Table 1
LBGs used in the fitting.
| LBG_IDUV | RA | Dec | z gb | M V | FWHM | #spec | #points | Grism_ID | |
| (deg) | (deg) | (mag) | (arcsec) | ||||||
|
|
|||||||||
| 46190 | 53.18483 | –27.92041 | — | 23.34 | 10.0 | 4 | 39 | HAG_J033244.36-275513.5_J9FA43BIQ | |
| 47362 | 53.17793 | –27.90950 | 1.1041 | 22.46 | 7.1 | 4 | 68 | HAG_J033242.70-275434.2_J9FA43BIQ | |
| 49138 | 53.13903 | –27.89262 | 0.6792 | 23.46 | 6.1 | 1 | 18 | HAG_J033233.37-275333.4_J9FA43BIQ | |
| 53929 | 53.03306 | –27.84798 | 1.0431 | 23.79 | 16.6 | 1 | 9 | HAG_J033207.93-275052.7_UDFNICP2 | |
| 58236 | 53.07825 | –27.80578 | 0.9993 | 24.53 | 12.7 | 2 | 9 | HAG_J033218.78-274820.8_J94SA3CIQ | |
| 59257 | 53.17618 | –27.79613 | 0.9961 | 22.39 | 22.8 | 9 | 34 | HAG_J033242.28-274746.1_J8G6I3PEQ | |
| 61554 | 53.14792 | –27.77405 | 1.0874 | 22.25 | 34.3 | 10 | 16 | HAG_J033235.50-274626.6_J8G6I3PEQ | |
| 61983 | 53.00104 | –27.77013 | 1.0321 | 23.70 | — | 2 | 14 | HAG_J033200.25-274612.5_UDFNICP2 | |
| 62478 | 53.01969 | –27.76527 | 1.0795 | 23.36 | 16.4 | 1 | 5 | HAG_J033204.72-274555.0_UDFNICP2 | |
| 62522 | 53.06233 | –27.76517 | 1.2262 | 23.73 | 12.9 | 1 | 15 | HAG_J033214.96-274554.6_J94SPDCSQ | |
| 63294 | 53.12040 | –27.75701 | 0.9535 | 23.50 | 14.9 | 5 | 39 | HAG_J033228.90-274525.2_J94SPDCSQ | |
| 63984 | 53.10560 | –27.75079 | 0.9731 | 23.18 | 6.3 | 4 | 56 | HAG_J033225.34-274502.9_J94SPDCSQ | |
| 66235 | 53.04549 | –27.72864 | 0.9983 | 22.69 | 29.7 | 3 | 6 | HAG_J033210.92-274343.1_J9FAA3IBQ | |
| 69377 | 53.07893 | –27.69774 | — | 22.74 | 12.2 | 3 | 24 | HAG_J033218.94-274151.9_J9FAA3IBQ | |
| 69919 | 53.04692 | –27.69087 | 1.0595 | 23.31 | 7.0 | 4 | 64 | HAG_J033211.26-274127.1_J9FAA3IBQ | |
Notes. IDs are from Burgarella et al. (2007); RA and Dec (in J2000) from the grism position; MV is the isophotal magnitude from the GOODS-S catalogue v.2.0; FWHM are measured in the z band from the GOODS-S catalogue. The last columns give number of overlapping grism spectra on each source (with different orientation angles), the number of extracted SED points for each object, and an example ID for the grism spectra. Notes on redshifts give the source of the ground-based redshift: 1) VVDS (Le Fèvre et al. 2005); 2) IMAGES (Ravikumar et al. 2007); 3) FORS (Vanzella et al. 2008); 4) K20 (Mignoli et al. 2005) and 5) VIMOS (Balestra et al. 2010).
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