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ZENODO
Dataset . 2024
License: CC BY
Data sources: ZENODO
ZENODO
Dataset . 2024
License: CC BY
Data sources: Datacite
ZENODO
Dataset . 2024
License: CC BY
Data sources: Datacite
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Data products for Unresolved lensed SNe Ia in LSST (arxiv: 2404.15389)

Authors: Bag, Satadru;

Data products for Unresolved lensed SNe Ia in LSST (arxiv: 2404.15389)

Abstract

This data release is a part of arxiv 2404.15389. If needed, the ipython notebooks to analyse these datasets are availble at https://github.com/deltasata/Unresolved_LSNeIa_in_LSST There are two zip files stemming from two directories. 1. unresolved_catalog: contains the catalogs of lensed type-Ia supernovae (LSNe Ia) -- all and unresolved ones, separately. The notebook at the following path can provides statistics of the unresolved systems (please place the notebook in the same directory).https://github.com/deltasata/Unresolved_LSNeIa_in_LSST/tree/main/unresolved_stat There are two subdirectories: (i) catalog data: contains two catalogs - one listing all LSNe Ia expected over 10 effective years of LSST observations, and another specifically detailing the unresolved systems. See the "unresolved_catalog/catalog data/read_me.txt" for more details. There is also a subdirectory called "down_sampled_data" which contains details of the downsampled unresolved LSNe Ia systems. It is needed for running the ipython notebook.(ii) save_micro_mag_res: needed for running the ipython notebook. 2. build_blended_lc: contains necessary data files to create blended light curves for the unresolved systems. The subdirectory, "ML_downsampled_data" contains microlensed light curves for the downsampled unresolved LSNeIa. The file "Good_cadence_systems_fiveSigmaDepth_riyz.pkl" contains multi-band cadence distributions from the LSST baseline3.2 observing strategy.The required codes are availble at:https://github.com/deltasata/Unresolved_LSNeIa_in_LSST/tree/main/build_blended_lcplease put all the codes from the above in the same directory (build_blended_lc). References: Bag, S. et al 2024, arxiv:2404.15389 Oguri, M. & Marshall, P. J. 2010, MNRAS, 405, 2579 Oguri, M. 2018, MNRAS, 480, 3842

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
0
Average
Average
Average