학술논문

The Zwicky Transient Facility: Science Objectives
Document Type
Report
Author
Matthew J. GrahamS. R. KulkarniEric C. BellmScott M. AdamsCristina BarbarinoNadejda BlagorodnovaDennis BodewitsBryce BolinPatrick R. BradyS. Bradley CenkoChan-Kao ChangMichael W. CoughlinKishalay DeGwendolyn EadieTony L. FarnhamUlrich FeindtAnna FranckowiakChristoffer FremlingSuvi GezariShaon GhoshDaniel A. GoldsteinV. Zach GolkhouAriel GoobarAnna Y. Q. HoDaniela HuppenkothenŽeljko IvezićR. Lynne JonesMario JuricDavid L. KaplanMansi M. KasliwalMichael S. P. KelleyThomas KupferChien-De LeeHsing Wen LinRagnhild LunnanAshish A. MahabalAdam A. MillerChow-Choong NgeowPeter NugentEran O. OfekThomas A. PrinceLudwig RauchJan van RoestelSteve SchulzeLeo P. SingerJesper SollermanFrancesco TaddiaLin YanQuan-Zhi YePo-Chieh YuTom BarlowJames BauerRon BeckJustin BelickiRahul BiswasValery BrinnelTim BrookeBrian BueMattia BullaRick BurrussAndrew ConnollyJohn CromerVirginia CunninghamRichard DekanyAlex DelacroixVandana DesaiDmitry A. DuevMichael FeeneyDavid FlynnSara FrederickAvishay Gal-YamMatteo GiomiSteven GroomEugean HacopiansDavid HaleGeorge HelouJohn HenningDavid HoverLynne A. HillenbrandJustin HowellTiara HungDavid ImelWing-Huen IpEdward JacksonShai KaspiStephen KayeMarek KowalskiEmily KramerMichael KuhnWalter LandryRuss R. LaherPeter MaoFrank J. MasciSerge MonkewitzPatrick MurphyJakob NordinMaria T. PattersonBryan PenpraseMichael PorterUmaa RebbapragadaDan ReileyReed RiddleMickael Rigault3Hector RodriguezBen RusholmeJakob van SantenDavid L. ShupeRoger M. SmithMaayane T. SoumagnacRobert SteinJason SuracePaula SzkodyScott TerekAngela Van SistineSjoert van VelzenW. Thomas Vestrand3Richard WaltersCharlotte WardChaoran ZhangJeffry Zolkower
Source
Publications of the Astronomical Society of the Pacific. 131(1001)
Subject
Astronomy
Language
English
ISSN
1538-3873
0004-6280
Abstract
The Zwicky Transient Facility (ZTF), a public–private enterprise, is a new time-domain survey employing a dedicated camera on the Palomar 48-inch Schmidt telescope with a 47 sq. deg field of view and an 8 second readout time. It is well positioned in the development of time-domain astronomy, offering operations at 10% of the scale and style of the Large Synoptic Survey Telescope (LSST) with a single 1-m class survey telescope. The public surveys will cover the observable northern sky every three nights in g and r filters and the visible Galactic plane every night in g and r. Alerts generated by these surveys are sent in real time to brokers. A consortium of universities that provided funding (“partnership”) are undertaking several boutique surveys. The combination of these surveys producing one million alerts per night allows for exploration of transient and variable astrophysical phenomena brighter than r ~20.5 on timescales of minutes to years. We describe the primary science objectives driving ZTF, including the physics of supernovae and relativistic explosions, multi-messenger astrophysics, supernova cosmology, active galactic nuclei, and tidal disruption events, stellar variability, and solar system objects.