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FIRST J102347.6+003841: The First Radio-Selected Cataclysmic Variable

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TLDR
In this article, the 1.4 GHz radio source First J102347.6+003841 (hereafter FIRSTJ1023+00 38) with a previously unknown 17th-mag Galactic cataclysmic variable (CV) was identified.
Abstract
We have identified the 1.4 GHz radio source FIRST J102347.6+003841 (hereafter FIRST J1023+0038) with a previously unknown 17th-mag Galactic cataclysmic variable (CV). The optical spectrum resembles that of a magnetic (AM Herculis- or DQ Herculis-type) CV. Five nights of optical CCD photometry showed variations on timescales of minutes to hours, along with rapid flickering. A re-examination of the FIRST radio survey data reveals that the radio detection was based on a single 6.6 mJy flare; on two other occasions the source was below the ~1 mJy survey limit. Several other magnetic CVs are known to be variable radio sources, suggesting that FIRST J1023+0038 is a new member of this class (and the first CV to be discovered on the basis of radio emission). However, FIRST J1023+0038 is several optical magnitudes fainter than the other radio-detected magnetic CVs. It remains unclear whether the source simply had a very rare and extraordinarily intense radio flare at the time of the FIRST observation, or is really an unusually radio-luminous CV; thus further observations are urged.

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Science with ASKAP: The Australian square-kilometre-array pathfinder

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A State Change in the Missing Link Binary Pulsar System PSR J1023+0038

TL;DR: In this article, radio and γ-ray observations along with concurrent X-ray data were used to reveal that the binary millisecond pulsar (MSP)/low-mass Xray binary transition system PSR J1023+0038 has undergone a transformation in state, and the radio pulsations at frequencies between 300 to 5000 MHz have now become undetectable.
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A new accretion disk around the missing link binary system psr j1023+0038

TL;DR: In this paper, the first targeted X-ray observations were performed of the active phase and complementing them with UV/optical and radio observations collected in 2013 October, and they found strong evidence that indeed an accretion disk has recently formed in the system and reported the detection of fast Xray changes spanning about two orders of magnitude in luminosity.
References
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Journal ArticleDOI

The NRAO VLA Sky Survey

TL;DR: The NRAO VLA Sky Survey (NVSS) covers the sky north of J2000 at 1.4 GHz as discussed by the authors, including a set of 2326 4?? 4? continuum cubes with three planes containing Stokes I, Q, and U images plus a catalog of almost 2? 106 discrete sources stronger than S 2.5 mJy.
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The FIRST Survey: Faint Images of the Radio Sky at twenty centimeters

TL;DR: The first year of the First Radio Sky at Twenty centimeters (FIRST) survey as discussed by the authors was performed using the NRAO Very Large Array (VLA) with a total of 144 hr of time in 1993 April and May was used for a variety of tests, as well as to cover an initial strip of the survey extending between 07{sup h}15{sup m} and 16{suph}30{supm} in a 2{sq_bullet}8 wide declination zone passing through the local zenith.
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Sloan digital sky survey: Early data release

Chris Stoughton, +212 more
TL;DR: The Sloan Digital Sky Survey (SDSS) is an imaging and spectroscopic survey that will eventually cover approximately one-quarter of the celestial sphere and collect spectra of ≈106 galaxies, 100,000 quasars, 30,000 stars, and 30, 000 serendipity targets as discussed by the authors.
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A Catalog of 1.4 GHz Radio Sources from the FIRST Survey

TL;DR: In this article, the authors presented a catalog of 138,665 radio sources derived from the initial 1550 deg2 of the FIRST survey, which they used to construct a log N-log S relation for 20 cm radio sources over four decades of flux density, finding excellent agreement with previous determinations from smaller surveys.
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Several other magnetic CVs are known to be variable radio sources, suggesting that FIRST J1023+0038 is a new member of this class (and the first CV to be discovered on the basis of radio emission).