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相关论文: Clustering properties of TGSS radio sources

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We study the angular clustering of point sources in The GMRT (Giant Meter Wave Telescope) Sky Survey (TGSS). The survey at 150 MHz with delta > -53.5 degrees has a sky coverage of 3.6 pi steradians, i.e., 90% of the whole sky. We created…

星系天体物理 · 物理学 2019-06-04 Sandeep Rana , J. S. Bagla

We explore the large to moderate scale anisotropy in distant radio sources using the TGSS ADR1 catalog. We use different measures, i.e. number counts, sky brightness and flux per source, for this study. In agreement with earlier results, we…

宇宙学与河外天体物理 · 物理学 2019-12-20 Prabhakar Tiwari , Shamik Ghosh , Pankaj Jain

We measure the angular correlation function of radio galaxies selected by the 843 MHz Sydney University Molonglo Sky Survey (SUMSS). We find that the characteristic imprint of large-scale structure is clearly detectable, and that the survey…

天体物理学 · 物理学 2009-11-10 Chris Blake , Tom Mauch , Elaine M. Sadler

The radio spectral index is a powerful probe for classifying cosmic radio sources and understanding the origin of the radio emission. Combining data at 147 MHz and 1.4 GHz from the TIFR GMRT Sky Survey (TGSS) and the NRAO VLA Sky Survey…

天体物理仪器与方法 · 物理学 2018-01-10 F. de Gasperin , H. T. Intema , D. A. Frail

We investigate the origin of the large clustering signal detected in the angular distribution of the radio sources in the TGSS catalog. To do so, we cross-correlate the angular position of the radio sources with the Cosmic Microwave…

宇宙学与河外天体物理 · 物理学 2023-03-08 Giulia Piccirilli , Marina Migliaccio , Enzo Branchini , Arianna Dolfi

I extract the radio spectral index, $\alpha$, from 541,195 common sources observed in the 150 MHz TIFR GMRT Sky Survey (TGSS) and the 1.4 GHz NRAO VLA Sky Survey (NVSS). This large common source catalogue covers about $80\%$ of the sky. The…

星系天体物理 · 物理学 2019-07-26 Prabhakar Tiwari

Covering $\sim$5600 deg$^2$ to rms sensitivities of $\sim$70$-$100 $\mu$Jy beam$^{-1}$, the LOFAR Two-metre Sky Survey Data Release 2 (LoTSS-DR2) provides the largest low-frequency ($\sim$150 MHz) radio catalogue to date, making it an…

This Rescaled Subset of the Alternative Data Release 1 to the Tata Institute of Fundamental Physics Giant Metrewave Radio Telescope Sky Survey (TGSS-RSADR1) modifies the initial data release of TGSS-ADR1 (Intema et al. 2017) to bring that…

天体物理仪器与方法 · 物理学 2017-05-04 Natasha Hurley-Walker

Studying the spatial distribution of extragalactic source populations is vital in understanding the matter distribution in the Universe. It also enables understanding the cosmological evolution of dark matter density fields and the…

宇宙学与河外天体物理 · 物理学 2022-10-12 Aishrila Mazumder , Arnab Chakraborty , Abhirup Datta

Investigations of the cluster environment of radio sources have not shown a correlation between radio power and degree of clustering. However, it has been demonstrated that extended X-ray luminosity and galaxy clustering do exhibit a…

天体物理学 · 物理学 2009-10-31 N. A. Miller , F. N. Owen , J. O. Burns , M. J. Ledlow , W. Voges

We quantify the angular clustering of radio galaxies in the NVSS and FIRST radio surveys using the two-point correlation function and the moments of counts-in-cells - both important points of comparison with theory. These investigations…

天体物理学 · 物理学 2009-11-07 Chris Blake , Jasper Wall

The knowledge of the origin and statistical properties of diffuse radio emission in galaxy clusters has appreciably improved thanks to the GMRT Radio Halo Survey, a project based on 610 MHz observations of clusters belonging to a…

宇宙学与河外天体物理 · 物理学 2011-02-10 Simona Giacintucci

Giant radio sources (GRSs) are the single largest astrophysical objects known in the universe that have grown to megaparsec scales ($\ge$ 0.7 Mpc). GRSs are much rarer compared with normal-sized radio galaxies. Still, the reason for the…

星系天体物理 · 物理学 2024-05-31 Netai Bhukta , Souvik Manik , Sabyasachi Pal , Sushanta K. Mondal

The angular power spectrum is a powerful statistic for analysing cosmological signals imprinted in the clustering of matter. However, current galaxy and quasar surveys cover limited portions of the sky, and are contaminated by systematics…

宇宙学与河外天体物理 · 物理学 2013-10-29 Boris Leistedt , Hiranya V. Peiris , Daniel J. Mortlock , Aurélien Benoit-Lévy , Andrew Pontzen

We detect a highly significant excess of X-ray (2RXS) and radio (NVSS, GMRT, VLSSr) catalog sources when stacked around MCXC galaxy clusters and groups, narrowly confined within $\lesssim100\mathrm{\,kpc}$ of the $\sim2.4 R_{500}$ virial…

高能天体物理现象 · 物理学 2024-12-09 Gideon Ilani , Kuan-Chou Hou , Uri Keshet

Measurements of the Galactic synchrotron emission is relevant for the 21-cm studies from the Epoch of Reionization. The study of the synchrotron emission is also useful to quantify the fluctuations in the magnetic field and the cosmic ray…

宇宙学与河外天体物理 · 物理学 2021-01-13 Samir Choudhuri , Abhik Ghosh , Nirupam Roy , Somnath Bharadwaj , Huib. T. Intema , Sk. Saiyad Ali

We present the first full release of a survey of the 150 MHz radio sky, observed with the Giant Metrewave Radio Telescope between April 2010 and March 2012 as part of the TGSS project. Aimed at producing a reliable compact source survey,…

宇宙学与河外天体物理 · 物理学 2017-02-08 H. T. Intema , P. Jagannathan , K. P. Mooley , D. A. Frail

This is the third paper in a series that reports on our investigation of the clustering properties of AGNs identified in the ROSAT All-Sky Survey (RASS) and Sloan Digital Sky Survey (SDSS). In this paper, we extend the redshift range to…

宇宙学与河外天体物理 · 物理学 2015-05-30 Mirko Krumpe , Takamitsu Miyaji , Alison L. Coil , Hector Aceves

We present predictions on the angular power spectrum of CMB fluctuations due to extragalactic point sources (EPS) by using a method for simulating realistic 2D distributions of clustered EPS. Both radio and far--IR selected source…

天体物理学 · 物理学 2009-11-10 J. González-Nuevo , L. Toffolatti , F. Argüeso

We present the results from a pilot study with the Karl G. Jansky Very Large Array (JVLA) to determine the radio morphologies of extended radio sources and the properties of their host-galaxies in 10 massive galaxy clusters at z~1, an epoch…

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