Search Publications

Characterizing motion types of G-band bright points in the quiet Sun
DOI: 10.1088/1674-4527/15/4/009 Bibcode: 2015RAA....15..569Y

Feng, Song; Wang, Feng; Deng, Hui +4 more

We study the motion of G-band bright points (GBPs) in the quiet Sun to obtain the characteristics of different motion types. A high resolution image sequence taken with the Hinode/Solar Optical Telescope (SOT) is used, and GBPs are automatically tracked by segmenting 3D evolutional structures in a space-time cube. After putting the GBPs that do no…

2015 Research in Astronomy and Astrophysics
Hinode 46
Suzaku observation of Be/X-ray binary pulsar EXO 2030+375
DOI: 10.1088/1674-4527/15/4/007 Bibcode: 2015RAA....15..537N

Naik, Sachindra; Jaisawal, Gaurava K.

We study the timing and spectral properties of Be/X-ray binary pulsar EXO 2030+375 using a Suzaku observation taken on 2012 May 23, during a less intense Type I outburst. Pulsations were clearly detected in the X-ray light curves at a barycentric period of 41.2852 s, which suggest that the pulsar is spinning-up. The pulse profiles were found to be…

2015 Research in Astronomy and Astrophysics
Suzaku 17
Photometric Calibration of the Lunar-based Ultraviolet Telescope for Its First Six Months of Operation on the Lunar Surface
DOI: 10.1088/1674-4527/15/7/014 Bibcode: 2015RAA....15.1068W

Wang, Shen; Wang, Jing; Meng, Xian-Min +10 more

We describe the photometric calibration of the Lunar-based Ultraviolet Telescope (LUT), the first robotic astronomical telescope working on the lunar surface, for its first six months of operation on the lunar surface. Two spectral datasets (set A and B) from near-ultraviolet (NUV) to the optical band were constructed with 44 International Ultravi…

2015 Research in Astronomy and Astrophysics
IUE 17
Morphology and structure of BzK-selected galaxies at z ∼ 2 in the CANDELS-COSMOS field
DOI: 10.1088/1674-4527/15/6/005 Bibcode: 2015RAA....15..819F

Kong, Xu; Chen, Yang; Fang, Guan-Wen +1 more

Utilizing a BzK-selection technique, we obtain 14550 star-forming galaxies (sBzKs) and 1763 passive galaxies (pBzKs) at z ∼ 2 from the K-selected (KAB < 22.5) catalog in the COSMOS/UltraVISTA field. The differential number counts of sBzKs and pBzKs are consistent with the results from the literature. Compared to the observed results,…

2015 Research in Astronomy and Astrophysics
eHST 7
Propagating disturbances along fan-like coronal loops in an active region
DOI: 10.1088/1674-4527/15/11/006 Bibcode: 2015RAA....15.1832M

Teriaca, Luca; Krishna Prasad, S.; Banerjee, Dipankar +2 more

Propagating disturbances are often observed in active region fan-like coronal loops. They were thought to be due to slow mode magnetohydrodynamic waves based on some of the observed properties. However, recent studies involving spectroscopy indicate that they could be due to high speed quasi-periodic upflows which are difficult to distinguish from…

2015 Research in Astronomy and Astrophysics
Hinode 6
Differential measurement of atmospheric refraction using a telescope with double fields of view
DOI: 10.1088/1674-4527/15/10/011 Bibcode: 2015RAA....15.1742Y

Zhao, Ming; Yu, Yong; Cao, Jian-Jun +2 more

For the sake of advancing theoretical research about atmospheric refraction, the atmospheric refraction observed at lower angles of elevation is still worth analyzing and exploring. In some engineering applications, objects with a larger zenith distance must sometimes be observed. Carrying out observational research on atmospheric refraction at lo…

2015 Research in Astronomy and Astrophysics
Hipparcos 5
Understanding the X-ray spectrum of anomalous X-ray pulsars and soft gamma-ray repeaters
DOI: 10.1088/1674-4527/15/4/006 Bibcode: 2015RAA....15..525G

Liu, Yuan; Guo, Yan-Jun; Tong, Hao +3 more

Hard X-rays above 10 keV are detected from several anomalous X-ray pulsars (AXPs) and soft gamma-ray repeaters (SGRs), and different models have been proposed to explain the physical origin within the frame of either a magnetar model or a fallback disk system. Using data from Suzaku and INTEGRAL, we study the soft and hard X-ray spectra of four AX…

2015 Research in Astronomy and Astrophysics
INTEGRAL Suzaku 5
High resolution deep imaging of a bright radio quiet QSO at z ~ 3
DOI: 10.1088/1674-4527/15/5/006 Bibcode: 2015RAA....15..673W

Tanaka, Ichi; Yamada, Toru; Iye, Masanori +3 more

We have obtained deep J and Ks-band images centered on a bright radio quiet QSO UM 402 (zem = 2.856) using the IRCS camera and adaptive optics systems that are part of the Subaru Telescope, as well as retrieved WFC3/F140W archive images of this object. A faint galaxy (mk = 23.32±0.05 in the Vega magnitude system) that lies ~ …

2015 Research in Astronomy and Astrophysics
eHST 4
Galactic coordinate system based on multi-wavelength catalogs
DOI: 10.1088/1674-4527/15/7/012 Bibcode: 2015RAA....15.1045D

Zhu, Zi; Liu, Jia-Cheng; Ding, Ping-Jie

The currently used Galactic coordinate system (GalCS) is based on the FK5 system at J2000.0, which was transformed from the FK4 system at B1950.0. The limitations and misunderstandings related to this transformed GalCS can be avoided by defining a new GalCS that is directly connected to the International Celestial Reference System (ICRS). With mor…

2015 Research in Astronomy and Astrophysics
AKARI 3
Morphology and structure of extremely red objects at z ∼ 1 in the CANDELS-COSMOS field
DOI: 10.1088/1674-4527/15/6/004 Bibcode: 2015RAA....15..811F

Kong, Xu; Chen, Yang; Fang, Guan-Wen +1 more

Using high-resolution HST/Wide Field Camera 3 F125W imaging from the CANDELS-COSMOS field, we report the structural and morphological properties of extremely red objects (EROs) at z ∼ 1. Based on the UVJ color criteria, we separate EROs into two types: old passive galaxies (OGs) and dusty star-forming galaxies (DGs). For a given stellar mass, we f…

2015 Research in Astronomy and Astrophysics
eHST 3