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K-band images of star-forming regions
We present deep, wide-field, Ks-band (2.14-micron) images towards 87 southern massive star formation regions traced by methanol maser emission. Using point-spread function... -
FLAIR II spectroscopy of DENIS samples
As a pilot survey for the forthcoming 6dF Galaxy Redshift Survey, spectroscopy of galaxies selected in the 1.2 micron J waveband with the DENIS imaging survey was performed at... -
IRAS observations of Be stars
The IRAS associations for 193 Be stars are identified in this paper. From the infrared colors, the IRAS low-resolution spectra (LRS) and the spectral types, some physical... -
NLS1s 2MASS and WISE photometry
The infrared photometric study of SDSS selected Narrow Line Seyfert 1 Galaxies (NLS1s) is presented in this paper. We have made cross-identifications for such NLS1s with 2MASS... -
Star-forming complex S254-S258 HII regions
The S254-258 star-forming complex is a place of massive star formation where five OB-stars have created HII regions, visible as optical nebulae, and disrupted the parental... -
Bootes field source catalogue at 400MHz
The dominant source of radio continuum emissions at low frequencies is synchrotron radiation, which originates from star-forming regions in disc galaxies and from powerful jets... -
NIR spectral atlas of early-type galaxies
We present a near infrared spectroscopic atlas of nearby, bright early-type galaxies with radio emission, containing 163 galaxies observed by the Palomar 200" TripleSpec... -
Metal-rich galaxies dust, CO and [CI]
We present a self-consistent cross-calibration of the three main molecular gas mass tracers in galaxies, namely the ^12^CO(1-0), CI lines,and the submm dust continuum emission,... -
Infrared-faint radio sources redshifts
Infrared-faint radio sources (IFRSs) are an important class of high-redshift active galaxy, and potentially important as a means of discovering more high-redshift radio sources,... -
WISE view of narrow-line Seyfert 1 galaxies
We present the colour and flux variability analysis at 3.4{mu}m (W1 band) and 4.6{mu}m (W2 band) of 492 narrow-line Seyfert 1 (NLSy1) galaxies using archival data from the... -
HAWK-I JHK photometry of the Orion Nebula Cloud
Due to its youth, proximity and richness, the Orion nebula cloud (ONC) is an ideal testbed to obtain a comprehensive view on the initial mass function (IMF) down to the... -
HST Frontier Fields Herschel sources
We present a complete census of all Herschel-detected sources within the six massive lensing clusters of the HST Frontier Fields (HFF). We provide a robust legacy catalogue of... -
NGC 7538 IRS 1-3 and IRS 9 sources
We present deep and high-resolution (FWHM~0.4-arcsec) near-infrared (NIR) imaging observations of the NGC 7538 IRS 1-3 region (in JHK bands), and IRS 9 region (in HK bands)... -
CO lines in luminous IR galaxies
We report results from a large molecular line survey of luminous infrared galaxies (LIRGs; L_IR_>~10^11^L_{sun}) in the local Universe (z<=0.1), conducted during the last... -
Multiwavelength survey of AGNs
We aim to study the effect of environment on the presence and fuelling of active galactic nuclei (AGNs) in massive galaxy clusters. We explore the use of different AGN detection... -
Catalog of bubbles from Milky Way Project
We present a new catalogue of 5106 infrared bubbles created through visual classification via the online citizen science website The Milky Way Project. Bubbles in the new... -
MIPS photometry for Herschel SAG2 Programs
We provide an overview of ancillary 24, 70, and 160 micron data from the Multiband Imaging Photometer for Spitzer (MIPS) that are intended to complement the 70-500 micron... -
Ultraluminous IRAS galaxies
We present a new, large sample of ultraluminous (L_60_>10^11.4^L_{sun} for H_0=100km/s/Mpc) IRAS galaxies selected for the IRAS Faint Source Survey using a novel optical... -
IRAS Galactic star-forming regions. II.
The results of the analysis of the occurrence of 22.2-GHz H_2_O maser emission in a sample of 1409 IRAS sources north of declination -30deg associated with star-forming regions... -
Surveys of clumps & cores in Cygnus X. I. ~0.1pc MDCs
Using infrared to (sub)millimeter data from Spitzer, Herschel, the James Clerk Maxwell Telescope, and the IRAM 30m telescope, we conducted an unbiased survey of the massive...