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Am and Ap star candidates from LAMOST DR10
Large samples of Am and Ap stars are helpful in studying the interplay between phenomena like atomic diffusion, magnetic fields, and stellar rotation in stellar astrophysics.... -
PN LF distances using VLT-MUSE. II. Archival data
Thanks to the MUSE integral field spectrograph on board the Very Large Telescope (VLT), extragalactic distance measurements with the [OIII]{lambda}5007 planetary nebula... -
Cataclysmic variables from LAMOST DR6
In this work, we present a catalog of cataclysmic variables (CVs) identified from the sixth data release (DR6) of the Large Sky Area Multi-Object Fiber Spectroscopic Telescope... -
Probing the Gal. halo with RR Lyrae stars. I.
We present a catalog of 5290 RR Lyrae stars (RRLs) with metallicities estimated from spectra of the LAMOST Experiment for Galactic Understanding and Exploration (LEGUE) and the... -
RV photon limits of well-characterized F-M stars
The determination of extrasolar planet masses with the radial velocity (RV) technique requires spectroscopic Doppler information from the planet's host star, which varies with... -
The first three quarters of Kepler mission
We present the results of a search for potential transit signals in the first three quarters of photometry data acquired by the Kepler mission. The targets of the search include... -
A GALEX UV imaging survey of nearby galaxies
We present results from a GALEX ultraviolet (UV) survey of a complete sample of 390 galaxies within ~11Mpc of the Milky Way. The UV data are a key component of the composite... -
HST astrometry of TNOs
We present 1428 individual astrometric measurements of 256 trans-Neptunian objects made with Hubble Space Telescope (HST). The observations were collected over three years with... -
A 3.5mm polarimetric survey of radio-loud AGNs
We present the results from the first large (>100 sources) 3.5mm polarimetric survey of radio-loud active galactic nuclei (AGNs). This wavelength is favorable within the... -
WIYN spectroscopy in the deep SWIRE field
We present the results of spectroscopy using HYDRA on the WIYN 3.5m telescope of objects in the deep SWIRE radio field. The goal of the project was to determine spectroscopic... -
H{alpha} and [NII] survey in local 11 Mpc
As part of a broader effort to characterize the population of star-forming galaxies in the local universe, we have carried out an H{alpha}+[NII] imaging survey for an... -
M dwarf UV flares in GALEX
We present the preliminary results from implementing a new software tool that enables inspection of time-tagged photon data for the astronomical sources contained within... -
UV-Optical galaxy color-magnitude diagram I.
We have analyzed the bivariate distribution of galaxies as a function of ultraviolet-optical colors and absolute magnitudes in the local universe. The sample consists of... -
Infrared observations of the Pleiades
We make use of new near- and mid-IR photometry of the Pleiades cluster in order to help identify proposed cluster members. We also use the new photometry with previously... -
Population synthesis in the blue. IV
We present a new set of model predictions for 16 Lick absorption line indices from H{delta} through Fe5335 and UBV colors for single stellar populations with ages ranging... -
Virgo intracluster planetary nebula candidates
Intracluster stars - stars outside of individual galaxies - are a sensitive measure of the poorly understood processes of galactic mergers, cluster accretion, and tidal... -
The FIRST bright quasar survey. III.
We present the results of an extension of the FIRST Bright Quasar Survey (FBQS) to the South Galactic cap, and to a fainter optical magnitude limit. Radio source counterparts... -
Einstein X-ray survey of galaxies. I.
We present the results of a complete Einstein imaging proportional counter X-ray survey of optically-selected galaxies from the Shapley-Ames Catalog (Cat. ), the Uppsala General... -
MRC/1Jy Radio source survey. I.
This is the first in a series of papers discussing the properties of a complete set of radio sources selected near S408=1Jy. We present optical or infrared identifications for a... -
Pleiades members & escapee candidates with Gaia EDR3
We search through an eight million cubic parsec volume surrounding the Pleiades star cluster and the Sun to identify both the current and past members of the Pleiades cluster...
