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The metal-poor tail of APOGEE I
The most metal-poor stars in our Galaxy contain important clues of its earliest history, particularly those occupying the inner regions of the Galaxy. In the search for such... -
The birth of Be star disks. I.
Classical Be stars are well known to eject mass to build up a disk, but the details governing the initial distribution and subsequent evolution of this matter into a disk are in... -
BPS CS 29529-0089 and TYC 9219-2422-1 abund.
R-process enhanced metal-poor stars ([Eu/Fe]>=+0.3 and [Fe/H]<=-1.0) are rare objects, the study of which can provide clues as to the astrophysical sites of the rapid... -
Variability of active galaxies. I.
Accreting supermassive black holes at the centres of galaxies are the engine of active galactic nuclei (AGN). X-ray light curves of unabsorbed AGN show dramatic random... -
Photometry & parameters of eclipsing contact binairies
We performed photometric and spectroscopic studies of three large amplitude contact binaries: NSVS 2418361, ATLAS J057.1170+31.2384, and NSVS 7377875. The amplitudes of these... -
HL Tau spectral data cubes + map
Protoplanetary disks inherit their chemical composition from their natal molecular cloud, although the extent to which this material is preserved versus reset through chemical... -
Accretion luminosity of Class I protostars
The value of the accretion luminosity during the early phases of star formation is crucial information that aids in understanding how stars form, but it is still very difficult... -
Anatomy of L1489 IRS with NOEMA II
Streamers are newly identified channels that transport mass from large, molecular-cloud scales down to small, protoplanetary-disk scales. To better understand their impact on... -
ESO TAP_CAT: a TAP service to query the astronomical catalogs generated by ES...
TAP_CAT is the ESO Science Archive service that provides programmatic access onto the astronomical catalogues produced by the principal investigators of ESO... -
CLIMSO DaCHS portal TAP service
The CLIMSO DaCHS portal's TAP end point. The Table Access Protocol (TAP) lets you execute queries against our database tables, inspect various metadata, and upload your own... -
CLIMSO DaCHS portal Registry
The publishing registry for the CLIMSO DaCHS portal. -
IAP - DaCHS Services TAP service
The IAP - DaCHS Services's TAP end point. The Table Access Protocol (TAP) lets you execute queries against our database tables, inspect various metadata, and upload your own... -
Line doublets in near-infrared sky emission spectra
Subtracting the changing sky contribution from the near-infrared (NIR) spectra of faint astronomical objects is challenging and crucial to a wide range of science cases such as... -
IAP - DaCHS Services Registry
The publishing registry for the IAP - DaCHS Services. -
1782 Mira variables candidates with VVV survey
The properties of the Milky Way's nuclear stellar disc give crucial information on the epoch of bar formation. Mira variables are promising bright candidates to study the... -
Star-spots properties of Pleiades and M67 stars
We measure star-spot filling fractions for 240 stars in the Pleiades and M67 open star clusters using APOGEE high-resolution H-band spectra. For this work, we developed a... -
Physical parameters of RRab stars with OGLE
In this paper, we report on the detection of RRab stars with quasi-identical-shape light curves but period differences as large as 0.05-0.21 d using the Galactic bulge data of... -
Radial velocities of HD 101581 & exoplanets search
We report the validation of multiple planets transiting the nearby (d=12.8pc) K5V dwarf HD 101581 (GJ 435, TOI-6276, TIC 397362481). This system consists of at least two... -
Plaskett's star photographic spectra from DAO
Photographic spectra of Plaskett's Star (HR 2420, HD 47129, V640 Monocerotis) that were recorded at the Dominion Astrophysical Observatory have been digitized with a flatbed... -
M3DIS. II. CEMP abundances
Understanding the origin and evolution of carbon-enhanced metal-poor (CEMP) stars is key to tracing the early chemical enrichment of the Galaxy. In this work, we investigate how...
