Rubin 2020 Metrics Hackathon

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This metric hackathon will take place on August 6 and 7, right before the Rubin LSST PCW. The hackathon is organized to collaboratively take a final look at the existing MAF metrics to evaluate the effectiveness of Rubin LSST observing strategies to provide data that enables the pursuit of a specific science goal. This event will comply with the Rubin LSST PCW Code of Conduct: please read the Code of Conduct at https://project.lsst.org/meetings/rubin2020/resources/coc and answer the questions below to complete your registration. If you have any questions check out our website https://lsst-tvssc.github.io/metricshackathon2020/ or contact Rachel Street (rstreet@lgo.global) and Federica Bianco (fbianco@udel.edu)

Family name *

First name *

Preferred pronoun *

he/him/his

she/her/hers

they/them/theirs

Other:

Time zone from which you will participate *

Academic role *

Undergraduate Student

Graduate Student

Postdoc

Staff or Researcher

Faculty

Other:

Rubin affiliation (check all that apply) *

Science Collaboration - TVS

Science Collaboration - DESC

Science Collaboration - SSSC

Science Collaboration - SMWLV

Science Collaboration - ISSC

Science Collaboration - AGN

Science Collaboration - Galaxies

Science Collaboration - SLSC

Rubin Observatory - DM

Rubin Observatory - PST

LSST Corporation

Other:

Required

Metrics you are interested in *

Let us know if you re most interested in working on some kind of metrics. This does not imply a commitment to work on that kind of metrics: you will be able to choose what to work on during the hackathon.

Transient and variable metrics

Depth metrics

Footprint metrics

Other:

Required

Observing Strategy white papers

Please select all Opsim white papers you were involved in responding to the 2019 call for observing strategy proposals

A Big Sky Approach to Cadence Diplomacy

A Cadence to Reduce Aliasing in LSST

A Higher Cadence Subsurvey Located in the Galactic Plane

A near-Sun Solar System Twilight Survey with LSST

A Northern Ecliptic Survey for Solar System Science

A Smart and Colorful Cadence for the Wide-Fast Deep Survey

A strategy for LSST to unveil a population of kilonovae

Active Galaxy Science in the LSST Deep-Drilling Fields: Footprints, Cadence Requirements, and Total-Depth Requirements

Blazars and Fast Radio Bursts with LSST

Calibrating Milky Way Maps: An LSST Bright(ish) Star Survey

Characterizing Variable Stars in a Single Night with LSST

Continuous Cadence Acquisition of the LSST Deep Drilling Fields

Deep Drilling Fields for Solar System Science

Discovery of Strongly-lensed Gravitational Waves –Implications for the LSST Observing Strategy

Enabling Cosmological Synergies between the LSST and WFIRST High Latitude Survey

Enabling Deep All-Sky Searches of Outer Solar System Objects

Enhancing LSST Science with Euclid Synergy

Investigating the population of Galactic star formation regions and star clusters within a Wide-Fast-Deep Coverage of the Galactic Plane

Large Synoptic Survey Telescope White Paper; The Case for Matching U-band on Deep Drilling Fields

Leveraging Differential Chromatic Refraction in LSST

LSST Cadence Optimization White Paper in Support of Observations of Unresolved Tidal Stellar Streams in Galaxies beyond the Local Group

LSST Local Volume mini-survey

LSST Observations of WFIRST Deep Fields

LSST Target of Opportunity proposal for locating a core collapse supernova in our galaxy triggered by a neutrino supernova alert

Mapping the Periphery and Variability of the Magellanic Clouds

Maximizing the Joint Science Return of LSST and DESI

Mini-survey of the northern sky to Dec < +30

Optimizing the LSST Observing Strategy for Dark Energy Science: DESC Recommendations for the Deep Drilling Fields and other Special Programs

Optimizing the LSST Observing Strategy for Dark Energy Science: DESC Recommendations for the Wide-Fast-Deep Survey

Presto-Color: An LSST Cadence for Explosive Physics & Fast Transients

Searching for white dwarf transits with LSST

Simultaneous LSST and Euclid observations –advantages for Solar System Objects

Strong Lensing considerations for the LSST observing strategy

Target of Opportunity Observations of Gravitational Wave Events with LSST

TDEs with LSST

Testing of LSST AGN Selection Using Rolling Cadences

The Definitive Map of the Galactic bulge

The Diverse Science Return from a Wide-Area Survey of the Galactic Plane

The Effects of Filter Choice on Outer Solar System Science with LSST

The First Extragalactic Exoplanets — What We Gain From High Cadence Observations of the Small Magellanic Cloud?

The Gaia-LSST Synergy: resolved stellar populations in selected Local Group stellar systems

The Plane’s The Thing: The Case for Wide-Fast-Deep Coverage of the Galactic Plane and Bulge

Unique Science from a Coordinated LSST-WFIRST Survey of the Galactic Bulge

unVEil the darknesS of The gAlactic bulge (VESTALE)

Unveiling the Rich and Diverse Universe of Subsecond Astrophysics through LSST Star Trails

Young Stars and their Variability with LSST

Other:

Experience with metrics *

What is your experience with the MAF metrics concept and syntax?

I do not know what a MAF metric is

I wrote MAF metrics that have been integrated in the MAF contrib portfolio

If you have a GitHub account, please give us your GitHub handle

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