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Phys443: Extragalactic Astronomy and Cosmology
Papers for Thursday, March 28
Add your name and a reference to your paper to the list below.
You may not choose a paper which someone else has already
selected. The paper must have some connection to AGN and
must have been published since 2010.
Photometric reverberation mapping of 3C120
Spitzer Mid-IR Spectroscopy of Powerful 2 Jy and 3CRR Radio Galaxies
A near-infrared relationship for estimating black hole masses in active galactic nuclei
Measuring the dark matter halo mass of X-ray AGN at z ∼ 1using photometric redshifts
Thermal and Dynamical Properties of Gas Accreting onto a SMBH in an AGN
Integral Field Spectroscopy of Massive, Kiloparsec-Scale Outflows in the Infrared-Luminous QSO Mrk 231
Cause and Effect of Feedback: Multiphase Gas in Cluster Cores Heated by AGN Jets
Quasar feedback: accelerated star formation and chaotic accretion
Far-infrared Properties of Type 1 Quasars
Galaxy Zoo : Bulgeless Galaxies with Growing Black Holes
Orientation Effects on the Inner Region of Dusty Torus of AGN
Feeding versus feedback in AGNs from near-infrared IFU observations: the case of Mrk 79
Identification of Outflows and Candidate Dual Active Galactic Nuclei in SDSS Quasars at z=0.8-1.6
A deep X-ray observation of NGC 4258 and its surrounding field
THE BLACK HOLE-BULGE MASS RELATION OF ACTIVE GALACTIC NUCLEI IN THE EXTENDED CHANDRA DEEP FIELD-SOUTH SURVEY
Papers for Thursday, April 18
Choose a paper which describes a method for determining the distance to the LMC,
and a result. You may not choose a paper which someone else has already chosen.
On the distance of the Magellanic Clouds using Cepheid NIR and optical-NIR Period Wesenheit Relations
An eclipsing-binary distance to the Large Magellanic Cloud accurate to two per cent
Distance To The Large Magellanic Cluster: The RR Lyrae Star
The Properties of the Large Magellanic Cloud Based on OGLE III Photometry of RR Lyrae Stars
The Distance to the Large Magellanic Cloud from the Eclipsing Binary HV 2274
The Distance to the Large Magellanic Cloud Cluster NGC 1866 and the Surrounding Field
A new Large Magellanic Cloud K-band distance from precision measurements of nearby red clump stars
Distance to SN 1987A and the LMC
Distances of the Galactic Cepheids, Magellanic Clouds, and Globular Clusters
Dmitry "Flux Capacitor" Vorobiev:
The tip of the red giant branch and distance of the Magellanic Clouds
A ``Pulsational'' Distance Determination for the Large Magellanic Cloud
Globular clusters and the Mira period–luminosity relation
Three-dimensional Maps of the Magellanic Clouds using RR Lyrae Stars and Cepheids. I. The Large Magellanic Cloud
Calibrating the Cepheid period-luminosity relation from the infrared surface brightness technique. II. The effect of metallicity and the distance to the LMC
The Araucaria Project. Determination of the Large Magellanic Cloud Distance from Late-Type Eclipsing Binary Systems. I.
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