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JADES and FRESCO Ha-emitting galaxies at z=5.1-5.5
HDF850.1 is the brightest submillimeter galaxy (SMG) in the Hubble Deep Field. It is known as a heavily dust-obscured star-forming galaxy embedded in an overdense environment at... -
California-Kepler Survey. VII. Planet radius gap
The distribution of planet sizes encodes details of planet formation and evolution. We present the most precise planet size distribution to date based on Gaia parallaxes, Kepler... -
M99 dust properties and photometry with NIKA2
Large dust grains in thermal equilibrium dominate the far-infrared emission of star-forming galaxies and contribute substantially to their millimetre continuum. Constraining... -
Deep UNCOVER-ALMA Legacy high-Z survey (DUALZ)
We present the survey design and initial results of the Atacama Large Millimeter/submillimeter Array (ALMA) Cycle 9 program of DUALZ, which aims to establish a joint ALMA and... -
Milky Way field giants from Gaia & APASS I-band
The calibration of the tip of the red giant branch (TRGB) in the I-band has a direct role in determinations of the Hubble constant, a subject of recent interest due to the... -
The UNCOVER phot. catalog of A2744 with HST+JWST
In 2022 November, the James Webb Space Telescope (JWST) returned deep near-infrared images of A2744-a powerful lensing cluster capable of magnifying distant, incipient galaxies... -
DESI observations of the Andromeda galaxy
We present Dark Energy Spectroscopic Instrument (DESI) observations of the inner halo of M31, which reveal the kinematics of a recent merger-a galactic immigration event-in... -
SEAMBHs. XI. Mrk 142 X-ray to optical light curves
We performed an intensive accretion disk reverberation mapping campaign on the high accretion rate active galactic nucleus Mrk142 in early 2019. Mrk 142 was monitored with the... -
SEAMBHs. V. The third year
This paper reports results of the third-year campaign of monitoring super-Eddington accreting massive black holes (SEAMBHs) in active galactic nuclei (AGNs) between 2014 and... -
Milky Way as seen by classical Cepheids. I. WISE
Classical Cepheids are the archetype of the standard candle, thanks to the period-luminosity relation, which allows us to measure their intrinsic brightness. They are also... -
Galactic center maser-bearing Miras
This sample of 370 Mira variables that are likely near the Galactic center (GC) has been selected from the OGLE and BAaDE surveys based on their sky coordinates, OGLE... -
EL COSMOS DR1 spectra
Synthetic spectra of COSMOS2015 sources -
KMTNet Synoptic Survey of Southern Sky (KS4) DR1
We present the first public data release (DR1) of the KMTNet Synoptic Survey of Southern Sky (KS4). This deep, wide-field imaging survey covers a southern footprint of... -
EL COSMOS DR1 catalogue
Modeled magnitudes and emission line fluxes of COSMOS2015 sources -
ASPIC VIPERS catalogue on W4 field
Photometry, physical parameters and spectral features of VIPERS PDR-2 sources on W4 field. -
ASPIC VIPERS catalogue on W1-VIDEO field
Photometry, physical parameters and spectral features of VIPERS PDR-2 sources on W1-VIDEO field. -
ASPIC GAMA catalogue on G09 G12 G15 fields
ASPIC value-added catalogue on GAMA G09, G12, and G15 fields. -
ASPIC GAMA catalogue on G02 field
ASPIC value-added catalogue on GAMA G02 field. -
ASPIC VUDS-DR1 catalogue on ECDFS field
Photometry, spectral features, and physical parameters of VUDS (DR1) sources on ECDFS field. -
ASPIC VIPERS catalogue on W1 field
Photometry, physical parameters and spectral features of VIPERS PDR-2 sources on W1 field.
