The ISO view of Palomar-Green quasars

By M. Haas, U. Klaas, S. A. H. Müller, F. Bertoldi, M. Camenzind, Rolf Chini, O. Krause, D. Lemke, K. Meisenheimer, P. J. Richards and 1 more. 2003

142 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Instrumentation

View Paper: https://www.semanticscholar.org/paper/fac01a464395236c90c01a77adcf02938a4be811

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Citations in the corpus

The X-Ray Spectral Properties of SCUBA Galaxies (2005, background): “Although the large fraction of obscured AGNs in our sample suggests that the dust-covering factor is large in these SMGs, the dust-covering factor of quasars is uncertain and may depend on the evolutionary state or nature of individual objects (e.g., Haas et al. 2003; Page et al. 2004).”
Spitzer Quasar and ULIRG Evolution Study (QUEST). I. The Origin of the Far-Infrared Continuum of QSOs (2006, background): “A similar test remains to be done for the highest luminosity members of the Haas et al. (2003) sample, which are not sufficiently represented in our local PG sample or in the IRS spectra of radio galaxies and radio-loud QSOs of Haas et al. (2005).”
The Distribution of Silicate Strength in Spitzer Spectra of AGNs and ULIRGs (2006, background): “The distribution of the mid-IR properties of different types of known AGNs has been discussed in various studies (Heckman et al. 1994; Haas et al. 2003; Siebenmorgen et al. 2004; Clavel et al. 2000; Shi et al. 2006; Buchanan et al. 2006).”
Spitzer Quasar and ULIRG Evolution Study (QUEST). II. The Spectral Energy Distributions of Palomar-Green Quasars (2007, methodology): “We also test the correlation of L(5100) with L(PAH 7.7µm) which was not available in the Haas et al. (2003) sample.”
Spitzer Observations of Massive, Red Galaxies at High Redshift (2005, background): “These IR luminosities are comparable to those of PG quasars at zk 1, which have warm thermal dust temperatures (Haas et al. 2003).”
A 158 μm [C ii] LINE SURVEY OF GALAXIES AT z ∼ 1–2: AN INDICATOR OF STAR FORMATION IN THE EARLY UNIVERSE (2010, methodology): “Based on their infrared SEDs, Haas et al. (2003) have argued that much, if not most of the FIR luminosity, has its origins in AGN activity.”
Radiation Pressure-supported Starburst Disks and Active Galactic Nucleus Fueling (2005, result): “Indeed, thebroad but sub-dominant IR peak and the magnitude of the AGN luminosity in our models are reasonably consistent with composite quasar spectra (Elvis et al. 1994; Haas et al. 2003).”
Dust covering factor, silicate emission, and star formation in luminous QSOs (2007, result): “We also note that a similar, independent result was obtained by Haas et al. (2003), who found that in a large sample of QSOs the ratio between LFIR (powered by star formation) and LB decreases at high luminosities.”
A DEEP HUBBLE SPACE TELESCOPE H-BAND IMAGING SURVEY OF MASSIVE GAS-RICH MERGERS. II. THE QUEST QSOs (2006, background): “…between ‘‘cool’’ ULIRGs (IRAS [Infrared Astronomical Satellite] 25 to 60 mflux ratio f25 /f60 < 0:2), ‘‘warm’’ ULIRGs, and QSOs (Sanders et al. 1988b; Haas et al. 2003) bring qualitative support to an evolutionary connection between these various classes of objects, but key elements remain…”