A search for radio pulses from GBS0526-66

Alan Vaughan; M. I. Large

A search for radio pulses from GBS0526-66

Alan Vaughan, M. I. Large

Research output: Contribution to journal › Article › peer-review

Abstract

Observations of GBS0526-66 collected from December 29, 1984-January 3, 1985 with the Molonglo Observatory Synthesis Telescope are examined. The events were accepted based on the instrumental detection thresholds which ranged from about 10 to the -29th J/sq m Hz for 1 microsecond pulses to about 10 to the -26th J/sq m Hz for 1 sec pulses. The effect of interference on the detection of events is discussed. It is observed that no event, other than recognized interference, with a pulse energy density rate greater than that of the acceptance threshold was detected.

Original language	English
Pages (from-to)	159-162
Number of pages	4
Journal	Astrophysical letters & communications
Volume	25
Issue number	3
Publication status	Published - 1987

Cite this

@article{476489416cb94068a6a520311bbc0300,

title = "A search for radio pulses from GBS0526-66",

abstract = "Observations of GBS0526-66 collected from December 29, 1984-January 3, 1985 with the Molonglo Observatory Synthesis Telescope are examined. The events were accepted based on the instrumental detection thresholds which ranged from about 10 to the -29th J/sq m Hz for 1 microsecond pulses to about 10 to the -26th J/sq m Hz for 1 sec pulses. The effect of interference on the detection of events is discussed. It is observed that no event, other than recognized interference, with a pulse energy density rate greater than that of the acceptance threshold was detected.",

author = "Alan Vaughan and Large, \{M. I.\}",

year = "1987",

language = "English",

volume = "25",

pages = "159--162",

journal = "Astrophysical letters \& communications",

issn = "0888-6512",

publisher = "Harwood Academic Publishers GmbH",

number = "3",

}

TY - JOUR

T1 - A search for radio pulses from GBS0526-66

AU - Vaughan, Alan

AU - Large, M. I.

PY - 1987

Y1 - 1987

N2 - Observations of GBS0526-66 collected from December 29, 1984-January 3, 1985 with the Molonglo Observatory Synthesis Telescope are examined. The events were accepted based on the instrumental detection thresholds which ranged from about 10 to the -29th J/sq m Hz for 1 microsecond pulses to about 10 to the -26th J/sq m Hz for 1 sec pulses. The effect of interference on the detection of events is discussed. It is observed that no event, other than recognized interference, with a pulse energy density rate greater than that of the acceptance threshold was detected.

AB - Observations of GBS0526-66 collected from December 29, 1984-January 3, 1985 with the Molonglo Observatory Synthesis Telescope are examined. The events were accepted based on the instrumental detection thresholds which ranged from about 10 to the -29th J/sq m Hz for 1 microsecond pulses to about 10 to the -26th J/sq m Hz for 1 sec pulses. The effect of interference on the detection of events is discussed. It is observed that no event, other than recognized interference, with a pulse energy density rate greater than that of the acceptance threshold was detected.

M3 - Article

SN - 0888-6512

VL - 25

SP - 159

EP - 162

JO - Astrophysical letters & communications

JF - Astrophysical letters & communications

IS - 3

ER -

A search for radio pulses from GBS0526-66

Abstract

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