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HST/WFC3 spectroscopy of WISEP J182831.08+265037.8
We present a Hubble Space Telescope/Wide-Field Camera 3 near-infrared spectrum of the archetype Y-dwarf WISEPJ182831.08+265037.8. The spectrum covers the 0.9-1.7{mu}m wavelength... -
AT 2019qyl UV-to-IR photometry and spectroscopy
Nova eruptions, thermonuclear explosions on the surfaces of white dwarfs (WDs), are now recognized to be among the most common shock-powered astrophysical transients. We present... -
HST-WFC3/IR grism sp. for CANDELS z~1-2 galaxies
We present a new measurement of the gas-phase mass-metallicity relation (MZR) and its dependence on star formation rates (SFRs) at 1.3<z<2.3. Our sample comprises 1056... -
High-resolution NIR spectra of IRAS 16316-1540
Outbursts of young stellar objects occur when the mass accretion rate suddenly increases. However, such outbursts are difficult to detect for deeply embedded protostars due to... -
Opt-to-IR monitoring obs. of V1057 Cyg
Among the low-mass pre-main sequence stars, a small group called FU Orionis-type objects (FUors) are notable for undergoing powerful accretion outbursts. V1057 Cyg, a classical... -
Metallicities of Coma Berenices bona fide members
We present a study of metallicities in a sample of main-sequence stars with spectral types M, K, G, and F (T_eff_~3200-6500K and logg~4.3-5.0dex) belonging to the solar... -
Follow-up Opt. and NIR obs. of the SNIa SN2015bp
Unburned carbon is potentially a powerful probe of Type Ia supernova (SN) explosion mechanisms. We present comprehensive optical and near-infrared (NIR) data on the... -
Opt. phot. and GMOS & NIRES spectra of SN2019yvq
We present new photometric and spectroscopic observations of SN2019yvq, a Type Ia supernova (SN Ia) exhibiting several peculiar properties including an excess of UV/optical flux... -
G305 star-forming region. II. Irregular var. stars
We present a catalog of 167 newly discovered, irregular variables spanning a ~7deg^2^ area that encompasses the G305 star-forming complex, one of the most luminous giant HII... -
Stellar polarimetry with Gaia DR2 data
Optical stellar polarimetry in the Perseus molecular cloud direction is known to show a fully mixed bimodal distribution of position angles across the cloud. We study the Gaia... -
Superthin galaxies with 5yr sp. and NIR phot.
We conduct spectral observations of 138 superthin galaxies (STGs) with high radial-to-vertical stellar disk scale ratios with the Dual Imaging Spectrograph on the 3.5m telescope... -
Follow-up phot. & sp. of 12 PGIR novae
The nova rate in the Milky Way remains largely uncertain, despite its vital importance in constraining models of Galactic chemical evolution as well as understanding progenitor... -
Metallicity of Gal. RR Lyrae from opt. & IR LCs
We present newly calibrated period-{phi}31-[Fe/H] relations for fundamental-mode RR Lyrae stars in the optical and, for the first time, mid-infrared. This work's calibration... -
The CGM-GRB study. I. GRB hosts at z~2-6
Recent studies have revealed a dynamic interplay between the galaxy ecosystem and circumgalactic medium (CGM). We investigate the CGM at high redshifts (z>~2) by using bright... -
Exploring 6 AGN dusty torus models. II.
This is the second in a series of papers devoted to exploring a set of six dusty models of active galactic nuclei (AGN) with available spectral energy distributions. These... -
Ultracool SpeXtroscopic survey. I. M7-L5 sample
We present a volume-limited, spectroscopically verified sample of M7-L5 ultracool dwarfs (UCDs) within 25pc. The sample contains 410 sources, of which 93% have trigonometric... -
Magellan/IMACS spectra of Crater II & Hercules
We investigate the possibility that the dwarf galaxies Crater II and Hercules have previously been tidally stripped by the Milky Way. We present Magellan/IMACS spectra of... -
Subaru obs. of Vesta in MIR spectral range
Plagioclase feldspars are among the most prevalent minerals in the solar system, and are present in many chondritic and achondritic meteorite families. Nevertheless, spectral... -
Hot subdwarf stars from LAMOST DR5 & Gaia DR2
Combing Gaia DR2 with LAMOST DR5, we spectroscopically identified 924 hot subdwarf stars, among which 32 stars exhibit strong double-lined composite spectra. We measured the... -
Ages & [Fe/H] of the MW bulge using APOGEE
We present stellar age distributions of the Milky Way bulge region using ages for ~6000 high-luminosity (log(g)<2.0), metal-rich ([Fe/H]>=-0.5) bulge stars observed by the...
