LensWatch. II. Improved Photometry and Time-delay Constraints on the Strongly Lensed Type Ia Supernova 2022qmx ("SN Zwicky") with Hubble Space Telescope Template Observations

被引:0
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作者
Larison, C. [1 ]
Pierel, J. D. R. [2 ]
Newman, M. J. B. [1 ]
Jha, S. W. [1 ]
Gilman, D. [3 ]
Hayes, E. E. [4 ]
Agrawal, A. [5 ]
Arendse, N. [6 ]
Birrer, S. [7 ]
Bronikowski, M. [8 ]
Chakrabarti, S. [9 ]
Della Costa, J. M. [10 ]
Coulter, D. A. [2 ]
Courbin, F. [11 ,12 ]
Dalrymple, K. A. [13 ]
Dhawan, S. [4 ]
Diego, J. M. [14 ]
Gall, C. [15 ]
Goobar, A. [6 ]
Hjorth, J. [15 ]
Huang, X. [16 ]
Johansson, J. [6 ]
Mao, S. [17 ]
Marques-Chaves, R. [18 ]
Mazzali, P. A. [19 ,20 ]
More, A. [21 ,22 ]
Moustakas, L. A. [23 ]
Perez-Fournon, I. [24 ,25 ]
Petrushevska, T. [8 ]
Poidevin, F. [25 ,26 ]
Rest, A. [2 ,13 ]
Shajib, A. J. [3 ,27 ]
Shirley, R. [28 ]
Strolger, L. G. [2 ]
Suyu, S. H. [20 ,29 ]
Treu, T. [30 ]
Zenati, Y. [2 ,13 ]
机构
[1] Rutgers State Univ, Dept Phys & Astron, 136 Frelinghuysen Rd, Piscataway, NJ 08854 USA
[2] Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21218 USA
[3] Univ Chicago, Dept Astron & Astrophys, Chicago, IL 60637 USA
[4] Univ Cambridge, Inst Astron, Kavli Inst Cosmol, Madingley Rd, Cambridge CB3 0HA, England
[5] Univ Illinois, Dept Astron, 1002 W Green St, Champaign, IL 61801 USA
[6] Stockholm Univ, Oskar Klein Ctr, Dept Phys, SE-10691 Stockholm, Sweden
[7] SUNY Stony Brook, Dept Phys & Astron, Stony Brook, NY 11794 USA
[8] Univ Nova Gorica, Ctr Astrophys & Cosmol, Vipavska 11c, Ajdovscina 5270, Slovenia
[9] Univ Alabama, Dept Phys & Astron, Huntsville, AL 35899 USA
[10] NSFs NOIRLab, 950 N Cherry Ave, Tucson, AZ 85719 USA
[11] Univ Barcelona, ICC UB Inst Ciencies Cosmos, Marti Franques 1, E-08028 Barcelona, Spain
[12] ICREA, Pg Lluis Co 23, E-08010 Barcelona, Spain
[13] Johns Hopkins Univ, William H Miller Dept Phys & Astron, 3400 North Charles St, Baltimore, MD 21218 USA
[14] Inst Fis Cantabria CSIC UC, Avda Castros s-n, Santander 39005, Spain
[15] Univ Copenhagen, Niels Bohr Inst, DARK, Jagtvej 155A, DK-2200 Copenhagen, Denmark
[16] Univ San Francisco, Dept Phys & Astron, San Francisco, CA 94117 USA
[17] Tsinghua Univ, Dept Astron, Beijing 100084, Peoples R China
[18] Univ Geneva, Dept Astron, 51 Chemin Pegasi, CH-1290 Versoix, Switzerland
[19] Liverpool John Moores Univ, Astrophys Res Inst, IC 2,Liverpool Sci Pk,146 Brownlow Hill, Liverpool L3 5RF, England
[20] Max Planck Inst Astrophys, Karl Schwarzschild Str 1, D-85748 Garching, Germany
[21] Interuniv Ctr Astron & Astrophys, Pune 411007, India
[22] Univ Tokyo, Kavli Inst Phys & Math Universe WPI, 5-1-5 Kashiwa, Chiba 2778583, Japan
[23] CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA 91109 USA
[24] Inst Astrofis Canarias, C Via Lactea S-N, E-38205 Tenerife, Spain
[25] Univ La Laguna, Dept Astrofis, E-38206 Tenerife, Spain
[26] Inst Astrofis Canarias, Via Lactea, Tenerife 38205, Spain
[27] Univ Chicago, Kavli Inst Cosmol Phys, Chicago, IL 60637 USA
[28] Max Planck Inst Extraterr Phys, Giessenbachstr 1, D-85748 Garching, Germany
[29] Tech Univ Munich, TUM Sch Nat Sci, Phys Dept, James Franck Str 1, Garching, Germany
[30] Univ Calif Los Angeles, Phys & Astron Dept, Los Angeles, CA 90095 USA
来源
ASTROPHYSICAL JOURNAL | 2025年 / 980卷 / 02期
基金
美国国家航空航天局; 美国国家科学基金会; 欧洲研究理事会;
关键词
DARK-MATTER; COSMOLOGICAL CONSTRAINTS; GRAVITATIONAL TELESCOPE; DISTANT SUPERNOVAE; COSMOGRAIL; GALAXIES; CONSTANT; PACKAGE; H0PE; MAGNIFICATION;
D O I
10.3847/1538-4357/ada776
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Strongly lensed supernovae (SNe) are a rare class of transient that can offer tight cosmological constraints that are complementary to methods from other astronomical events. We present a follow-up study of one recently discovered strongly lensed SN, the quadruply imaged type Ia SN 2022qmx (aka "SN Zwicky"), at z = 0.3544. We measure updated, template-subtracted photometry for SN Zwicky and derive improved time delays and magnifications. This is possible because SNe are transient, fading away after reaching their peak brightness. Specifically, we measure point-spread-function photometry for all four images of SN Zwicky in three Hubble Space Telescope WFC3/UVIS passbands (F475W, F625W, and F814W) and one WFC3/IR passband (F160W), with template images taken similar to 11 months after the epoch in which the SN images appear. We find consistency to within 2 sigma between lens-model-predicted time delays (less than or similar to 1 day) and measured time delays with HST colors (less than or similar to 2 days), including the uncertainty from chromatic microlensing that may arise from stars in the lensing galaxy. The standardizable nature of SNe Ia allows us to estimate absolute magnifications for the four images, with images A and C being elevated in magnification compared to lens model predictions by about 6 sigma and 3 sigma, respectively, confirming previous work. We show that millilensing or differential dust extinction is unable to explain these discrepancies, and we find evidence for the existence of microlensing in images A, C, and potentially D that may contribute to the anomalous magnification.
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页数:13
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