The overarching goal of our project is to characterize planetary systems orbiting cool dwarfs observed by K2. Accordingly, we selected our targets from the set of planet...

Our initial stellar sample is retrieved from version 7 of the TESS Input Catalog (TIC-7), which is accessed via the Barbara A. Mikulski Archive for Space Telescope (MAST) Portal...

Coordinates, VIJHKs photometry, stellar surface parameters, [Fe/H], [Mg/Fe] and [Ca/Fe] abundance ratios for a sample of 400 red clump stars in the four high-resolution GIBS...

Absolute photometry (ROSAT X-ray, GALEX UV, APASS gri, 2MASS JHKs, and WISE W1 to W4) and physical parameters of the Hyades single-star sequence members. The "Resolution" column...

Observations were made with the Wide Field and Planetary Camera 2 (WFPC2) aboard HST as part of General Observer program 6685. The data consist of multiple images through the...

Our study utilizes the public data and catalogs from multi-band deep surveys of the COSMOS field. The UltraVISTA survey (McCracken+ 2012, J/A+A/544/A156) provides ultra-deep...

TESS (Ricker et al. 2015JATIS...1a4003R) is currently conducting a year-long photometric monitoring campaign of the southern sky. TESS scans the sky in a series of sectors for...

Library of 30 rest-frame FUV-to-FIR stacked SEDs and templates of LBGs at z~3. For each stacked LBG, the library includes the stacked photometry at optical (BVriz bands),...

The WASP FP catalogue contains entries for each star that has been dispositioned after additional observation.

The HCV catalog (tableb2) lists for each source the equatorial coordinates, MatchID, GroupID, subgroup, the pipeline classification flag, the expert-validation classification...

Table A.1: List of new asteroid models. For each asteroid, we list one or two pole directions in the ecliptic coordinates ({lambda}, {beta}), the sidereal rotation period P, the...

V and I time-series CCD photometry for known variables in the 5.4'x5.4' filed of view of NGC 1261.

The Hipparcos and Tycho Catalogues are the primary products of the European Space Agency's astrometric mission, Hipparcos. The satellite, which operated for four years,...

Our paper is based on images acquired with the 1.0-m Swope telescope using the 2048x3150 SITE3 camera. The field of view was 14.8x22.8arcmin^2^ at a scale of 0.435 arcsec/pixel....

Light curve files for the 20573 simulated TESS light curves. The directory structure flows through the different parameters used in the simulations: Spectral class >...

The photometric detection of the exoplanets presented in this work was made with the HATSouth units based in Las Campanas Observatory (LCO; HS-1 and HS-2), at the HESS site in...

OGLE 4 Galactic Cepheids.

Two data sets are used for the analysis here: stars with unusually deep transits in NASA's four-year Kepler mission (Borucki et al. 2010Sci...327..977B), and stars with...

A first spectroscopic run carried out in 2006 March with the du Pont telescope at Las Campanas Observatory (LCO) allowed us to corroborate the quasar nature of our sample and...

We selected our sample of star-forming galaxies from the COSMOS2015 photometric catalog (Laigle+ 2016, J/ApJS/224/24). After applying the selection criteria described in Section...