The First VERA Astrometry Catalog

Author:

Hirota Tomoya12, ,Nagayama Takumi3,Honma Mareki345,Adachi Yuuki3,Burns Ross A1,Chibueze James O67,Choi Yoon Kyung8,Hachisuka Kazuya3,Hada Kazuhiro34,Hagiwara Yoshiaki9,Hamada Shota10,Handa Toshihiro1011,Hashimoto Mao12,Hirano Ken3,Hirata Yushi10,Ichikawa Takanori10,Imai Hiroshi101113ORCID,Inenaga Daichi12,Ishikawa Toshio3,Jike Takaaki34,Kameya Osamu34,Kaseda Daichi10,Kim Jeong Sook14,Kim Jungha2,Kim Mi Kyoung3,Kobayashi Hideyuki12,Kono Yusuke12,Kurayama Tomoharu15,Matsuno Masako10,Morita Atsushi10,Motogi Kazuhito16,Murase Takeru10,Nakagawa Akiharu1011,Nakanishi Hiroyuki1011,Niinuma Kotaro16,Nishi Junya12,Oh Chung Sik14,Omodaka Toshihiro10,Oyadomari Miyako13,Oyama Tomoaki3,Sakai Daisuke3,Sakai Nobuyuki14,Sawada-Satoh Satoko16,Shibata Katsunori M12,Shizugami Makoto117,Sudo Jumpei10,Sugiyama Koichiro18,Sunada Kazuyoshi34,Suzuki Syunsaku1,Takahashi Ken3,Tamura Yoshiaki34,Tazaki Fumie3,Ueno Yuji3,Uno Yuri10,Urago Riku10,Wada Koji10,Wu Yuan Wei19,Yamashita Kazuyoshi3,Yamashita Yuto10,Yamauchi Aya3,Yuda Akito10

Affiliation:

1. Mizusawa VLBI Observatory, National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan

2. Department of Astronomical Sciences, SOKENDAI (The Graduate University for Advanced Studies), 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan

3. Mizusawa VLBI Observatory, National Astronomical Observatory of Japan, 2-12 Hoshigaoka, Mizusawa-ku, Oshu, Iwate 023-0861, Japan

4. Department of Astronomical Sciences, SOKENDAI (The Graduate University for Advanced Studies), 2-12 Hoshigaoka, Mizusawa-ku, Oshu, Iwate 023-0861, Japan

5. Department of Astronomy, Graduate School of Science, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan

6. Centre for Space Research, Physics Department, North-West University, Potchefstroom 2520, South Africa

7. Department of Physics and Astronomy, Faculty of Physical Sciences, University of Nigeria, Carver Building, 1 University Road, Nsukka, Nigeria

8. Max-Planck-Institut für Radioastronomy, Auf dem Hügel 69, D-53121-Bonn, Germany

9. Toyo University, 5-28-20 Hakusan, Bunkyo-ku, Tokyo 112-8606, Japan

10. Graduate School of Science and Engineering, Kagoshima University, 1-21-35 Korimoto, Kagoshima, Kagoshima 890-0065, Japan

11. Amanogawa Galaxy Astronomy Research Center, Graduate School of Science and Engineering, Kagoshima University, 1-21-35 Korimoto, Kagoshima, Kagoshima 890-0065, Japan

12. Faculty of Science, Kagoshima University, 1-21-35 Korimoto, Kagoshima, Kagoshima 890-0065, Japan

13. Center for General Education, Institute for Comprehensive Education, Kagoshima University, 1-21-30 Korimoto, Kagoshima, Kagoshima 890-0065, Japan

14. Korea Astronomy and Space Science Institute, Hwaam-dong 61-1, Yuseong-gu, Daejeon, 305-348, Republic of Korea

15. Teikyo University of Science, 2-2-1 Senju-Sakuragi, Adachi-ku, Tokyo 120-0045, Japan

16. Graduate School of Sciences and Technology for Innovation, Yamaguchi University, 1677-1 Yoshida, Yamaguchi, Yamaguchi 753-8512, Japan

17. NAOJ ALMA Project, National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan

18. National Astronomical Research Institute of Thailand, 260 Moo 4, T. Donkaew, Amphur Maerim, Chiang Mai, 50180, Thailand

19. National Time Service Center, Key Laboratory of Precise Positioning and Timing Technology, Chinese Academy of Sciences, Xi’an 710600, People’s Republic of China

Abstract

AbstractWe 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 the 78 sources are referred to in previously published results or those in preparation for forthcoming papers. The accuracy in the VERA astrometry is revisited and compared with that 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 parameters of $R_{0}=7.92\pm 0.16_{\rm {stat.}}\pm 0.3_{\rm {sys.}}\:$kpc and $\Omega _{\odot }=30.17\pm 0.27_{\rm {stat.}}\pm 0.3_{\rm {sys.}}\:$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.

Funder

NAOJ

Japan Society for the Promotion of Science

South African Department of Science and Technology National Research Foundation

ISARP

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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