GaLactic and Extragalactic All-sky Murchison Widefield Array (GLEAM) survey II: Galactic Plane $345^\circ < l < 67^\circ$, $180^\circ < l < 240^\circ
This work makes available a further 2,860deg$^2$ of the GLEAM survey, covering half of the accessible Galactic Plane, across twenty frequency bands sampling $72-231$MHz, with resolution $4'-2'$. Unlike previous GLEAM data releases, we used multi-scale clean to better deconvolve large-scale...
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creator | Hurley-Walker, Natasha Hancock, Paul J Franzen, Thomas M. O Callingham, Joseph R Offringa, Andre R Hindson, Luke Wu, Chen Bell, Martin E For, Bi-Qing Gaensler, Bryan M Johnston-Hollitt, Melanie Kapinska, Anna D Morgan, John Murphy, Tara McKinley, Benjamin Procopio, Pietro Staveley-Smith, Lister Wayth, Randall B Zheng, Cathie Q |
description | This work makes available a further 2,860deg$^2$ of the GLEAM survey,
covering half of the accessible Galactic Plane, across twenty frequency bands
sampling $72-231$MHz, with resolution $4'-2'$. Unlike previous GLEAM data
releases, we used multi-scale clean to better deconvolve large-scale Galactic
structure. For the Galactic longitude ranges $345^\circ < l < 67^\circ$,
$180^\circ < l < 240^\circ$, we provide a compact source catalogue of 22,037
components selected from a 60-MHz bandwidth image centred at 200-MHz, with RMS
noise $\approx10-20$mJy beam$^{-1}$ and position accuracy better than $2"$. The
catalogue has a completeness of 50% at $\approx120$mJy, and a reliability of
99.86%. It covers Galactic latitudes $1^\circ\leq|b|\leq10^\circ$ toward the
Galactic Centre and $|b|\leq10^\circ$ for other regions, and is available from
Vizier; images covering $|b|\leq10^\circ$ for all longitudes are made available
on the GLEAM VO server and SkyView. |
doi_str_mv | 10.48550/arxiv.1911.08127 |
format | Article |
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covering half of the accessible Galactic Plane, across twenty frequency bands
sampling $72-231$MHz, with resolution $4'-2'$. Unlike previous GLEAM data
releases, we used multi-scale clean to better deconvolve large-scale Galactic
structure. For the Galactic longitude ranges $345^\circ < l < 67^\circ$,
$180^\circ < l < 240^\circ$, we provide a compact source catalogue of 22,037
components selected from a 60-MHz bandwidth image centred at 200-MHz, with RMS
noise $\approx10-20$mJy beam$^{-1}$ and position accuracy better than $2"$. The
catalogue has a completeness of 50% at $\approx120$mJy, and a reliability of
99.86%. It covers Galactic latitudes $1^\circ\leq|b|\leq10^\circ$ toward the
Galactic Centre and $|b|\leq10^\circ$ for other regions, and is available from
Vizier; images covering $|b|\leq10^\circ$ for all longitudes are made available
on the GLEAM VO server and SkyView.</description><identifier>DOI: 10.48550/arxiv.1911.08127</identifier><language>eng</language><subject>Physics - Astrophysics of Galaxies ; Physics - Instrumentation and Methods for Astrophysics</subject><creationdate>2019-11</creationdate><rights>http://arxiv.org/licenses/nonexclusive-distrib/1.0</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,780,885</link.rule.ids><linktorsrc>$$Uhttps://arxiv.org/abs/1911.08127$$EView_record_in_Cornell_University$$FView_record_in_$$GCornell_University$$Hfree_for_read</linktorsrc><backlink>$$Uhttps://doi.org/10.48550/arXiv.1911.08127$$DView paper in arXiv$$Hfree_for_read</backlink><backlink>$$Uhttps://doi.org/10.1017/pasa.2019.37$$DView published paper (Access to full text may be restricted)$$Hfree_for_read</backlink></links><search><creatorcontrib>Hurley-Walker, Natasha</creatorcontrib><creatorcontrib>Hancock, Paul J</creatorcontrib><creatorcontrib>Franzen, Thomas M. O</creatorcontrib><creatorcontrib>Callingham, Joseph R</creatorcontrib><creatorcontrib>Offringa, Andre R</creatorcontrib><creatorcontrib>Hindson, Luke</creatorcontrib><creatorcontrib>Wu, Chen</creatorcontrib><creatorcontrib>Bell, Martin E</creatorcontrib><creatorcontrib>For, Bi-Qing</creatorcontrib><creatorcontrib>Gaensler, Bryan M</creatorcontrib><creatorcontrib>Johnston-Hollitt, Melanie</creatorcontrib><creatorcontrib>Kapinska, Anna D</creatorcontrib><creatorcontrib>Morgan, John</creatorcontrib><creatorcontrib>Murphy, Tara</creatorcontrib><creatorcontrib>McKinley, Benjamin</creatorcontrib><creatorcontrib>Procopio, Pietro</creatorcontrib><creatorcontrib>Staveley-Smith, Lister</creatorcontrib><creatorcontrib>Wayth, Randall B</creatorcontrib><creatorcontrib>Zheng, Cathie Q</creatorcontrib><title>GaLactic and Extragalactic All-sky Murchison Widefield Array (GLEAM) survey II: Galactic Plane $345^\circ < l < 67^\circ$, $180^\circ < l < 240^\circ</title><description>This work makes available a further 2,860deg$^2$ of the GLEAM survey,
covering half of the accessible Galactic Plane, across twenty frequency bands
sampling $72-231$MHz, with resolution $4'-2'$. Unlike previous GLEAM data
releases, we used multi-scale clean to better deconvolve large-scale Galactic
structure. For the Galactic longitude ranges $345^\circ < l < 67^\circ$,
$180^\circ < l < 240^\circ$, we provide a compact source catalogue of 22,037
components selected from a 60-MHz bandwidth image centred at 200-MHz, with RMS
noise $\approx10-20$mJy beam$^{-1}$ and position accuracy better than $2"$. The
catalogue has a completeness of 50% at $\approx120$mJy, and a reliability of
99.86%. It covers Galactic latitudes $1^\circ\leq|b|\leq10^\circ$ toward the
Galactic Centre and $|b|\leq10^\circ$ for other regions, and is available from
Vizier; images covering $|b|\leq10^\circ$ for all longitudes are made available
on the GLEAM VO server and SkyView.</description><subject>Physics - Astrophysics of Galaxies</subject><subject>Physics - Instrumentation and Methods for Astrophysics</subject><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2019</creationdate><recordtype>article</recordtype><sourceid>GOX</sourceid><recordid>eNpjYJA0NNAzsTA1NdBPLKrILNMztDQ01DOwMDQy52SY6p7ok5hckpmskJiXouBaUVKUmJ6YAxFxzMnRLc6uVPAtLUrOyCzOz1MIz0xJTctMzUlRcCwqSqxU0HD3cXX01VQoLi0qS61U8PS0UnCH6Q7IScxLVVAxNjGNi0nOLEpWsFHIAWIzcwhXRUdBxdDCAEXOyATK52FgTUvMKU7lhdLcDPJuriHOHrpgD8QXFGXmJhZVxoM8Eg_2iDFhFQA7Ak9I</recordid><startdate>20191119</startdate><enddate>20191119</enddate><creator>Hurley-Walker, Natasha</creator><creator>Hancock, Paul J</creator><creator>Franzen, Thomas M. O</creator><creator>Callingham, Joseph R</creator><creator>Offringa, Andre R</creator><creator>Hindson, Luke</creator><creator>Wu, Chen</creator><creator>Bell, Martin E</creator><creator>For, Bi-Qing</creator><creator>Gaensler, Bryan M</creator><creator>Johnston-Hollitt, Melanie</creator><creator>Kapinska, Anna D</creator><creator>Morgan, John</creator><creator>Murphy, Tara</creator><creator>McKinley, Benjamin</creator><creator>Procopio, Pietro</creator><creator>Staveley-Smith, Lister</creator><creator>Wayth, Randall B</creator><creator>Zheng, Cathie Q</creator><scope>GOX</scope></search><sort><creationdate>20191119</creationdate><title>GaLactic and Extragalactic All-sky Murchison Widefield Array (GLEAM) survey II: Galactic Plane $345^\circ < l < 67^\circ$, $180^\circ < l < 240^\circ</title><author>Hurley-Walker, Natasha ; Hancock, Paul J ; Franzen, Thomas M. O ; Callingham, Joseph R ; Offringa, Andre R ; Hindson, Luke ; Wu, Chen ; Bell, Martin E ; For, Bi-Qing ; Gaensler, Bryan M ; Johnston-Hollitt, Melanie ; Kapinska, Anna D ; Morgan, John ; Murphy, Tara ; McKinley, Benjamin ; Procopio, Pietro ; Staveley-Smith, Lister ; Wayth, Randall B ; Zheng, Cathie Q</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-arxiv_primary_1911_081273</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2019</creationdate><topic>Physics - Astrophysics of Galaxies</topic><topic>Physics - Instrumentation and Methods for Astrophysics</topic><toplevel>online_resources</toplevel><creatorcontrib>Hurley-Walker, Natasha</creatorcontrib><creatorcontrib>Hancock, Paul J</creatorcontrib><creatorcontrib>Franzen, Thomas M. O</creatorcontrib><creatorcontrib>Callingham, Joseph R</creatorcontrib><creatorcontrib>Offringa, Andre R</creatorcontrib><creatorcontrib>Hindson, Luke</creatorcontrib><creatorcontrib>Wu, Chen</creatorcontrib><creatorcontrib>Bell, Martin E</creatorcontrib><creatorcontrib>For, Bi-Qing</creatorcontrib><creatorcontrib>Gaensler, Bryan M</creatorcontrib><creatorcontrib>Johnston-Hollitt, Melanie</creatorcontrib><creatorcontrib>Kapinska, Anna D</creatorcontrib><creatorcontrib>Morgan, John</creatorcontrib><creatorcontrib>Murphy, Tara</creatorcontrib><creatorcontrib>McKinley, Benjamin</creatorcontrib><creatorcontrib>Procopio, Pietro</creatorcontrib><creatorcontrib>Staveley-Smith, Lister</creatorcontrib><creatorcontrib>Wayth, Randall B</creatorcontrib><creatorcontrib>Zheng, Cathie Q</creatorcontrib><collection>arXiv.org</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Hurley-Walker, Natasha</au><au>Hancock, Paul J</au><au>Franzen, Thomas M. O</au><au>Callingham, Joseph R</au><au>Offringa, Andre R</au><au>Hindson, Luke</au><au>Wu, Chen</au><au>Bell, Martin E</au><au>For, Bi-Qing</au><au>Gaensler, Bryan M</au><au>Johnston-Hollitt, Melanie</au><au>Kapinska, Anna D</au><au>Morgan, John</au><au>Murphy, Tara</au><au>McKinley, Benjamin</au><au>Procopio, Pietro</au><au>Staveley-Smith, Lister</au><au>Wayth, Randall B</au><au>Zheng, Cathie Q</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>GaLactic and Extragalactic All-sky Murchison Widefield Array (GLEAM) survey II: Galactic Plane $345^\circ < l < 67^\circ$, $180^\circ < l < 240^\circ</atitle><date>2019-11-19</date><risdate>2019</risdate><abstract>This work makes available a further 2,860deg$^2$ of the GLEAM survey,
covering half of the accessible Galactic Plane, across twenty frequency bands
sampling $72-231$MHz, with resolution $4'-2'$. Unlike previous GLEAM data
releases, we used multi-scale clean to better deconvolve large-scale Galactic
structure. For the Galactic longitude ranges $345^\circ < l < 67^\circ$,
$180^\circ < l < 240^\circ$, we provide a compact source catalogue of 22,037
components selected from a 60-MHz bandwidth image centred at 200-MHz, with RMS
noise $\approx10-20$mJy beam$^{-1}$ and position accuracy better than $2"$. The
catalogue has a completeness of 50% at $\approx120$mJy, and a reliability of
99.86%. It covers Galactic latitudes $1^\circ\leq|b|\leq10^\circ$ toward the
Galactic Centre and $|b|\leq10^\circ$ for other regions, and is available from
Vizier; images covering $|b|\leq10^\circ$ for all longitudes are made available
on the GLEAM VO server and SkyView.</abstract><doi>10.48550/arxiv.1911.08127</doi><oa>free_for_read</oa></addata></record> |
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source | arXiv.org |
subjects | Physics - Astrophysics of Galaxies Physics - Instrumentation and Methods for Astrophysics |
title | GaLactic and Extragalactic All-sky Murchison Widefield Array (GLEAM) survey II: Galactic Plane $345^\circ < l < 67^\circ$, $180^\circ < l < 240^\circ |
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