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X-shaped radio galaxies from FIRST
We present a catalog of 290 "winged" or X-shaped radio galaxies (XRGs) extracted from the latest (2014 December 17) data release of the "Very Large Array Faint Images of the... -
Linear structural param. of SDSS+UKIDSS+WISE gal.
Accurate measurements of galaxy structure are prerequisites for quantitative investigation of galaxy properties or evolution. Yet galaxy inclination, through projection and... -
CANDELS/SHARDS multiwavelength cat. in GOODS-N
We present a WFC3 F160W (H-band) selected catalog in the CANDELS/GOODS-N field containing photometry from the ultraviolet (UV) to the far-infrared (IR), photometric redshifts,... -
Parallaxes of late-T and Y dwarfs
We present preliminary trigonometric parallaxes of 184 late-T and Y dwarfs using observations from Spitzer (143), the U.S. Naval Observatory (18), the New Technology Telescope... -
Opt. & NIR spectral atlas of 16 2MASS NIR-red AGNs
We present medium-resolution spectra (R~2000-4000) at 0.4-1.0{mu}m and 0.7-2.5{mu}m of 16 active galactic nuclei (AGNs) selected with red color in the near-infrared (NIR) of... -
SPLASH-SXDF multi-wavelength photometric catalog
We present a multi-wavelength catalog in the Subaru/XMM-Newton Deep Field (SXDF) as part of the Spitzer Large Area Survey with Hyper-Suprime-Cam (SPLASH). We include the newly... -
Physical parameters of ~300000 SDSS-DR12 QSOs
We use the Sloan Digital Sky Survey (SDSS) Quasar Data Release 12 (DR12Q), containing nearly 300000 active galactic nuclei (AGNs), to calculate the monochromatic luminosities at... -
Luminosity profiles of BCGs
We have derived detailed R-band luminosity profiles and structural parameters for a total of 430 brightest cluster galaxies (BCGs), down to a limiting surface brightness of... -
New HIP-based parallaxes for 424 faint stars
We present a catalog of 424 common proper-motion companions to Hipparcos stars with good (>3{sigma}) parallaxes, thereby effectively providing new parallaxes for these... -
SNII during ZTF 1st phase survey with follow-up sp.
Narrow transient emission lines (flash-ionization features) in early supernova (SN) spectra trace the presence of circumstellar material (CSM) around the massive progenitor... -
Spectroscopic analysis of ASAS-SN SNe Ia
We present a spectroscopic analysis of 44 low-luminosity host galaxies of Type Ia supernovae (SNe Ia) detected by the All-Sky Automated Survey for Supernovae (ASAS-SN), using... -
High-z galaxies from JWST ERO
This paper highlights initial photometric analyses of JWST NIRCam imaging data in the sightline of SMACS0723, aiming to identify galaxies at redshift z>7. By applying a... -
Phot. metallicity & distances for Gaia RR Lyrae stars
We present a sample of 135,873 RR Lyrae stars (RRLs) with precise photometric metallicity and distance estimates from our newly calibrated P-{Phi}31-R_21_-[Fe/H]/P-R_21_-[Fe/H]... -
PS1 z>5.6 QSO Survey. III. z~6 quasar LF
We present the z~6 type-1 quasar luminosity function (QLF), based on the Pan-STARRS1 (PS1) quasar survey. The PS1 sample includes 125 quasars at z~5.7-6.2, with... -
Ap stars from LAMOST DR9 sp. and Gaia DR3
We present a sample of 2700 Ap stars in the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) DR9 catalog. The candidates are first selected to be in a... -
CII em-line stars in LMC. II. Final results
We present the final results of an imaging and spectroscopic search for stars in the Large Magellanic Cloud (LMC) with CII{lambda}{lambda}7231,7236 emission lines. The goal is... -
X-SHOOTER/ALMA QSOs at 5.7<~z<~7.6. II. BH masses
We present measurements of black hole masses and Eddington ratios ({lambda}Edd) for a sample of 38 bright (M_1450_<-24.4mag) quasars at 5.8<~z<~7.5, derived from Very... -
Cataclysmic variable orb. periods from Gaia phot.
The orbital-period (Porb) gap in the population of cataclysmic variables (CVs) informs the theoretical narrative of CV evolution, yet a complete understanding of the driving... -
WISE-2MASS (W2M) quasars and red QSOs with sp.
We present a highly complete sample of broad-line (Type 1) QSOs out to z~3 selected by their mid-infrared colors, a method that is minimally affected by dust reddening. We... -
Photometry of comet Bernardinelli-Bernstein
Cometary activity may be driven by ices with very low sublimation temperatures, such as carbon monoxide ice, which can sublimate at distances well beyond 20au. This point is...
