The First VERA Astrometry Catalog
We present the first astrometry catalog from the Japanese VLBI (very long baseline interferometer) project VERA (VLBI Exploration of Radio Astrometry). We have compiled all the astrometry results from VERA, providing accurate trigonometric annual parallax and proper motion measurements. In total, 99...
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creator | collaboration, VERA Hirota, Tomoya Nagayama, Takumi Honma, Mareki Adachi, Yuuki Burns, Ross A Chibueze, James O Choi, Yoon Kyung Hachisuka, Kazuya Hada, Kazuhiro Hagiwara, Yoshiaki Hamada, Shota Handa, Toshihiro Hashimoto, Mao Hirano, Ken Hirata, Yushi Ichikawa, Takanori Imai, Hiroshi Inenaga, Daichi Ishikawa, Toshio Jike, Takaaki Kameya, Osamu Kaseda, Daichi Kim, Jeong Sook Kim, Jungha Kim, Mi Kyoung Kobayashi, Hideyuki Kono, Yusuke Kurayama, Tomoharu Matsuno, Masako Morita, Atsushi Motogi, Kazuhito Murase, Takeru Nakagawa, Akiharu Nakanishi, Hiroyuki Niinuma, Kotaro Nishi, Junya Oh, Chung Sik Omodaka, Toshihiro Oyadomari, Miyako Oyama, Tomoaki Sakai, Daisuke Sakai, Nobuyuki Sawada-Satoh, Satoko Shibata, Katsunori M Shizugami, Makoto Sudo, Jumpei Sugiyama, Koichiro Sunada, Kazuyoshi Suzuki, Syunsaku Takahashi, Ken Tamura, Yoshiaki Tazaki, Fumie Ueno, Yuji Uno, Yuri Urago, Riku Wada, Koji Yuan Wei Wu Yamashita, Kazuyoshi Yamashita, Yuto Yamauchi, Aya Yuda, Akito |
description | We present the first astrometry catalog from the Japanese VLBI (very long baseline interferometer) project VERA (VLBI Exploration of Radio Astrometry). We have compiled all the astrometry results from VERA, providing accurate trigonometric annual parallax and proper motion measurements. In total, 99 maser sources are listed in the VERA catalog. Among them, 21 maser sources are newly reported while the rest of 78 sources are referred to previously published results or those in preparation for forthcoming papers. The accuracy in the VERA astrometry are revisited and compared with those from the other VLBI astrometry projects such as BeSSeL (The Bar and Spiral Structure Legacy) Survey and GOBELINS (the Gould's Belt Distances Survey) with the VLBA (Very Long Baseline Array). We have confirmed that most of the astrometry results are consistent with each other, and the largest error sources are due to source structure of the maser features and their rapid variation, along with the systematic calibration errors and different analysis methods. Combined with the BeSSeL results, we estimate the up-to-date fundamental Galactic parameter of \(R_{0}=7.92\pm0.16_{\rm{stat.}}\pm0.3_{\rm{sys.}}\)~kpc and \(\Omega_{\odot}=30.17\pm0.27_{\rm{stat.}}\pm0.3_{\rm{sys.}}\)~km~s\(^{-1}\)~kpc\(^{-1}\), where \(R_{0}\) and \(\Omega_{\odot}\) are the distance from the Sun to the Galactic center and the Sun's angular velocity of the Galactic circular rotation, respectively. |
doi_str_mv | 10.48550/arxiv.2002.03089 |
format | Article |
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We have compiled all the astrometry results from VERA, providing accurate trigonometric annual parallax and proper motion measurements. In total, 99 maser sources are listed in the VERA catalog. Among them, 21 maser sources are newly reported while the rest of 78 sources are referred to previously published results or those in preparation for forthcoming papers. The accuracy in the VERA astrometry are revisited and compared with those from the other VLBI astrometry projects such as BeSSeL (The Bar and Spiral Structure Legacy) Survey and GOBELINS (the Gould's Belt Distances Survey) with the VLBA (Very Long Baseline Array). We have confirmed that most of the astrometry results are consistent with each other, and the largest error sources are due to source structure of the maser features and their rapid variation, along with the systematic calibration errors and different analysis methods. Combined with the BeSSeL results, we estimate the up-to-date fundamental Galactic parameter of \(R_{0}=7.92\pm0.16_{\rm{stat.}}\pm0.3_{\rm{sys.}}\)~kpc and \(\Omega_{\odot}=30.17\pm0.27_{\rm{stat.}}\pm0.3_{\rm{sys.}}\)~km~s\(^{-1}\)~kpc\(^{-1}\), where \(R_{0}\) and \(\Omega_{\odot}\) are the distance from the Sun to the Galactic center and the Sun's angular velocity of the Galactic circular rotation, respectively.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.2002.03089</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Angular velocity ; Astrometry ; Galactic rotation ; Parallax ; Parameter estimation ; Physics - Astrophysics of Galaxies</subject><ispartof>arXiv.org, 2020-02</ispartof><rights>2020. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). 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We have compiled all the astrometry results from VERA, providing accurate trigonometric annual parallax and proper motion measurements. In total, 99 maser sources are listed in the VERA catalog. Among them, 21 maser sources are newly reported while the rest of 78 sources are referred to previously published results or those in preparation for forthcoming papers. The accuracy in the VERA astrometry are revisited and compared with those from the other VLBI astrometry projects such as BeSSeL (The Bar and Spiral Structure Legacy) Survey and GOBELINS (the Gould's Belt Distances Survey) with the VLBA (Very Long Baseline Array). We have confirmed that most of the astrometry results are consistent with each other, and the largest error sources are due to source structure of the maser features and their rapid variation, along with the systematic calibration errors and different analysis methods. Combined with the BeSSeL results, we estimate the up-to-date fundamental Galactic parameter of \(R_{0}=7.92\pm0.16_{\rm{stat.}}\pm0.3_{\rm{sys.}}\)~kpc and \(\Omega_{\odot}=30.17\pm0.27_{\rm{stat.}}\pm0.3_{\rm{sys.}}\)~km~s\(^{-1}\)~kpc\(^{-1}\), where \(R_{0}\) and \(\Omega_{\odot}\) are the distance from the Sun to the Galactic center and the Sun's angular velocity of the Galactic circular rotation, respectively.</description><subject>Angular velocity</subject><subject>Astrometry</subject><subject>Galactic rotation</subject><subject>Parallax</subject><subject>Parameter estimation</subject><subject>Physics - Astrophysics of 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Kono, Yusuke ; Kurayama, Tomoharu ; Matsuno, Masako ; Morita, Atsushi ; Motogi, Kazuhito ; Murase, Takeru ; Nakagawa, Akiharu ; Nakanishi, Hiroyuki ; Niinuma, Kotaro ; Nishi, Junya ; Oh, Chung Sik ; Omodaka, Toshihiro ; Oyadomari, Miyako ; Oyama, Tomoaki ; Sakai, Daisuke ; Sakai, Nobuyuki ; Sawada-Satoh, Satoko ; Shibata, Katsunori M ; Shizugami, Makoto ; Sudo, Jumpei ; Sugiyama, Koichiro ; Sunada, Kazuyoshi ; Suzuki, Syunsaku ; Takahashi, Ken ; Tamura, Yoshiaki ; Tazaki, Fumie ; Ueno, Yuji ; Uno, Yuri ; Urago, Riku ; Wada, Koji ; Yuan Wei Wu ; Yamashita, Kazuyoshi ; Yamashita, Yuto ; Yamauchi, Aya ; Yuda, Akito</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a527-13c9269a55359ec6863ad0002334312618f7fb03bd36bd35cbcea59111278c0a3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2020</creationdate><topic>Angular velocity</topic><topic>Astrometry</topic><topic>Galactic 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Kazuyoshi</creatorcontrib><creatorcontrib>Yamashita, Yuto</creatorcontrib><creatorcontrib>Yamauchi, Aya</creatorcontrib><creatorcontrib>Yuda, Akito</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science & Engineering Collection</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest Central UK/Ireland</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>SciTech Premium Collection</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>Publicly Available Content Database</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>Engineering Collection</collection><collection>arXiv.org</collection><jtitle>arXiv.org</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>collaboration, VERA</au><au>Hirota, Tomoya</au><au>Nagayama, Takumi</au><au>Honma, Mareki</au><au>Adachi, Yuuki</au><au>Burns, Ross A</au><au>Chibueze, James O</au><au>Choi, Yoon Kyung</au><au>Hachisuka, Kazuya</au><au>Hada, Kazuhiro</au><au>Hagiwara, Yoshiaki</au><au>Hamada, Shota</au><au>Handa, Toshihiro</au><au>Hashimoto, Mao</au><au>Hirano, Ken</au><au>Hirata, Yushi</au><au>Ichikawa, Takanori</au><au>Imai, Hiroshi</au><au>Inenaga, Daichi</au><au>Ishikawa, Toshio</au><au>Jike, Takaaki</au><au>Kameya, Osamu</au><au>Kaseda, Daichi</au><au>Kim, Jeong Sook</au><au>Kim, Jungha</au><au>Kim, Mi Kyoung</au><au>Kobayashi, Hideyuki</au><au>Kono, Yusuke</au><au>Kurayama, Tomoharu</au><au>Matsuno, Masako</au><au>Morita, Atsushi</au><au>Motogi, Kazuhito</au><au>Murase, Takeru</au><au>Nakagawa, Akiharu</au><au>Nakanishi, Hiroyuki</au><au>Niinuma, Kotaro</au><au>Nishi, Junya</au><au>Oh, Chung Sik</au><au>Omodaka, Toshihiro</au><au>Oyadomari, Miyako</au><au>Oyama, Tomoaki</au><au>Sakai, Daisuke</au><au>Sakai, Nobuyuki</au><au>Sawada-Satoh, Satoko</au><au>Shibata, Katsunori M</au><au>Shizugami, Makoto</au><au>Sudo, Jumpei</au><au>Sugiyama, Koichiro</au><au>Sunada, Kazuyoshi</au><au>Suzuki, Syunsaku</au><au>Takahashi, Ken</au><au>Tamura, Yoshiaki</au><au>Tazaki, Fumie</au><au>Ueno, Yuji</au><au>Uno, Yuri</au><au>Urago, Riku</au><au>Wada, Koji</au><au>Yuan Wei Wu</au><au>Yamashita, Kazuyoshi</au><au>Yamashita, Yuto</au><au>Yamauchi, Aya</au><au>Yuda, Akito</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>The First VERA Astrometry Catalog</atitle><jtitle>arXiv.org</jtitle><date>2020-02-08</date><risdate>2020</risdate><eissn>2331-8422</eissn><abstract>We present the first astrometry catalog from the Japanese VLBI (very long baseline interferometer) project VERA (VLBI Exploration of Radio Astrometry). We have compiled all the astrometry results from VERA, providing accurate trigonometric annual parallax and proper motion measurements. In total, 99 maser sources are listed in the VERA catalog. Among them, 21 maser sources are newly reported while the rest of 78 sources are referred to previously published results or those in preparation for forthcoming papers. The accuracy in the VERA astrometry are revisited and compared with those from the other VLBI astrometry projects such as BeSSeL (The Bar and Spiral Structure Legacy) Survey and GOBELINS (the Gould's Belt Distances Survey) with the VLBA (Very Long Baseline Array). We have confirmed that most of the astrometry results are consistent with each other, and the largest error sources are due to source structure of the maser features and their rapid variation, along with the systematic calibration errors and different analysis methods. Combined with the BeSSeL results, we estimate the up-to-date fundamental Galactic parameter of \(R_{0}=7.92\pm0.16_{\rm{stat.}}\pm0.3_{\rm{sys.}}\)~kpc and \(\Omega_{\odot}=30.17\pm0.27_{\rm{stat.}}\pm0.3_{\rm{sys.}}\)~km~s\(^{-1}\)~kpc\(^{-1}\), where \(R_{0}\) and \(\Omega_{\odot}\) are the distance from the Sun to the Galactic center and the Sun's angular velocity of the Galactic circular rotation, respectively.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.2002.03089</doi><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | EISSN: 2331-8422 |
ispartof | arXiv.org, 2020-02 |
issn | 2331-8422 |
language | eng |
recordid | cdi_arxiv_primary_2002_03089 |
source | arXiv.org; Free E- Journals |
subjects | Angular velocity Astrometry Galactic rotation Parallax Parameter estimation Physics - Astrophysics of Galaxies |
title | The First VERA Astrometry Catalog |
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