The Table 8 contains the chemical abundances obtained through the EW-spectral analysis (DOOp-FAMA tools). They are determined from high-resolution stellar spectra collected by...

We analyse spectra from the FEROS, HARPS, ELODIE, SOPHIE, UVES, and CAFE spectrographs. We refer to section 2 for a detailed description of the observations and data analysis.

Table 1. Cname, spectrum used for the measurements, object name, signal-to-noise ratio, FWZI(H{alpha}) ({AA}) and velocities of the wings (blue and red part of the profile) of...

The 20 tables, which conform Appendix C in our paper, show the results of our analysis and the final selections of candidate members for each cluster, as well as the lists of...

Table 2 lists radial velocity variable stars in NGC 2516 which can be considered radial velocity binaries. Their radial velocities were acquired from various sources in the...

The spectroscopic analysis of NGC 2546 is based on 177 spectra collected between the years 2000 and 2018. These observations were carried out using the 2.15m telescope and the...

For this program, the field was observed using Spitzer from 2011 May through June (starting on about MJD 55700); these data are referred to as Young Stellar Object VARiability...

New candidate members of Sco OB1, including normal M-type stars, NIR- and uv-excess stars, and H-alpha emission stars. Also tabulated are previously unpublished lists of X-ray...

NGC 2070 was observed as part of the MUSE SV program at the VLT in August 2014. Four overlapping fields, each with an individual field of 1'x1' and a pixel scale of 0.2''/pixel,...

We used the cluster members identified by Cantat-Gaudin et sl. (2018, Cat. J/A+A/615/A49) to cross-match with the LAMOST spectroscopic catalog (Luo et al., 2019, Cat. V/164). A...

Thanks to the INfrared Spectra of Young Nebulous Clusters (IN-SYNC) program, more than 3000 stars in NGC 1333, IC 348, and the Orion A molecular cloud have been observed with...

The observations were carried out on the night of 2004 November 30 at the W. M. Keck Observatory under photometric conditions and a typical seeing of 1.1".

Photometry of stars in the Westerlund 1 cluster field of view and inferred masses. The catalog contains new photometric measurements using data from the SofI instrument on the...

List of member candidates of Coma Ber with UKIDSS GCG DR9 (Cat. II/319/), Pan-STARR DR1 (Cat. II/349) and SDSS DR12 (Cat. V/147) photometry.

In this paper we compile and derive lists of members for 2017 open clusters. We employ an artificial neural network to estimate cluster parameters (extinction Av, distance...

The dataset contains stellar spectra collected by the HARPS spectrograph. The instrument is installed on the 3.6m telescope at the La Silla Observatory (Chile) and delivers a...

We present classifications of a further 69 members of Wd1, producing a current census of 166 massive, evolved stars.

JHKs individual photometric measurements for all sources in the observed field. Near-IR images were collected on the night of 2009 June 12 using the Perssons Auxiliary Nasmyth...

All the data used in this paper were acquired with the X-shooter spectrograph at the VLT. The capabilities of X-shooter in terms of wide spectral coverage (310-2500nm),...

Observations of M48 candidate members were made using the Wisconsin-Indiana-Yale-NOAO (WIYN) 3.5m telescope and Hydra multi-fiber spectrograph during four runs in 2017-October,...