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Optical interferometry of 6 O-type HD stars
We present interferometric observations of six O-type stars that were made with the Precision Astronomical Visible Observations beam combiner at the Center for High Angular... -
Sgr A* 1.3mm VLBI observations with the EHT in 2013
We report results from very long baseline interferometric (VLBI) observations of the supermassive black hole in the Galactic center, Sgr A, at 1.3mm (230GHz). The observations... -
Radial profiles of 5 nearby galaxies
We use new ALMA observations to investigate the connection between dense gas fraction, star formation rate (SFR), and local environment across the inner region of four local... -
CHARA array obs. of 13 AB Dor moving group stars
We present interferometric measurements obtained with the CHARA Array of 13 adolescent-age stars in nearby moving groups. The motivation was to spatially resolve the largest... -
The Megamaser Cosmology Project. X.
We present high-resolution (submas) Very Long Baseline Interferometry maps of nuclear H_2_O megamasers for seven galaxies. In UGC 6093, the well-aligned systemic masers and... -
Molecular transitions toward NGC5128 with ALMA
Centaurus A, with its gas-rich elliptical host galaxy, NGC 5128, is the nearest radio galaxy at a distance of 3.8Mpc. Its proximity allows us to study the interaction among an... -
Jet kinematics of blazars at 43GHz with the VLBA
We analyze the parsec-scale jet kinematics from 2007 June to 2013 January of a sample of {gamma}-ray bright blazars monitored roughly monthly with the Very Long Baseline Array... -
Interferometric CO obs. of 126 CALIFA galaxies
We present interferometric CO observations, made with the Combined Array for Millimeter-wave Astronomy (CARMA) interferometer, of galaxies from the Extragalactic Database for... -
H{alpha} interferometry obs. of the Be star 48 Per
We utilize a multi-step modeling process to produce synthetic interferometric and spectroscopic observables, which are then compared to their observed counterparts. Our... -
SUPER GOODS. I. Ultradeep SCUBA-2 survey
In this first paper in the SUPER GOODS series on powerfully star-forming galaxies in the two GOODS fields, we present a deep SCUBA-2 survey of the GOODS-N at both 850 and... -
HST FGS-1r parallaxes for 8 metal-poor stars
Hubble Space Telescope (HST) fine guidance sensor observations were used to obtain parallaxes of eight metal-poor ([Fe/H]< -1.4) stars. The parallaxes of these stars... -
The Megamaser Cosmology Project (MCP). IX.
As part of the Megamaser Cosmology Project, we present VLBI maps of nuclear water masers toward five galaxies. The masers originate in sub-parsec circumnuclear disks. For three... -
Radio obs. of NGC 6251 jet
The structure of the NGC 6251 jet on the milliarcsecond scale is investigated using images taken with the European VLBI Network and the Very Long Baseline Array. We detect a... -
Radio sources in the NCP region with the 21CMA
We present a catalog of 624 radio sources detected around the North Celestial Pole (NCP) with the 21 Centimeter Array (21CMA), a radio interferometer dedicated to the... -
CLASSy: CARMA obs. in L1451 region of Perseus
We present a 3mm spectral line and continuum survey of L1451 in the Perseus Molecular Cloud. These observations are from the CARMA Large Area Star Formation Survey (CLASSy),... -
4yr 1.3mm VLBI observations of SgrA* with EHT
The Galactic Center black hole Sagittarius A (Sgr A) is a prime observing target for the Event Horizon Telescope (EHT), which can resolve the 1.3mm emission from this source on... -
Gould's Belt VLA survey. V. Perseus region
We present multiepoch, large-scale (~2000 arcmin^2^), fairly deep (~16 {mu}Jy), high-resolution (~1") radio observations of the Perseus star-forming complex obtained with the... -
Megamaser Cosmology Project. VIII. NGC5765B
As part of the Megamaser Cosmology Project, here we present a new geometric distance measurement to the megamaser galaxy NGC 5765b. Through a series of very long baseline... -
H{alpha} interferometric visibilities of o Aqr
Omicron Aquarii is a late-type, Be shell star with a stable and nearly symmetric H{alpha} emission line. We combine H{alpha} interferometric observations obtained with the Navy... -
LIGO gravitational-wave (GW) searches from SNRs
We describe directed searches for continuous gravitational waves (GWs) in data from the sixth Laser Interferometer Gravitational-wave Observatory (LIGO) science data run. The...
