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2 Description of the sample

BCGs are typically rich in H  I gas. Many large H  I surveys of BCGs were carried out, in particular by Gordon & Gottesman (1981), Thuan & Martin (1981), Thuan et al. (1999) and Smoker et al. (2000). Since we want to combine the optical spectra we obtain with HI data to constrain simultaneously the stars and gas contents of BCGs, we therefore select our sample on the basis of these surveys.

Considering the observatory site, instruments and possible observation times, we selected our sample according to the following criteria: (1) $m_B^{\rm c} < 17.0$ mag; (2)  $\delta_{2000} > -12^{\circ}$; (3) $M_B^{\rm c} < -17$ mag. Using these criteria, 83 BCGs were selected. 14 additional "dwarf'' ( $M_B^{\rm c} > -17$ mag) BCGs were also included because we want to compare their properties with those of "luminous'' ( $M_B^{\rm c} < -17$ mag) BCGs. The final sample consists of 97 BCGs. We emphasize that there is no guarantee that our sample has any statistical completeness.

Most (92/97) of the galaxies in our sample come from Gordon & Gottesman (1981). These authors assembled a list of 99 blue compact galaxies from the Markarian, Haro and Zwicky lists. The H  I observations were made using the 91-m transit radio telescope of the National Radio Astronomy Observatory and the 305-m spherical radio telescope of the Arecibo Observatory. Three other galaxies in our sample come from Kinney et al. (1993). One galaxy comes from Thuan & Martin (1981); these authors assembled a list of 115 blue compact dwarf galaxies (BCDs, MB > -18 mag) known at that time from the objective prism surveys of Markarian and Haro, with a few objects from Zwicky and other investigators (we are presently observing most of these BCDs and will present our results in the future). Finally, one galaxy in our sample comes from Thuan et al. (1999).

 
Table 1: Global parameters of observed blue compact galaxies.
Galaxy RA(2000) Dec(2000) $m_B^{\rm c}$ Dist. $M_B^{\rm c}$ $E(B-V)_{\rm G}$ Other
Name (hms) (dms) (mag) (Mpc) (mag)   Name
Mrk 335 00:06:19.5 +20:12:10 13.72 102.0 -21.3 0.035 PGC 473
IIIZw12 00:47:56.5 +22:22:23 14.58 80.0 -19.9 0.045 Mrk 347
Haro15 00:48:35.4 -12:42:59 13.48 86.0 -21.2 0.023 Mrk 960
Mrk 352 00:59:53.3 +31:49:37 14.24 62.0 -19.7 0.061 PGC 3575
Mrk 1 01:16:07.2 +33:05:22 14.69 67.0 -19.4 0.060 NGC 449
IIIZw33 01:43:56.5 +17:03:43 14.56 109.0 -20.6 0.068 Mrk 360
VZw155 01:57:49.4 +27:51:56 15.00 111.0 -20.2 0.082 Mrk 364
IIIZw42 02:11:33.5 +13:55:02 14.51 107.0 -20.6 0.088 Mrk 366
IIIZw43 02:13:45.0 +04:06:07 14.05 47.0 -19.3 0.042 Mrk 589
VZw372 04:13:56.0 +29:09:28 15.19R 74.0 -19.2 0.709 UGC 2989
IIZw18 04:38:39.7 +11:14:28 16.41R 59.0 -17.4 0.391 PGC 15715
IIZw23 04:49:44.4 +03:20:03 13.88 110.0 -21.3 0.063 Mrk 1087
IIZw28 05:01:42.0 +03:34:28 14.94 113.0 -20.3 0.060 VV790B
IIZw33 05:10:48.1 -02:40:54 13.48 36.0 -19.3 0.102 Mrk 1094
IIZw35 05:16:59.3 +00:55:20 16.90N 95.0 -18.0 0.140 PGC 17037
IIZw40 05:55:42.8 +03:23:30 14.22 9.0 -15.6 0.820 UGCA 116
IIZw42 06:03:11.4 +07:49:37 15.37 69.0 -18.8 0.417 UGC3 393
Mrk 5 06:42:15.5 +75:37:33 15.12 13.3 -15.5 0.084 UGCA 130
Mrk 6 06:52:12.2 +74:25:37 13.86 76.0 -20.5 0.136 UGC 3547
VIIZw153 07:28:12.0 +72:34:29 13.40 43.0 -19.8 0.030 Mrk 7
VIIZw156 07:29:25.4 +72:07:44 13.17 50.0 -20.3 0.026 Mrk 8
Haro1 07:36:56.4 +35:14:31 12.39 50.0 -21.1 0.043 NGC 2415
Mrk 385 08:03:28.0 +25:06:10 14.57 110.0 -20.6 0.030 PGC 22615
Mrk 622 08:07:41.0 +39:00:15 14.33 94.0 -20.5 0.051 UGC 4229
Mrk 390 08:35:33.1 +30:32:03 14.58 101.0 -20.4 0.041 PGC 24127
Zw0855 08:58:27.4 +06:19:41 14.50 47.0 -18.9 0.069 UGC 4703
Mrk 105 09:20:26.3 +71:24:16 15.88 49.0 -17.6 0.066 PGC 26416
IZw18 09:34:02.0 +55:14:28 15.80 10.9 -14.4 0.032 Mrk 116
Mrk 402 09:35:19.2 +30:24:31 15.66R 98.0 -19.3 0.020 PGC 27258
IZw21 09:46:28.6 +45:45:09 14.59 67.0 -19.5 0.015 UGC 5225
Haro22 09:50:11.0 +28:00:47 14.94 18.4 -16.4 0.025 PGC 28305
Haro23 10:06:18.1 +28:56:40 14.33 17.5 -16.9 0.024 UGCA 201
IIZw44 10:15:14.7 +21:06:34 15.75 81.0 -18.8 0.023 PGC 29934
Haro2 10:32:31.9 +54:24:03 13.15 21.0 -18.5 0.012 Mrk 33
Mrk 148 10:35:34.8 +44:18:57 14.65R 96.0 -20.3 0.019 UGC 5747
Haro3 10:45:22.4 +55:57:37 12.81 13.6 -17.9 0.007 Mrk 35
Haro25 10:48:44.2 +26:03:12 15.52 101.0 -19.5 0.033 Mrk 727
Mrk 1267 10:53:03.9 +04:37:54 14.48 77.8 -20.0 0.034 Ark 264r1
Haro4 11:04:58.5 +29:08:22 15.51 7.9 -14.0 0.030 Mrk 36
IZw26 11:25:36.2 +54:22:57 16.80 83.0 -17.8 0.014 Mrk 40
Mrk169 11:26:44.4 +59:09:20 13.95 17.5 -17.3 0.014 UGC 6447
Haro27 11:40:24.8 +28:22:26 14.13 24.0 -17.8 0.022 Mrk 1507
Mrk198 12:09:14.1 +47:03:30 14.56 97.0 -20.4 0.017 PGC 38613
IIZw57 12:09:32.9 +17:00:51 13.60 88.0 -21.1 0.036 PGC 38634
Mrk201 12:14:09.7 +54:31:38 12.86 35.0 -19.9 0.015 IZw 33r1
Haro28 12:15:46.1 +48:07:54 13.21 10.6 -16.9 0.016 NGC 4218
Haro8 12:19:09.9 +03:51:21 14.49 18.6 -16.9 0.017 Mrk 49
Mrk50 12:23:24.1 +02:40:45 14.89R 92.0 -19.9 0.016 PGC 40220
Haro29 12:26:16.0 +48:29:37 14.24 4.8 -14.2 0.015 IZw 36



 
Table 1: continued.
Galaxy RA (2000) Dec. (2000) $m_B^{\rm c}$ Dist. $M_B^{\rm c}$ $E(B-V)_{\rm G}$ Other
Name (hms) (dms) (mag) (Mpc) (mag)   Name
Mrk 213 12:31:22.2 +57:57:52 13.03R 41.7 -20.1 0.012 NGC 4500r1
Mrk 215 12:32:34.7 +45:46:04 14.47 79.0 -20.0 0.017 PGC 41591
Haro32 12:43:48.6 +54:54:02 13.70 67.0 -20.4 0.016 IZw41
Haro33 12:44:38.3 +28:28:19 14.39 12.5 -16.1 0.016 UGCA 294
Haro34 12:45:06.6 +21:10:10 14.86 93.0 -20.0 0.041 Ark 386
Haro36 12:46:56.4 +51:36:46 14.67 8.0 -14.8 0.015 UGC 7950
Haro35 12:47:08.5 +27:47:35 15.89R 99.0 -19.1 0.013 PGC 43139
Haro37 12:48:41.0 +34:28:39 15.18 57.0 -18.6 0.014 Mrk 444
IIIZw68 12:58:02.4 +26:51:34 14.34 76.0 -20.1 0.009 UGC 8080
IIZw67 12:58:35.2 +27:35:47 13.69 101.0 -21.3 0.010 NGC 4853
Mrk 57 12:58:37.2 +27:10:34 15.08 102.0 -20.0 0.014 PGC 44486r2
Mrk 235 13:00:02.1 +33:26:15 15.07 100.0 -19.9 0.012 PGC 44694
Mrk 241 13:06:19.8 +32:58:25 15.87 105.0 -19.2 0.014 PGC 45363
IZw53 13:13:57.7 +35:18:55 15.00R 69.0 -19.2 0.011 PGC 45993
IZw56 13:20:35.3 +34:08:22 14.10 93.0 -20.7 0.013 UGC 8387
Haro38 13:35:35.6 +29:13:01 14.87 11.9 -15.5 0.012 UGC 8578
Mrk 270 13:41:05.7 +67:40:20 13.61 38.0 -19.3 0.020 NGC 5283
Mrk 275 13:48:40.5 +31:27:39 14.52 106.0 -20.6 0.019 PGC 48992
Haro39 13:58:23.8 +25:33:00 14.49 35.0 -18.2 0.016 PGC 49732
Haro42 14:31:09.0 +27:14:14 14.74 60.0 -19.2 0.015 Mrk 685
Haro43 14:36:08.8 +28:26:59 15.08 27.0 -17.1 0.020 PGC 52193
Haro44 14:43:24.7 +28:18:04 16.05R 51.0 -17.5 0.017 PGC 52587
IIZw70 14:50:56.5 +35:34:18 14.04 18.0 -17.2 0.012 Mrk 829
IIZw71 14:51:14.4 +35:32:31 13.34 18.0 -17.9 0.013 PGC 53039
IZw97 14:54:39.2 +42:01:26 14.47 36.0 -18.3 0.020 PGC 53299
IZw98 14:55:15.6 +42:30:25 13.91 75.0 -20.5 0.019 NGC 5787
IZw101 15:03:45.8 +42:41:59 15.19 68.0 -19.0 0.019 Ark467
IZw117 15:35:53.6 +38:40:37 14.15 77.0 -20.3 0.017 UGC 9922
IZw123 15:37:04.2 +55:15:48 15.44 11.6 -14.9 0.014 Mrk 487
VIIZw631 15:59:11.9 +20:45:31 12.98 62.0 -21.0 0.055 NGC 6027
Mrk 297 16:05:12.9 +20:32:32 12.98 65.0 -21.1 0.076 NGC 6052
IZw147 16:23:12.0 +54:08:36 15.80R 75.0 -18.6 0.009 PGC 57975
IZw159 16:35:21.1 +52:12:53 15.70 38.0 -17.2 0.029 Mrk 1499
IZw166 16:48:24.1 +48:42:33 15.03 106.0 -20.1 0.016 Mrk 499
Mrk 893 17:15:02.2 +60:12:59 16.34 83.7 -18.3 0.021 1714+602r3
IZw191 17:40:24.8 +47:43:59 14.70R 81.0 -19.8 0.019 PGC 60671
IZw199 17:50:05.1 +56:40:27 14.82 74.0 -19.5 0.048 PGC 60950
IZw207 18:31:10.4 +55:16:32 15.31R 79.0 -19.2 0.042 PGC 61982
IIZw82 20:23:15.6 +00:39:52 13.46 56.0 -20.3 0.191 UGC 11546
IVZw67 21:02:18.8 +36:41:44 14.00N 38.0 -18.9 0.280 UGC 11668
IIZw172 22:14:45.9 +13:50:37 13.23 108.0 -21.9 0.065 NGC 7237
IVZw93 22:16:07.7 +22:56:33 15.44R 55.0 -18.3 0.069 PGC 68454
Mrk 303 22:16:26.8 +16:28:17 14.62 104.0 -20.5 0.051 NGC 7244
Zw2220 22:23:02.0 +30:55:29 13.52 93.0 -21.3 0.078 UGC 12011
Mrk 314 23:02:59.2 +16:36:19 13.45 31.0 -19.0 0.085 Mrk 314
IVZw142 23:20:03.1 +26:12:58 14.89 109.0 -20.3 0.086 Mrk 322
IVZw149 23:27:41.2 +23:35:21 12.66 80.0 -21.9 0.043 Mrk 325
Zw2335 23:37:39.6 +30:07:47 15.37 22.0 -16.3 0.093 Mrk 328

r1: Kinney et al. (1993); r2: Thuan & Martin (1981); r3: Thuan et al. (1999);
The other BCGs were selected from Gordon & Gottesman (1981).

In total our sample contains 97 blue compact galaxies, the general parameters of which are listed in Table 1. Column 1 lists the galaxy name following Haro (Haro 1956), Markarian (Mrk, Markarian et al. 1989), and Zwicky (Zw, Zwicky 1971). Columns 2 and 3 list the right ascension and declination at epoch 2000, taken from NED[*]. Column 4 lists the apparent blue magnitude ( $m_B^{\rm c}$) corrected for instrumental effects, extinction, inclination, and doppler velocity. Most magnitudes were taken from Gordon & Gottesman (1981). The other galaxies were corrected for instrumental effects, extinction, inclination based on de Vaucouleurs et al. (1991, RC3) and NED, as indicated by "R'', "N''. Column 5 lists the distance (D) to the galaxy, in megaparsecs, assuming a Hubble constant of H0=75 km s-1 Mpc-1 and q0=0.5. Column 6 lists the absolute blue magnitude ( $M_B^{\rm c}$,), derived from Col. 4 and Col. 5 with $M_B^{\rm c} =m_B^{\rm c} - 5~{\log D} +5 $. Column 7 lists the Galactic foreground reddening, E(B-V). The last Col. 8 lists other commonly used designations for the galaxies.

The spatial distribution of the 97 sample galaxies on the sky is show in Fig. 1. The absolute blue magnitude ( $M_B^{\rm c}$) distribution of the 97 sample galaxies is presented in Fig. 2.

  \begin{figure}
\par\includegraphics[angle=-90,width=9cm,clip]{MS2390f1.ps} %
\end{figure} Figure 1: The distribution of blue compact galaxies in the sky shown in equal-area projection, centered on Declination (latitude) 0, Right Ascension (longitude) 0.


  \begin{figure}
\par\includegraphics[angle=-90,width=9cm,clip]{MS2390f2.ps}\end{figure} Figure 2: The distribution of absolute blue magnitudes (MB) of the 97 blue compact galaxies in our sample, 83 have MB < -17 mag.


 
Table 2: The observation date and instrumental parameters.
Obs. Observation date Number cw. slit arc Spec. Standard stars
No.   of nights (Å) ( $^{\prime\prime}$) lamp num.  
 1 2002 Jan. 08-Jan. 12 5 5500 2.5 He/Ar 20 G191B2B Hilt600 Feige56 Feige25 HZ44
 2 2001 Oct. 12 1 5500 2.5 He/Ar  4 Hilt600 HD192281 G191B2B BD174708
 3 2001 Feb. 24-Mar. 01 4 5500 2.5 He/Ar 33 G191B2B Feige34 BD332642 HZ44
 4 2000 Apr. 29-May. 01 3 6000 2.3 He/Ar 24 Feige34 BD332642 HZ44
 5 2000 Feb. 25 1 6000 2.2 He/Ar  4 Hilt600 Feige34
 6 2000 Jan. 01-Jan. 02 2 5500 3.0 He/Ar 17 G191B2B Hilt600 Feige34
 7 1999 Aug. 03-Aug. 09 2 5500 2.0 He/Ar  4 BD284211 HD192281
 8 1998 Aug. 14-Aug. 20 4 5500 2.5 He/Ar 15 BD284211 Kopff27 Feige15 BD332642
 9 1998 Feb. 17 1 5500 2.0 He/Ar  2 Hilt600 Feige98
10 1997 Mar. 18-Mar. 20 3 6000 2.0 Fe/Ar 13 Feige34 Feige98 Sa29130



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