Published October 3, 2020
| Version 1
Dataset
Open
BPASS Stellar Models in DataFrames
Contributors
Research groups:
- 1. University of Auckland
- 2. University of Warwick
Description
This data set is made of 26 binary files (.pckl) that contain pandas DataFrames compiling all the BPASS stellar models for the fiducial IMF (img135_300 - see BPASS manual for more info or contact hfstevance@gmail or @sydonahi on Twitter).
If you end up using this data set please also cite hoki - which was used to create these data.
The BibTex is as follows.
@ARTICLE{2020JOSS....5.1987S, author = {{Stevance}, Heloise and {Eldridge}, J. and {Stanway}, Elizabeth}, title = "{Hoki: Making BPASS accessible through Python}", journal = {The Journal of Open Source Software}, keywords = {Python, galaxies, Batchfile, SED, astronomy, binary stars, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Astrophysics of Galaxies, Astrophysics - Instrumentation and Methods for Astrophysics}, year = "2020", month = "Jan", volume = {5}, number = {45}, eid = {1987}, pages = {1987}, doi = {10.21105/joss.01987}, archivePrefix = {arXiv}, eprint = {2001.11069}, primaryClass = {astro-ph.SR}, adsurl = {https://ui.adsabs.harvard.edu/abs/2020JOSS....5.1987S}, adsnote = {Provided by the SAO/NASA Astrophysics Data System} }
Files
Files
(29.6 GB)
Name | Size | Download all |
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md5:64e942bb2c5f9f844f12508946af6bd4
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2.2 GB | Download |
md5:787d8cbdca4c40e8668fe4d9dfd4ef2c
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188.2 MB | Download |
md5:94f2db8ddf3535ab5ea41014233adfc3
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2.3 GB | Download |
md5:5edb3bea6912ff0d1410b6dc3b04b266
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180.7 MB | Download |
md5:4426a6651a5e62f7fcecf097ae24e2f1
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2.4 GB | Download |
md5:b4b7fc939759926f2f40bceb907635fb
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204.4 MB | Download |
md5:486ac2f855b722a6c8512d53aed5bd31
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2.4 GB | Download |
md5:6be7e6d4466f659e63fac67f60b1eb21
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190.8 MB | Download |
md5:bae8983fbb195788e2c330488d19114d
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2.5 GB | Download |
md5:cce24041b89abdd501e62c674e63eb8e
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187.9 MB | Download |
md5:cfacf907400793e7fd413da00dfc8b9f
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2.3 GB | Download |
md5:4a95aa166622c7ee66cbb256ec2f809f
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191.7 MB | Download |
md5:c29bf457e607a77d27d7bd45e0f679e2
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1.9 GB | Download |
md5:0da147887401176db628d4361bfbf638
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236.1 MB | Download |
md5:aaeb5aaa6e1e94ebb1c08f9192375ca0
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2.0 GB | Download |
md5:4afb3f2ce9e0947d6d17e94daa693ff0
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240.9 MB | Download |
md5:6d38f068da860ee46a8475472870d726
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2.1 GB | Download |
md5:eb40d09e58c64690241d441342ff756d
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201.2 MB | Download |
md5:55c1b77da2d2623a085d1fa52d1ae45f
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1.8 GB | Download |
md5:735300d2ee6512ac9680ee0e0f9cd557
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271.5 MB | Download |
md5:22a03d237116cc5e0a7d8bdb496342df
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1.8 GB | Download |
md5:b9c49c45d31e915cb05161dd1cc22f71
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285.6 MB | Download |
md5:ba9822e703354708725b16c6f3d15764
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1.6 GB | Download |
md5:4a24ccd09e332249032d05a3b53f6553
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212.5 MB | Download |
md5:9f182c425a94f06e8c265bd50b4dd2cb
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1.7 GB | Download |
md5:4a8c760fa4c9a0f6c30ece35ae0833a3
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175.2 MB | Download |
Additional details
Related works
- Cites
- Journal article: https://joss.theoj.org/papers/10.21105/joss.01987 (URL)