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The Last Global extinction foraminifera data, Appendix 39 to 44
This dataset has no description
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YSOs in GRSMC 045.49+00.04 from IR obs.
Understanding the characteristics of young stellar populations is essential for deriving insights into star formation processes within parent molecular clouds and the influence... -
SPICY. II. Spectroscopic observations of 26 YSOs
Wide-field searches for young stellar objects (YSOs) can place useful constraints on the prevalence of clustered versus distributed star formation. The Spitzer/IRAC Candidate... -
OB stars in Carina Arm
In large-scale maps of the Galactic disc, the Carina Arm stands out as a clear spiral feature, hosting prominent star clusters and associations rich in massive stars. We study... -
Stars groups in CMa OB 1 with Gaia DR2
Canis Major OB1 (CMa OB1) is a Galactic stellar association with a very intriguing star-formation scenario. There are more than two dozen known star clusters in its line of... -
An all-sky catalogue of stellar reddening values
When observing astronomical objects, we have to deal with extinction (i.e. the absorption and scattering of the emitted radiation by dust and gas between the source and the... -
Stellar parameters from GALANTE
In this paper, we analyse how to extract the physical properties from the GALANTE photometry of a stellar sample. We propose a direct comparison between the observational... -
Unclassified B[e] stars in the MW, SMC and LMC
We investigated 12 unclassified B[e] stars or candidates, 8 from the Galaxy, 2 from the Large Magellanic Cloud (LMC), and 2 from the Small Magellanic Cloud (SMC). Based on the... -
Variable dust emission by WC type Wolf-Rayets
Photometry at 3.4 and 4.6{mu}m of 128 Population I WC type Wolf-Rayet stars in the Galaxy and 12 in the Large Magellanic Cloud (LMC) observed in the WISE NEOWISE-R survey was... -
WISE-2MASS (W2M) quasars and red QSOs with sp.
We present a highly complete sample of broad-line (Type 1) QSOs out to z~3 selected by their mid-infrared colors, a method that is minimally affected by dust reddening. We... -
Local Bubble & Gould Belt polarization
We create and analyse the largest up-to-date all-sky compilation of the interstellar optical polarization data supplemented by the reddening data This compilation includes 13... -
Metals, depletion, and dimming: decrypting dust
Dust plays a pivotal role in the chemical enrichment of the interstellar medium. In the era of mid-/high-resolution spectra and multiband spectral energy distributions, testing... -
SUMaC I
We present the first results from the Swift Ultraviolet Survey of the Magellanic Clouds, the highest resolution ultraviolet (UV) survey of the Magellanic Clouds yet completed.... -
High-resolution census data of Extinction Group species in the Late Pliocene-...
This dataset has no description
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High-resolution census data of Extinction Group species n the Late Pliocene-P...
This dataset has no description
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High-resolution census data of Extinction Group species in the Pliocene-Pleis...
This dataset has no description
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The last Global Extinction in the deep sea - foraminiferal and related data
Part 1. The Last Global Extinction in the Deep Sea:During the Last Global Extinction (LGE) c. 20% (30 genera, 105 species) of cosmopolitan, mainly deep-sea (600–4000 m), benthic... -
Aircraft measurements of aerosol particles and trace gases over the Southern ...
During the BALTIC'15 campaign, conducted in August 2015 over the Southern Baltic Sea, trace gasses (CO2/O3/NOy/SO2) and aerosol particles (number concentration of... -
{beta} Cephei pulsating variables from TESS and Gaia
{beta} Cephei pulsating variable (BCEP) stars are the most massive pulsating variable stars in the main sequence, exhibiting both p- and g-mode pulsations. In this study, we... -
Low resolution census data of Extinction Group species in Oligocene-Pleistoce...
a = abundant, c = common, f = frequent, o = occasional, r = rare; p = present (no assessment of abundance)
