G. Clementini

Computation of the Fourier parameters of RR Lyrae stars by template fitting

The Luminous Type Ic Supernova 1992ar at z = 0.145

The influence of chemical composition on the properties of Cepheid stars

Na-O anticorrelation and horizontal branches

Abundances of four open clusters from solar stars

Big-bang nucleosynthesis in a Brans-Dicke cosmology with a varying $\mathsf{\Lambda}$ term related to WMAP

The distance to the Galactic centre based on Population II Cepheids and RR Lyrae stars

The effect of metallicity on Cepheid period-luminosity relations from a Baade-Wesselink analysis of Cepheids in the Milky Way and Magellanic Clouds

Simulations of the formation, evolution and clustering of galaxies and quasars

Phantom Energy: Dark Energy withw<−1Causes a Cosmic Doomsday

Properties of galaxies reproduced by a hydrodynamic simulation

ANALYSIS OF SPIN-ORBIT ALIGNMENT IN THE WASP-32, WASP-38, AND HAT-P-27/WASP-40 SYSTEMS

NO EXCESS OF RR LYRAE STARS IN THE CANIS MAJOR OVERDENSITY

The Galactic Center massive black hole and nuclear star cluster

HipparcosParallaxes and the Cepheid Distance Scale

47 Tucanae: The Spectroscopic versus Color‐Magnitude Diagram Age Discrepancy

The cosmological constant and dark energy

WASP-128b: a transiting brown dwarf in the dynamical-tide regime

A Local Hubble Bubble from Type Ia Supernovae?

EXTENDING THE NEARBY GALAXY HERITAGE WITHWISE: FIRST RESULTS FROM THEWISEENHANCED RESOLUTION GALAXY ATLAS

The Distance to the Galactic Center

Cepheid Calibrations from theHubble Space Telescopeof the Luminosity of Two Recent Type Ia Supernovae and a Redetermination of the Hubble Constant

Results from the High-z Supernova Search Team

Near-infrared variability study of the central 2.3 × 2.3 arcmin2 of the Galactic Centre – II. Identification of RR Lyrae stars in the Milky Way nuclear star cluster

High‐Redshift Supernova Rates

Type Ia Supernova Discoveries atz> 1 from theHubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution

Accurate spectroscopic parameters of WASP planet host stars★

Supernova Ia Constraints on a Time‐variable Cosmological “Constant”

Updated Big Bang Nucleosynthesis Compared withWilkinson Microwave Anisotropy ProbeObservations and the Abundance of Light Elements

Microwave cavity searches for dark-matter axions

Stellar Orbits around the Galactic Center Black Hole

Cosmic Microwave Background Anisotropy Constraints on Open and Flat‐Λ Cold Dark Matter Cosmogonies from UCSB South Pole, ARGO, MAX, White Dish, and SuZIE Data

Particle dark matter: evidence, candidates and constraints

Evidence for a Long‐standing Top‐heavy Initial Mass Function in the Central Parsec of the Galaxy

f(R)theories of gravity

Will Jets Identify the Progenitors of Type I[CLC]a[/CLC] Supernovae?

The Carnegie-Chicago Hubble Program. VIII. An Independent Determination of the Hubble Constant Based on the Tip of the Red Giant Branch*

Molecular and atomic gas along and across the main sequence of star-forming galaxies

Hubble tension or a transition of the Cepheid SnIa calibrator parameters?

The Luminous Type Ic Supernova 1992ar at \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $z=0.145$ \end{document}

The effect of metal enrichment and galactic winds on galaxy formation in cosmological zoom simulations

On the variation of the initial mass function

Stellar population synthesis at the resolution of 2003

Snapshot Distances to Type Ia Supernovae: All in “One” Night's Work

Monte Carlo Simulations of Type Ia Supernova Observations in Supernova Surveys

USING ULTRA LONG PERIOD CEPHEIDS TO EXTEND THE COSMIC DISTANCE LADDER TO 100 Mpc AND BEYOND

Rossiter-McLaughlin effect measurements for WASP-16, WASP-25 and WASP-31★

New Low-mass Eclipsing Binary Systems in Praesepe Discovered by K2

A Large Stellar Evolution Database for Population Synthesis Studies. I. Scaled Solar Models and Isochrones

On the Globular Cluster Initial Mass Function below 1 \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $M_{\odot }$ \end{document}

THE UNIVERSAL STELLAR MASS-STELLAR METALLICITY RELATION FOR DWARF GALAXIES

LINE DERIVED INFRARED EXTINCTION TOWARD THE GALACTIC CENTER

Cepheid theoretical models and observations in HST/WFC3 filters: the effect on the Hubble constant H0

Discovery of an Unbound Hypervelocity Star in the Milky Way Halo

M31 PAndromeda Cepheid Sample Observed in Four HST Bands

Stellar populations and surface brightness fluctuations: new observations and models

Uniformity of (V−Near‐Infrared) Color Evolution of Type Ia Supernovae and Implications for Host Galaxy Extinction Determination

MONITORING STELLAR ORBITS AROUND THE MASSIVE BLACK HOLE IN THE GALACTIC CENTER

The Spectroscopic Orbit of the Planetary Companion Transiting HD 209458

The Age of Globular Clusters in Light ofHipparcos: Resolving the Age Problem?

A Definitive Measurement of Time Dilation in the Spectral Evolution of the Moderate-Redshift Type Ia Supernova 1997ex

A REDETERMINATION OF THE HUBBLE CONSTANT WITH THEHUBBLE SPACE TELESCOPEFROM A DIFFERENTIAL DISTANCE LADDER

First‐Year Wilkinson Microwave Anisotropy Probe ( WMAP ) Observations: Determination of Cosmological Parameters

The First Type Ia Supernovae: An Empirical Approach to Taming Evolutionary Effects in Dark Energy Surveys from SNe Ia atz > 2

Near-infrared variability study of the central 2.3 arcmin × 2.3 arcmin of the Galactic Centre – I. Catalogue of variable sources

THE RISE AND FALL OF TYPE Ia SUPERNOVA LIGHT CURVES IN THE SDSS-II SUPERNOVA SURVEY

A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km s⁻¹ Mpc⁻¹ Uncertainty from the Hubble Space Telescope and the SH0ES Team

The Adequacy of Stellar Evolution Models for the Interpretation of the Color-Magnitude Diagrams of Resolved Stellar Populations

A 3% SOLUTION: DETERMINATION OF THE HUBBLE CONSTANT WITH THEHUBBLE SPACE TELESCOPEAND WIDE FIELD CAMERA 3

The Magnification of SN 1997[CLC]ff[/CLC], the Farthest Known Supernova

Improved Distances to Type Ia Supernovae with Multicolor Light‐Curve Shapes: MLCS2k2

An interferometric CO survey of luminous submillimetre galaxies

SINFONI Integral Field Spectroscopy ofz∼ 2 UV‐selected Galaxies: Rotation Curves and Dynamical Evolution

TheCOBEDiffuse Infrared Background Experiment Search for the Cosmic Infrared Background. IV. Cosmological Implications

Updated nucleosynthesis constraints on unstable relic particles

Reconciliation of the Surface Brightness Fluctuation and Type Ia Supernova Distance Scales

On the Origin of the UV Upturn in Elliptical Galaxies. I. Sensitivity of UV Population Synthesis to Various Input Parameters

ellc: A fast, flexible light curve model for detached eclipsing binary stars and transiting exoplanets

A Geometric Determination of the Distance to the Galactic Center

Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant

Metal abundances of RR Lyrae stars in the bar of the Large Magellanic Cloud

Distances and ages of NGC 6397, NGC 6752 and 47 Tuc

Period–luminosity–metallicity relation of classical Cepheids

Variable Stars in the Newly Discovered Milky Way Dwarf Spheroidal Satellite Canes Venatici I

Standard Galactic Field RR Lyrae. I. Optical to Mid-infrared Phased Photometry

The VMC survey – XXV. The 3D structure of the Small Magellanic Cloud from Classical Cepheids

The metal abundance distribution of the oldest stellar component in the Sculptor dwarf spheroidal galaxy^★

RR Lyrae Variable Stars in the Dwarf Spheroidal Galaxy Leo I

Metallicities for Double-Mode RR Lyrae Stars in the Large Magellanic Cloud

A δ Scuti Distance to the Large Magellanic Cloud

The Composition of HB Stars: RR Lyrae Variables

On the Newly Discovered Canes Venatici II dSph Galaxy

I Zw 18 Revisited withHSTACS and Cepheids: New Distance and Age

Ages of Globular Clusters fromHIPPARCOSParallaxes of Local Subdwarfs

Gaia’s Cepheids and RR Lyrae stars and luminosity calibrations based on Tycho-Gaia Astrometric Solution

MULTI-EPOCHHUBBLE SPACE TELESCOPEOBSERVATIONS OF IZw18: CHARACTERIZATION OF VARIABLE STARS AT ULTRA-LOW METALLICITIES

The VMC survey – XXVI. Structure of the Small Magellanic Cloud from RR Lyrae stars

On the giant, horizontal and asymptotic branches of Galactic globular clusters - IV. CCD photometry of NGC 1904

Eclipsing binary stars in the Large Magellanic Cloud: results from the EROS-2, OGLE and VMC surveys★

Distance to the Large Magellanic Cloud: The RR Lyrae Stars

Cepheid metallicity in the Leavitt law (C-metall) survey – I. HARPS-N@TNG spectroscopy of 47 classical Cepheids and 1 BL Her variables

RR Lyrae and Short-Period Variable Stars in the Dwarf Irregular Galaxy NGC 6822

The lithium content of the globular cluster\nNGC 6397

The VMC survey. I. Strategy and first data

Metal Abundances of RR Lyrae Stars in the Metal-rich Globular Cluster NGC 6441

PULSATION MODELS FOR ULTRA-LOW (Z= 0.0004) METALLICITY CLASSICAL CEPHEIDS