| Q | Description |
|---|---|
| 4 | Rock-solid z value with at lest two clear features |
| 3 | Good z value, probability > 90% that it is correct, two features still required |
| 2 | Not usable, but spectrum should be revisited |
| 1 | Not usable and the data will never yield a redshift |
| 0 | Have not yet looked at the spectrum |
| -1 | Star |
| -2 | Cannot obtain a redshift due to bad reduction and/or instrumental effects |
| Code | Reference |
|---|---|
| 1 | Cowie, L. L. et al. 2004, A.J. submitted |
| 2 | Cohen, J. et al. 1996, Ap.J. 471, 5 |
| 3 | Cohen, J. et al. 2000, Ap.J. 538, 29 |
| 8 | Cohen, J., 2001 A.J. 121, 2895 |
| 9 | Phillips, A., et al. 1997, Ap.J. 489, 543 and Lowenthal, J., et al. 1997, Ap.J., 481, 673 |
| 11 | Dawson, S., et al. 2001, A.J., 122 598 |
| 12 | Steidel, C., et al. 2003, Ap.J. 592, 728 and Steidel, C., et al. 1999, Ap.J. 519, 1 |
| 15 | Dickinson, M., 1998, The Hubble Deep Field: (Edited by Mario Livio, S. Michael Fall, and Piero Madau. New York : Cambridge University Press) 219 |
| 17 | Zepf, S. E., Moustakas, L. A., & Davis, M. 1997, ApJ, 474, L1 and Moustakas (private communication, data available at http://www-astro.physics.ox.ac.uk/~leonidas/ucbhdf/ |
| 18 | Cowie et al. 1996, http://www.ifa.hawaii.edu/~cowie/hdflank/hdflank.html |
| 19 | Bunker. A., Spinrad, H. Stern, D., Thompson, Ro.m Moustakas, L., Davis, M. and Dey, A. 2000, Proceedings of the "Galaxies in the Young Universe II" , eds. H. Hippelein and K. Meisenheimer (Berlin: Springer-Verlag), astroph/0004348 |