output
19992026
most citedHigh-Sensitivity 86GHz (3.5mm) VLBI Observations of M87: Deep Imaging of the Jet Base at a 10 Schwarzschild-Radius Resolution

173 citations

Showing 2021Show all

7 papers · 1 filter

astro-ph.HE2021★ 27 cited

The intrinsic structure of Sagittarius A* at 1.3 cm and 7 mm

Ilje Cho, Guang-Yao Zhao, Tomohisa Kawashima +63

Sagittarius A* (Sgr A*), the Galactic Center supermassive black hole (SMBH), is one of the best targets to resolve the innermost region of SMBH with very long baseline interferomet…

hep-ph2021★ 29 cited

Non-resonant new physics search at the LHC for the anomalies

Motoi Endo, Syuhei Iguro, Teppei Kitahara +2

Motivated by the anomalies, we study non-resonant searches for new physics at the large hadron collider (LHC) by considering final states with an energetic an…

astro-ph.GA2021★ 10 cited

Second Epoch ALMA Observations of 321 GHz Water Maser Emission in NGC 4945 and the Circinus Galaxy

Yoshiaki Hagiwara, Shinji Horiuchi, Masatoshi Imanishi +1

We present the results of second epoch ALMA observations of 321 GHz HO emission toward two nearby active galactic nuclei, NGC 4945 and the Circinus galaxy, together with Tidbin…

astro-ph.GA2021★ 19 cited

East Asian VLBI Network Observations of Active Galactic Nuclei Jets: Imaging with KaVA+Tianma+Nanshan

Yuzhu Cui, Kazuhiro Hada, Motoki Kino +74

The East Asian very-long-baseline interferometry (VLBI) Network (EAVN) is a rapidly evolving international VLBI array that is currently promoted under joint efforts among China, Ja…

math.NT2021

Variations of Ramanujan's Euler Products

Shin-ya Koyama, Nobushige Kurokawa

We study the meromorphy of various Euler products of degree two attached to cusp forms including Ramanujan's -function.

astro-ph.GA2021★ 8 cited

ALMA detection of millimetre 183 GHz H2O maser emission in the Superantennae galaxy at z ~ 0.06

Masatoshi Imanishi, Yoshiaki Hagiwara, Shinji Horiuchi +2

We present the results of ALMA band-5 (~170 GHz) observations of the merging ultraluminous infrared galaxy, the "Superantennae" (IRAS 19254-7245) at z=0.0617, which has been diagno…