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= = 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.
 * Phys443: Extragalactic Astronomy and Cosmology**
 * Papers for Thursday, March 28**
 * Richmond: [|Photometric reverberation mapping of 3C120]
 * Magagnoli: [|Spitzer Mid-IR Spectroscopy of Powerful 2 Jy and 3CRR Radio Galaxies]
 * Punzi: [|A near-infrared relationship for estimating black hole masses in active galactic nuclei]
 * Elspeth Ochs: Measuring the dark matter halo mass of X-ray AGN at z ∼ 1using photometric redshifts
 * Bowen: [|Thermal and Dynamical Properties of Gas Accreting onto a SMBH in an AGN]
 * Rasskazov: [|Integral Field Spectroscopy of Massive, Kiloparsec-Scale Outflows in the Infrared-Luminous QSO Mrk 231]
 * Varnado: [|Cause and Effect of Feedback: Multiphase Gas in Cluster Cores Heated by AGN Jets]
 * Alex Hensley: [|Quasar feedback: accelerated star formation and chaotic accretion]
 * Zhang:Far-infrared Properties of Type 1 Quasars
 * Dmitry: [|Galaxy Zoo : Bulgeless Galaxies with Growing Black Holes]
 * Almeyda: [|Orientation Effects on the Inner Region of Dusty Torus of AGN]
 * Lipnicky: [|Feeding versus feedback in AGNs from near-infrared IFU observations: the case of Mrk 79]
 * Trinker: [|Identification of Outflows and Candidate Dual Active Galactic Nuclei in SDSS Quasars at z=0.8-1.6]
 * Bero: [|A deep X-ray observation of NGC 4258 and its surrounding field]
 * Alex Hab: THE BLACK HOLE-BULGE MASS RELATION OF ACTIVE GALACTIC NUCLEI IN THE EXTENDED CHANDRA DEEP FIELD-SOUTH SURVEY

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.
 * Papers for Thursday, April 18**


 * Punzi: [|On the distance of the Magellanic Clouds using Cepheid NIR and optical-NIR Period Wesenheit Relations]
 * Richmond: [|An eclipsing-binary distance to the Large Magellanic Cloud accurate to two per cent]
 * Varnado: [|Distance To The Large Magellanic Cluster: The RR Lyrae Star]
 * Almeyda: [|The Properties of the Large Magellanic Cloud Based on OGLE III Photometry of RR Lyrae Stars]
 * Bowen [|The Distance to the Large Magellanic Cloud from the Eclipsing Binary HV 2274]
 * Hensley: [|The Distance to the Large Magellanic Cloud Cluster NGC 1866 and the Surrounding Field]
 * Rasskazov: [| A new Large Magellanic Cloud K-band distance from precision measurements of nearby red clump stars]
 * Magagnoli: [|Distance to SN 1987A and the LMC]
 * Lipnicky: [|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]
 * Elspeth Ochs: [|A ``Pulsational'' Distance Determination for the Large Magellanic Cloud]
 * Zhang:Globular clusters and the Mira period–luminosity relation
 * Trinker: [|Three-dimensional Maps of the Magellanic Clouds using RR Lyrae Stars and Cepheids. I. The Large Magellanic Cloud]
 * Bero: [|Calibrating the Cepheid period-luminosity relation from the infrared surface brightness technique. II. The effect of metallicity and the distance to the LMC]-[|full text]
 * Habermann: [|The Araucaria Project. Determination of the Large Magellanic Cloud Distance from Late-Type Eclipsing Binary Systems. I.]

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