Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- California Institute of TechnologyUS2.6k papers
- Centre National de la Recherche ScientifiqueFR2k papers
- Massachusetts Institute of TechnologyUS1.9k papers
- University of FloridaUS1.8k papers
- Carnegie Mellon UniversityUS1.7k papers
- Princeton UniversityUS1.7k papers
- University of RochesterUS1.7k papers
- Purdue University West LafayetteUS1.6k papers
- Johns Hopkins UniversityUS1.6k papers
- University of Maryland, College ParkUS1.6k papers
- The Ohio State UniversityUS1.6k papers
- University of California, Santa BarbaraUS1.6k papers
39 papers · 2 filters
SOFIA Far Infrared Imaging Polarimetry of M82 and NGC 253: Exploring the Super-Galactic Wind
Terry Jay Jones, C. Darren Dowell, Enrique Lopez Rodriguez +22
We present Far-Infrared polarimetry observations of M82 at 53 and and NGC 253 at , which were taken with HAWC+ in polarimetry mode on the Stratospheric Ob…
The ISM Properties and Gas Kinematics of a Redshift 3 Massive Dusty Star-forming Galaxy
T. K. Daisy Leung, Dominik A. Riechers, Andrew J. Baker +9
We present CO(J= 1-0; 3-2; 5-4; 10-9) and 1.2-kpc resolution [CII] line observations of the dusty star-forming galaxy (SFG) HXMM05 -- carried out with the Karl G. Jansky Very Large…
The Arecibo Pisces-Perseus Supercluster Survey I: Harvesting ALFALFA
Aileen A. O'Donoghue, Martha P. Haynes, Rebecca A. Koopmann +9
We report a multi-objective campaign of targeted 21 cm HI line observations of sources selected from the Arecibo Legacy Fast ALFA (Arecibo L-band Feed Array) survey (ALFALFA) and g…
The NANOGrav 11-Year Data Set: Limits on Gravitational Waves from Individual Supermassive Black Hole Binaries
K. Aggarwal, Z. Arzoumanian, P. T. Baker +60
Observations indicate that nearly all galaxies contain supermassive black holes (SMBHs) at their centers. When galaxies merge, their component black holes form SMBH binaries (SMBHB…
Low star formation efficiency in typical galaxies at z=5-6
Riccardo Pavesi, Dominik A. Riechers, Andreas L. Faisst +2
Using the VLA and ALMA, we have obtained CO(2-1), [C II], [N II] line emission and multiple dust continuum measurements in a sample of "normal" galaxies at . We report the h…
No evidence for enhanced [OIII] 88um emission in a z~6 quasar compared to its companion starbursting galaxy
Fabian Walter, Dominik Riechers, Mladen Novak +14
We present ALMA band 8 observations of the [OIII] 88um line and the underlying thermal infrared continuum emission in the z=6.08 quasar CFHQS J2100-1715 and its dust-obscured starb…
The Frequency Dependence of Scintillation Arc Thickness in Pulsar B1133+16
Dan R. Stinebring, Barney J. Rickett, Stella Koch Ocker
Scintillation arcs have become a powerful tool for exploring scattering in the ionized interstellar medium. There is accumulating evidence that the scattering from many pulsars is…
Multiple Ultralight Axionic Wave Dark Matter and Astronomical Structures
Hoang Nhan Luu, S. -H. Henry Tye, Tom Broadhurst
An ultralight scalar boson with mass eV is gaining credence as a Dark Matter (DM) candidate that explains the dark cores of dwarf galaxies as soliton waves. S…
Dust emission in an accretion-rate-limited sample of z>6 quasars
Bram Venemans, Roberto Decarli, Fabian Walter +9
We present Atacama Large Millimeter Array 1mm observations of the rest-frame far-infrared (FIR) dust continuum in 27 quasars at redshifts 6.0 < z < 6.7. We detect FIR emission at >…
Science with an ngVLA. Cold gas in High-z Galaxies: CO as redshift beacon
R. Decarli, C. Carilli, C. Casey +7
The goal of this science case is to address the use of a ngVLA as a CO redshift machine for dust-obscured high-redshift galaxies which lack of clear counterparts at other wavelengt…
Resolving Star Formation on Sub-Kiloparsec Scales in the High-Redshift Galaxy SDP.11 Using Gravitational Lensing
C. Lamarche, A. Verma, A. Vishwas +7
We investigate the properties of the interstellar medium, star formation, and the current-day stellar population in the strongly-lensed star-forming galaxy H-ATLAS J091043.1-000321…
Mirach's Goblin: Discovery of a dwarf spheroidal galaxy behind the Andromeda galaxy
David Martinez-Delgado, Eva K. Grebel, Behnam Javanmardi +9
It is of broad interest for galaxy formation theory to carry out a full inventory of the numbers and properties of dwarf galaxies in the Local Volume, both satellites and isolated…
No Evidence for Millimeter Continuum Source Overdensities in the Environments of Quasars
Jaclyn B. Champagne, Roberto Decarli, Caitlin M. Casey +11
Bright high-redshift quasars (), hosting supermassive black holes (), are expected to reside in massive host galaxies embedded within some of the…
Gemini GNIRS near-infrared spectroscopy of 50 quasars at z>~5.7
Yue Shen, Jin Wu, Linhua Jiang +12
We report initial results from a large Gemini program to observe z>~5.7 quasars with GNIRS near-IR spectroscopy. Our sample includes 50 quasars with simultaneous ~0.85-2.5 micron s…
The CO Luminosity Density at High-z (COLDz) Survey: A Sensitive, Large Area Blind Search for Low-J CO Emission from Cold Gas in the Early Universe with the Karl G. Jansky Very Large Array
Riccardo Pavesi, Chelsea E. Sharon, Dominik A. Riechers +16
We describe the CO Luminosity Density at High-z (COLDz) survey, the first spectral line deep field targeting CO(1-0) emission from galaxies at and CO(2-1) at $z=4.91-…
COLDz: Shape of the CO Luminosity Function at High Redshift and the Cold Gas History of the Universe
Dominik A. Riechers, Riccardo Pavesi, Chelsea E. Sharon +14
We report the first detailed measurement of the shape of the CO luminosity function at high redshift, based on 320 hr of the NSF's Karl G. Jansky Very Large Array (VLA) observat…
SOFIA/HAWC+ detection of a gravitationally lensed starburst galaxy at = 1.03
Jingzhe Ma, Arianna Brown, Asantha Cooray +13
We present the detection at 89 m (observed frame) of the {\it Herschel}-selected gravitationally lensed starburst galaxy HATLASJ1429-0028 (also known as G15v2.19) in 15 minutes…
Far-infrared Herschel SPIRE spectroscopy of lensed starbursts reveals physical conditions of ionised gas
Zhi-Yu Zhang, R. J. Ivison, R. D. George +15
The most intensively star-forming galaxies are extremely luminous at far-infrared (FIR) wavelengths, highly obscured at optical and ultraviolet wavelengths, and lie at .…
CCAT-prime: Science with an Ultra-widefield Submillimeter Observatory at Cerro Chajnantor
G. J. Stacey, M. Aravena, K. Basu +37
We present the detailed science case, and brief descriptions of the telescope design, site, and first light instrument plans for a new ultra-wide field submillimeter observatory, C…
The Local Cluster Survey I: Evidence of Outside-In Quenching in Dense Environments
Rose A. Finn, Vandana Desai, Gregory Rudnick +9
The goal of the Local Cluster Survey is to look for evidence of environmentally driven quenching among star-forming galaxies in nearby galaxy groups and clusters. Quenching is link…
The Atacama Cosmology Telescope: CO(J = 3 - 2) mapping and lens modeling of an ACT-selected dusty star-forming galaxy
J. Rivera, A. J. Baker, P. A. Gallardo +13
We report Northern Extended Millimeter Array (NOEMA) CO() observations of the dusty star-forming galaxy ACT-S\,J020941+001557 at , which was detected as an u…
The Arecibo Legacy Fast ALFA Survey: The ALFALFA Extragalactic HI Source Catalog
Martha P. Haynes, Riccardo Giovanelli, Brian R. Kent +22
We present the catalog of ~31500 extragalactic HI line sources detected by the completed ALFALFA survey out to z < 0.06 including both high signal-to-noise ratio (> 6.5) detections…
Warm Molecular Hydrogen in Nearby, Luminous Infrared Galaxies
Andreea O. Petric, Lee Armus, Nicolas Flagey +19
Mid-infrared molecular hydrogen (H) emission is a powerful cooling agent in galaxy mergers and in radio galaxies; it is a potential key tracer of gas evolution and energy dissi…
Quantifying the AGN-driven outflows in ULIRGs (QUADROS) II: evidence for compact outflow regions from HST [OIII] imaging observations
C. Tadhunter, J. Rodríguez Zaurín, M. Rose +7
The true importance of the warm, AGN-driven outflows for the evolution of galaxies remains uncertain. Measurements of the radial extents of the outflows are key for quantifying the…