RAVE stellar elemental abundances (DR1)

VizieR online Data Catalogue associated with article published in journal Astronomical Journal (AAS) with title 'The RAVE catalog of stellar elemental abundances: first data release.' (bibcode: 2011AJ....142..193B

VizieR Online Data Catalog: Stellar kinematics in CALIFA survey (Falcon-Barroso+, 2017)

This study is based on observations of 300 galaxies drawn from the CALIFA mother and extended samples1, which are part of the photometric catalog of the seventh data release (Abazajian et al., 2009ApJS..182..543A) of the Sloan Digital Sky Survey (SDSS). (1 data file)

VizieR Online Data Catalog: Stellar kinematics in CALIFA survey (Falcon-Barroso+, 2017)

This study is based on observations of 300 galaxies drawn from the CALIFA mother and extended samples1, which are part of the photometric catalog of the seventh data release (Abazajian et al., 2009ApJS..182..543A) of the Sloan Digital Sky Survey (SDSS). (1 data file)

CasA, CygA, TauA, VirA 30MHz & 77MHz models

VizieR online Data Catalogue associated with article published in journal Astronomy & Astrophysics with title 'Cassiopeia A, Cygnus A, Taurus A, and Virgo A at ultra-low radio frequencies.' (bibcode: 2020A&A...635A.150D

Cas A LOFAR and VLA images

VizieR online Data Catalogue associated with article published in journal Astronomy & Astrophysics with title 'Low frequency radio absorption in Cassiopeia A.' (bibcode: 2018A&A...612A.110A

LOFAR Long-Baseline Calibrator Survey. II.

VizieR online Data Catalogue associated with article published in journal Astronomy & Astrophysics with title 'Sub-arcsecond imaging with the International LOFAR Telescope. II. Completion of the LOFAR Long-Baseline Calibrator Survey.' (bibcode: 2022A&A...658A...2J

LOFAR Bootes and 3C295 field sources

The Bootes and 3C 295 fields were simultaneously observed on 2012 April 12 as part of a multi-beam observation with the LOFAR LBA stations. The idea behind the multi-beam setup is that we use the 3C 295 observations as a calibrator field to transfer the gain amplitudes to the (target) Bootes field. The total integration time on both fields was 10.25 hr. Complete frequency coverage was obtained between 54 and 70 MHz for both fields, while non-contiguous frequency coverage was obtained between 30 and 54 MHz for the 3C 295 only. All four correlation products were recorded. By default, the frequency band was divided into sub-bands, each 195.3125 kHz wide. Each sub-band was further divided in 64 channels and the integration time was 1 s