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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... -
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... -
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... -
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... -
Variations of RS CVn primaries. II. o Dra
To measure the stellar and orbital properties of the metal-poor RS CVn binary o Draconis (o Dra), we directly detect the companion using interferometric observations obtained... -
Companions of RS CVn primaries. I. sig Gem
To measure the properties of both components of the RS Canum Venaticorum binary {sigma} Geminorum ({sigma} Gem), we directly detect the faint companion, measure the orbit,... -
230GHz VLBI observations of M87
We report on 230GHz (1.3mm) very long baseline interferometry (VLBI) observations of M87 with the Event Horizon Telescope using antennas on Mauna Kea in Hawaii, Mt. Graham in... -
Electromagnetic follow-up with LIGO/Virgo
We anticipate the first direct detections of gravitational waves (GWs) with Advanced LIGO and Virgo later this decade. Though this groundbreaking technical achievement will be... -
LOFAR Bootes and 3C295 field sources
We present Low Frequency Array (LOFAR) Low Band observations of the Bootes and 3C 295 fields. Our images made at 34, 46, and 62 MHz reach noise levels of 12, 8, and 5 mJy/beam,... -
PTI carbon star angular size survey
We report new interferometric angular diameter observations of 41 carbon stars observed with the Palomar Testbed Interferometer. Two of these stars are CH carbon stars and... -
VLBI observations of 3C 279 at 230GHz
We report results from five day very long baseline interferometry (VLBI) observations of the well-known quasar 3C 279 at 1.3mm (230GHz) in 2011. The measured nonzero closure... -
MWA Stokes I 189MHz sources
We present a Stokes I, Q and U survey at 189MHz with the Murchison Widefield Array 32 element prototype covering 2400deg^2^. The survey has a 15.6' angular resolution and... -
PHIBSS: CO observations of star-forming galaxies
We present PHIBSS, the IRAM Plateau de Bure high-z blue sequence CO(3-2) survey of the molecular gas properties in massive, main-sequence star-forming galaxies (SFGs) near the... -
K-band calibrated visibilities of 24 Be stars
We report on a high angular resolution survey of circumstellar disks around 24 northern sky Be stars. The K-band continuum survey was made using the CHARA Array long baseline... -
Murchison Widefield Array 110-200MHz observations
The Murchison Widefield Array (MWA) is a new low-frequency, wide field-of-view radio interferometer under development at the Murchison Radio-astronomy Observatory in Western...
