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For refcode 2009ApJS..182..628V:
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2009ApJS..182..628V Spitzer Quasar and Ulirg Evolution Study (QUEST). IV. Comparison of 1 Jy Ultraluminous Infrared Galaxies with Palomar-Green Quasars Veilleux, S.; Rupke, D. S. N.; Kim, D.-C.; Genzel, R.; Sturm, E.; Lutz, D.; Contursi, A.; Schweitzer, M.; Tacconi, L. J.; Netzer, H.; Sternberg, A.; Mihos, J. C.; Baker, A. J.; Mazzarella, J. M.; Lord, S.; Sanders, D. B.; Stockton, A.; Joseph, R. D.; Barnes, J. E. Abstract. We report the results from a comprehensive study of 74 ultraluminous infrared galaxies (ULIRGs) and 34 Palomar-Green (PG) quasars within z ~ 0.3 observed with the Spitzer Infrared Spectrograph (IRS). The contribution of nuclear activity to the bolometric luminosity in these systems is quantified using six independent methods that span a range in wavelength and give consistent results within ~+/-10%-15% on average. This agreement suggests that deeply buried active galactic nuclei (AGNs) invisible to Spitzer IRS but bright in the far-infrared are not common in this sample. The average derived AGN contribution in ULIRGs is ~35%-40%, ranging from ~15%-35% among "cool" (f_25_/f_60_ <= 0.2) optically classified H II-like and LINER ULIRGs to ~50 and ~75% among warm Seyfert 2 and Seyfert 1 ULIRGs, respectively. This number exceeds ~80% in PG QSOs. ULIRGs fall in one of three distinct AGN classes: (1) objects with small extinctions and large polycyclic aromatic hydrocarbon (PAH) equivalent widths are highly starburst-dominated; (2) systems with large extinctions and modest PAH equivalent widths have larger AGN contributions, but still tend to be starburst-dominated; and (3) ULIRGs with both small extinctions and small PAH equivalent widths host AGN that are at least as powerful as the starbursts. The AGN contributions in class 2 ULIRGs are more uncertain than in the other objects, and we cannot formally rule out the possibility that these objects represent a physically distinct type of ULIRGs. A morphological trend is seen along the sequence (1)-(2)-(3), in general agreement with the standard ULIRG--QSO evolution scenario and suggestive of a broad peak in extinction during the intermediate stages of merger evolution. However, the scatter in this sequence, including the presence of a significant number of AGN-dominated systems prior to coalescence and starburst-dominated but fully merged systems, implies that black hole accretion, in addition to depending on the merger phase, also has a strong chaotic/random component, as in local AGNs. Key words: galaxies: active, galaxies: interactions, galaxies: Seyfert, galaxies: starburst, infrared: galaxies, quasars: general =========================================================================== 2014ApJS..213...36V Erratum: "Spitzer Quasar and ULIRG Evolution Study (QUEST). IV. Comparison of 1 Jy Ultraluminous Infrared Galaxies with Palomar-Green Quasars" (2009, ApJS, 182, 628) Veilleux, S.; Rupke, D. S. N.; Kim, D.-C.; Genzel, R.; Sturm, E.; Lutz, D.; Contursi, A.; Schweitzer, M.; Tacconi, L. J.; Netzer, H.; Sternberg, A.; Mihos, J. C.; Baker, A. J.; Mazzarella, J. M.; Lord, S.; Sanders, D. B.; Stockton, A.; Joseph, R. D.; Barnes, J. E. Abstract. Some of the entries listed in Tables 12 and 16 of the published manuscript were mistakenly transposed. 1. In Table 12, the entries under Column 6 should have been listed under Column 7, and vice versa. 2. In Table 16, the entries under Column 6 should have been listed under Column 7, and vice versa. Similarly, the entries under Column 13 should have been listed under Column 14, and vice versa. These errors only affect these tables; they have no impact on the results reported in the paper ===========================================================================
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