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new drp version 1.0.2
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ajmejia committed May 28, 2024
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45 changes: 23 additions & 22 deletions CHANGELOG.rst
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Expand Up @@ -6,35 +6,36 @@ Change Log

This document records the main changes to the drp code.

1.0.2dev (unrealeased)
-------------------
1.0.2 (28-05-2024)
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- Speed up tracing by skipping model evaluation
- Fixes bug with missing astrometry headers
- Some other minor bug fixes


1.0.1 (23-05-2024)
------------------

* Fixed minor bugs in thermal shifts reports, sky QA plots, fetching of metadata, drpall product and more
* Implemented cleaning of ancillary paths
* Serial runs are default now
- Fixed minor bugs in thermal shifts reports, sky QA plots, fetching of metadata, drpall product and more
- Implemented cleaning of ancillary paths
- Serial runs are default now

1.0.0 (22-05-2024)
------------------

* Retired the quick-reduction now all science reductions use drp run
* Integrated the calibration reductions with the drp
* Use of twilight flats to flatfield
* Remove the illumination gradient across the IFU in twilight exposures
* Detect and correct for the pixel shifts in raw frames
* Adjust the wavelength solutions to the sky lines in each frame
* Shift the traces to account for thermal motions in the spectrographs
* Implemented cosmic ray rejection
* Better pixel flats and bad pixel masks
* Subtract the scattered light for all reductions
* Better sky subtraction by separating sky continuum from sky lines
* Astrometry in the slitmap for each fiber, also guider astrometry in headers
* Have smaller calibration frames
* Provide new products: lvmFrame, lvmFFrame, lvmCFrame, lvmSFrame, lvmRSS
* A lot of bug fixes and small improvements
- Retired the quick-reduction now all science reductions use drp run
- Integrated the calibration reductions with the drp
- Use of twilight flats to flatfield
- Remove the illumination gradient across the IFU in twilight exposures
- Detect and correct for the pixel shifts in raw frames
- Adjust the wavelength solutions to the sky lines in each frame
- Shift the traces to account for thermal motions in the spectrographs
- Implemented cosmic ray rejection
- Better pixel flats and bad pixel masks
- Subtract the scattered light for all reductions
- Better sky subtraction by separating sky continuum from sky lines
- Astrometry in the slitmap for each fiber, also guider astrometry in headers
- Have smaller calibration frames
- Provide new products: lvmFrame, lvmFFrame, lvmCFrame, lvmSFrame, lvmRSS
- A lot of bug fixes and small improvements

0.1.1 (11-08-2023)
------------------
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2 changes: 1 addition & 1 deletion setup.cfg
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[metadata]
name = lvmdrp
version = 1.0.2dev
version = 1.0.2
author = Alfredo Mejia-Narvaez
author_email = [email protected]
description = SDSSV-LVM Data Reduction Pipeline
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