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physlitetoopendata
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for-research/limitations/Limitations.ipynb

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"- Some signals/variations/systematics are not publicly released: if you need a specific sample, you can request it.\n",
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"- Producing large bespoke MC yourself is possible but discouraged, as it is resource-heavy, and easy to mismatch conditions.\n",
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"\n",
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"Regarding the first point, we can explore the GRL and filter data with measured in good runs and good lumiblocks. We are going to do it with proton-proton collisions data, but this also applies to heavy ion data."
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"Regarding the first point, we can explore the GRL and filter data with measured in good runs and good lumiblocks. We are going to do it with proton-proton collisions data, but this also applies to heavy ion data. "
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"id": "26df10da",
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"metadata": {},
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"source": [
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"The GRL are publicly available [here](cern.ch). There are two files for the proton-proton data corresponding to 2015 and 2016 runs, and one for the HI collisions. They are saved in .xml format. The data for each run with its LB's looks something like this:\n",
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"The GRL are publicly available [here](https://github.com/atlas-outreach-data-tools/notebooks-collection-opendata/tree/master/for-research/limitations/). There are two files for the proton-proton data corresponding to 2015 and 2016 runs, and one for the HI minimum bias stream from 2015. They are saved in .xml format. The data for each run with its LB's looks something like this:\n",
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"```xml\n",
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"<LumiBlockCollection>\n",
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"<Run>276262</Run>\n",
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"id": "53335bc5",
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"metadata": {},
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"source": [
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"And just like that, we checked that the quality of the dataset is suitable for physics analysis!"
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"And just like that, we checked that the quality of the dataset is suitable for physics analysis!\n",
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"\n",
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"It's worth noting that our [PHYSLITEtoOpenData](https://gitlab.cern.ch/atlas-outreach-data-tools/physlitetoopendata) ntuple maker filters out events that aren't included in a GRL, so you don't need to do this yourself if you are using the framework."
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