- Bibliography (1) Tripp, T.M., Jenkins, E.B., Bowen, D.V., Prochaska, J.X., Aracil, B., & Ganguly,
- ApJL: Accepted November 11, 1998 Preprint typeset using L A T E X style emulateapj
- The Evolution of Galaxies on Cosmological Timescales ASP Conference Series, Vol. 3 10 8
- Draft version March 6, 2000 Preprint typeset using L A T E X style emulateapj
- Draft version May 18, 2000 Preprint typeset using L A T E X style emulateapj v. 20/04/00
- AJ: December 15, 1998 Preprint typeset using L A T E X style emulateapj
- Table 8. ABUNDANCES FOR G66-51 Ion N [X/Fe]d [X/Fe]n [X/Fe]
- Table 19. HFS TABLES Ion ( A) EP (eV) log gf
- Accepted to the Astrophysical Journal Supplements: June 8, 2001 Preprint typeset using L A T E X style emulateapj v. 20/04/00
- arXiv:astro-ph/0602172v17Feb2006 Accepted to ApJ: January 30, 2006 Preprint typeset using LATEX style emulateapj v. 20/04/00
- Probing the IGM/Galaxy Connection IV: The LCO/WFCCD Galaxy Survey of 20 Fields Surrounding UV Bright Quasars
- HIRedux Pipeline Jason X. Prochaska
- arXiv:0706.1285v1[astro-ph]9Jun2007 Draft 1: June 12, 2007
- arXiv:astroph/0202140 Accepted to the Astrophysical Journal: Feb 5, 2002
- Accepted to ApJ: August 15, 2005 Preprint typeset using L A T E X style emulateapj v. 20/04/00
- arXiv:astroph/0002449 Mon. Not. R. Astron. Soc. 000, 000--000 (0000) Printed 24 February 2000 (MN L A T E X style file v1.4)
- arXiv:astroph/0009081 accepted by the Astrophysical Journal August 5, 2000
- Accepted to the Astronomical Journal July 21, 2000 Preprint typeset using L A T E X style emulateapj v. 20/04/00
- Accepted to the Astrophysical Journal: Oct 12, 2001 Preprint typeset using L A T E X style emulateapj v. 20/04/00
- Determining the Physical Nature of the Damped Lyff Systems by Investigating their Kinematic Characteristics
- Damped Lyman Alpha Systems at High Redshift and Models of Protogalactic Disks
- 4000 4200 4400 4600 4800 5000 5200 5400 Row Arc 2D FIT (Res x500) nx=4 ny=4 RMS=0.1054Ang*Order#Arc 2D FIT (Res x500) nx=4 ny=4 RMS=0.1054Ang*Order#Arc 2D FIT (Res x500) nx=4 ny=4 RMS=0.1054Ang*Order#Arc 2D FIT (Res x500) nx=4 ny=4 RMS=0.1054Ang*Order#Arc
- arXiv:astro-ph/0408294v116Aug2004 Accepted to the Astrophysical Journal: August 12, 2004 Preprint typeset using LATEX style emulateapj v. 20/04/00
- arXiv:astroph/0009082 accepted by the Astrophysical Journal August 5, 2000
- arXiv:astro-ph/0507621v126Jul2005 Accepted for publication in the Astrophysical Journal Letters Preprint typeset using LATEX style emulateapj v. 20/04/00
- Wavelength (Ang) Residual(Pix)
- ApJ: Accepted May 21, 1998 Preprint typeset using L A T E X style emulateapj
