Hello, I am now learning the lsst pipeline, I have installed two verions: w_2021_48 and w_2021_33 cause the tutorial series were developed using the w_2021_33 version. At the very begining of the tutorial, Getting started tutorial part 2: calibrating single frames with Pipeline Tasks , when I execut…

It was pointed out to me that the change in the query-data-ids results was a known issue, and I just didn’t recognize that it was what you had run into (despite being the person responsible for the change). In short, the old behavior with w_2021_33 was incorrect, because you didn’t pass the dimensi…

[image] Yuanyu: /home/yu/butler/daf_butler/tests/.tests/pytest-daf_butler.xml.failed You have to look in there to see the failure. If you are running scons locally you have to make sure you use setup -k -r . or something similar so that EUPS knows you are wanting to run the tests on the loca…

Thank you! The comannd work! butler query-datasets SMALL_HSC raw --collections HSC/RC2/defaults Here are part of the result: (lsst-scipipe-0.7.0) [yu@localhost rc2_subset]$ butler query-datasets SMALL_HSC raw --collections HSC/RC2/defaults type run id …

I have run the whole LSST and HSC pipeline now, since my teacher gives me a mission to develop a pipeline for a new observatory(not the whole pipeline, only the very beginning include removing instrumental signatures with dark, bias and flat field and then do photometric and astrometric ). like HSC’…

[image] Yuanyu: Where should I change? You need to create an “obs” package describing your instrument. This is a good place to start: How to create a new LSST obs package — LSST Science Pipelines

I have a question, it may be kinda stupid, I want to know how LSST’s pipeline do astrometry,and I want to read and modify these codes, and finally use them to do astrometry for other observatory’s images, and I follow the Command editting (lsst-scipipe-0.7.0) [yu@localhost astrom]$ which singleFr…

I am now reading the website you give me: How to create a new LSST obs package — LSST Science Pipelines . But I didn’t know how to Creating a MetadataTranslator named ExampleTranslator which should be imported later on from astro_metadata_translator import ExampleTranslator by reading the Metadata…

ExampleTranslator is a placeholder for whatever translator you write – it is not a translator that is available to use as an example. For your instrument metadata translator you can either write a new package, send a pull request to GitHub - lsst/astro_metadata_translator: Observation metadata hand…

Thank you! You and other people really help me a lot! And your detailed documents about pipeline are pretty useful! I am a postgraduate student new to astronomy, and I am working on WFST in China.

How do you solve this ValueError problem “Labels {‘TE4’, ‘nsrcMeasVisit’, ‘TE3’} were not found in the declared pipeline” ? I faced this, too.

Problems using version w_2021_48 and w_2021_33

Support

ktl (K-T Lim) December 20, 2021, 7:03pm 11

(Answer posted in original topic.)

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Problems using version w_2021_48 and w_2021_33

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