← Back to rubinobservatory.org

Survey Cadence Notes 2021

Authors

Title

Link

Abrams

Microlensing Discovery and CharacterizationEfficiency at Different Timescales

DocuShare

Andreoni

MaximizingSerendipitous Kilonova and Fast Transient Discovery

DocuShare

Anguita

LSST Strong Lensing Science Collaboration responseto the SurveyCadence Optimization Committee Call on Cadence

DocuShare

Assef

Type-1 Quasar Colors in the Context of Photometric Redshifts

DocuShare

Assef

Quasar Counts

DocuShare

Assef

Type-1 Quasar Variability in the Context of Photometric Redshifts

DocuShare

Bachelet

On the observational synergies between all-sky surveys for thecharacterization of microlensing events

DocuShare

Bellm

Give Me a Few Hours: Missing Timescales in Rubin Cadence Simulations

DocuShare

Blaineau

Microlensing towards the Magellanic Clouds:searching for long events

DocuShare

Bonito

Young stellar objects and their variability with Rubin Observatory LSST

DocuShare

Brandt

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

DocuShare

Buckley

Accreting Binaries

DocuShare

Carlin

A resolved census of dwarfsatellites around Local Volume galaxies

DocuShare

Clarkson

Saturation and Bright Objects

DocuShare

Clarkson

Bulge stellar populations with LSST

DocuShare

Cuillandre

Enhancing LSST Science withEuclidsynergyand a mini-survey of the northern sky to Dec<+30

DocuShare

D’Orazio

Double AGN: Binary-Lens Lighthouses in VRO’s 10-year Survey

DocuShare

Ferguson

The LSST Galaxies Science Collaboration Response to the Survey Cadence Optimization Committee Call

DocuShare

Frohmaier

The Time-Domain Extragalactic Survey Cadence Note

DocuShare

Gizis

Brown Dwarf Astrometry

DocuShare

Graham

WFD Photo-z

DocuShare

Graham

Supernova Science

DocuShare

Hernitschek

Cadence impacts on reliable classification of standard-candle variable stars

DocuShare

Hundertmark

Alerting transient phenomena in theGalactic Plane in time to coordinate follow-up

DocuShare

Jaimes

Milky Way Globular Clusters

DocuShare

Kovačević

Two metrics on AGN variability observables

DocuShare

Li

Anomaly Detection

DocuShare

Lochner

The LSST Dark Energy Science CollaborationCadence Note

DocuShare

Moniez

Detection of interstellar scintillation by highfrequency imaging of the LMC or SMC

DocuShare

Musella

Classical variable stars in different Galacticenvironments: pulsation behaviour recovery

DocuShare

Olsen

A census of dwarf satellites and substructure around the Magellanic Clouds

DocuShare

Prisinzano

Maximize volume and uniformitycoverage of Star Forming Regions in the Galactic Plane

DocuShare

Raiteri

BLAZAR VARIABILITY

DocuShare

Schwamb

Vera C. Rubin Observatory Legacy Survey of Spaceand Time (LSST) Solar System Science Collaboration (SSSC)

DocuShare

Street

LSST Survey Footprint in the Galactic Plane and Magellanic Clouds

DocuShare

Tisanić

Simulations of multiband Lomb-Scargle-derived variable star periods

DocuShare

van Velzen

Tidal Disruption Events

DocuShare

Yu

Non-Parametric Structure Function Metric

DocuShare

Yu

Differential Chromatic Refraction

DocuShare

 

Financial support for Rubin Observatory comes from the National Science Foundation (NSF) through Cooperative Agreement No. 1258333, the Department of Energy (DOE) Office of Science under Contract No. DE-AC02-76SF00515, and private funding raised by the LSST Corporation. The NSF-funded Rubin Observatory Project Office for construction was established as an operating center under management of the Association of Universities for Research in Astronomy (AURA).  The DOE-funded effort to build the Rubin Observatory LSST Camera (LSSTCam) is managed by the SLAC National Accelerator Laboratory (SLAC).
The National Science Foundation (NSF) is an independent federal agency created by Congress in 1950 to promote the progress of science. NSF supports basic research and people to create knowledge that transforms the future.
NSF and DOE will continue to support Rubin Observatory in its Operations phase. They will also provide support for scientific research with LSST data.   




Contact   |   We are Hiring

Admin Login

Back to Top