EDP Sciences logo
Subscriber Authentication Point
Search
Menu
Home All issues Volume 558 (October 2013) A&A, 558 (2013) A18 Full HTML
Free Access

Table 3

The optical data for the 140 XMP galaxies in the local Universe.

Name RA(J2000) Dec(J2000) m g r opt sin   i 12    +   log  (O/H) Optical Spatial
h m s °   ′  ″ mag ′′ morphology offset
(1) (2) (3) (4) (5) (6) (7) (8) (9)
UGC 12894 00 00 22 +39 29 44 ... 27.0⋆ ... 7.64 ... ...
J0004+0025 00 04 22 +00 25 36 19.4 5.23 0.70 7.37 symmetric∗ ...
J0014-0044a 00 14 29 –00 44 44 18.7 1.43⋆ 0.89⋆ 7.63 ... ...
J0015+0104 00 15 21 +01 04 37 18.3 15.25 0.62 7.07 multi-knot∗ ...
J0016+0108 00 16 28 +01 08 02 18.9 4.54 0.57 7.53 symmetric∗ ...
HS0017+1055 00 20 21 +11 12 21 ... ... ... 7.63 cometary∗ 0.2
J0029-0108 00 29 05 –01 08 26 19.2 5.3 0.88 7.35 cometary∗ 0.4
J0029-0025 00 29 49 –00 25 40 20.4 17.34⋆ 0.50⋆ 7.29 symmetric∗ ...
ESO 473-G024 00 31 22 –22 45 57 ... 25.5† 0.89† 7.45 ... ...
J0036+0052 00 36 30 +00 52 34 18.8 2.32 0.48 7.64‡ symmetric ...
AndromedaIV 00 42 32 +40 34 19 ... 34.5† 0.68† 7.49 ... ...
J0057-0022 00 57 13 –00 21 58 19.1 1.51⋆ 0.42⋆ 7.60 symmetric∗ ...
IC1613 01 04 48 +02 07 04 ... 460.5† 0.48† 7.64 multi-knot∗ ...
J0107+0001 01 07 51 +00 01 28 19.4 1.30 0.63 7.23 cometary∗ 0.4
AM0106-382 01 08 22 –38 12 34 ... 17.1† 0.88† 7.56 ... ...
J0113+0052 01 13 40 +00 52 39 20.1 3.23 0.42 7.24 multi-knot∗ 0.5
J0119-0935 01 19 14 –09 35 46 19.5 2.04 0.61 7.31 cometary∗ 0.4
HS0122+0743 01 25 34 +07 59 24 15.7 10.14 0.67 7.60 multi-knot 0.5
J0126-0038 01 26 46 –00 38 39 18.4 3.36⋆ 0.78⋆ 7.51 cometary∗ 0.2
J0133+1342 01 33 53 +13 42 09 18.1 5.64 0.81 7.56 symmetric∗ ...
J0135-0023 01 35 44 –00 23 17 18.9 2.23⋆ 0.94⋆ 7.38 symmetric∗ ...
UGCA20 01 43 15 +19 58 32 18.0 58.5† 1.03† 7.60 cometary∗ 0.7
UM133 01 44 42 +04 53 42 15.4 ... ... 7.63 cometary∗ 0.8
J0158+0006 01 58 09 +00 06 37 18.1 5.16 0.78 7.75‡ cometary ...
HKK97L14 02 00 10 +28 49 53 ... 13.5† 0.92† 7.56 cometary∗ 0.5
J0204-1009 02 04 26 –10 09 35 17.1 10.09 0.94 7.36 cometary∗ ...
J0205-0949 02 05 49 –09 49 18 15.3 21.39 0.98 7.61 multi-knot∗ ...
J0216+0115 02 16 29 +01 15 21 17.4 9.22 0.73 7.44 cometary∗ 0.6
096632 02 51 47 –30 06 32 16.3 17.55† 0.74† 7.51 ... ...
J0254+0035 02 54 29 +00 35 50 19.8 3.29 0.83 7.28 cometary∗ 0.3
J0301-0059 03 01 26 –00 59 26 21.5 3.18⋆ 0.82⋆ 7.64 cometary∗ 0.1
J0301-0052 03 01 49 –00 52 57 18.8 2.48⋆ 0.87⋆ 7.52 cometary∗ 0.8
J0303-0109 03 03 31 –01 09 47 19.8 4.69 0.69 7.22 two-knot 0.7
J0313+0006 03 13 00 +00 06 12 19.2 3.80 0.82 7.82‡ cometary 0.5
J0313+0010 03 13 02 +00 10 40 18.9 4.35 0.43 7.44 symmetric∗ ...
J0315-0024 03 16 00 –00 24 26 20.2 1.48⋆ 0.59⋆ 7.41 cometary∗ 0.7
UGC 2684 03 20 24 +17 17 45 22.8 2.47 0.77 7.60 cometary∗ 0.0
SBS 0335-052W 03 37 38 –05 02 37 19.0 3.45† 0.68† 7.11 ... ...
SBS 0335-052E 03 37 44 –05 02 40 16.3 6.45† 0.53† 7.31 ... ...
J0338+0013 03 38 12 +00 13 13 24.4 4.31 0.84 7.64 cometary∗ 0.7
J0341-0026 03 41 18 –00 26 28 18.8 1.72⋆ 0.97⋆ 7.26 cometary∗ 0.7
ESO358-G060 03 45 12 –35 34 15 ... 31.5† 1.04† 7.26 ... ...
G0405-3648 04 05 19 –36 48 49 ... 12.45† 0.73† 7.25 ... ...
J0519+0007 05 19 03 +00 07 29 18.4 2.16 0.47 7.44 symmetric∗ ...
Tol0618-402 06 20 02 –40 18 09 ... 10.5† 0.71† 7.56 ... ...
ESO 489-G56 06 26 17 –26 15 56 15.6 22.5† 0.80† 7.49 ... ...
J0808+1728 08 08 41 +17 28 56 19.2 0.56⋆ 0.75⋆ 7.48 symmetric ...
J0812+4836 08 12 39 +48 36 46 16.0 13.10 0.89 7.28 cometary∗ 0.2
UGC 4305 08 19 05 +70 43 12 ... 213.0† 0.64† 7.65 ... ...
J0825+1846 08 25 40 +18 46 17 19.0 2.16 0.58 7.75‡ symmetric ...
HS0822+03542 08 25 55 +35 32 31 17.8 4.45 0.92 7.35 cometary∗ 0.3
DD053 08 34 07 +66 10 54 20.3 42.0† 0.53† 7.62 multi-knot∗ ...
UGC 4483 08 37 03 +69 46 31 15.1 31.5† 0.92† 7.58 ... ...
HS0837+4717 08 40 30 +47 07 10 17.6 2.31 0.69 7.64 cometary∗ 0.3
J0842+1033 08 42 36 +10 33 13 17.7 5.65 0.87 7.58‡ cometary 0.4
HS0846+3522 08 49 40 +35 11 39 18.2 5.80 0.79 7.65 cometary∗ 0.2
J0859+3923 08 59 47 +39 23 06 17.2 10.62 0.74 7.57 two-knot∗ ...
J0910+0711 09 10 29 +07 11 18 16.9 11.61 0.94 7.63 cometary∗ 0.5
J0911+3135 09 11 59 +31 35 36 17.8 6.04 0.71 7.51 cometary∗ 0.3
J0926+3343 09 26 09 +33 43 04 17.8 15.58 1.00 7.12 cometary∗ 0.9
IZw18 09 34 02 +55 14 25 16.4 4.47 0.51 7.17 two-knot ...
J0940+2935 09 40 13 +29 35 30 16.5 16.44 0.95 7.65 cometary∗ 0.3
J0942+3404 09 42 54 +34 04 11 19.1 2.29 0.68 7.67‡ cometary 0.4
CGCG007-025 09 44 02 –00 38 32 16.0 9.47 0.82 7.65 multi-knot∗ ...
SBS940+544 09 44 17 +54 11 34 19.1 0.63⋆ 0.36⋆ 7.46 cometary 0.7
CS0953-174 09 55 00 –17 00 00 ... ... ... 7.58 ... ...
J0956+2849 09 56 46 +28 49 44 15.9 32.05 0.97 7.13 multi-knot∗ ...
LeoA 09 59 26 +30 44 47 19.0 124.5† 0.86† 7.30 multi-knot∗ ...
SextansB 10 00 00 +05 19 56 20.5 129.0† 0.78† 7.53 multi-knot∗ ...
J1003+4504 10 03 48 +45 04 57 17.5 3.40 0.59 7.65‡ symmetric ...
SextansA 10 11 00 –04 41 34 ... 162.0† 0.59† 7.54 ... ...
KUG1013+381 10 16 24 +37 54 44 15.9 1.62 ... 7.58 cometary 0.2
SDSSJ1025+1402 10 25 30 +14 02 07 20.4 0.60⋆ 0.54⋆ 7.36 symmetric∗ ...
UGCA211 10 27 02 +56 16 14 16.2 2.11 0.38 7.56 cometary∗ 0.4
J1031+0434 10 31 37 +04 34 22 16.2 6.08 0.70 7.70 cometary 0.3
HS1033+4757 10 36 25 +47 41 52 17.5 6.92 0.67 7.65 symmetric∗ ...
J1044+0353 10 44 58 +03 53 13 17.5 4.16 0.86 7.44 cometary 0.4
HS1059+3934 11 02 10 +39 18 45 17.9 7.89 0.71 7.62 multi-knot∗ ...
J1105+6022 11 05 54 +60 22 29 16.4 17.08 0.91 7.64 cometary∗ 0.4
J1119+5130 11 19 34 +51 30 12 16.9 4.52 0.73 7.51 cometary∗ 0.2
J1121+0324 11 21 53 +03 24 21 18.1 9.62 0.80 7.64 cometary∗ 0.5
UGC6456 11 28 00 +78 59 39 ... 33.0† 0.88† 7.35 ... ...
SBS1129+576 11 32 02 +57 22 46 16.7 6.59⋆ 0.97⋆ 7.36 cometary∗ 0.5
J1145+5018 11 45 06 +50 18 02 17.8 5.50 0.89 7.71‡ cometary 0.4
J1151-0222 11 51 32 –02 22 22 16.8 11.30 0.52 7.78 two-knot 0.6
J1157+5638 11 57 54 +56 38 16 16.9 10.39 0.61 7.83‡ cometary 0.5
J1201+0211 12 01 22 +02 11 08 17.6 10.28 0.88 7.49 cometary 0.6
SBS1159+545 12 02 02 +54 15 50 18.7 2.33 0.40 7.41 two-knot∗ 0.8
SBS1211+540 12 14 02 +53 45 17 17.4 5.72 0.79 7.64 cometary 0.1
J1215+5223 12 15 47 +52 23 14 15.2 24.67 0.85 7.43 multi-knot∗ ...
Tol1214-277 12 17 17 –28 02 33 ... 2.4† ... 7.55 ... ...
VCC0428 12 20 40 +13 53 22 17.0 11.73 0.91 7.64 cometary∗ 0.1
HS1222+3741 12 24 37 +37 24 37 17.9 2.19 0.47 7.64 symmetric∗ ...
Tol65 12 25 47 –36 14 01 17.5 6.0† ... 7.54 ... ...
J1230+1202 12 30 49 +12 02 43 16.7 4.88 0.86 7.73 cometary 0.3
KISSR85 12 37 18 +29 14 55 19.9 3.16 0.56 7.61 cometary∗ 0.3
UGCA292 12 38 40 +32 46 01 18.9 1.51 0.14 7.28 multi-knot∗ ...
HS1236+3937 12 39 20 +39 21 05 18.5 8.54 1.00 7.47 two-knot∗ 0.4
J1239+1456 12 39 45 +14 56 13 19.8 1.47 0.56 7.65 symmetric∗ ...
SBS1249+493 12 51 52 +49 03 28 18.0 3.00 0.84 7.64 cometary∗ 0.7
J1255-0213 12 55 26 –02 13 34 19.1 0.83⋆ 0.64⋆ 7.83 symmetric ...
GR8 12 58 40 +14 13 03 17.9 23.54 0.88 7.65 multi-knot∗ ...
KISSR1490 13 13 16 +44 02 30 19.0 5.60 0.85 7.56 cometary∗ 0.4
DD0167 13 13 23 +46 19 22 ... 19.64 0.82 7.20 multi-knot∗ 0.8
HS1319+3224 13 21 20 +32 08 25 18.6 4.57 0.66 7.59 cometary∗ 0.2
J1323-0132 13 23 47 –01 32 52 18.2 0.66⋆ 0.39⋆ 7.78 symmetric ...
J1327+4022 13 27 23 +40 22 04 19.0 2.83 0.46 7.67‡ symmetric ...
J1331+4151 13 31 27 +41 51 48 17.1 3.80 0.74 7.75 cometary 0.3
ESO577-G27 13 42 47 –19 34 54 ... 28.5† 0.46† 7.57 ... ...
J1355+4651 13 55 26 +46 51 51 19.3 2.20 0.79 7.63 cometary∗ 0.4
J1414-0208 14 14 54 –02 08 23 18.0 8.47 0.72 7.28 cometary∗ 0.5
SBS1415+437 14 17 01 +43 30 05 17.8 1.40 0.57 7.43 multi-knot∗ 0.8
J1418+2102 14 18 51 +21 02 39 17.6 2.87 0.85 7.64‡ cometary 0.4
J1422+5145 14 22 51 +51 45 16 20.2 2.01 0.73 7.41 symmetric∗ ...
J1423+2257 14 23 43 +22 57 29 17.9 2.36 0.66 7.72 symmetric ...
J1441+2914 14 41 58 +29 14 34 20.1 2.25 0.55 7.47 symmetric∗ ...
HS1442+4250 14 44 13 +42 37 44 15.9 20.04 1.00 7.54 cometary∗ 0.3
J1509+3731 15 09 34 +37 31 46 17.3 2.87 0.75 7.85 cometary∗ 0.6
KISSR666 15 15 42 +29 01 40 19.1 4.24 0.87 7.53 cometary∗ 0.4
KISSR1013 16 16 39 +29 03 33 18.2 1.28 0.37 7.63 two-knot∗ ...
J1644+2734 16 44 03 +27 34 05 17.7 10.05 1.00 7.48 symmetric∗ ...
J1647+2105 16 47 11 +21 05 15 17.3 9.16 0.82 7.75 multi-knot ...
W1702+18 17 02 33 +18 03 06 18.4 1.57 0.56 7.63 symmetric∗ ...
HS1704+4332 17 05 45 +43 28 49 18.4 3.49 0.75 7.55 cometary∗ 0.5
SagDIG 19 29 59 –17 40 41 ... ... ... 7.44 ... ...
J2053+0039 20 53 13 +00 39 15 19.4 6.48 0.83 7.33 two-knot∗ 0.4
J2104-0035 21 04 55 –00 35 22 17.9 ... ... 7.05 cometary∗ 0.8
J2105+0032 21 05 09 +00 32 23 19.0 0.43⋆ 0.47⋆ 7.42 cometary∗ 0.3
J2120-0058 21 20 26 –00 58 27 18.8 1.02⋆ 0.74⋆ 7.65 symmetric∗ ...
HS2134+0400 21 36 59 +04 14 04 ... ... ... 7.44 cometary∗ 0.2
J2150+0033 21 50 32 +00 33 05 19.3 6.12 0.71 7.60 symmetric∗ ...
ESO 146-G14 22 13 00 –62 04 03 ... 52.5† 1.06† 7.59 ... ...
2dF171716 22 13 26 –25 26 43 ... 5.55† 0.56† 7.54 ... ...
PHL293B 22 30 37 –00 06 37 17.2 2.13⋆ 0.53⋆ 7.62 cometary∗ 0.4
2dF115901 22 37 02 –28 52 41 ... 3.6† 0.75† 7.57 ... ...
J2238+1400 22 38 31 +14 00 30 19.0 3.00 0.80 7.45 two-knot 0.1
J2250+0000 22 50 59 +00 00 33 19.8 1.71 0.57 7.61 symmetric∗ ...
J2259+1413 22 59 01 +14 13 43 19.1 4.03 0.85 7.37 cometary∗ 0.5
J2302+0049 23 02 10 +00 49 39 18.8 2.19 0.66 7.71 two-knot ...
J2354-0005 23 54 37 –00 05 02 18.7 2.68⋆ 0.75⋆ 7.35 two-knot∗ 0.8

Notes. Column 1: Source name. Column 2: Right Ascension. Column 3: Declination. Column 4: SDSS g-band Petrosian magnitude, from ML11. Column 5: Optical radius containing 90% of the g-band galaxy light, from the SDSS. Otherwise, NED SDSS r-band Petrosian radius (⋆) or the average source size at isophote 25 mag arcsec-2 (†), is used. Column 6: Inclination angle of the source from the SDSS g-band data, NED SDSS r-band Petrosian data (⋆) or estimated from the NED source size (†). Column 7: Metallicity, 12 +log  (O/H), from ML11. Tabulated values are based on the direct method or strong-line method (‡; see ML11 for details). Column 8: SDSS optical morphology adapted from ML11 or obtained from SDSS DR9 images (∗). Symmetric (spherical, elliptical or disk-like symmetric structure), two-knot (two-knot structure), multi-knot (multiple knot structure) and cometary (head-tail structure), are used. Column 9: Spatial offset, ΔR/r, where ΔR is the difference between the position of the brightest star-formation region and the position of the center of the galaxy and r is the radius of the outer isophote.

(a)

Although this source has been selected as an XMP galaxy in ML11, NED has flagged this as a Western H ii region of UGC 139 (Sect. 3.2.2).

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.