J. Dickey
Dickey, John M.
VIAF ID: 93271390 (Personal)
Permalink: http://viaf.org/viaf/93271390
Preferred Forms
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- 100 1 _ ‡a Dickey, John M.
- 100 1 0 ‡a Dickey, John M.
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- 100 1 _ ‡a Dickey, John M.
- 100 1 _ ‡a Dickey, John M.
- 100 0 _ ‡a J. Dickey
4xx's: Alternate Name Forms (9)
Works
Title | Sources |
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Enhanced Small-Scale Faraday Rotation in the Galactic Spiral Arms | |
Evolution of the parsec-scale structure of PKS 1934-638 revisited: first science with the ASKAP and new zealand telescopes | |
Expert uncertainty and the use of subjective-probability models | |
The Fan Region at 1.5 GHz – I. Polarized synchrotron emission extending beyond the Perseus Arm | |
Fast rotation in the nuclear region of the galaxy NGC 1808 | |
A galactic example of a massive chimney | |
Galaxies on the blue edge | |
A GLIMPSE of star formation in the giant H II region RCW 49 | |
A GLIMPSE of the Southern Jellyfish Nebula and its massive YSO | |
The Global Magneto-Ionic Medium Survey: polarimetry of the southern sky from 300 to 480 MHz | |
GSH 23.0-0.7+117: a neutral hydrogen shell in the inner galaxy | |
H I absorption toward H II regions at small Galactic longitudes | |
An HI absorption survey of M 31 and M 33 : the mixture ofwarm and cool phases in the interstellar media of spiral galaxies | |
HI, CO, and Planck/IRAS dust properties in the high latitude cloud complex, MBM 53, 54, 55 and HLCG 92-35. Possible evidence for an optically thick HI envelope around the CO clouds | |
HI distribution and kinematics in the peculiar spiral galaxy NGC 5474 | |
The HI gas kinetic temperature of high galactic latitude cirrus clouds | |
HI synthesis of the Hercules cluster of galaxies | |
High-latutude HI structure and the soft X-ray background | |
High-resolution images of diffuse neutral clouds in the Milky Way. I. Observations, imaging, and basic cloud properties | |
High resolution rapid response observations of compact radio sources with the Ceduna Hobart Interferometer (CHI) | |
Identification of Main‐Sequence Stars with Mid‐Infrared Excesses Using GLIMPSE: β Pictoris Analogs? | |
An improved method to derive HI absorption spectra through the disks of galaxies: application to the Sculptor Group | |
Infrared polarimetry and the galactic magnetic field. II. Improved models | |
The interchangeability of CO and H I in the Tully-Fisher relation | |
Interstellar scintillation and compact sources in SNR | |
The joint far-infrared-optical luminosity function for spiral galaxies and data for the Abell 400 and Cancer clusters | |
Kinematic distance assignments with H I absorption | |
Low-Mach-number turbulence in interstellar gas revealed by radio polarization gradients. | |
The Magnetic Field of the Large Magellanic Cloud Revealed Through Faraday Rotation | |
Magnetically Dominated Strands of Cold Hydrogen in the Riegel‐Crutcher Cloud | |
Measurement of spin temperatures in a rapidly moving HI shell | |
Methanol absorption in PKS B1830−211 at milliarcsecond scales | |
Milky way kinematics. I. Measurements at the subcentral point of the fourth quadrant | |
Milky Way kinematics. II. A uniform inner galaxy H I terminal velocity curve | |
The Minnesota lectures on clusters of galaxies and large-scale structure | |
“Missing Link” Clouds in the Southern Galactic Plane Survey | |
Molecular clouds in supershells: a case study of three objects in the walls of GSH 287+04-17 and GSH 277+00+36 | |
Neutral hydrogen gas in interacting galaxies: the NGC 6221/6215 galaxy group | |
New star clusters discovered in the GLIMPSE survey | |
NGC 1058: gas motions in an extended, quiescent spiral disk | |
Non-confirmation of reported H I clouds without optical counterparts in the Hercules cluster | |
Observations of the ^57^Fe^+23^ hyperfine transition in clusters of galaxies | |
The phases of the interstellar medium : proceedings of a workshop held at the National Radio Astronomy Observatory, Green Bank, West Virginia, May 10-13, 1981 | |
Polarization Angular Spectra of Galactic Synchrotron Emission on Arcminute Scales | |
The radial distribution of cold hydrogen in the Galaxy | |
RCW 49 at mid-infrared wavelengths: a GLIMPSE from the Spitzer Space Telescope | |
Recovering galaxy rotation speeds from irregular emission profiles | |
Recovering interstellar gas properties with HI spectral lines: a comparison between synthetic spectra and 21-SPONGE | |
Resolving the kinematic ambiguity toward galactic H II regions | |
Rotation Measures of Extragalactic Sources behind the Southern Galactic Plane: New Insights into the Large‐Scale Magnetic Field of the Inner Milky Way | |
Search for OH megamaser emission from the FIR ultraluminous radio galaxy 4C 12.50 | |
SKA studies of atomic gas in the interstellar medium of the Milky Way | |
The small-scale structure of the Magellanic stream | |
The Southern Galactic Plane Survey: Polarized Radio Continuum Observations and Analysis | |
The Southern H II Region Discovery Survey. I. The bright catalog | |
The spatial power spectrum of galactic neutral hydrogen from observations of the 21-cm emission line | |
SPLASH: the Southern Parkes Large-Area Survey in Hydroxyl – first science from the pilot region | |
Statistics of neutral hydrogen absorption toward pulsars | |
A Stellar Wind Bubble Coincident with the Anomalous X-Ray Pulsar 1E 1048.1-5937: Are Magnetars Formed from Massive Progenitors? | |
Studies of interstellar neutral hydrogen at twenty-one centimeter wavelenght : a thesis | |
A study of the pulsed radio emission from XTE J1810-197 | |
A successful automated search for crouching giants | |
Supergiant shells and molecular cloud formation in the Large Magellanic Cloud | |
A survey of HI absorption at low latitudes | |
Temporal evolution of the Vela pulsar's pulse profile | |
Through thick or thin: multiple components of the magneto-ionic medium towards the nearby H II region Sharpless 2-27 revealed by Faraday tomography | |
Tracking the Outer Spiral Arms of the Galaxy in HiAbsorption | |
VLA observations of the Seyfert galaxy NGC 1068 | |
A VLA snapshot continuum survey of the first quadrant of the Galactic Plane at 1.5 GHz | |
The wavelength dependence of interstellar extinction from 1.25 to 8.0 {mu}m using GLIMPSE data | |
Westerbork and VLA observations of G 127.1+0.5 |