2009PASP..121.1334R


Query : 2009PASP..121.1334R

2009PASP..121.1334R - Publ. Astron. Soc. Pac., 121, 1334-1351 (2009/December-0)

Exploring the optical transient sky with the Palomar Transient Factory.

RAU A., KULKARNI S.R., LAW N.M., BLOOM J.S., CIARDI D., DJORGOVSKI G.S., FOX D.B., GAL-YAM A., GRILLMAIR C.C., KASLIWAL M.M., NUGENT P.E., OFEK E.O., QUIMBY R.M., REACH W.T., SHARA M., BILDSTEN L., CENKO S.B., DRAKE A.J., FILIPPENKO A.V., HELFAND D.J., HELOU G., HOWELL D.A., POZNANSKI D. and SULLIVAN M.

Abstract (from CDS):

The Palomar Transient Factory (PTF) is a wide-field experiment designed to investigate the optical transient and variable sky on time scales from minutes to years. PTF uses the CFH12k mosaic camera, with a field of view of and a plate scale of, mounted on the Palomar Observatory 48 inch Samuel Oschin Telescope. The PTF operation strategy is devised to probe the existing gaps in the transient phase space and to search for theoretically predicted, but not yet detected, phenomena, such as fallback supernovae, macronovae, .Ia supernovae, and the orphan afterglows of gamma-ray bursts. PTF will also discover many new members of known source classes, from cataclysmic variables in their various avatars to supernovae and active galactic nuclei, and will provide important insights into understanding galactic dynamics (through RR Lyrae stars) and the solar system (asteroids and near-Earth objects). The lessons that can be learned from PTF will be essential for the preparation of future large synoptic sky surveys like the Large Synoptic Survey Telescope. In this article we present the scientific motivation for PTF and describe in detail the goals and expectations for this experiment.

Abstract Copyright: ∼

Journal keyword(s): Supernovae

CDS comments: Fig.4 : SNF 2004-023 not identified

Simbad objects: 25

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Number of rows : 25
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 2004dh SN* 00 18 00.39 +24 33 44.5   18.364 17.5     SNII 16 1
2 WASP-1b Pl 00 20 40.0745768856 +31 59 23.954809596           ~ 134 1
3 M 31 AGN 00 42 44.330 +41 16 07.50 4.86 4.36 3.44     ~ 13622 1
4 NAME M31 RV No* 00 43 02.433 +41 12 56.17           M0 113 0
5 NAME SMC G 00 52 38.0 -72 48 01   2.79 2.2     ~ 12317 1
6 AT 2008jd ev 00 54 34.16 -37 38 28.6           ~ 134 1
7 SN 2005E SN* 02 39 14.34 +01 05 55.0     16.8     SNIb/c 128 1
8 SN 2006gy SN* 03 17 27.06 +41 24 19.5       14.20   SNIIn 372 1
9 ACO S 373 ClG 03 38 29.4 -35 27 08           ~ 2029 0
10 NAME LMC G 05 23 34.6 -69 45 22     0.4     ~ 19090 0
11 NAME Ori Region reg 05 35 17.30 -05 23 28.0           ~ 623 0
12 V* V838 Mon CV* 07 04 04.8221494992 -03 50 50.648894412       15.181 14.51 M10+B3V 462 1
13 SN 2009an SN* 12 22 47.40 +65 51 04.0           SNIa-norm 53 1
14 NAME M85 OT2006-1 No* 12 25 23.82 +18 10 56.2     19.30     ~ 70 1
15 M 85 GiP 12 25 24.053 +18 11 27.89   10.2       ~ 678 0
16 NAME Virgo Cluster ClG 12 30 47.8 +12 23 07           ~ 7107 0
17 SN 2005ap SN* 13 01 14.84 +27 43 31.4       18.20   SLSN-I 146 1
18 M 13 GlC 16 41 41.634 +36 27 40.75     5.8     ~ 2291 0
19 V* V4332 Sgr CV* 18 50 36.6958376520 -21 23 28.925017944         14.37 K8/M0e 194 0
20 NAME Orphan Stream St* 19 09 -23.           ~ 281 0
21 SN 2008S ev 20 34 45.33 +60 05 58.4   19.89 18.79 17.93   SNIIn? 253 1
22 NAME GD-1 Stream St* 22 40 +31.           ~ 319 0
23 NAME BD+37 4734Bb Pl 22 57 46.8442481880 +38 40 30.358351704           ~ 268 1
24 SN 2008ha SN* 23 34 52.69 +18 13 35.4           SNIax 203 1
25 NAME Local Group GrG ~ ~           ~ 9325 0

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