Showing 1–20 of 20 results
/ Date/ Name
Dec 9, 2025Near-IR CO and CN in classical CepheidsOct 4, 2019Standard Galactic Field RR Lyrae II: A Gaia DR2 calibration of the period-Wesenheit-metallicity relationAug 16, 2019The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch MethodDec 14, 2018The Carnegie-Chicago Hubble Program: Calibration of the Near-Infrared RR Lyrae Period-Luminosity Relation With HSTSep 5, 2018The Carnegie-Chicago Hubble Program. V. The Distances to NGC 1448 and NGC 1316 via the Tip of the Red Giant BranchJul 19, 2018The Carnegie RR Lyrae Program: Mid-infrared Period-Luminosity relations of RR Lyrae stars in ReticulumJun 7, 2018The Carnegie-Chicago Hubble Program. IV. The Distances to NGC 4424, NGC 4526, and NGC 4536 via the Tip of the Red Giant BranchMay 4, 2017On a new theoretical framework for RR Lyrae stars II: Mid--Infrared Period--Luminosity--Metallicity RelationsMar 4, 2017Standard Galactic Field RR Lyrae. I. Optical to Mid-infrared Phased PhotometryApr 6, 2016The Carnegie-Chicago Hubble Program. I. An Independent Approach to the Extragalactic Distance Scale Using only Population II Distance IndicatorsMar 11, 2016The Carnegie Chicago Hubble Program: The Mid-Infrared Colours of Cepheids and the Effect of Metallicity on the CO Band-head at $4.6μ$mFeb 24, 2015The Carnegie Hubble Program: The Distance and Structure of the SMC as Revealed by Mid-infrared Observations of CepheidsSep 24, 2014A New Cepheid Distance Measurement and Method for NGC 6822Jul 28, 2014The Calibration of the WISE W1 and W2 Tully-Fisher RelationJun 24, 2013The Carnegie Hubble Program: The Infrared Leavitt Law in IC 1613Jan 21, 2013Calibration of the Mid-Infrared Tully-Fisher RelationSep 22, 2012The Carnegie Hubble Program: The Leavitt Law at 3.6 and 4.5 micron in the Milky WayAug 16, 2012Carnegie Hubble Program: A Mid-Infrared Calibration of the Hubble ConstantJun 18, 2012Stellar Archaeology in the Galactic halo with Ultra-Faint Dwarfs: VII. HerculesAug 23, 2011The Carnegie Hubble Program: The Leavitt Law at 3.6 μm and 4.5 μm in the Large Magellanic Cloud