DECam photometric data collected and used in this work (no table in the article, see Section 2).

In the second work of our project PATHOS, we applied our PSF-based approach to TESS FFIs in order to extract high-precision light curves of stars that belong to open clusters...

The data used in this work were obtained from two sites. The first set of data was obtained with the 0.80m IAC80 telescope at the Observatorio del Teide (Tenerife, Spain),...

Properties of variable stars and disk around "dippers" in 5 young stellar associations (ChI, ChII, CrA, Lup and Vel).

For this pilot work, we used FFIs collected in Sector-1. FFIs are obtained on board by co-adding series of 2s exposures into a 30min exposure time image. Observations have been...

The images used are the 16 target pixel files (TPFs) that make up the M4 superstamp from the Mikulski Archive for Space Telescopes; taken by the Kepler space telescope during...

The observations have been collected under the program 095.D-0290 (PI: Mucciarelli) and performed during the night of 2015 May 28 with the multi-object spectrograph FLAMES at...

We used Advanced Camera for Surveys (ACS) images for NGC4589 from the Hubble Space Telescope (HST) archive (PI: Smartt, ID: 10498 -- observations from November 2006). The...

The data come from the Magellanic Clouds Photometric Survey (MCPS) described by Zaritsky et al. (2002, Cat. ). In summary, we have obtained U, B, V, and I drift-scan images of...

We chose to make use of the Harris+ (2013, J/ApJ/772/82) catalog of 422 galaxies with published measurements of globular cluster (GC) population properties. See Section 2 for...

The twin method is applied to determine parallaxes for stars in the RAVE survey. The method is based on the proposition that if two stars have the same spectra (hence twins)...

We combined 180ks of new Chandra ACIS data on 47 Tuc with 370ks of archival data, and used improved algorithms to generate a new source catalogue, finding 81 new sources for a...

We derive ugri photometry of ~1.7 million sources over the ~21 square degree area of the Fornax Deep Survey (FDS) centered on the bright galaxy NGC1399 (fds.dat). For a wider...

The images analysed in this paper were collected within the CASE project between the years 1997 and 2015. Observations in V and B filters were obtained using the 1-m Swope...

We have revisited M87 in a new era high-precision wide-field survey of GCs. The main component of our data set is presented and discussed in detail in Strader et al. (2011, Cat....

The stars x,y positions in the *.dat file are converted to RA and Dec using the F606W fits image.

Building upon the early pilot study of Jarrett+ (2013AJ....145....6J), this is the first paper in a series that encompasses the Wide-field Infrared Survey Explorer (WISE)...

Since 2014, 27 Galactic globular clusters were observed (PI: S. Kamann, formerly S. Dreizler) with the integral field spectrograph Multi Unit Spectroscopic Explorer (MUSE) at...

Chemodynamical associations of stars in the vicinity of globular clusters with those very globular clusters are presented. Moreover, we provide possible associations of Galactic...

The work uses Stroemgren photometry of the globular cluster NGC 6205 (M13), obtained from archival images from the Wide-Field Camera on the Isaac Newton Telescope (INT-WFC)....