Targeted search for young radio pulsars in the SMC: discovery of two new pulsars

N. Titus; B. W.  Stappers; V. Morello; Manisha Caleb; M. D. FilipoviÄ‡; V. A. McBride; W C G Ho; David Buckley

doi:10.1093/mnras/stz1578

Targeted search for young radio pulsars in the SMC: discovery of two new pulsars

N. Titus, B. W. Stappers, V. Morello, Manisha Caleb, M. D. FilipoviÄ‡, V. A. McBride, W C G Ho, David Buckley

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

Abstract

We report the first rotation powered pulsars discovered in the Small Magellanic Cloud (SMC) in more than a decade. PSR J0043–73 and PSR J0052–72 were discovered during a Parkes Multi-Beam (PMB) survey of MCSNR J0127–7332, and five new, optically selected, supernova remnant (SNR) candidates identified by the XMM–Newton survey. In addition to the candidates, we adjusted the PMB rotation to include additional nine SNRs and pulsar wind nebulae. We searched for young pulsars (1–200 ms) employing a Fourier analysis with PRESTO, as well as a search for longer period pulsars (200 ms–360 s) with a fast folding algorithm. Our targeted survey had a limiting flux density of 0.039 mJy for periods greater than 50 ms. Although not the main target of this search it was also sensitive to millisecond pulsars. PSR J0043–73 has a period and dispersion measure of 937.429 37 (26) ms and 115.1 (3.4) pc cm−3, respectively, and PSR J0052–72 has a period of 191.444 328 (46) ms and a DM of 158.6 (1.6) pc cm−3.

Original language	English
Pages (from-to)	4332-4342
Journal	Monthly Notices of the Royal Astronomical Society
Volume	487
Issue number	3
DOIs	https://doi.org/10.1093/mnras/stz1578
Publication status	Published - 2019

Access to Document

10.1093/mnras/stz1578

Cite this

@article{54ef509e89f046f6a66778da2c473ba0,

title = "Targeted search for young radio pulsars in the SMC: discovery of two new pulsars",

abstract = "We report the first rotation powered pulsars discovered in the Small Magellanic Cloud (SMC) in more than a decade. PSR J0043–73 and PSR J0052–72 were discovered during a Parkes Multi-Beam (PMB) survey of MCSNR J0127–7332, and five new, optically selected, supernova remnant (SNR) candidates identified by the XMM–Newton survey. In addition to the candidates, we adjusted the PMB rotation to include additional nine SNRs and pulsar wind nebulae. We searched for young pulsars (1–200 ms) employing a Fourier analysis with PRESTO, as well as a search for longer period pulsars (200 ms–360 s) with a fast folding algorithm. Our targeted survey had a limiting flux density of 0.039 mJy for periods greater than 50 ms. Although not the main target of this search it was also sensitive to millisecond pulsars. PSR J0043–73 has a period and dispersion measure of 937.429 37 (26) ms and 115.1 (3.4) pc cm−3, respectively, and PSR J0052–72 has a period of 191.444 328 (46) ms and a DM of 158.6 (1.6) pc cm−3.",

author = "N. Titus and Stappers, {B. W.} and V. Morello and Manisha Caleb and Filipovi{\"A}‡, {M. D.} and McBride, {V. A.} and Ho, {W C G} and David Buckley",

year = "2019",

doi = "10.1093/mnras/stz1578",

language = "English",

volume = "487",

pages = "4332--4342",

journal = "Monthly Notices of the Royal Astronomical Society",

issn = "1365-2966",

publisher = "Oxford University Press ",

number = "3",

}

TY - JOUR

T1 - Targeted search for young radio pulsars in the SMC: discovery of two new pulsars

AU - Titus, N.

AU - Stappers, B. W.

AU - Morello, V.

AU - Caleb, Manisha

AU - FilipoviÄ‡, M. D.

AU - McBride, V. A.

AU - Ho, W C G

AU - Buckley, David

PY - 2019

Y1 - 2019

N2 - We report the first rotation powered pulsars discovered in the Small Magellanic Cloud (SMC) in more than a decade. PSR J0043–73 and PSR J0052–72 were discovered during a Parkes Multi-Beam (PMB) survey of MCSNR J0127–7332, and five new, optically selected, supernova remnant (SNR) candidates identified by the XMM–Newton survey. In addition to the candidates, we adjusted the PMB rotation to include additional nine SNRs and pulsar wind nebulae. We searched for young pulsars (1–200 ms) employing a Fourier analysis with PRESTO, as well as a search for longer period pulsars (200 ms–360 s) with a fast folding algorithm. Our targeted survey had a limiting flux density of 0.039 mJy for periods greater than 50 ms. Although not the main target of this search it was also sensitive to millisecond pulsars. PSR J0043–73 has a period and dispersion measure of 937.429 37 (26) ms and 115.1 (3.4) pc cm−3, respectively, and PSR J0052–72 has a period of 191.444 328 (46) ms and a DM of 158.6 (1.6) pc cm−3.

AB - We report the first rotation powered pulsars discovered in the Small Magellanic Cloud (SMC) in more than a decade. PSR J0043–73 and PSR J0052–72 were discovered during a Parkes Multi-Beam (PMB) survey of MCSNR J0127–7332, and five new, optically selected, supernova remnant (SNR) candidates identified by the XMM–Newton survey. In addition to the candidates, we adjusted the PMB rotation to include additional nine SNRs and pulsar wind nebulae. We searched for young pulsars (1–200 ms) employing a Fourier analysis with PRESTO, as well as a search for longer period pulsars (200 ms–360 s) with a fast folding algorithm. Our targeted survey had a limiting flux density of 0.039 mJy for periods greater than 50 ms. Although not the main target of this search it was also sensitive to millisecond pulsars. PSR J0043–73 has a period and dispersion measure of 937.429 37 (26) ms and 115.1 (3.4) pc cm−3, respectively, and PSR J0052–72 has a period of 191.444 328 (46) ms and a DM of 158.6 (1.6) pc cm−3.

U2 - 10.1093/mnras/stz1578

DO - 10.1093/mnras/stz1578

M3 - Article

SN - 1365-2966

VL - 487

SP - 4332

EP - 4342

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

IS - 3

ER -

Targeted search for young radio pulsars in the SMC: discovery of two new pulsars

Abstract

Access to Document

Fingerprint

Cite this