Articles 30
-
Gaia Data Release 3. A golden sample of astrophysical parameters
-
Classical Cepheid period-Wesenheit-metallicity relation in the Gaia bands
-
Gaia Early Data Release 3: Structure and properties of the Magellanic Clouds
-
Galactic spiral structure revealed by Gaia EDR3
-
Eridanus II: A Fossil from Reionization with an Off-center Star Cluster
-
Born in a Pair (?): Pisces II and Pegasus III*
-
Gaia Data Release 2. Variable stars in the colour-absolute magnitude diagram
-
Gaia Data Release 2. All-sky classification of high-amplitude pulsating stars
-
Gaia Data Release 2. Kinematics of globular clusters and dwarf galaxies around the Milky Way
-
Gaia Data Release 2. Mapping the Milky Way disc kinematics
-
Gaia Data Release 2. Observational Hertzsprung-Russell diagrams
-
Gaia Data Release 2. Observations of solar system objects
-
Gaia Data Release 2. The celestial reference frame (Gaia-CRF2)
-
SMHASH: a new mid-infrared RR Lyrae distance determination for the Local Group dwarf spheroidal galaxy Sculptor
-
The Carnegie-Chicago Hubble Program: Calibration of the Near-infrared RR Lyrae Period–Luminosity Relation with HST
-
Standard Galactic Field RR Lyrae. I. Optical to Mid-infrared Phased Photometry
-
Pulsating star research and the Gaia revolution
-
The Carnegie-Chicago Hubble Program. I. An independent approach to the extragalactic distance scale using only population II distance indicators
-
MOONS: the Multi-Object Optical and Near-infrared Spectrograph for the VLT
-
The star formation history of the very metal-poor blue compact dwarf I zw 18 from HST/ACS data
-
MOONS: a multi-object optical and near-infrared spectrograph for the VLT
-
Ultra long period Cepheids: a primary standard candle out to the Hubble flow
-
The ancient stellar population of M 32: RR Lyrae variable stars confirmed
-
Spatial distribution and evolution of the stellar populations and candidate star clusters in the blue compact dwarf I Zwicky 18
-
Pulsation models for ultra-low (Z = 0.0004) metallicity classical Cepheids
-
Multi-epoch Hubble space telescope observations of IZw18: characterization of variable stars at ultra-low metallicities
-
Variable Stars in the Newly Discovered Milky Way Dwarf Spheroidal Satellite Canes Venatici I
-
On the Newly Discovered Canes Venatici II dSph Galaxy
-
A New Age and Distance for I Zw 18, the Most Metal-Poor Galaxy in the Nearby Universe
-
I Zw 18 Revisited withHSTACS and Cepheids: New Distance and Age
Human - wd:Q61470581