论文标题

第一个Vera天文测量目录

The First VERA Astrometry Catalog

论文作者

VERA collaboration, 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, Wu, Yuan Wei, Yamashita, Kazuyoshi, Yamashita, Yuto, Yamauchi, Aya, Yuda, Akito

论文摘要

我们介绍了日本VLBI(非常长的基线干涉仪)项目Vera(VLBI探索射射线标准)的第一个天文统计目录。我们已经汇编了Vera的所有天体结果,提供了准确的三角年度视差和适当的运动测量。 Vera目录中总共列出了99个MASER来源。其中,新报道了21个MASER来源,而其他78个来源中的其余资料则提到了先前发表的结果或准备即将发表的论文的结果。重新审视了Vera天文标准的准确性,并将其与其他VLBI天文标准项目(例如BESSEL(酒吧和螺旋结构)遗留)和Gobelins(Guld's Belt距离调查)(非常长的基线阵列)进行了比较。我们已经证实,大多数天文统计结果彼此一致,最大的误差源是由于MASER特征的源结构及其快速变化,以及系统的校准误差和不同的分析方法。结合贝塞尔结果,我们估计$ r_ {0} = 7.92 \ pm0.16 _ {\ rm {stat。}} \ pm0.3 _ {\ rm {\ rm {sys。 $ω_ {\ odot} = 30.17 \ pm0.27 _ {\ rm {stat。分别是从太阳到银河中心的距离以及银河圆形旋转的太阳角速度。

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 $Ω_{\odot}=30.17\pm0.27_{\rm{stat.}}\pm0.3_{\rm{sys.}}$~km~s$^{-1}$~kpc$^{-1}$, where $R_{0}$ and $Ω_{\odot}$ are the distance from the Sun to the Galactic center and the Sun's angular velocity of the Galactic circular rotation, respectively.

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