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Detailed study of ELAIS N1 field with the uGMRT -- II. Source Properties and Spectral Variation Of Foreground Power Spectrum from 300-500 MHz Observations

, , , , , , , , , , and . (2019)cite arxiv:1908.10380Comment: There are 14 figures. The revised draft after getting the first favourable comments and resubmitted for publication in MNRAS.

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Scalability model for the LOFAR direction independent pipeline., , , , , and . Astron. Comput., (2019)Fast and Reproducible LOFAR Workflows with AGLOW., , , , , and . eScience, page 136-144. IEEE Computer Society, (2018)Detailed study of ELAIS N1 field with the uGMRT -- II. Source Properties and Spectral Variation Of Foreground Power Spectrum from 300-500 MHz Observations, , , , , , , , , and 1 other author(s). (2019)cite arxiv:1908.10380Comment: There are 14 figures. The revised draft after getting the first favourable comments and resubmitted for publication in MNRAS.Detailed study of the ELAIS N1 field with the uGMRT - I. Characterizing the 325 MHz foreground for redshifted 21 cm observations, , , , , , , , , and 1 other author(s). (2019)cite arxiv:1906.01655Comment: 13 pages, 5figures, 4 tables; accepted for publication in MNRAS.323 MHz GMRT Observations of Radio-loud Quasars at z>5, , , , , , , and . (2020)cite arxiv:2006.13762Comment: 13 pages; Accepted by A&A.Unexpected Circular Radio Objects at High Galactic Latitude, , , , , , , , , and 19 other author(s). (2020)cite arxiv:2006.14805Comment: Accepted for publication by PASA.Calibration of ultraviolet, mid-infrared and radio star formation rate indicators, , , , , , , , , and 5 other author(s). (2017)cite arxiv:1709.00183Comment: Accepted for publication in the Astrophysical Journal; 39 pages, 14 figures and 4 tables.