2010AJ....140.1868W


Query : 2010AJ....140.1868W

2010AJ....140.1868W - Astron. J., 140, 1868-1881 (2010/December-0)

The wide-field infrared survey explorer (WISE): mission description and initial on-orbit performance.

WRIGHT E.L., EISENHARDT P.R.M., MAINZER A.K., RESSLER M.E., CUTRI R.M., JARRETT T., KIRKPATRICK J.D., PADGETT D., McMILLAN R.S., SKRUTSKIE M., STANFORD S.A., COHEN M., WALKER R.G., MATHER J.C., LEISAWITZ D., GAUTIER T.N., McLEAN I., BENFORD D., LONSDALE C.J., BLAIN A., MENDEZ B., IRACE W.R., DUVAL V., LIU F., ROYER D., HEINRICHSEN I., HOWARD J., SHANNON M., KENDALL M., WALSH A.L., LARSEN M., CARDON J.G., SCHICK S., SCHWALM M., ABID M., FABINSKY B., NAES L. and TSAI C.-W.

Abstract (from CDS):

The all sky surveys done by the Palomar Observatory Schmidt, the European Southern Observatory Schmidt, and the United Kingdom Schmidt, the InfraRed Astronomical Satellite, and the Two Micron All Sky Survey have proven to be extremely useful tools for astronomy with value that lasts for decades. The Wide-field Infrared Survey Explorer (WISE) is mapping the whole sky following its launch on 2009 December 14. WISE began surveying the sky on 2010 January 14 and completed its first full coverage of the sky on July 17. The survey will continue to cover the sky a second time until the cryogen is exhausted (anticipated in 2010 November). WISE is achieving 5σ point source sensitivities better than 0.08, 0.11, 1, and 6 mJy in unconfused regions on the ecliptic in bands centered at wavelengths of 3.4, 4.6, 12, and 22 µm. Sensitivity improves toward the ecliptic poles due to denser coverage and lower zodiacal background. The angular resolution is 6".1, 6".4, 6".5, and 12".0 at 3.4, 4.6, 12, and 22 µm, and the astrometric precision for high signal-to-noise sources is better than 0".15.

Abstract Copyright: ∼

Journal keyword(s): infrared: general - space vehicles - surveys

Simbad objects: 19

goto Full paper

goto View the references in ADS

Number of rows : 19
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 IC 10 rG 00 20 17.33520 +59 18 13.6480   13.6 9.5     ~ 1185 1
2 NGC 1365 Sy1 03 33 36.458 -36 08 26.37 10.48 10.08 9.63 8.79 9.7 ~ 1987 2
3 NAME Taurus Complex SFR 04 41.0 +25 52           ~ 4971 0
4 * zet Lep * 05 46 57.3413646658 -14 49 19.020570470   3.637 3.525     A2IV-V(n) 308 0
5 NAME Orion Molecular Cloud MoC 05 56 -01.8           ~ 1227 1
6 NAME SEP reg 06 00 00.000 -66 33 38.55           ~ 198 0
7 HD 42581B BD* 06 10 34.80 -21 52 00.0           T6.5 549 0
8 NGC 2359 HII 07 18 30.000 -13 13 36.00           ~ 170 0
9 V* TW Hya TT* 11 01 51.9053285064 -34 42 17.033218380   11.94 10.50 10.626 9.18 K6Ve 2144 1
10 NAME TW Hya Association As* 11 01.9 -34 42           ~ 1018 0
11 SDSS J114816.64+525150.3 QSO 11 48 16.647 +52 51 50.31   25.73 25.04     ~ 487 0
12 HD 109573 TT* 12 36 01.0317461592 -39 52 10.220465388   5.786 5.774   5.81 A0V 684 1
13 M 83 SBG 13 37 00.91920 -29 51 56.7400 8.85 8.11 7.52 7.21   ~ 2778 2
14 M 101 GiP 14 03 12.583 +54 20 55.50   8.46 7.86 7.76   ~ 3138 2
15 THA 15-12 Or* 15 56 09.2066646912 -37 56 06.126118692   13.12 11.93 11.45   M0e 554 0
16 NAME Ophiuchus Molecular Cloud SFR 16 28 06 -24 32.5           ~ 3969 1
17 NAME NEP reg 18 00 00.000 +66 33 38.55           ~ 430 0
18 * alf Lyr dS* 18 36 56.33635 +38 47 01.2802 0.03 0.03 0.03 0.07 0.10 A0V 2787 1
19 NAME Gould Belt PoG ~ ~           ~ 956 1

To bookmark this query, right click on this link: simbad:objects in 2010AJ....140.1868W and select 'bookmark this link' or equivalent in the popup menu