JWST's PEARLS: Transients in the MACS J0416.1−2403 Field

With its unprecedented sensitivity and spatial resolution, the James Webb Space Telescope (JWST) has opened a new window for time-domain discoveries in the infrared. Here we report observations in the only field that has received four epochs (spanning 126 days) of JWST NIRCam observations in Cycle 1...
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Autor*in:	Haojing Yan [verfasserIn] Zhiyuan Ma [verfasserIn] Bangzheng Sun [verfasserIn] Lifan Wang [verfasserIn] Patrick Kelly [verfasserIn] José M. Diego [verfasserIn] Seth H. Cohen [verfasserIn] Rogier A. Windhorst [verfasserIn] Rolf A. Jansen [verfasserIn] Norman A. Grogin [verfasserIn] John F. Beacom [verfasserIn] Christopher J. Conselice [verfasserIn] Simon P. Driver [verfasserIn] Brenda Frye [verfasserIn] Dan Coe [verfasserIn] Madeline A. Marshall [verfasserIn] Anton Koekemoer [verfasserIn] Christopher N. A. Willmer [verfasserIn] Aaron Robotham [verfasserIn] Jordan C. J. D’Silva [verfasserIn] Jake Summers [verfasserIn] Mario Nonino [verfasserIn] Nor Pirzkal [verfasserIn] Russell E. Ryan Jr. [verfasserIn] Rafael Ortiz III [verfasserIn] Scott Tompkins [verfasserIn] Rachana A. Bhatawdekar [verfasserIn] Cheng Cheng [verfasserIn] Adi Zitrin [verfasserIn] S. P. Willner [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2023

Schlagwörter:	Transient sources Infrared sources Gravitational lensing Supernovae Surveys

Übergeordnetes Werk:	In: The Astrophysical Journal Supplement Series - IOP Publishing, 2022, 269(2023), 2, p 43
Übergeordnetes Werk:	volume:269 ; year:2023 ; number:2, p 43

Links:	Link aufrufen Link aufrufen Link aufrufen Journal toc

DOI / URN:	10.3847/1538-4365/ad0298

Katalog-ID:	DOAJ092561047

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allfields	10.3847/1538-4365/ad0298 doi (DE-627)DOAJ092561047 (DE-599)DOAJ0eb82ce4cf0246e28b542391545aec43 DE-627 ger DE-627 rakwb eng QB460-466 Haojing Yan verfasserin aut JWST's PEARLS: Transients in the MACS J0416.1−2403 Field 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier With its unprecedented sensitivity and spatial resolution, the James Webb Space Telescope (JWST) has opened a new window for time-domain discoveries in the infrared. Here we report observations in the only field that has received four epochs (spanning 126 days) of JWST NIRCam observations in Cycle 1. This field is toward MACS J0416.1−2403, which is a rich galaxy cluster at redshift z = 0.4 and is one of the Hubble Frontier Fields. We have discovered 14 transients from these data. Twelve of these transients happened in three galaxies (with z = 0.94, 1.01, and 2.091) crossing a lensing caustic of the cluster, and these transients are highly magnified by gravitational lensing. These 12 transients are likely of a similar nature to those previously reported based on the Hubble Space Telescope (HST) data in this field, i.e., individual stars in the highly magnified arcs. However, these 12 could not have been found by HST because they were too red and too faint. The other two transients are associated with background galaxies ( z = 2.205 and 0.7093) that are only moderately magnified, and they are likely supernovae. They indicate a demagnified supernova surface density, when monitored at a time cadence of a few months to a ∼3–4 μ m survey limit of AB ∼28.5 mag, of ∼0.5 arcmin ^−2 integrated to z ≈ 2. This survey depth is beyond the capability of HST but can be easily reached by JWST. Transient sources Infrared sources Gravitational lensing Supernovae Surveys Astrophysics Zhiyuan Ma verfasserin aut Bangzheng Sun verfasserin aut Lifan Wang verfasserin aut Patrick Kelly verfasserin aut José M. Diego verfasserin aut Seth H. Cohen verfasserin aut Rogier A. Windhorst verfasserin aut Rolf A. Jansen verfasserin aut Norman A. Grogin verfasserin aut John F. Beacom verfasserin aut Christopher J. Conselice verfasserin aut Simon P. Driver verfasserin aut Brenda Frye verfasserin aut Dan Coe verfasserin aut Madeline A. Marshall verfasserin aut Anton Koekemoer verfasserin aut Christopher N. A. Willmer verfasserin aut Aaron Robotham verfasserin aut Jordan C. J. D’Silva verfasserin aut Jake Summers verfasserin aut Mario Nonino verfasserin aut Nor Pirzkal verfasserin aut Russell E. Ryan Jr. verfasserin aut Rafael Ortiz III verfasserin aut Scott Tompkins verfasserin aut Rachana A. Bhatawdekar verfasserin aut Cheng Cheng verfasserin aut Adi Zitrin verfasserin aut S. P. Willner verfasserin aut In The Astrophysical Journal Supplement Series IOP Publishing, 2022 269(2023), 2, p 43 (DE-627)312200196 (DE-600)2006860-8 15384365 nnns volume:269 year:2023 number:2, p 43 https://doi.org/10.3847/1538-4365/ad0298 kostenfrei https://doaj.org/article/0eb82ce4cf0246e28b542391545aec43 kostenfrei https://doi.org/10.3847/1538-4365/ad0298 kostenfrei https://doaj.org/toc/0067-0049 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_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 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 269 2023 2, p 43
spelling	10.3847/1538-4365/ad0298 doi (DE-627)DOAJ092561047 (DE-599)DOAJ0eb82ce4cf0246e28b542391545aec43 DE-627 ger DE-627 rakwb eng QB460-466 Haojing Yan verfasserin aut JWST's PEARLS: Transients in the MACS J0416.1−2403 Field 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier With its unprecedented sensitivity and spatial resolution, the James Webb Space Telescope (JWST) has opened a new window for time-domain discoveries in the infrared. Here we report observations in the only field that has received four epochs (spanning 126 days) of JWST NIRCam observations in Cycle 1. This field is toward MACS J0416.1−2403, which is a rich galaxy cluster at redshift z = 0.4 and is one of the Hubble Frontier Fields. We have discovered 14 transients from these data. Twelve of these transients happened in three galaxies (with z = 0.94, 1.01, and 2.091) crossing a lensing caustic of the cluster, and these transients are highly magnified by gravitational lensing. These 12 transients are likely of a similar nature to those previously reported based on the Hubble Space Telescope (HST) data in this field, i.e., individual stars in the highly magnified arcs. However, these 12 could not have been found by HST because they were too red and too faint. The other two transients are associated with background galaxies ( z = 2.205 and 0.7093) that are only moderately magnified, and they are likely supernovae. They indicate a demagnified supernova surface density, when monitored at a time cadence of a few months to a ∼3–4 μ m survey limit of AB ∼28.5 mag, of ∼0.5 arcmin ^−2 integrated to z ≈ 2. This survey depth is beyond the capability of HST but can be easily reached by JWST. Transient sources Infrared sources Gravitational lensing Supernovae Surveys Astrophysics Zhiyuan Ma verfasserin aut Bangzheng Sun verfasserin aut Lifan Wang verfasserin aut Patrick Kelly verfasserin aut José M. Diego verfasserin aut Seth H. Cohen verfasserin aut Rogier A. Windhorst verfasserin aut Rolf A. Jansen verfasserin aut Norman A. Grogin verfasserin aut John F. Beacom verfasserin aut Christopher J. Conselice verfasserin aut Simon P. Driver verfasserin aut Brenda Frye verfasserin aut Dan Coe verfasserin aut Madeline A. Marshall verfasserin aut Anton Koekemoer verfasserin aut Christopher N. A. Willmer verfasserin aut Aaron Robotham verfasserin aut Jordan C. J. D’Silva verfasserin aut Jake Summers verfasserin aut Mario Nonino verfasserin aut Nor Pirzkal verfasserin aut Russell E. Ryan Jr. verfasserin aut Rafael Ortiz III verfasserin aut Scott Tompkins verfasserin aut Rachana A. Bhatawdekar verfasserin aut Cheng Cheng verfasserin aut Adi Zitrin verfasserin aut S. P. Willner verfasserin aut In The Astrophysical Journal Supplement Series IOP Publishing, 2022 269(2023), 2, p 43 (DE-627)312200196 (DE-600)2006860-8 15384365 nnns volume:269 year:2023 number:2, p 43 https://doi.org/10.3847/1538-4365/ad0298 kostenfrei https://doaj.org/article/0eb82ce4cf0246e28b542391545aec43 kostenfrei https://doi.org/10.3847/1538-4365/ad0298 kostenfrei https://doaj.org/toc/0067-0049 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_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 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 269 2023 2, p 43
allfields_unstemmed	10.3847/1538-4365/ad0298 doi (DE-627)DOAJ092561047 (DE-599)DOAJ0eb82ce4cf0246e28b542391545aec43 DE-627 ger DE-627 rakwb eng QB460-466 Haojing Yan verfasserin aut JWST's PEARLS: Transients in the MACS J0416.1−2403 Field 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier With its unprecedented sensitivity and spatial resolution, the James Webb Space Telescope (JWST) has opened a new window for time-domain discoveries in the infrared. Here we report observations in the only field that has received four epochs (spanning 126 days) of JWST NIRCam observations in Cycle 1. This field is toward MACS J0416.1−2403, which is a rich galaxy cluster at redshift z = 0.4 and is one of the Hubble Frontier Fields. We have discovered 14 transients from these data. Twelve of these transients happened in three galaxies (with z = 0.94, 1.01, and 2.091) crossing a lensing caustic of the cluster, and these transients are highly magnified by gravitational lensing. These 12 transients are likely of a similar nature to those previously reported based on the Hubble Space Telescope (HST) data in this field, i.e., individual stars in the highly magnified arcs. However, these 12 could not have been found by HST because they were too red and too faint. The other two transients are associated with background galaxies ( z = 2.205 and 0.7093) that are only moderately magnified, and they are likely supernovae. They indicate a demagnified supernova surface density, when monitored at a time cadence of a few months to a ∼3–4 μ m survey limit of AB ∼28.5 mag, of ∼0.5 arcmin ^−2 integrated to z ≈ 2. This survey depth is beyond the capability of HST but can be easily reached by JWST. Transient sources Infrared sources Gravitational lensing Supernovae Surveys Astrophysics Zhiyuan Ma verfasserin aut Bangzheng Sun verfasserin aut Lifan Wang verfasserin aut Patrick Kelly verfasserin aut José M. Diego verfasserin aut Seth H. Cohen verfasserin aut Rogier A. Windhorst verfasserin aut Rolf A. Jansen verfasserin aut Norman A. Grogin verfasserin aut John F. Beacom verfasserin aut Christopher J. Conselice verfasserin aut Simon P. Driver verfasserin aut Brenda Frye verfasserin aut Dan Coe verfasserin aut Madeline A. Marshall verfasserin aut Anton Koekemoer verfasserin aut Christopher N. A. Willmer verfasserin aut Aaron Robotham verfasserin aut Jordan C. J. D’Silva verfasserin aut Jake Summers verfasserin aut Mario Nonino verfasserin aut Nor Pirzkal verfasserin aut Russell E. Ryan Jr. verfasserin aut Rafael Ortiz III verfasserin aut Scott Tompkins verfasserin aut Rachana A. Bhatawdekar verfasserin aut Cheng Cheng verfasserin aut Adi Zitrin verfasserin aut S. P. Willner verfasserin aut In The Astrophysical Journal Supplement Series IOP Publishing, 2022 269(2023), 2, p 43 (DE-627)312200196 (DE-600)2006860-8 15384365 nnns volume:269 year:2023 number:2, p 43 https://doi.org/10.3847/1538-4365/ad0298 kostenfrei https://doaj.org/article/0eb82ce4cf0246e28b542391545aec43 kostenfrei https://doi.org/10.3847/1538-4365/ad0298 kostenfrei https://doaj.org/toc/0067-0049 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_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 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 269 2023 2, p 43
allfieldsGer	10.3847/1538-4365/ad0298 doi (DE-627)DOAJ092561047 (DE-599)DOAJ0eb82ce4cf0246e28b542391545aec43 DE-627 ger DE-627 rakwb eng QB460-466 Haojing Yan verfasserin aut JWST's PEARLS: Transients in the MACS J0416.1−2403 Field 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier With its unprecedented sensitivity and spatial resolution, the James Webb Space Telescope (JWST) has opened a new window for time-domain discoveries in the infrared. Here we report observations in the only field that has received four epochs (spanning 126 days) of JWST NIRCam observations in Cycle 1. This field is toward MACS J0416.1−2403, which is a rich galaxy cluster at redshift z = 0.4 and is one of the Hubble Frontier Fields. We have discovered 14 transients from these data. Twelve of these transients happened in three galaxies (with z = 0.94, 1.01, and 2.091) crossing a lensing caustic of the cluster, and these transients are highly magnified by gravitational lensing. These 12 transients are likely of a similar nature to those previously reported based on the Hubble Space Telescope (HST) data in this field, i.e., individual stars in the highly magnified arcs. However, these 12 could not have been found by HST because they were too red and too faint. The other two transients are associated with background galaxies ( z = 2.205 and 0.7093) that are only moderately magnified, and they are likely supernovae. They indicate a demagnified supernova surface density, when monitored at a time cadence of a few months to a ∼3–4 μ m survey limit of AB ∼28.5 mag, of ∼0.5 arcmin ^−2 integrated to z ≈ 2. This survey depth is beyond the capability of HST but can be easily reached by JWST. Transient sources Infrared sources Gravitational lensing Supernovae Surveys Astrophysics Zhiyuan Ma verfasserin aut Bangzheng Sun verfasserin aut Lifan Wang verfasserin aut Patrick Kelly verfasserin aut José M. Diego verfasserin aut Seth H. Cohen verfasserin aut Rogier A. Windhorst verfasserin aut Rolf A. Jansen verfasserin aut Norman A. Grogin verfasserin aut John F. Beacom verfasserin aut Christopher J. Conselice verfasserin aut Simon P. Driver verfasserin aut Brenda Frye verfasserin aut Dan Coe verfasserin aut Madeline A. Marshall verfasserin aut Anton Koekemoer verfasserin aut Christopher N. A. Willmer verfasserin aut Aaron Robotham verfasserin aut Jordan C. J. D’Silva verfasserin aut Jake Summers verfasserin aut Mario Nonino verfasserin aut Nor Pirzkal verfasserin aut Russell E. Ryan Jr. verfasserin aut Rafael Ortiz III verfasserin aut Scott Tompkins verfasserin aut Rachana A. Bhatawdekar verfasserin aut Cheng Cheng verfasserin aut Adi Zitrin verfasserin aut S. P. Willner verfasserin aut In The Astrophysical Journal Supplement Series IOP Publishing, 2022 269(2023), 2, p 43 (DE-627)312200196 (DE-600)2006860-8 15384365 nnns volume:269 year:2023 number:2, p 43 https://doi.org/10.3847/1538-4365/ad0298 kostenfrei https://doaj.org/article/0eb82ce4cf0246e28b542391545aec43 kostenfrei https://doi.org/10.3847/1538-4365/ad0298 kostenfrei https://doaj.org/toc/0067-0049 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_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 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 269 2023 2, p 43
allfieldsSound	10.3847/1538-4365/ad0298 doi (DE-627)DOAJ092561047 (DE-599)DOAJ0eb82ce4cf0246e28b542391545aec43 DE-627 ger DE-627 rakwb eng QB460-466 Haojing Yan verfasserin aut JWST's PEARLS: Transients in the MACS J0416.1−2403 Field 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier With its unprecedented sensitivity and spatial resolution, the James Webb Space Telescope (JWST) has opened a new window for time-domain discoveries in the infrared. Here we report observations in the only field that has received four epochs (spanning 126 days) of JWST NIRCam observations in Cycle 1. This field is toward MACS J0416.1−2403, which is a rich galaxy cluster at redshift z = 0.4 and is one of the Hubble Frontier Fields. We have discovered 14 transients from these data. Twelve of these transients happened in three galaxies (with z = 0.94, 1.01, and 2.091) crossing a lensing caustic of the cluster, and these transients are highly magnified by gravitational lensing. These 12 transients are likely of a similar nature to those previously reported based on the Hubble Space Telescope (HST) data in this field, i.e., individual stars in the highly magnified arcs. However, these 12 could not have been found by HST because they were too red and too faint. The other two transients are associated with background galaxies ( z = 2.205 and 0.7093) that are only moderately magnified, and they are likely supernovae. They indicate a demagnified supernova surface density, when monitored at a time cadence of a few months to a ∼3–4 μ m survey limit of AB ∼28.5 mag, of ∼0.5 arcmin ^−2 integrated to z ≈ 2. This survey depth is beyond the capability of HST but can be easily reached by JWST. Transient sources Infrared sources Gravitational lensing Supernovae Surveys Astrophysics Zhiyuan Ma verfasserin aut Bangzheng Sun verfasserin aut Lifan Wang verfasserin aut Patrick Kelly verfasserin aut José M. Diego verfasserin aut Seth H. Cohen verfasserin aut Rogier A. Windhorst verfasserin aut Rolf A. Jansen verfasserin aut Norman A. Grogin verfasserin aut John F. Beacom verfasserin aut Christopher J. Conselice verfasserin aut Simon P. Driver verfasserin aut Brenda Frye verfasserin aut Dan Coe verfasserin aut Madeline A. Marshall verfasserin aut Anton Koekemoer verfasserin aut Christopher N. A. Willmer verfasserin aut Aaron Robotham verfasserin aut Jordan C. J. D’Silva verfasserin aut Jake Summers verfasserin aut Mario Nonino verfasserin aut Nor Pirzkal verfasserin aut Russell E. Ryan Jr. verfasserin aut Rafael Ortiz III verfasserin aut Scott Tompkins verfasserin aut Rachana A. Bhatawdekar verfasserin aut Cheng Cheng verfasserin aut Adi Zitrin verfasserin aut S. P. Willner verfasserin aut In The Astrophysical Journal Supplement Series IOP Publishing, 2022 269(2023), 2, p 43 (DE-627)312200196 (DE-600)2006860-8 15384365 nnns volume:269 year:2023 number:2, p 43 https://doi.org/10.3847/1538-4365/ad0298 kostenfrei https://doaj.org/article/0eb82ce4cf0246e28b542391545aec43 kostenfrei https://doi.org/10.3847/1538-4365/ad0298 kostenfrei https://doaj.org/toc/0067-0049 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_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 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 269 2023 2, p 43
language	English
source	In The Astrophysical Journal Supplement Series 269(2023), 2, p 43 volume:269 year:2023 number:2, p 43
sourceStr	In The Astrophysical Journal Supplement Series 269(2023), 2, p 43 volume:269 year:2023 number:2, p 43
format_phy_str_mv	Article
institution	findex.gbv.de
topic_facet	Transient sources Infrared sources Gravitational lensing Supernovae Surveys Astrophysics
isfreeaccess_bool	true
container_title	The Astrophysical Journal Supplement Series
authorswithroles_txt_mv	Haojing Yan @@aut@@ Zhiyuan Ma @@aut@@ Bangzheng Sun @@aut@@ Lifan Wang @@aut@@ Patrick Kelly @@aut@@ José M. Diego @@aut@@ Seth H. Cohen @@aut@@ Rogier A. Windhorst @@aut@@ Rolf A. Jansen @@aut@@ Norman A. Grogin @@aut@@ John F. Beacom @@aut@@ Christopher J. Conselice @@aut@@ Simon P. Driver @@aut@@ Brenda Frye @@aut@@ Dan Coe @@aut@@ Madeline A. Marshall @@aut@@ Anton Koekemoer @@aut@@ Christopher N. A. Willmer @@aut@@ Aaron Robotham @@aut@@ Jordan C. J. D’Silva @@aut@@ Jake Summers @@aut@@ Mario Nonino @@aut@@ Nor Pirzkal @@aut@@ Russell E. Ryan Jr. @@aut@@ Rafael Ortiz III @@aut@@ Scott Tompkins @@aut@@ Rachana A. Bhatawdekar @@aut@@ Cheng Cheng @@aut@@ Adi Zitrin @@aut@@ S. P. Willner @@aut@@
publishDateDaySort_date	2023-01-01T00:00:00Z
hierarchy_top_id	312200196
id	DOAJ092561047
language_de	englisch
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callnumber-first	Q - Science
author	Haojing Yan
spellingShingle	Haojing Yan misc QB460-466 misc Transient sources misc Infrared sources misc Gravitational lensing misc Supernovae misc Surveys misc Astrophysics JWST's PEARLS: Transients in the MACS J0416.1−2403 Field
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topic_title	QB460-466 JWST's PEARLS: Transients in the MACS J0416.1−2403 Field Transient sources Infrared sources Gravitational lensing Supernovae Surveys
topic	misc QB460-466 misc Transient sources misc Infrared sources misc Gravitational lensing misc Supernovae misc Surveys misc Astrophysics
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title	JWST's PEARLS: Transients in the MACS J0416.1−2403 Field
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author_browse	Haojing Yan Zhiyuan Ma Bangzheng Sun Lifan Wang Patrick Kelly José M. Diego Seth H. Cohen Rogier A. Windhorst Rolf A. Jansen Norman A. Grogin John F. Beacom Christopher J. Conselice Simon P. Driver Brenda Frye Dan Coe Madeline A. Marshall Anton Koekemoer Christopher N. A. Willmer Aaron Robotham Jordan C. J. D’Silva Jake Summers Mario Nonino Nor Pirzkal Russell E. Ryan Jr. Rafael Ortiz III Scott Tompkins Rachana A. Bhatawdekar Cheng Cheng Adi Zitrin S. P. Willner
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title_sort	jwst's pearls: transients in the macs j0416.1−2403 field
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title_auth	JWST's PEARLS: Transients in the MACS J0416.1−2403 Field
abstract	With its unprecedented sensitivity and spatial resolution, the James Webb Space Telescope (JWST) has opened a new window for time-domain discoveries in the infrared. Here we report observations in the only field that has received four epochs (spanning 126 days) of JWST NIRCam observations in Cycle 1. This field is toward MACS J0416.1−2403, which is a rich galaxy cluster at redshift z = 0.4 and is one of the Hubble Frontier Fields. We have discovered 14 transients from these data. Twelve of these transients happened in three galaxies (with z = 0.94, 1.01, and 2.091) crossing a lensing caustic of the cluster, and these transients are highly magnified by gravitational lensing. These 12 transients are likely of a similar nature to those previously reported based on the Hubble Space Telescope (HST) data in this field, i.e., individual stars in the highly magnified arcs. However, these 12 could not have been found by HST because they were too red and too faint. The other two transients are associated with background galaxies ( z = 2.205 and 0.7093) that are only moderately magnified, and they are likely supernovae. They indicate a demagnified supernova surface density, when monitored at a time cadence of a few months to a ∼3–4 μ m survey limit of AB ∼28.5 mag, of ∼0.5 arcmin ^−2 integrated to z ≈ 2. This survey depth is beyond the capability of HST but can be easily reached by JWST.
abstractGer	With its unprecedented sensitivity and spatial resolution, the James Webb Space Telescope (JWST) has opened a new window for time-domain discoveries in the infrared. Here we report observations in the only field that has received four epochs (spanning 126 days) of JWST NIRCam observations in Cycle 1. This field is toward MACS J0416.1−2403, which is a rich galaxy cluster at redshift z = 0.4 and is one of the Hubble Frontier Fields. We have discovered 14 transients from these data. Twelve of these transients happened in three galaxies (with z = 0.94, 1.01, and 2.091) crossing a lensing caustic of the cluster, and these transients are highly magnified by gravitational lensing. These 12 transients are likely of a similar nature to those previously reported based on the Hubble Space Telescope (HST) data in this field, i.e., individual stars in the highly magnified arcs. However, these 12 could not have been found by HST because they were too red and too faint. The other two transients are associated with background galaxies ( z = 2.205 and 0.7093) that are only moderately magnified, and they are likely supernovae. They indicate a demagnified supernova surface density, when monitored at a time cadence of a few months to a ∼3–4 μ m survey limit of AB ∼28.5 mag, of ∼0.5 arcmin ^−2 integrated to z ≈ 2. This survey depth is beyond the capability of HST but can be easily reached by JWST.
abstract_unstemmed	With its unprecedented sensitivity and spatial resolution, the James Webb Space Telescope (JWST) has opened a new window for time-domain discoveries in the infrared. Here we report observations in the only field that has received four epochs (spanning 126 days) of JWST NIRCam observations in Cycle 1. This field is toward MACS J0416.1−2403, which is a rich galaxy cluster at redshift z = 0.4 and is one of the Hubble Frontier Fields. We have discovered 14 transients from these data. Twelve of these transients happened in three galaxies (with z = 0.94, 1.01, and 2.091) crossing a lensing caustic of the cluster, and these transients are highly magnified by gravitational lensing. These 12 transients are likely of a similar nature to those previously reported based on the Hubble Space Telescope (HST) data in this field, i.e., individual stars in the highly magnified arcs. However, these 12 could not have been found by HST because they were too red and too faint. The other two transients are associated with background galaxies ( z = 2.205 and 0.7093) that are only moderately magnified, and they are likely supernovae. They indicate a demagnified supernova surface density, when monitored at a time cadence of a few months to a ∼3–4 μ m survey limit of AB ∼28.5 mag, of ∼0.5 arcmin ^−2 integrated to z ≈ 2. This survey depth is beyond the capability of HST but can be easily reached by JWST.
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title_short	JWST's PEARLS: Transients in the MACS J0416.1−2403 Field
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JWST's PEARLS: Transients in the MACS J0416.1−2403 Field

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