LSST Project and Community Workshop 2018 • Tucson • August 13 - 17
An Introduction to Alert Follow-up Networks
Bryan Miller
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An Introduction to Alert Follow-up Networks Bryan Miller 1 LSST - - PowerPoint PPT Presentation
An Introduction to Alert Follow-up Networks Bryan Miller 1 LSST Project and Community Workshop 2018 Tucson August 13 - 17 Why all the fuss? In operation LSST will generate ~10 7 transient alerts per night! CANDELS
LSST Project and Community Workshop 2018 • Tucson • August 13 - 17
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LSST Project and Community Workshop 2018 • Tucson • August 13 - 17
2 CANDELS (http://www.spacetelescope.org/images/heic1306d/) 104 alerts every ~2 min
Science teams must select interesting targets. Observatories must prepare for Order(10-100) triggers/night/tel
LSST Project and Community Workshop 2018 • Tucson • August 13 - 17
At Gemini, ToOs make up about 20-25%
scheduling process and observers
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At CTIO/SOAR, ToOs interrupt visitor nights
disruptive to standard programs
LSST Project and Community Workshop 2018 • Tucson • August 13 - 17
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Talk by Soraisam on ANTARES. Talk by Bianco ZTF example: talk by Ridgway
LSST Project and Community Workshop 2018 • Tucson • August 13 - 17
Scheduling needs to be automatic, update frequently or as new
Targets assigned to nodes based on site conditions, target visibility, requested resource, etc.
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LSST Project and Community Workshop 2018 • Tucson • August 13 - 17
21 robotic telescopes: 0.4m, 1m, 2m Imaging and spectroscopy (on 1m and 2m) Both hemispheres and nearly complete longitudinal coverage
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LSST Project and Community Workshop 2018 • Tucson • August 13 - 17
Rachel Street (LCOgt, PS) Bryan Miller (Gemini, PS) Stephen Ridgway (NOAO, PS) Cesar Briceno (NOAO/SOAR) Andy Adamson (Gemini) John Blakeslee (Gemini) Adam Bolton (NOAO) Bob Blum (NOAO/LSST) Todd Boroson (LCOgt) Jay Elias (SOAR) Steve Heathcote (NOAO) Catherine Merrill (NOAO) Joanna Thomas-Osip (Gemini)
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LSST Project and Community Workshop 2018 • Tucson • August 13 - 17
1. Develop interfaces (APIs) a. Receive requests from TOMs b. Send schedule to telescopes c. Receive status 2. Incorporate SOAR into LCOgt network, execute observations on dedicated nights 3. Coordinate data pipelining and archiving efforts 4. Incorporate Gemini, modify scheduler to handle queue 5. Be ready to incorporate other facilities (Blanco, etc)
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LSST Project and Community Workshop 2018 • Tucson • August 13 - 17
Automating Goodman spectrograph
Modifying LCOgt scheduler Will develop interfaces to accept a schedule and create scripts for taking observations. Tests in late 2019
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LSST Project and Community Workshop 2018 • Tucson • August 13 - 17
Gemini has developed a pure python image reduction package (2019) SOAR and Gemini are collaborating on spectroscopy reduction in python starting in 2018 New Gemini instruments come with reduction tools that work in our pipeline environment (DRAGONS). Automated processing is a goal for the LSST era
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LSST Project and Community Workshop 2018 • Tucson • August 13 - 17
Current weaknesses:
plans as conditions change.
cadences (eg. observe every N days, logarithmic cadences)
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LSST Project and Community Workshop 2018 • Tucson • August 13 - 17
Rethink system from first principles. New UIs for ease of use. AEON APIs for search, status, and triggering. Automated scheduling built on LCOgt adapts to ToOs and changing conditions. Part of AEON in ~2020+
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See Oct 2017 Gemini Focus, pg. 20
LSST Project and Community Workshop 2018 • Tucson • August 13 - 17
▪ Allocates time on all network resources ▪ Avoids multiple jeopardy from different TACs
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LSST Project and Community Workshop 2018 • Tucson • August 13 - 17
NOAO/SOAR/Gemini/LCOgt are developing an instance of an alert follow-up network that includes:
There are many implications for how we will use or the network and facilities. We want your feedback so that we can develop a system that works for everyone and delivers the best science.
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LSST Project and Community Workshop 2018 • Tucson • August 13 - 17
Goals:
from first principles
much easier
not possible in the current code
and scalable
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See Oct 2017 Gemini Focus, pg. 20
LSST Project and Community Workshop 2018 • Tucson • August 13 - 17 16
Task-specific but consistent UIs ⇒ lower learning curve Calibration steps and observations automatically added, configs linked Physical conditions on target (FWHM) instead of conditions bins
LSST Project and Community Workshop 2018 • Tucson • August 13 - 17
Include tools for visibilities, planning, etc
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Programmatic access (eg. APIs for scripts) for search, full control, and access to services (ITCs, AGS).