Phase 1 submission for cluster-scale lensed SN program with HST + JWST. 2092107672 Assigned ID: 7717 ----- Attempting Submission 1 (Thu Apr 16 22:17:35 GMT 2026) ----- Phase II submission for generic targets following our nominal observing plan. -1056160992 ----- Attempting Submission 1 (Tue Aug 18 15:50:32 GMT 2026) ----- Orbit planner was run to check that orbit was packed for each epoch. Actual exposure times/filters/instruments will change when fixed targets are found. The Visit Planner is not needed as these are generic targets. LensTrove: Unlocking the Cosmological Power of Cluster-lensed Supernovae The discovery rate of cluster-lensed supernovae (SNe) has exploded since the launch of JWST, opening a powerful new route to time-delay cosmography. In these systems, the measured delays between multiple SN images, combined with a model of the lensing cluster mass distribution, provide a direct geometrical probe of cosmic expansion. We propose coordinated HST+JWST ToO follow-up of three cosmologically useful cluster-lensed SNe in Cycle 34. This program will double the current cosmological sample of cluster-lensed SNe and enable a combined measurement of H0 with ~2.5% precision, sufficient to distinguish between the two ends of the Hubble tension at ~3 sigma. This result is comparable to that achieved from decades of monitoring lensed quasars but can be reached more efficiently with SNe and with reduced susceptibility to key systematics that hinder galaxy-scale systems. Cluster-lensed SNe therefore provide a uniquely powerful and independent probe for cosmology and of the potential systematics underlying current leading cosmological methods. This program will produce the comprehensive HST (27 orbits) + JWST (21.9 hours) dataset needed to enable the first statistically significant, sample-level test of the Hubble tension using only lensed SNe. For this phase II submission we are submitting three generic ToO targets following the nominal observing strategy of our proposal. This program is as follows: three epochs of imaging when the SN is brightest, following the quickest possible non-disruptive turnaround time and three additional epochs after it has begun to fade. These first three epochs nominally consist of one orbit each (the number of epochs and orbits assigned to each target are subject to change depending on the target properties, as specified in the proposal). For our nominal case, we split these orbits equally between F110W and F160W, although UVIS or other IR detectors may be used instead depending on the need. For the last three epochs, 1.5 orbits are assigned to F160W and 0.5 orbit to F110W. Again, we require flexibility in the assignment of these orbit, the filters and detector chosen, etc. Each epoch that required two orbits was separated into separate visits and then grouped within 1 orbit. PI Dr. Conor Larison is an expert in strongly lensed SN observations with space-based facilities, having worked on SN Zwicky, SN Encore, SN Ares, and SN Eos. co-PI Ana Acebron is an expert on strong lensing models in galaxy clusters and time-delay cosmography with lensed transients. co-PI Justin Pierel is an expert in strongly lensed SN observations with HST and JWST co-I Jose Diego. Expert on modeling gravitational lenses and on microlensing near caustics co-I Aadya Agrawal is an expert on Lensed SN lightcurve modeling and TD analysis. co-I Suhail Dhawan. Expert on time-delay estimation, lensed modelling and unlensed Type Ia supernova analyses. co-I Masamune Oguri. Expert on strong lens mass modeling. co-I Dr. David Coulter is an expert transient observer and software engineer, with experience in ground-based and space-based image reduction, photometry, and transient analysis, including electromagnetic follow-up of gravitational wave sources. He has worked on high-z transients and kilonovae, and in optimizing coordinated follow-up strategies. co-I Mateusz Bronikowski is an expert in strongly-lensed supernova yield predictions for telescopic surveys, and has received training on JWST data analysis for transient science. co-I Dr. Tanja Petrushevska is an expert on strongly-lensed supernova yield predictions for telescopic surveys and on tidal disruption events, and has received training on JWST data analysis for transient science. co-I Stefan Schuldt is an expert on strong lens mass modeling ranging from galaxy scale to cluster scale. co-I Frederick Poidevin is an expert on supernovae with experience in ground-based follow-up using photometry, spectroscopy and polarimetry, data analysis and time-delay estimations. co-I Leonidas Moustakas is an expert on strong lens modeling. co-I Armin Rest is an expert in transient science, in particular SN Ia cosmology, light echoes of historic SN, and exotic transients. His technical expertise lies in data reduction, image analysis, photometry, and their application to wide-field time-domain surveys. co-I Massimo Pascale is an expert on strong lens modeling and time-delay cosmography co-I Simon Birrer is an expert in lens modeling, software development and cosmographic inference. co-I Dr. Wenlei Chen is an expert on lens modeling and HST + JWST data analysis. co-I Erin Hayes is an expert on time-delay estimation for time-delay cosmography and SN Ia cosmology. co-I Nikhil Garuda is an expert in multi-band photometry, fitting SED models based on imaging and on imaging + spectroscopy, fitting and analyzing spatially-resolved SEDs. co-I Sherry Suyu is an expert on time-delay cosmography with lensed transients. co-I Anton Koekemoer has extensive observational expertise in building JWST imaging mosaics of strong lensing clusters and numerous other large extragalactic programs, and scientific expertise in high-redshift galaxies, clusters, transients, and AGN science. co-I Sangjun Cha is an expert in strong and weak lens modeling co-I Ashish Kumar Meena (ashishmeena766@gmail.com) has expertise in strong lens modeling and caustic-crossing events. co-Is Saurabh W.~Jha and Lindsey Kwok have expertise in observations of supernovae, including with JWST. co-I Claudio Grillo is an expert on strong lensing models in galaxy clusters for cosmological applications. co-I Giovanni Granata is an expert on strong lensing models and stellar kinematics in galaxy clusters co-I Patrick Kamieneski is an expert on gravitational lens modeling and in identifying candidates for time-delay cosmography. co-I Ismael Perez-Fournon is an expert in supernova discovery and classification, lensed supernovae and lensed galaxies, superluminous supernovae and space infrared surveys co-I Xiaosheng Huang is an expert in supernova spectroscopy and strong lens modeling co-I Gautham Narayan has expertise with real-time alerts from wide-field surveys, AI to identify lensed sources and anomalous objects, flux calibration, photometry and lightcurve fitting of supernovae, cosmology with type Ia supernovae. co-I Jens Hjorth, expert in JWST hi-z galaxies and Hubble constant determination. co-I Mike Engesser is an expert in image reduction and analysis with JWST, near- and mid-infrared detectors, as well as detecting transients using modern alignment, subtraction, source detection, and photometry techniques. co-I Dr. Melissa Shahbandeh is an expert in IR spectroscopy and observations of transients, as well as JWST data analysis. She is experienced with modeling dust evolution in SNe. She is the PI and co-I of many programs using both ground and space-based telescopes, and thus can support supplementary multiwavelength observations. co-I Dr. Sebastian Gomez is an expert on the study of exotic transients, particularly superluminous supernovae and tidal disruption events. He has experience leading programs on optical photometric and spectroscopic observations of transients from a wide array of telescopes including HST, Magellan, MMT, Gemini, and WHT. co-I Dr. Yossef Zenati is an expert on theory and simulation of transients, type Ia SNe and exotic SNe such as SESN. He is also a member of the few groups at the STScI. He will help with the simulation and interpretation of the data of these exotic SNe. co-I Dr. Jacob Jencson is an expert in transient science, particularly in infrared studies of obscured or dusty transients. He has worked on several transient searches, including ones with Spitzer and HST, and has experience in reduction/analysis of spectroscopic and imaging data. co-I Dr. Russell Ryan is an expert in space-based slitless spectral reduction co-I Dr. Qinan Wang is an expert in supernova photometry and spectroscopy with a focus on the rapid early features of SNe Ia and CCSNe. He has extensive experience on transients alert, coordinating follow-up with ground-based and space-based telescopes, data reduction and light curve fitting. co-I Dr. Lou Strolger is an expert in supernova rates, progenitor studies, and SN Ia cosmology. His technical expertise lies in data reduction and analysis, photometry, and spectroscopy. co-I Dr. Ori Fox is an expert in transient science and mid-IR observations of dust, in particular. He is a member of the JWST MIRI team and has built up significant experience working with JWST data, specifically NIRCam and MIRI imaging, as well as MIRI spectroscopy. co-I Dr. Egami is an expert in galaxy evolution and deep space-based surveys co-I Christa DeCoursey has lead the JADES high-z transient analysis co-I Dr. DerKacy has lead several papers of JWST observations of nearby SN Ia co-I Dr. Padilla Gonzalez is an expert in subtypes of SN Ia co-I Dr. Griggio is an expert in JWST astrometry and photometry co-I M. Karmen is an expert in TDEs at high redshifts. He is the PI of JWST DD 9356, a follow-up program following up high-redshift TDE candidates, and is PI of numerous ground-based follow-up programs for TDEs. He has extensive experience in photometric selection of TDEs, and in modeling their rates. co-I K. Shukawa is an expert in data reduction of both ground- and space-based telescopes, including difference imaging, high-precision photometry and astrometry. co-I Dr. Xiaolong Li is an expert in transient science, specializing in light echoes from SN and variable stars. His work focuses on developing data analysis tools to detect and characterize faint and extended transients in preparation for the Rubin LSST. co-I R Angulo is an expert in data reduction including difference imaging and in transient science, specifically on light echoes from supernovae and other transients. co-I Dr. Thomas Moore is an expert on the discovery and characterization of exotic transients, particularly unusual stripped-envelope supernovae. He has experience leading programs for UV-NIR spectrophotometric observations of transients using VLT, NTT, Gemini, Swift, and Pan-STARRS. co-I Dr. Matthew Siebert is an expert transient observer with specific expertise in UV/optical/NIR spectroscopy of SN Ia and their host galaxies. He has extensive experience coordinating space- and ground-based follow up observations, and has developed techniques for the interpretation of high-z transients observed with low-resolution spectroscopy. He has also developed data reduction pipelines for a variety of optical spectrographs. Stellar Physics and Stellar Types Galaxies 0 false false false false false false false true PRIMARY 21.9 true SUPPORTED STAR SUPERNOVA This target represents the nominal case for our follow-up program. Strongly lensed, cluster-scale SN at z > 1, with time delays > 20 days STAR SUPERNOVA This target represents the nominal case for our follow-up program. Strongly lensed, cluster-scale SN at z > 1, with time delays > 20 days STAR SUPERNOVA This target represents the nominal case for our follow-up program. 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