the H α -line fluxes corrected for stellar absorption, dust extinction, and slit losses. Another group centered on a strongly lensed dusty star-forming galaxy is at z = 2.24. The total (unobscured and obscured) SFR of this second galaxy group is estimated to be (≳ 100 M _⊙ yr ^−1 ), which translates to a supernova rate of ∼1 SNe yr ^−1 , suggesting that regular monitoring of this cluster may yield additional SNe. Strong gravitational lensing Rich galaxy clusters High-redshift galaxy clusters Galaxy cluster counts Galaxy spectroscopy Astrophysics Massimo Pascale verfasserin aut Justin Pierel verfasserin aut Wenlei Chen verfasserin aut Nicholas Foo verfasserin aut Reagen Leimbach verfasserin aut Nikhil Garuda verfasserin aut Seth H. Cohen verfasserin aut Patrick S. Kamieneski verfasserin aut Rogier A. Windhorst verfasserin aut Anton M. Koekemoer verfasserin aut Pat Kelly verfasserin aut Jake Summers verfasserin aut Michael Engesser verfasserin aut Daizhong Liu verfasserin aut Lukas J. Furtak verfasserin aut Maria del Carmen Polletta verfasserin aut Kevin C. Harrington verfasserin aut S. P. Willner verfasserin aut Jose M. Diego verfasserin aut Rolf A. Jansen verfasserin aut Dan Coe verfasserin aut Christopher J. Conselice verfasserin aut Liang Dai verfasserin aut Hervé Dole verfasserin aut Jordan C. J. D’Silva verfasserin aut Simon P. Driver verfasserin aut Norman A. Grogin verfasserin aut Madeline A. Marshall verfasserin aut Ashish K. Meena verfasserin aut Mario Nonino verfasserin aut Rafael Ortiz III verfasserin aut Nor Pirzkal verfasserin aut Aaron Robotham verfasserin aut Russell E. Ryan Jr. verfasserin aut Lou Strolger verfasserin aut Scott Tompkins verfasserin aut Christopher N. A. Willmer verfasserin aut Haojing Yan verfasserin aut Min S. Yun verfasserin aut Adi Zitrin verfasserin aut In The Astrophysical Journal IOP Publishing, 2022 961(2024), 2, p 171 (DE-627)269019219 (DE-600)1473835-1 15384357 nnns volume:961 year:2024 number:2, p 171 https://doi.org/10.3847/1538-4357/ad1034 kostenfrei https://doaj.org/article/6cc49a5947ac4a70931e819d2c75b613 kostenfrei https://doi.org/10.3847/1538-4357/ad1034 kostenfrei https://doaj.org/toc/1538-4357 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 961 2024 2, p 171
allfieldsGer	10.3847/1538-4357/ad1034 doi (DE-627)DOAJ096516925 (DE-599)DOAJ6cc49a5947ac4a70931e819d2c75b613 DE-627 ger DE-627 rakwb eng QB460-466 Brenda L. Frye verfasserin aut The JWST Discovery of the Triply Imaged Type Ia “Supernova H0pe” and Observations of the Galaxy Cluster PLCK G165.7+67.0 2024 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier A Type Ia supernova (SN) at z = 1.78 was discovered in James Webb Space Telescope Near Infrared Camera imaging of the galaxy cluster PLCK G165.7+67.0 (G165; z = 0.35). The SN is situated 1.5–2 kpc from the host-galaxy nucleus and appears in three different locations as a result of gravitational lensing by G165. These data can yield a value for Hubble’s constant using time delays from this multiply imaged SN Ia that we call “SN H0pe.” Over the cluster, we identified 21 image multiplicities, confirmed five of them using the Near-Infrared Spectrograph, and constructed a new lens model that gives a total mass within 600 kpc of (2.6 ± 0.3) × 10 ^14 M _⊙ . The photometry uncovered a galaxy overdensity coincident with the SN host galaxy. NIRSpec confirmed six member galaxies, four of which surround the SN host galaxy with relative velocity ≲900 km s ^−1 and projected physical extent ≲33 kpc. This compact galaxy group is dominated by the SN host galaxy, which has a stellar mass of (5.0 ± 0.1) × 10 ^11 M _⊙ . The group members have specific star formation rates of 2–260 Gyr ^−1 derived from the H α -line fluxes corrected for stellar absorption, dust extinction, and slit losses. Another group centered on a strongly lensed dusty star-forming galaxy is at z = 2.24. The total (unobscured and obscured) SFR of this second galaxy group is estimated to be (≳ 100 M _⊙ yr ^−1 ), which translates to a supernova rate of ∼1 SNe yr ^−1 , suggesting that regular monitoring of this cluster may yield additional SNe. Strong gravitational lensing Rich galaxy clusters High-redshift galaxy clusters Galaxy cluster counts Galaxy spectroscopy Astrophysics Massimo Pascale verfasserin aut Justin Pierel verfasserin aut Wenlei Chen verfasserin aut Nicholas Foo verfasserin aut Reagen Leimbach verfasserin aut Nikhil Garuda verfasserin aut Seth H. Cohen verfasserin aut Patrick S. Kamieneski verfasserin aut Rogier A. Windhorst verfasserin aut Anton M. Koekemoer verfasserin aut Pat Kelly verfasserin aut Jake Summers verfasserin aut Michael Engesser verfasserin aut Daizhong Liu verfasserin aut Lukas J. Furtak verfasserin aut Maria del Carmen Polletta verfasserin aut Kevin C. Harrington verfasserin aut S. P. Willner verfasserin aut Jose M. Diego verfasserin aut Rolf A. Jansen verfasserin aut Dan Coe verfasserin aut Christopher J. Conselice verfasserin aut Liang Dai verfasserin aut Hervé Dole verfasserin aut Jordan C. J. D’Silva verfasserin aut Simon P. Driver verfasserin aut Norman A. Grogin verfasserin aut Madeline A. Marshall verfasserin aut Ashish K. Meena verfasserin aut Mario Nonino verfasserin aut Rafael Ortiz III verfasserin aut Nor Pirzkal verfasserin aut Aaron Robotham verfasserin aut Russell E. Ryan Jr. verfasserin aut Lou Strolger verfasserin aut Scott Tompkins verfasserin aut Christopher N. A. Willmer verfasserin aut Haojing Yan verfasserin aut Min S. Yun verfasserin aut Adi Zitrin verfasserin aut In The Astrophysical Journal IOP Publishing, 2022 961(2024), 2, p 171 (DE-627)269019219 (DE-600)1473835-1 15384357 nnns volume:961 year:2024 number:2, p 171 https://doi.org/10.3847/1538-4357/ad1034 kostenfrei https://doaj.org/article/6cc49a5947ac4a70931e819d2c75b613 kostenfrei https://doi.org/10.3847/1538-4357/ad1034 kostenfrei https://doaj.org/toc/1538-4357 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 961 2024 2, p 171
allfieldsSound	10.3847/1538-4357/ad1034 doi (DE-627)DOAJ096516925 (DE-599)DOAJ6cc49a5947ac4a70931e819d2c75b613 DE-627 ger DE-627 rakwb eng QB460-466 Brenda L. Frye verfasserin aut The JWST Discovery of the Triply Imaged Type Ia “Supernova H0pe” and Observations of the Galaxy Cluster PLCK G165.7+67.0 2024 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier A Type Ia supernova (SN) at z = 1.78 was discovered in James Webb Space Telescope Near Infrared Camera imaging of the galaxy cluster PLCK G165.7+67.0 (G165; z = 0.35). The SN is situated 1.5–2 kpc from the host-galaxy nucleus and appears in three different locations as a result of gravitational lensing by G165. These data can yield a value for Hubble’s constant using time delays from this multiply imaged SN Ia that we call “SN H0pe.” Over the cluster, we identified 21 image multiplicities, confirmed five of them using the Near-Infrared Spectrograph, and constructed a new lens model that gives a total mass within 600 kpc of (2.6 ± 0.3) × 10 ^14 M _⊙ . The photometry uncovered a galaxy overdensity coincident with the SN host galaxy. NIRSpec confirmed six member galaxies, four of which surround the SN host galaxy with relative velocity ≲900 km s ^−1 and projected physical extent ≲33 kpc. This compact galaxy group is dominated by the SN host galaxy, which has a stellar mass of (5.0 ± 0.1) × 10 ^11 M _⊙ . The group members have specific star formation rates of 2–260 Gyr ^−1 derived from the H α -line fluxes corrected for stellar absorption, dust extinction, and slit losses. Another group centered on a strongly lensed dusty star-forming galaxy is at z = 2.24. The total (unobscured and obscured) SFR of this second galaxy group is estimated to be (≳ 100 M _⊙ yr ^−1 ), which translates to a supernova rate of ∼1 SNe yr ^−1 , suggesting that regular monitoring of this cluster may yield additional SNe. Strong gravitational lensing Rich galaxy clusters High-redshift galaxy clusters Galaxy cluster counts Galaxy spectroscopy Astrophysics Massimo Pascale verfasserin aut Justin Pierel verfasserin aut Wenlei Chen verfasserin aut Nicholas Foo verfasserin aut Reagen Leimbach verfasserin aut Nikhil Garuda verfasserin aut Seth H. Cohen verfasserin aut Patrick S. Kamieneski verfasserin aut Rogier A. Windhorst verfasserin aut Anton M. Koekemoer verfasserin aut Pat Kelly verfasserin aut Jake Summers verfasserin aut Michael Engesser verfasserin aut Daizhong Liu verfasserin aut Lukas J. Furtak verfasserin aut Maria del Carmen Polletta verfasserin aut Kevin C. Harrington verfasserin aut S. P. Willner verfasserin aut Jose M. Diego verfasserin aut Rolf A. Jansen verfasserin aut Dan Coe verfasserin aut Christopher J. Conselice verfasserin aut Liang Dai verfasserin aut Hervé Dole verfasserin aut Jordan C. J. D’Silva verfasserin aut Simon P. Driver verfasserin aut Norman A. Grogin verfasserin aut Madeline A. Marshall verfasserin aut Ashish K. Meena verfasserin aut Mario Nonino verfasserin aut Rafael Ortiz III verfasserin aut Nor Pirzkal verfasserin aut Aaron Robotham verfasserin aut Russell E. Ryan Jr. verfasserin aut Lou Strolger verfasserin aut Scott Tompkins verfasserin aut Christopher N. A. Willmer verfasserin aut Haojing Yan verfasserin aut Min S. Yun verfasserin aut Adi Zitrin verfasserin aut In The Astrophysical Journal IOP Publishing, 2022 961(2024), 2, p 171 (DE-627)269019219 (DE-600)1473835-1 15384357 nnns volume:961 year:2024 number:2, p 171 https://doi.org/10.3847/1538-4357/ad1034 kostenfrei https://doaj.org/article/6cc49a5947ac4a70931e819d2c75b613 kostenfrei https://doi.org/10.3847/1538-4357/ad1034 kostenfrei https://doaj.org/toc/1538-4357 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 961 2024 2, p 171
language	English
source	In The Astrophysical Journal 961(2024), 2, p 171 volume:961 year:2024 number:2, p 171
sourceStr	In The Astrophysical Journal 961(2024), 2, p 171 volume:961 year:2024 number:2, p 171
format_phy_str_mv	Article
institution	findex.gbv.de
topic_facet	Strong gravitational lensing Rich galaxy clusters High-redshift galaxy clusters Galaxy cluster counts Galaxy spectroscopy Astrophysics
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container_title	The Astrophysical Journal
authorswithroles_txt_mv	Brenda L. Frye @@aut@@ Massimo Pascale @@aut@@ Justin Pierel @@aut@@ Wenlei Chen @@aut@@ Nicholas Foo @@aut@@ Reagen Leimbach @@aut@@ Nikhil Garuda @@aut@@ Seth H. Cohen @@aut@@ Patrick S. Kamieneski @@aut@@ Rogier A. Windhorst @@aut@@ Anton M. Koekemoer @@aut@@ Pat Kelly @@aut@@ Jake Summers @@aut@@ Michael Engesser @@aut@@ Daizhong Liu @@aut@@ Lukas J. Furtak @@aut@@ Maria del Carmen Polletta @@aut@@ Kevin C. Harrington @@aut@@ S. P. Willner @@aut@@ Jose M. Diego @@aut@@ Rolf A. Jansen @@aut@@ Dan Coe @@aut@@ Christopher J. Conselice @@aut@@ Liang Dai @@aut@@ Hervé Dole @@aut@@ Jordan C. J. D’Silva @@aut@@ Simon P. Driver @@aut@@ Norman A. Grogin @@aut@@ Madeline A. Marshall @@aut@@ Ashish K. Meena @@aut@@ Mario Nonino @@aut@@ Rafael Ortiz III @@aut@@ Nor Pirzkal @@aut@@ Aaron Robotham @@aut@@ Russell E. Ryan Jr. @@aut@@ Lou Strolger @@aut@@ Scott Tompkins @@aut@@ Christopher N. A. Willmer @@aut@@ Haojing Yan @@aut@@ Min S. Yun @@aut@@ Adi Zitrin @@aut@@
publishDateDaySort_date	2024-01-01T00:00:00Z
hierarchy_top_id	269019219
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Frye</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="4"><subfield code="a">The JWST Discovery of the Triply Imaged Type Ia “Supernova H0pe” and Observations of the Galaxy Cluster PLCK G165.7+67.0</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2024</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">Computermedien</subfield><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Online-Ressource</subfield><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">A Type Ia supernova (SN) at z = 1.78 was discovered in James Webb Space Telescope Near Infrared Camera imaging of the galaxy cluster PLCK G165.7+67.0 (G165; z = 0.35). 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callnumber-first	Q - Science
author	Brenda L. Frye
spellingShingle	Brenda L. Frye misc QB460-466 misc Strong gravitational lensing misc Rich galaxy clusters misc High-redshift galaxy clusters misc Galaxy cluster counts misc Galaxy spectroscopy misc Astrophysics The JWST Discovery of the Triply Imaged Type Ia “Supernova H0pe” and Observations of the Galaxy Cluster PLCK G165.7+67.0
authorStr	Brenda L. Frye
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topic_title	QB460-466 The JWST Discovery of the Triply Imaged Type Ia “Supernova H0pe” and Observations of the Galaxy Cluster PLCK G165.7+67.0 Strong gravitational lensing Rich galaxy clusters High-redshift galaxy clusters Galaxy cluster counts Galaxy spectroscopy
topic	misc QB460-466 misc Strong gravitational lensing misc Rich galaxy clusters misc High-redshift galaxy clusters misc Galaxy cluster counts misc Galaxy spectroscopy misc Astrophysics
topic_unstemmed	misc QB460-466 misc Strong gravitational lensing misc Rich galaxy clusters misc High-redshift galaxy clusters misc Galaxy cluster counts misc Galaxy spectroscopy misc Astrophysics
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title	The JWST Discovery of the Triply Imaged Type Ia “Supernova H0pe” and Observations of the Galaxy Cluster PLCK G165.7+67.0
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title_full	The JWST Discovery of the Triply Imaged Type Ia “Supernova H0pe” and Observations of the Galaxy Cluster PLCK G165.7+67.0
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author_browse	Brenda L. Frye Massimo Pascale Justin Pierel Wenlei Chen Nicholas Foo Reagen Leimbach Nikhil Garuda Seth H. Cohen Patrick S. Kamieneski Rogier A. Windhorst Anton M. Koekemoer Pat Kelly Jake Summers Michael Engesser Daizhong Liu Lukas J. Furtak Maria del Carmen Polletta Kevin C. Harrington S. P. Willner Jose M. Diego Rolf A. Jansen Dan Coe Christopher J. Conselice Liang Dai Hervé Dole Jordan C. J. D’Silva Simon P. Driver Norman A. Grogin Madeline A. Marshall Ashish K. Meena Mario Nonino Rafael Ortiz III Nor Pirzkal Aaron Robotham Russell E. Ryan Jr. Lou Strolger Scott Tompkins Christopher N. A. Willmer Haojing Yan Min S. Yun Adi Zitrin
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title_sort	jwst discovery of the triply imaged type ia “supernova h0pe” and observations of the galaxy cluster plck g165.7+67.0
callnumber	QB460-466
title_auth	The JWST Discovery of the Triply Imaged Type Ia “Supernova H0pe” and Observations of the Galaxy Cluster PLCK G165.7+67.0
abstract	A Type Ia supernova (SN) at z = 1.78 was discovered in James Webb Space Telescope Near Infrared Camera imaging of the galaxy cluster PLCK G165.7+67.0 (G165; z = 0.35). The SN is situated 1.5–2 kpc from the host-galaxy nucleus and appears in three different locations as a result of gravitational lensing by G165. These data can yield a value for Hubble’s constant using time delays from this multiply imaged SN Ia that we call “SN H0pe.” Over the cluster, we identified 21 image multiplicities, confirmed five of them using the Near-Infrared Spectrograph, and constructed a new lens model that gives a total mass within 600 kpc of (2.6 ± 0.3) × 10 ^14 M _⊙ . The photometry uncovered a galaxy overdensity coincident with the SN host galaxy. NIRSpec confirmed six member galaxies, four of which surround the SN host galaxy with relative velocity ≲900 km s ^−1 and projected physical extent ≲33 kpc. This compact galaxy group is dominated by the SN host galaxy, which has a stellar mass of (5.0 ± 0.1) × 10 ^11 M _⊙ . The group members have specific star formation rates of 2–260 Gyr ^−1 derived from the H α -line fluxes corrected for stellar absorption, dust extinction, and slit losses. Another group centered on a strongly lensed dusty star-forming galaxy is at z = 2.24. The total (unobscured and obscured) SFR of this second galaxy group is estimated to be (≳ 100 M _⊙ yr ^−1 ), which translates to a supernova rate of ∼1 SNe yr ^−1 , suggesting that regular monitoring of this cluster may yield additional SNe.
abstractGer	A Type Ia supernova (SN) at z = 1.78 was discovered in James Webb Space Telescope Near Infrared Camera imaging of the galaxy cluster PLCK G165.7+67.0 (G165; z = 0.35). The SN is situated 1.5–2 kpc from the host-galaxy nucleus and appears in three different locations as a result of gravitational lensing by G165. These data can yield a value for Hubble’s constant using time delays from this multiply imaged SN Ia that we call “SN H0pe.” Over the cluster, we identified 21 image multiplicities, confirmed five of them using the Near-Infrared Spectrograph, and constructed a new lens model that gives a total mass within 600 kpc of (2.6 ± 0.3) × 10 ^14 M _⊙ . The photometry uncovered a galaxy overdensity coincident with the SN host galaxy. NIRSpec confirmed six member galaxies, four of which surround the SN host galaxy with relative velocity ≲900 km s ^−1 and projected physical extent ≲33 kpc. This compact galaxy group is dominated by the SN host galaxy, which has a stellar mass of (5.0 ± 0.1) × 10 ^11 M _⊙ . The group members have specific star formation rates of 2–260 Gyr ^−1 derived from the H α -line fluxes corrected for stellar absorption, dust extinction, and slit losses. Another group centered on a strongly lensed dusty star-forming galaxy is at z = 2.24. The total (unobscured and obscured) SFR of this second galaxy group is estimated to be (≳ 100 M _⊙ yr ^−1 ), which translates to a supernova rate of ∼1 SNe yr ^−1 , suggesting that regular monitoring of this cluster may yield additional SNe.
abstract_unstemmed	A Type Ia supernova (SN) at z = 1.78 was discovered in James Webb Space Telescope Near Infrared Camera imaging of the galaxy cluster PLCK G165.7+67.0 (G165; z = 0.35). The SN is situated 1.5–2 kpc from the host-galaxy nucleus and appears in three different locations as a result of gravitational lensing by G165. These data can yield a value for Hubble’s constant using time delays from this multiply imaged SN Ia that we call “SN H0pe.” Over the cluster, we identified 21 image multiplicities, confirmed five of them using the Near-Infrared Spectrograph, and constructed a new lens model that gives a total mass within 600 kpc of (2.6 ± 0.3) × 10 ^14 M _⊙ . The photometry uncovered a galaxy overdensity coincident with the SN host galaxy. NIRSpec confirmed six member galaxies, four of which surround the SN host galaxy with relative velocity ≲900 km s ^−1 and projected physical extent ≲33 kpc. This compact galaxy group is dominated by the SN host galaxy, which has a stellar mass of (5.0 ± 0.1) × 10 ^11 M _⊙ . The group members have specific star formation rates of 2–260 Gyr ^−1 derived from the H α -line fluxes corrected for stellar absorption, dust extinction, and slit losses. Another group centered on a strongly lensed dusty star-forming galaxy is at z = 2.24. The total (unobscured and obscured) SFR of this second galaxy group is estimated to be (≳ 100 M _⊙ yr ^−1 ), which translates to a supernova rate of ∼1 SNe yr ^−1 , suggesting that regular monitoring of this cluster may yield additional SNe.
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container_issue	2, p 171
title_short	The JWST Discovery of the Triply Imaged Type Ia “Supernova H0pe” and Observations of the Galaxy Cluster PLCK G165.7+67.0
url	https://doi.org/10.3847/1538-4357/ad1034 https://doaj.org/article/6cc49a5947ac4a70931e819d2c75b613 https://doaj.org/toc/1538-4357
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author2	Massimo Pascale Justin Pierel Wenlei Chen Nicholas Foo Reagen Leimbach Nikhil Garuda Seth H. Cohen Patrick S. Kamieneski Rogier A. Windhorst Anton M. Koekemoer Pat Kelly Jake Summers Michael Engesser Daizhong Liu Lukas J. Furtak Maria del Carmen Polletta Kevin C. Harrington S. P. Willner Jose M. Diego Rolf A. Jansen Dan Coe Christopher J. Conselice Liang Dai Hervé Dole Jordan C. J. D’Silva Simon P. Driver Norman A. Grogin Madeline A. Marshall Ashish K. Meena Mario Nonino Rafael Ortiz III Nor Pirzkal Aaron Robotham Russell E. Ryan Jr. Lou Strolger Scott Tompkins Christopher N. A. Willmer Haojing Yan Min S. Yun Adi Zitrin
author2Str	Massimo Pascale Justin Pierel Wenlei Chen Nicholas Foo Reagen Leimbach Nikhil Garuda Seth H. Cohen Patrick S. Kamieneski Rogier A. Windhorst Anton M. Koekemoer Pat Kelly Jake Summers Michael Engesser Daizhong Liu Lukas J. Furtak Maria del Carmen Polletta Kevin C. Harrington S. P. Willner Jose M. Diego Rolf A. Jansen Dan Coe Christopher J. Conselice Liang Dai Hervé Dole Jordan C. J. D’Silva Simon P. Driver Norman A. Grogin Madeline A. Marshall Ashish K. Meena Mario Nonino Rafael Ortiz III Nor Pirzkal Aaron Robotham Russell E. Ryan Jr. Lou Strolger Scott Tompkins Christopher N. A. Willmer Haojing Yan Min S. Yun Adi Zitrin
ppnlink	269019219
callnumber-subject	QB - Astronomy
mediatype_str_mv	c
isOA_txt	true
hochschulschrift_bool	false
doi_str	10.3847/1538-4357/ad1034
callnumber-a	QB460-466
up_date	2024-07-03T20:36:18.387Z
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The JWST Discovery of the Triply Imaged Type Ia “Supernova H0pe” and Observations of the Galaxy Cluster PLCK G165.7+67.0

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