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Onoddil opened this issue
Jun 25, 2020
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O1Understanding the effects of crowding on LSST astrometryO2Using that understanding to create a model of the astrometric uncertaintiesO3Combining model w/ photometric information to provide cross-matches between LSST & other catalogues
Similar to the stretch goal detailed in #3, a stretch goal of this working package could be to produce an analogous paper from the software side of things (in e.g. JOSS), giving the end product a DOI number and a citeable reference. This would be of benefit to the LUSC, allowing for the tracking of the number of users of the resulting data products.
The text was updated successfully, but these errors were encountered:
Onoddil
added
O1
Understanding the effects of crowding on LSST astrometry
O2
Using that understanding to create a model of the astrometric uncertainties
O3
Combining model w/ photometric information to provide cross-matches between LSST & other catalogues
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Jun 25, 2020
Onoddil
changed the title
D3.11.4.1.B: Software paper describing the code implementing the new cross-match algorithms
D3.11.4.1.C: Software paper describing the code implementing the new cross-match algorithms
Jul 8, 2020
Onoddil
changed the title
D3.11.4.1.C: Software paper describing the code implementing the new cross-match algorithms
D3.11.4.1.B: Software paper describing the code implementing the new cross-match algorithms
Sep 7, 2020
Onoddil
changed the title
D3.11.4.1.B: Software paper describing the code implementing the new cross-match algorithms
MS027.2: Software paper describing the code implementing the new cross-match algorithms
May 17, 2021
Onoddil
changed the title
MS027.2: Software paper describing the code implementing the new cross-match algorithms
27.2: Software paper describing the code implementing the new cross-match algorithms
Nov 28, 2022
Onoddil
changed the title
27.2: Software paper describing the code implementing the new cross-match algorithms
P2: Software paper describing the code implementing the new cross-match algorithms
Nov 28, 2022
O1Understanding the effects of crowding on LSST astrometryO2Using that understanding to create a model of the astrometric uncertaintiesO3Combining model w/ photometric information to provide cross-matches between LSST & other catalogues
Similar to the stretch goal detailed in #3, a stretch goal of this working package could be to produce an analogous paper from the software side of things (in e.g. JOSS), giving the end product a DOI number and a citeable reference. This would be of benefit to the LUSC, allowing for the tracking of the number of users of the resulting data products.
The text was updated successfully, but these errors were encountered: