|
Документ взят из кэша поисковой машины. Адрес
оригинального документа
: http://www.sao.ru/cats/doc/CL_Slee2.html
Дата изменения: Wed Mar 18 12:25:11 2015 Дата индексирования: Sun Apr 10 02:25:34 2016 Кодировка: Поисковые слова: m 5 |
1994AuJPh..47..145Slee, Roy & Savage; A VLA Survey of Rich Clusters
of Galaxies II. The stronger sources; (ctsy. A.Roy 4/94)
(ctsy. A.Roy 4/94) BEWARE: 1.5/4.9GHz polarization fraction has ranges of values!
(reformatted final version, 16-Oct-94)
==========================================================================
Table 1. Properties of observed clusters
Abell RA(1950)DEC rad_off D R m_10 BM Rc' Mpc z ref lgL_x
----+----1----+----2----+----3----+----4----+----5----+----6----+----7-
A 13 0011.1-1947 2.5 -81.1 2 5 16.6 5 17 1.59 0.0945 6
==========================================================================
Table 2. Radio source measurements * = Bandwidth smearing >= 7 arcsec
Cluster Source R.A. (1950) DEC Map Ang Dist S_1.5 S_4.9 Spectr. Ellipse Axes Lin. Polaris. lg10 LAS PTI References to
Field Number Number R/Rc Index Maj Min PA 1.5GHz 4.9GHz L_1.5 Size Core Other measurements
mJy mJy " " d % % W/Hz kpc mJy
----+----1----+----2----+----3----+----4----+----5----+----6----+----7----+----8----+----9----+----0----+----1----+----2----+----3--
A0013.1 000938.97-194042.4 1.30 84.0 17 3 89
A0013.6abc 001054.51-194647.7 1 0.19 3.85 -2.09 53 20 99 22.75 140 1,4,29
==========================================================================
Table 3. Measurements of double sources
# 4.9 GHz measurements; digital data not available at 1.5 GHz
* Bandwidth smearing >= 7 arc
Cluster Source Map Comp.Flux Flux Sp. Index Component Struct. Ratio of Comp. Linear
Field Number Number Sa Sb Ratio a b Maj.Axes Separ. Sep.
mJy mJy Sa/Sb a b " " d " " d a/b " d kpc
----+----1----+----2----+----3----+----4----+----5----+----6----+----7----+----8----+----9----+----
A0076.5ab 2 * 10.3 9.8 1.05 11 9 93 29.7 40
A0076.13ab 3,4 79.8 79.0 1.01 -0.97 -0.91 14 7 92 11 7 104 1.27 31.1 105
Column headings :
1,2 The cluster field and source number as listed by SPS89.
3 Contour map number within Figure 1.
4,5 The 1.5 GHz flux densities of the components.
6. Ratio of the flux densities of the components.
7,8 Spectral indices of the components between 1.5 & 4.9 GHz.
9,10 Deconvolved ellipse axes and position angles (from north through east) of the components.
11 Ratio of the major axes of the components.
12 Angular separation of the components and its position angle ( from north through east).
13 Linear separation of the components of doubles with redshifts (qo=0.5, Ho = 75km/s/Mpc)."
==========================================================================
Table 4. Measurements of triple sources
* Bandwidth smearing >= 7 arcsec
Cluster Source Map Component Flux Density Gaussian-fit Ellipses Component Separations
Field Number Number Sa Sb Sc a b c a - b b - c a - c
mJy mJy mJy " " deg " " deg " " deg " deg " deg " deg
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12)
----+----1----+----2----+----3----+----4----+----5----+----6----+----7----+----8----+----9----+----0----+----1----+--
A 13 6abc 1 1.83 1.36 0.74 32 11 120 9 3 8 37.9 104 20.3 130 21.6 79
==========================================================================
Table 5. Optical identifications
Cluster Source Radio Centroid Optical Position EF Ang. PA m_app m_app Ty z_hel Reference(s)
Field Source RA (B1950) Dec. RA (B1950)Dec. ID Dist PSSE SRC Morph to the redshift z
Number h m s d ' " h m s d ' " " d R B_J z
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13)
----+----1----+----2----+----3----+----4----+----5----+----6----+----7----+----8----+----9----+----0----
A0013.1 000938.97-194042.4 EF