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Table 1:

Log of the spectroscopic observations presented in this paper (see text for details).

(1)
(2) (3) (4) (5) (6) (7) (8)
Object RA Dec Telescope+instrument $\lambda$ range Disp. UT date & time Exposure
  (J2000) (J2000)   (Å) (Å/pix) at mid-exposure time (s)
Swift J0059.4+3150 00 59 53.28 +31 49 37.3 SPM 2.1m+B&C Spc. 3450-7650 4.0 30 Jun. 2008, 10:50 1800
Swift J0134.1-3625 01 33 57.75 -36 29 35.8 CTIO 1.5m+RC Spc. 3300-10 500 5.7 02 Jul. 2008, 09:02 1200
Swift J0342.0-2115 03 42 03.71 -21 14 39.6 AAT+6dF 3900-7600 1.6 30 Nov. 2003, 13:34 1200 + 600
Swift J0350.1-5019 03 50 23.78 -50 18 35.5 CTIO 1.5m+RC Spc. 3300-.10 500 5.7 04 Mar. 2008, 01:23 $2 \times 1800$
Swift J0505.7-2348 05 05 45.75 -23 51 14.0 SPM 2.1m+B&C Spc. 3450-7650 4.0 03 Feb. 2008, 04:04 $2 \times 1800$
Swift J0501.9-3239* 05 19 35.81 -32 39 28.0 AAT+6dF 3900-7600 1.6 30 Jan. 2003, 10:36 1200 + 600
Swift J0640.1-4328 06 40 37.99 -43 21 21.1 CTIO 1.5m+RC Spc. 3300-10 500 5.7 05 Mar. 2008, 1:26 $2 \times 1800$
Swift J0727.5-2406 07 27 21.05 -24 06 32.3 TNG+DOLoRes 3800-8000 2.5 07 Feb. 2008, 23:35 $2 \times 1200$
Swift J0739.6-3144 07 39 44.69 -31 43 02.5 SPM 2.1m+B&C Spc. 3450-7650 4.0 03 Feb. 2008, 07:15 $2 \times 1800$
Swift J0743.0-2543 07 43 14.72 -25 45 50.1 CTIO 1.5m+RC Spc. 3300-10 500 5.7 04 Mar. 2008, 03:56 $2 \times 1200$
Swift J0811.5+0937 08 11 30.83 +09 33 50.9 TNG+DOLoRes 3800-8000 2.5 08 Feb. 2008, 00:51 $2 \times 1800$
Swift J0902.0+6007 09 01 58.37 +60 09 06.2 Copernicus+AFOSC 4000-8000 4.2 22 Feb. 2008, 21:07 1200 + 600
Swift J0904.3+5538 09 04 36.97 +55 36 02.6 SDSS+CCD Spc. 3800-9200 1.0 29 Dec. 2000, 10:48 9000
Swift J0911.2+4533 09 11 30.00 +45 28 06.0 SDSS+CCD Spc. 3800-9200 1.0 07 Feb. 2002, 08:24 4803
Swift J0917.2-6221 09 16 09.37 -62 19 29.6 CTIO 1.5m+RC Spc. 3300-10 500 5.7 04 Mar. 2008, 06:02 600
Swift J0923.7+2255 09 23 43.01 +22 54 32.4 SPM 2.1m+B&C Spc. 3450-7650 4.0 02 Feb. 2008, 11:23 1800
Swift J1049.4+2258 10 49 30.89 +22 57 52.4 Cassini+BFOSC 3500-8000 4.0 08 May 2008, 21:17 $2 \times 1200$

Source coordinates are extracted from the 2MASS catalog and have an accuracy better than 0 $\hbox{$.\!\!^{\prime\prime}$ }$1. * The name of this source reported in Tueller et al. (2009) does not correspond to the actual coordinates.


Source LaTeX | All tables | In the text

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