Eric P. Rubenstein

The CORALIE survey for southern extra-solar planets

The HARPS search for southern extra-solar planets

WASP-8b: a retrograde transiting planet in a multiple system

Evidence of a massive planet candidate orbiting the young active K5V star BD+20 1790

The thermal emission of the young and massive planet CoRoT-2b at 4.5 and 8 μm

Evidence against the young hot-Jupiter around BD +20 1790

The HARPS search for southern extra-solar planets

The CORALIE survey for southern extra-solar planets

Lower limits on the Hubble constant from models of type Ia supernovae

The HARPS search for southern extra-solar planets

The HARPS search for southern extrasolar planets

The HARPS search for southern extra-solar planets

The HARPS search for southern extra-solar planets

The CORALIE survey for southern extrasolar planets

The CORALIE survey for southern extra-solar planets

The CORALIE survey for southern extra-solar planets

The HARPS search for southern extra-solar planets

SALT: a spectral adaptive light curve template for type Ia supernovae

The HARPS search for southern extra-solar planets

The HARPS search for Earth-like planets in the habitable zone

The HARPS search for southern extra-solar planets

The HARPS search for southern extra-solar planets

Lithium in stars with exoplanets

TheSpitzersearch for the transits of HARPS low-mass planets

The HARPS survey for southern extra-solar planets

The HARPS search for southern extra-solar planets

The HARPS search for southern extra-solar planets

TheSpitzersearch for the transits of HARPS low-mass planets

The HARPS search for southern extra-solar planets

A global analysis ofSpitzerand new HARPS data confirms the loneliness and metal-richness of GJ 436 b

Fundamental photon noise limit to radial velocity measurements

The HARPS search for southern extra-solar planets

An asymptotic-giant-branch star in the progenitor system of a type Ia supernova

Optical and Near‐Infrared Photometry of the Type Ia Supernova 2000E in NGC 6951

SECONDARY PARAMETERS OF TYPE Ia SUPERNOVA LIGHT CURVES

Formation of massive black holes through runaway collisions in dense young star clusters

Possible thermochemical disequilibrium in the atmosphere of the exoplanet GJ 436b

Optical Photometry and Spectroscopy of the SN 1998bw–like Type Ic Supernova 2002ap

Late‐Time Observations of SN 2006gy: Still Going Strong

SNLS Spectroscopy: Testing for Evolution in Type Ia Supernovae

Statistical Properties of Exoplanets

Variable Stars in Galactic Globular Clusters

Photometry of the Type Ia Supernovae 1999cc, 1999cl, and 2000cf

Optical and infrared observations of SN 2002dj: some possible common properties of fast-expanding Type Ia supernovae

Hot Jupiters and Hot Spots: The Short‐ and Long‐Term Chromospheric Activity on Stars with Giant Planets

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

Time Evolution of the Magnetic Activity Cycle Period. II. Results for an Expanded Stellar Sample

Anomalous extinction behaviour towards the Type Ia SN 2003cg

FIVE-YEARWILKINSON MICROWAVE ANISOTROPY PROBEOBSERVATIONS: COSMOLOGICAL INTERPRETATION

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

THE MOUNT WILSON OBSERVATORY S-INDEX OF THE SUN

Magnetic field, differential rotation and activity of the hot-Jupiter-hosting star HD 179949

THE MEAN TYPE IA SUPERNOVA SPECTRUM OVER THE PAST NINE GIGAYEARS

Extra-solar planets

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

SiFTO: An Empirical Method for Fitting SN Ia Light Curves

RESULTS OF THE LICK OBSERVATORY SUPERNOVA SEARCH FOLLOW-UP PHOTOMETRY PROGRAM: BVRI LIGHT CURVES OF 165 TYPE Ia SUPERNOVAE

The Deepest Supernova Search is Realized in the Hubble Ultra Deep Field Survey

Optical and Infrared Photometry of the Unusual Type Ia Supernova 2000cx

Is There Evidence for a Hubble Bubble? The Nature of Type Ia Supernova Colors and Dust in External Galaxies

A Light Echo from Type Ia SN 1995E?

On the ages of exoplanet host stars

Reddening, Absorption, and Decline Rate Corrections for a Complete Sample of Type Ia Supernovae Leading to a Fully Corrected Hubble Diagram tov< 30,000 km s⁻¹

The ExtendedHSTSupernova Survey: The Rate of SNe Ia atz> 1.4 Remains Low

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

WASP-80b has a dayside within the T-dwarf range

The farthest known supernova: Support for an accelerating universe and a glimpse of the \nepoch of deceleration

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

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

CEPHEID CALIBRATIONS OF MODERN TYPE Ia SUPERNOVAE: IMPLICATIONS FOR THE HUBBLE CONSTANT

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

GC-IRS13E—A PUZZLING ASSOCIATION OF THREE EARLY-TYPE STARS

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

Optical and Infrared Photometry of the Nearby Type I[CLC]a[/CLC] Supernova 2001[CLC]el[/CLC]

MODULES FOR EXPERIMENTS IN STELLAR ASTROPHYSICS (MESA): PLANETS, OSCILLATIONS, ROTATION, AND MASSIVE STARS

The Luminous Type Ic Supernova 1992ar at z = 0.145

The orbital period changes of UX Ursae Majoris

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}

Are Superflares on Solar Analogues Caused by Extrasolar Planets?

The Search for Main Sequence Binary Stars in Galactic Globular Clusters

[ITAL]Hubble Space Telescope[/ITAL] Observations of the Post–Core-Collapse Globular Cluster NGC 6752: A Search for Cataclysmic Variables

Optical Photometry of the Type I[CLC]a[/CLC] Supernova 1999[CLC]ee[/CLC] and the Type I[CLC]b[/CLC]/[CLC]c[/CLC] Supernova 1999[CLC]ex[/CLC] in IC 5179