SN 2022qmx , the SIMBAD biblio

SN 2022qmx , the SIMBAD biblio (20 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST10:16:24


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Title First 3 Authors
2023ApJ...948..115P 2247 T   A S   X C       49 3 4 LensWatch. I. Resolved HST Observations and Constraints on the Strongly Lensed Type Ia
Supernova 2022qmx (“
SN Zwicky”).
PIEREL J.D.R., ARENDSE N., ERTL S., et al.
2023ApJ...952...10S 87           X         2 8 1 Retrospective Search for Strongly Lensed Supernovae in the DESI Legacy Imaging Surveys. SHEU W., HUANG X., CIKOTA A., et al.
2023NatAs...7.1098G 1332 T   A S   X C       28 4 ~ Uncovering a population of gravitational lens galaxies with magnified standard candle
SN Zwicky.
GOOBAR A., JOHANSSON J., SCHULZE S., et al.
2023MNRAS.526.4296S 1288 T   A S   X C F     26 8 ~ Lensed Type Ia supernovae in light of
SN Zwicky and iPTF16geu.
SAINZ DE MURIETA A., COLLETT T.E., MAGEE M.R., et al.
2024ApJ...961..171F 45           X         1 10 ~ The JWST Discovery of the Triply Imaged Type Ia “Supernova H0pe” and Observations of the Galaxy Cluster PLCK G165.7+67.0. FRYE B.L., PASCALE M., PIEREL J., et al.
2024MNRAS.530.3942H 134           X         3 11 ~ GAUSSN: Bayesian time-delay estimation for strongly lensed supernovae. HAYES E.E., THORP S., MANDEL K.S., et al.
2024ApJ...967...50P 45           X         1 5 ~ JWST Photometric Time-delay and Magnification Measurements for the Triply Imaged Type Ia “SN H0pe” at z = 1.78. PIEREL J.D.R., FRYE B.L., PASCALE M., et al.
2024MNRAS.531.3509A 134           X         3 8 ~ Detecting strongly lensed type Ia supernovae with LSST. ARENDSE N., DHAWAN S., SAGUES CARRACEDO A., et al.
2024MNRAS.531.4349W 45           X         1 2 ~ How to break the mass sheet degeneracy with the light curves of microlensed Type Ia supernovae. WEISENBACH L., COLLETT T., SAINZ DE MURIETA A., et al.
2024ApJ...970..102C 90           X         2 25 ~ JWST Spectroscopy of SN H0pe: Classification and Time Delays of a Triply Imaged Type Ia Supernova at z = 1.78. CHEN W., KELLY P.L., FRYE B.L., et al.
2024A&A...689A.192D 90           X         2 10 ~ Forecast of strongly lensed supernovae rates in the China Space Station Telescope surveys. DONG J., SHU Y., LI G., et al.
2024MNRAS.535.2523S 134           X C       2 4 ~ Find the haystacks, then look for needles: the rate of strongly lensed supernovae in galaxy-galaxy strong gravitational lenses. SAINZ DE MURIETA A., COLLETT T.E., MAGEE M.R., et al.
2024MNRAS.535.2939D 45           X         1 12 ~ Spectroscopic analysis of the strongly lensed SN Encore: constraints on cosmic evolution of Type Ia supernovae. DHAWAN S., PIEREL J.D.R., GU M., et al.
2024A&A...692A.132H 45           X         1 6 ~ HOLISMOKES XII. Time-delay measurements of strongly lensed Type Ia supernovae using a long short-term memory network. HUBER S. and SUYU S.H.
2025ApJ...980..172L 1661 T   A S   X C       33 8 ~ LensWatch. II. Improved Photometry and Time-delay Constraints on the Strongly Lensed Type Ia
Supernova 2022qmx (“
SN Zwicky”) with Hubble Space Telescope Template Observations.
LARISON C., PIEREL J.D.R., NEWMAN M.J.B., et al.
2025A&A...697A.146B 140           X         3 75 ~ Cluster-lensed supernova yields from the Vera C. Rubin Observatory and Nancy Grace Roman Space Telescope. BRONIKOWSKI M., PETRUSHEVSKA T., PIEREL J.D.R., et al.
2025A&A...698A.266K 47           X         1 10 ~ Detection of unresolved strongly lensed supernovae with the 7-Dimensional Telescope. KHALOUEI E., SHAFIELOO A., KIM A.G., et al.
2025ApJ...994..117S 280           X C       5 2 ~ ML-driven Strong Lens Discoveries: Down to θE$\,\sim \,0\mathop{.}\limits^{\unicode{x02033}}03$ and Mhalo < 1011M⊙. SILVER E., WANG R., HUANG X., et al.
2025ApJ...995L..17J 47           X         1 9 ~ Discovery of SN 2025wny: A Strongly Gravitationally Lensed Superluminous Supernova at z = 2.01. JOHANSSON J., PERLEY D.A., GOOBAR A., et al.
2026ApJ...998..219P 50           X         1 7 ~ Cosmology with Supernova Encore in the Strong Lensing Cluster MACS J0138-2155: Time Delays and Hubble Constant Measurement. PIEREL J.D.R., HAYES E.E., MILLON M., et al.

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