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New brown dwarfs in upper Sco
This paper presents the results of a search for brown dwarfs in the Upper Scorpius Association using data from the UKIRT Infrared Deep Sky Survey (UKIDSS) Galactic Cluster... -
SPIRE (f250um>17.4mJy) GOODS-N galaxies
For the first time, we investigate the X-ray/infrared (IR) correlation for star-forming galaxies (SFGs) at z~1, using SPIRE submm data from the recently launched Herschel Space... -
Radio obs. of optically obscured galaxies
This paper analyses the radio properties of a subsample of optically obscured (R>=25.5) galaxies observed at 24um by the Spitzer Space Telescope within the First Look Survey.... -
Catalog of SDSS-DR5/2MASS spectroscopic quasars
We present a catalog of 13444 SDSS-DR5 spectroscopic quasars which have an 2MASS near-IR counterpart within 5" of their position. Cone search capability for table... -
QDOT all-sky IRAS redshift survey
The catalogue from the QDOT survey consists of infrared properties and redshifts of an all-sky sample of 2387 IRAS galaxies brighter than the IRAS PSC 60{mu}m completeness limit... -
Distances to RRab stars from WISE and Gaia
Pulsating stars, such as Cepheids, Miras, and RR Lyrae stars, are important distance indicators and calibrators of the "cosmic distance ladder," and yet their... -
The TESS-Keck survey. XXII. TOI-1437
Exoplanet discoveries have revealed a dramatic diversity of planet sizes across a vast array of orbital architectures. Sub-Neptunes are of particular interest; due to their... -
Massive galaxies at z>4 from JWST CEERS
We analyze the evolution of massive (log_10_[M_*/M{sun}_]>10) galaxies at z~1-4 selected from JWST Cosmic Evolution Early Release Survey (CEERS). We infer the physical... -
Avg pitch angles & spiral amplitudes in S4G
Spiral galaxies are very common in the local Universe, but their formation, evolution, and interplay with bars remain poorly understood after more than a century of astronomical... -
Properties of cores in OMC 2/3
We present new measurements of the dust emissivity index, {beta}, for the high-mass, star-forming OMC 2/3 filament. We combined 160-500um data from Herschel with long-wavelength... -
Catalogue enriched with R CrB stars
This catalogue contains 1602 entries. It was created to list objects that have similar near- and mid-infrared characteristics than R Coronae Borealis (RCB) stars which are... -
1.3mm and CO(2-1) maps of IRAS 20343+4129
IRAS 20343+4129 was suggested to harbor one of the most massive and embedded stars in the Cygnus OB2 association, IRS 1, which seemed to be associated with a north-south... -
ISOSS J23053+5953 maps
Due to the short timescales involved and observational difficulties, our knowledge of the earliest phases of massive star formation remains incomplete. We aim to explore the... -
Near-IR astrometry of Southern ICRF quasars
We present high quality astrometry, along with J, H, and Ks photometry, for 30 southern International Celestial Reference Frame (ICRF) quasars observed with the ESO NTT/SOFI at... -
86GHz SiO maser survey of late-type stars. III
We have determined extinction corrections for a sample of 441 late-type stars in the inner Galaxy, which we previously searched for SiO maser emission, using the 2MASS... -
Near-IR sources around IRAS 09002-4732
We present high-resolution near-infrared and mid-infrared imaging, mid-infrared spectroscopy and millimetre-wavelength continuum observations of the nearby massive star-forming... -
17OH spin-rotation transition frequencies
The frequencies and line strengths of the ^2^{Pi}3/2 J=5/2-3/2 rotational transition of ^17^OH have been calculated from an analysis of its far-infrared laser magnetic resonance... -
Mid-IR galaxies in Virgo cluster. III.
We present ISOCAM imaging data at 6.75 and 15{mu}m for 145 galaxies in the Virgo cluster and in the Coma/A1367 supercluster. Of these, 99 form a complete, optically-selected,... -
Galaxies in Southern Bright Star Fields I.
As a prerequisite for cosmological studies using adaptive optics techniques, we have begun to identify and characterize faint sources in the vicinity of bright stars at high... -
Unidentified infrared bands (UIR)
We present a set of 6-12{mu}m ISOPHOT-S spectra of the general interstellar medium of the Milky Way. This part of the spectrum is dominated by a series of strong, wide emission...