Erratum: ``An Investigation into the Prominence of Spiral Galaxy Bulges'' [Astron. J. 121, 820 (2001)]
Several proof corrections were not carried faithfully to the published version of this article. In particular, a central sentence of the abstract should...
Erratum: ``H I in the Shell Elliptical Galaxy NGC 3656'' [Astron. J. 122, 1758 (2001)]
As the result of an editorial oversight, the following two works were misattributed in the references:Schweizer, F. 1998, in Galaxies: Interactions and Induced...
ESO Very Large Telescope Optical Spectroscopy of BL Lacertae Objects. I. New Redshifts
We report redshift measurements for 12 BL Lacertae objects from a program aimed at obtaining high signal-to-noise ratio (up to ~500) optical spectroscopy of a...
ESO Very Large Telescope Optical Spectroscopy of BL Lacertae Objects. II. New Redshifts, Featureless Objects, and Classification Assessments
We report on ESO Very Large Telescope optical spectroscopy of 42 BL Lacertae objects of unknown redshift. Nuclear emission lines were observed in 12 objects...
Establishing the level of cylindrical rotation in boxy/peanut bulges
We present SAURON integral-field observations of a sample of 12 mid-to-high-inclination disc galaxies, to unveil hidden bars on the basis of their kinematics, i...
Estimation of kinematic parameters in CALIFA galaxies: no-assumption on internal dynamics
We propose a simple approach to homogeneously estimate kinematic parameters of a broad variety of galaxies (elliptical, spirals, irregulars or interacting...
Estimations of the magnetic field strength in the torus of IC 5063 using near-infrared polarimetry
An optically and geometrically thick torus obscures the central engine of active galactic nuclei (AGN) from some lines of sight. From a magnetohydrodynamical...
Euclid preparation - XXIII. Derivation of galaxy physical properties with deep machine learning using mock fluxes and H-band images
Next-generation telescopes, like Euclid, Rubin/LSST, and Roman, will open new windows on the Universe, allowing us to infer physical properties for tens of...