activity
20002024
most citedDetection of Sub-TeV Gamma-Rays from the Galactic Center Direction by CANGAROO-II

184 citations · 963 across the 25 of their papers we have counts for

collaborators

25 papers

astro-ph.CO2024

Velocity recostruction with graph neural networks

Hideki Tanimura, Albert Bonnefous, Jia Liu +1

In this work, we seek to improve the velocity reconstruction of clusters by using Graph Neural Networks -- a type of deep neural network designed to analyze sparse, unstructured da…

astro-ph.CO2023

Testing decaying dark matter models as a solution to the tension with the thermal Sunyaev-Zel'dovich effect

Hideki Tanimura, Marian Douspis, Nabila Aghanim +1

Considering possible solutions to the tension between the Planck cosmic microwave background (CMB) measurement and low-redshift probes, we extended the standard CDM cosmol…

astro-ph.CO2022★ 3 cited

Self-supervised component separation for the extragalactic submillimeter sky

V. Bonjean, H. Tanimura, N. Aghanim +2

We use a new approach based on self-supervised deep learning networks originally applied to transparency separation in order to simultaneously extract the components of the extraga…

astro-ph.CO2022★ 29 cited

X-ray emission from cosmic web filaments in SRG/eROSITA data

Hideki Tanimura, Nabila Aghanim, Marian Douspis +1

Using the publicly available eROSITA Final Equatorial Depth Survey (eFEDS) data, we detected the stacked X-ray emissions at the position of 463 filaments at a significance of 3.8 s…

astro-ph.CO2022★ 19 cited

Convolutional Neural Network-reconstructed velocity for kinetic SZ detection

Hideki Tanimura, Nabila Aghanim, Victor Bonjean +1

We report the detection of the kinetic Sunyaev-Zel'dovich (kSZ) effect in galaxy clusters with a 4.9 sigma significance using the latest 217 GHz Planck map from data release 4. For…

astro-ph.CO2021★ 1 cited

Constraining AGN feedback model with SZ profile

Hideki Tanimura, Gary Hinshaw, Ian G. McCarthy +7

Relativistic jets from AGN have a wide range of impacts on galaxy groups and clusters and are key for understanding their formation and physical properties. However, this non-gravi…

astro-ph.CO2021★ 1 cited

Cosmic backgrounds from the radio to the far-infrared: recent results and perspectives from cosmological and astrophysical surveys

Carlo Burigana, Elia Sefano Battistelli, Laura Bonavera +8

Cosmological and astrophysical surveys in various wavebands, in particular from the radio to the far-infrared, offer a unique view of the universe's properties and the formation an…

astro-ph.CO2021★ 33 cited

Constraining cosmology with a new all-sky Compton parameter map from the Planck PR4 data

Hideki Tanimura, Marian Douspis, Nabila Aghanim +1

We constructed a new all-sky Compton parameter map (y-map) of the thermal Sunyaev-Zel'dovich (tSZ) effect from the 100 to 857 GHz frequency channel maps delivered within the Planck…

astro-ph.CO2020★ 77 cited

First detection of stacked X-ray emission from cosmic web filaments

H. Tanimura, N. Aghanim, A. Kolodzig +2

We report the first statistical detection of X-ray emission from cosmic web filaments in ROSAT data. We selected 15,165 filaments at 0.2<z<0.6 ranging from 30 Mpc to 100 Mpc in len…

astro-ph.CO2020★ 81 cited

Properties of gas phases around cosmic filaments at z=0 in the Illustris-TNG simulation

Daniela Galárraga-Espinosa, Nabila Aghanim, Mathieu Langer +1

We present the study of gas phases around cosmic-web filaments detected in the TNG300-1 hydro-dynamical simulation at redshift z=0. We separate the gas in five different phases acc…

astro-ph.CO2020★ 34 cited

Direct detection of the kinetic Sunyaev-Zel'dovich effect in galaxy clusters

Hideki Tanimura, Saleem Zaroubi, Nabila Aghanim

We report the direct detection of the kinetic Sunyaev-Zel'dovich (kSZ) effect in galaxy clusters with a 3.5 sigma significance level. The measurement was performed by stacking the…

astro-ph.CO2020★ 62 cited

Characterising filaments in the SDSS volume from the galaxy distribution

Nicola Malavasi, Nabila Aghanim, Marian Douspis +2

Detecting the large-scale structure of the Universe based on the galaxy distribution and characterising its components is of fundamental importance in astrophysics but is also a di…

astro-ph.CO2019★ 45 cited

Filament profiles from WISExSCOS galaxies as probes of the impact of environmental effects

V. Bonjean, N. Aghanim, M. Douspis +2

The role played by the large-scale structures in the galaxy evolution is not quite well understood yet. In this study, we investigate properties of galaxy in the range 0.1<z<0.3 fr…

astro-ph.CO2019★ 50 cited

Like a spider in its web: a study of the Large Scale Structure around the Coma cluster

Nicola Malavasi, Nabila Aghanim, Hideki Tanimura +2

The Cosmic Web is a complex network of filaments, walls and voids that represent the largest structures in the Universe. In this network, which is the direct result of structure fo…

astro-ph.CO2019★ 57 cited

Density and temperature of cosmic-web filaments on scales of tens of megaparsecs

H. Tanimura, N. Aghanim, V. Bonjean +2

We studied physical properties of matter in 24,544 filaments ranging from 30 to 100 Mpc in length, identified in the Sloan Digital Sky Survey (SDSS). We stacked the Comptonization…

astro-ph.CO2019★ 6 cited

Probing galaxy cluster and intra-cluster gas with luminous red galaxies

Yan Gong, Yin-Zhe Ma, Hideki Tanimura

We use the cross-correlation between the thermal Sunyaev-Zeldovich (tSZ) signal measured by the Planck satellite and the luminous red galaxy (LRG) samples provided by the SDSS DR7…

astro-ph.CO2019★ 30 cited

Probing hot gas around luminous red galaxies through the Sunyaev-Zel'dovich effect

Hideki Tanimura, Gary Hinshaw, Ian G. McCarthy +7

We construct the mean thermal Sunyaev-Zel'dovich (tSZ) Comptonization y profile around Luminous Red Galaxies (LRGs) in the redshift range 0.16 < z < 0.47 from the Sloan Digital Sky…

astro-ph.CO2018★ 42 cited

Detection of intercluster gas in superclusters using the thermal Sunyaev-Zel'dovich effect

H. Tanimura, N. Aghanim, M. Douspis +2

Using a thermal Sunyaev-Zel'dovich (tSZ) signal, we search for hot gas in superclusters identified using the Sloan Digital Sky Survey Data Release 7 (SDSS/DR7) galaxies. We stack a…

astro-ph.CO2017★ 20 cited

Multi-wavelength scaling relations in galaxy groups: a detailed comparison of GAMA and KiDS observations to BAHAMAS simulations

Arthur Jakobs, Massimo Viola, Ian McCarthy +18

We study the scaling relations between the baryonic content and total mass of groups of galaxies, as these systems provide a unique way to examine the role of non-gravitational pro…

astro-ph.CO2016★ 65 cited

Cross-correlating Planck tSZ with RCSLenS weak lensing: Implications for cosmology and AGN feedback

Alireza Hojjati, Tilman Tröster, Joachim Harnois-Déraps +11

We present measurements of the spatial mapping between (hot) baryons and the total matter in the Universe, via the cross-correlation between the thermal Sunyaev-Zeldovich (tSZ) map…

astro-ph.HE2009★ 12 cited

Search for VHE gamma rays from SS433/W50 with the CANGAROO-II telescope

Sei. Hayashi, F. Kajino, T. Naito +48

SS433, located at the center of the supernova remnant W50, is a close proximity binary system consisting of a compact star and a normal star. Jets of material are directed outwards…

astro-ph2006★ 38 cited

CANGAROO-III Observations of the supernova remnant RX J0852.04622

R. Enomoto, S. Watanabe, T. Tanimori et al

Sub-TeV gamma-ray emission from the North-West rim of the supernova remnant RX J0852.04622 was detected with the CANGAROO-II telescope and recently confirmed by the H.E.S.S. gro…

astro-ph2005★ 73 cited

Detection of Gamma-rays around 1TeV from RX J0852.0-4622 by CANGAROO-II

H. Katagiri, R. Enomoto, L. T. Ksenofontov +1

We have detected gamma-ray emission at the 6sigma level at energies greater than 500GeV from the supernova remnant RX J0852.0-4622 (G266.2-1.2) using the CANGAROO-II Imaging Atmosp…

astro-ph2004★ 184 cited

Detection of Sub-TeV Gamma-Rays from the Galactic Center Direction by CANGAROO-II

K. Tsuchiya, R. Enomoto, L. T. Ksenofontov +3

We have detected sub-TeV gamma-ray emission from the direction of the Galactic Center (GC) using the CANGAROO-II Imaging Atmospheric Cherenkov Telescope (IACT). We detected a stati…