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Introduction
Save the date for the Rubin Observatory Project and Community Workshop! Rubin 2023 (also known as the PCW), is scheduled for August 7-11, 2023 in Tucson, AZ.
Those with ideas for future newsletter items should contact the LSST:UK Project Managers (George Beckett and Terry Sloanlusc_pm@mlist.is.ed.ac.uk), while everyone is encouraged to subscribe to the Rubin Observatory Digest for more general news from the US observatory team.
Update on efforts to create pipeline sky-subtraction that preserves low-surface-brightness flux
In December 2022, Aaron Watkins (lead of Work Package 3.7) spent two weeks at Princeton University, working directly with Rubin Data Management (DM) on sky-subtraction algorithms. From previous work done using simulated and real images, Watkins and DM have converged on a simple, easy-to-implement algorithm that is viable for preserving low-surface-brightness flux: aggressive masking of astrophysical sources accompanied by a simplistic sky model based on unmasked pixels. Kelvin (DM) and Watkins thus spent considerable time examining the existing Hyper Suprime-Cam pipeline sky-subtraction code to determine the feasibility of using an altered, LSB-flux-preserving version of it as the basis for the LSST pipeline sky-subtraction. They have determined this to be feasible and identified the parameters within the pipeline that need to be modified, from bin size used in creating different stages of the sky model, to the type of interpolation used across bins in reprojecting the sky models to the CCD frames. Watkins will therefore quantify the optimal set of such parameters via additional rounds of synthetic source injection, which he will then submit to DM as the quickest route to an LSB-flux-preserving sky-subtraction algorithm for LSST. In the meantime, to streamline future development, Kelvin and Watkins have cleaned up and updated the existing HSC sky-subtraction code substantially, including by creating more thorough and comprehensible documentation and by enabling the generation of new diagnostic images showing each step of the sky-model generation process.
In December 2022, Aaron Watkins (lead of Work Package 3.7) spent two weeks at Princeton University, working directly with Rubin Data Management (DM) on sky-subtraction algorithms. From previous work done using simulated and real images, Watkins and DM have converged on a simple, easy-to-implement algorithm that is viable for preserving low-surface-brightness flux: aggressive masking of astrophysical sources accompanied by a simplistic sky model based on unmasked pixels. Kelvin (DM) and Watkins thus spent considerable time examining the existing Hyper Suprime-Cam pipeline sky-subtraction code to determine the feasibility of using an altered, LSB-flux-preserving version of it as the basis for the LSST pipeline sky-subtraction. They have determined this to be feasible and identified the parameters within the pipeline that need to be modified, from bin size used in creating different stages of the sky model, to the type of interpolation used across bins in reprojecting the sky models to the CCD frames. Watkins will therefore quantify the optimal set of such parameters via additional rounds of synthetic source injection, which he will then submit to DM as the quickest route to an LSB-flux-preserving sky-subtraction algorithm for LSST. In the meantime, to streamline future development, Kelvin and Watkins have cleaned up and updated the existing HSC sky-subtraction code substantially, including by creating more thorough and comprehensible documentation and by enabling the generation of new diagnostic images showing each step of the sky-model generation process.
Creation of new Low-Surface-Brightness Coordination Group
Watkins, Mireia Montes (co-chair of the Low-Surface-Brightness Working Group within the Galaxies Science Collaboration) and Kaviraj have spearheaded the creation of a new Low-Surface-Brightness (LSB) Coordination Group. This is the first community-driven coordination group within the LSST ecosystem and has received strong support from the Project. While the initiative for its creation has come from the Galaxies Science Collaboration, the purpose of this group is provide a cross science collaboration forum to inform the pipeline efforts described above and prepare the community for LSB science in the coming years. Given that the discovery space of LSST is in the LSB regime, this coordination group will likely play a significant role in the LSST landscape as we ramp up to commissioning this year. The initial meeting of the coordination group was attended by 50 researchers from 5 science collaborations. The group will interact primarily via Slack, at meetings of the LSB Working Group within the Galaxies Science Collaboration and at dedicated sessions at LSST conferences like the Project and Community Workshop and the LSST@Europe meetings. It is currently co-chaired by Aaron Watkins and Mireia Montes.
Recent LSST:UK Science Centre outputs
The LSST:UK Science Centre has recently produced the following technical reports.
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Forthcoming meetings of interest
There are a number of meeting updates to report on this month. Please check-out the links below for more details.
The first announcement of the LSST@Europe 5 meeting has been made. The meeting will be held in Poreč, Croatia, during 25th--29th September 2023. Registration information is expected to be published by end of March 2023.
The dates have also been confirmed for the Rubin Project and Community Workshop 2023: it will be held on 7th--11th August in Tucson, Arizona. More details are expected in the coming weeks.
The IDAC coordinators (along with representatives from LSST:UK, LIneA, and the LINCC programme) are organising an IDAC workshop during 21st--22nd March 2023, entitled Supporting Computational Science with Rubin LSST. The workshop will be virtual and pre-signup is now available.
Other meetings of potential interest for the coming months include:
27th February – 3rd March: DESC Collaboration Meeting (virtual). Details to be published on DESC members website (login required).
24th - 28th July: DESC Collaboration Meeting (SLAC).
Members of the Consortium (not in receipt of travel funding through one of the Science Centre grants) may apply for travel support for meetings of this kind via the the LSST:UK Pool Travel Fund. Details are available at Forthcoming LSST-related Meetings .
Note that the current list of forthcoming meeting is always available on the Relevant Meetings page. You may also wish to check information held on the LSST organisation website LSST-organised events and the LSST Corporation website.
Announcements
If you have significant announcements that are directly relevant to LSST:UK and would like to share the announcement in a future newsletter, please contact the LSST:UK project managers.
Manda Banerji writes:
I have an opening in my group in Southampton for a research software scientist to work on one of the UK’s accepted in-kind software and dataset contributions to the Rubin LSST project. The project is delivering a pipeline for joint pixel processing of LSST and VISTA VIRCam imaging data and is in its second phase of funding. More details can be found here:
https://jobs.soton.ac.uk/Vacancy.aspx?ref=2152223WF
I would be grateful if you could please advertise this opportunity to any suitable candidates. We are particularly keen to attract those from under-represented groups in Physics who are typically severely under-represented in software/technical roles. Please do encourage anyone interested to get in touch with me directly to find out more about the role.
The application deadline for this post is Sunday, February 26th.