- (Submitted to ApJ comments welcome) Evidence for Two Kinematically Distinct Broad Emission Line
- Submitted to Publications of the Astronomical Society of the Pacific Preprint typeset using LATEX style emulateapj v. 03/07/07
- arXiv:0711.1025v1[astro-ph]7Nov2007 Submitted to Astrophysical Journal
- arXiv:0711.1013v1[astro-ph]7Nov2007 Submitted to Astrophysical Journal
- arXiv:0711.1019v1[astro-ph]7Nov2007 Submitted to ApJ Letters
- arXiv:0809.4742v2[astro-ph]30Sep2008 Astronomy Letters -in press
- The Astronomical Journal, 135:264267, 2008 January doi:10.1088/0004-6256/135/1/264 c 2008. The American Astronomical Society. All rights reserved. Printed in the U.S.A.
- THE CASE FOR OPTICALLY THICK HIGH-VELOCITY BROAD-LINE REGION GAS IN ACTIVE GALACTIC NUCLEI
- The Central Engine of Active Galactic Nuclei ASP Conference Series, Vol. 373, 2007
- arXiv:astro-ph/0701165v17Jan2007 Black Holes: from Stars to Galaxies across the Range of Masses Proceedings IAU Symposium No. 238, 2006
- The Central Engine of Active Galactic Nuclei ASP Conference Series, Vol. 373, 2007
- A&A 461, 121134 (2007) DOI: 10.1051/0004-6361:20065390
- arXiv:0711.2113v1[astro-ph]14Nov2007 To appear in "The Nuclear Region, Host Galaxy, and Environment ofActive Galaxies (2007)"RevMexAA(SC)
- A&A 465, 129145 (2007) DOI: 10.1051/0004-6361:20053555
- arXiv:0805.4258v3[astro-ph]29May2008 Submitted to Astrophysical Journal
- HUBBLE SPACE TELESCOPE ULTRAVIOLET SPECTROSCOPY OF 14 LOW-REDSHIFT QUASARS1 Rajib Ganguly,2
- arXiv:0711.4356v1[astro-ph]27Nov2007 Mon. Not. R. Astron. Soc. 000, 1?? (2007) Printed 29 November 2007 (MN LATEX style file v2.2)
- arXiv:0807.2889v1[astro-ph]17Jul2008 Mem. S.A.It. Vol. 79, 1
