2019PASP..131g8001G


Query : 2019PASP..131g8001G

2019PASP..131g8001G - Publ. Astron. Soc. Pac., 131, part no 7, 8001-78001 (2019/July-0)

The Zwicky Transient Facility: science objectives.

GRAHAM M.J., KULKARNI S.R., BELLM E.C., ADAMS S.M., BARBARINO C., BLAGORODNOVA N., BODEWITS D., BOLIN B., BRADY P.R., CENKO S.B., CHANG C.-K., COUGHLIN M.W., DE K., EADIE G., FARNHAM T.L., FEINDT U., FRANCKOWIAK A., FREMLING C., GEZARI S., GHOSH S., GOLDSTEIN D.A., GOLKHOU V.Z., GOOBAR A., HO A.Y.Q., HUPPENKOTHEN D., IVEZIC Z., JONES R.L., JURIC M., KAPLAN D.L., KASLIWAL M.M., KELLEY M.S.P., KUPFER T., LEE C.-D., LIN H.W., LUNNAN R., MAHABAL A.A., MILLER A.A., NGEOW C.-C., NUGENT P., OFEK E.O., PRINCE T.A., RAUCH L., VAN ROESTEL J., SCHULZE S., SINGER L.P., SOLLERMAN J., TADDIA F., YAN L., YE Q.-Z., YU P.-C., BARLOW T., BAUER J., BECK R., BELICKI J., BISWAS R., BRINNEL V., BROOKE T., BUE B., BULLA M., BURRUSS R., CONNOLLY A., CROMER J., CUNNINGHAM V., DEKANY R., DELACROIX A., DESAI V., DUEV D.A., FEENEY M., FLYNN D., FREDERICK S., GAL-YAM A., GIOMI M., GROOM S., HACOPIANS E., HALE D., HELOU G., HENNING J., HOVER D., HILLENBRAND L.A., HOWELL J., HUNG T., IMEL D., IP W.-H., JACKSON E., KASPI S., KAYE S., KOWALSKI M., KRAMER E., KUHN M., LANDRY W., LAHER R.R., MAO P., MASCI F.J., MONKEWITZ S., MURPHY P., NORDIN J., PATTERSON M.T., PENPRASE B., PORTER M., REBBAPRAGADA U., REILEY D., RIDDLE R., RIGAULT M., RODRIGUEZ H., RUSHOLME B., VAN SANTEN J., SHUPE D.L., SMITH R.M., SOUMAGNAC M.T., STEIN R., SURACE J., SZKODY P., TEREK S., VAN SISTINE A., VAN VELZEN S., VESTRAND W.T., WALTERS R., WARD C., ZHANG C. and ZOLKOWER J.

Abstract (from CDS):

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 deg2 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.

Abstract Copyright: © 2019. The Astronomical Society of the Pacific.

Journal keyword(s):

Simbad objects: 21

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Number of rows : 21
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 SN 2011kn SN* 00 34 13.25 +02 48 31.4           SNIc 27 0
2 SN 2005gl SN* 00 49 50.02 +32 16 56.8       17.0   SNIIn 162 2
3 SN 2015fn SN* 02 30 20.05 +37 14 06.7           SNIc 52 0
4 SN 2005ek SN* 03 05 48.96 +36 46 10.6     17.5     SNIc: 76 1
5 SN 2006aj SN* 03 21 39.670 +16 52 02.27 17.96 19.11 17.40     SNIc-BL 1007 1
6 SN 2010X SN* 04 48 27.90 +73 28 14.8           SNIc 85 1
7 PMN J0509+0541 BLL 05 09 25.9644373872 +05 41 35.333820420 15.32 14.95 14.78 15.12   ~ 589 2
8 SN 1987A SN* 05 35 27.98840 -69 16 11.1134           SNIIpec 5203 2
9 PTF 11agg SN* 08 22 17.195 +21 37 38.26           ~ 31 0
10 SN 2010jl SN* 09 42 53.33 +09 29 41.8           SNIIn 350 1
11 SN 1988Z SN* 10 51 50.10 +16 00 00.5   16.8       SNIIn 385 1
12 SN 1998S SN* 11 46 06.1 +47 28 55     12.2     SNIIn 517 1
13 iPTF 16asu SN* 12 59 09.28 +13 48 09.2           SLSN-I 49 0
14 GrW 170817 GWE 13 09 48.0850 -23 22 53.343           ~ 2683 0
15 PTF 12glz SN* 15 54 53.04 +03 32 07.5           SNIIn 13 0
16 PSST 16cgx SN? 16 01 18.60 +09 51 53.1           ~ 4 0
17 SN 2018cow SN* 16 16 00.254 +22 16 05.10           SNIb 305 0
18 SN 2010mc SN* 17 21 30.68 +48 07 47.4           SNIIn 101 1
19 SN 1998bw SN* 19 35 03.17 -52 50 46.1   14.09       SNIc 1928 2
20 SN 2016geu SN* 21 04 15.86 -06 20 24.5           SNIa 78 0
21 SN 2014ft SN* 23 33 27.95 +33 38 46.1           SNIc 58 0

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