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20202026
most citedBlind HI and OH absorption line search: first results with MALS and uGMRT processed using ARTIP

33 citations · 37 across the 6 of their papers we have counts for

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astro-ph.GA2026

HI 21-cm absorption in low- and high-excitation radio-loud AGNs at from MALS

P. P. Deka, N. Gupta, J-. K. Krogager +5

We present results from a search of cold neutral gas associated with radio-loud active galactic nuclei (AGNs) at using HI 21-cm absorption measurements from the MeerKAT A…

astro-ph.GA2025

Origin of gas in the Magellanic Bridge: MeerKAT detection of HI 21-cm absorption

A. P. M. Morelli, J. Kerp, N. Gupta +6

HI 21-cm absorption lines are investigated to determine the origin of the neutral atomic hydrogen (HI) of the Magellanic Bridge (MB). Using the MeerKat Absorption Line Survey (MALS…

astro-ph.GA2025★ 4 cited

The MeerKAT Absorption Line Survey (MALS) data release 3: Cold atomic gas associated with the Milky Way

N. Gupta, J. Kerp, S. A. Balashev +15

We present results of a blind search for Galactic HI 21-cm absorption lines toward 19130 radio sources, using 390 pointings of MALS, each pointing centered on a source brighter tha…

astro-ph.GA2023

MALS discovery of a rare HI 21-cm absorber at : origin of the absorbing gas in powerful AGN

P. P. Deka, N. Gupta, H. W. Chen +14

We report a new, rare detection of HI 21-cm absorption associated with a quasar (only six known at ) here towards J2339-5523 at = 1.3531, discovered through the Mee…

astro-ph.GA2023

The MeerKAT Absorption Line Survey (MALS) data release I: Stokes I image catalogs at 1-1.4 GHz

P. P. Deka, N. Gupta, P. Jagannathan +24

The MeerKAT Absorption Line Survey (MALS) has observed 391 telescope pointings at L-band (900 - 1670 MHz) at . We present radio continuum images and a catalog of…

astro-ph.GA2020★ 33 cited

Blind HI and OH absorption line search: first results with MALS and uGMRT processed using ARTIP

N. Gupta, P. Jagannathan, R. Srianand +32

We present details of the Automated Radio Telescope Imaging Pipeline (ARTIP) and results of a sensitive blind search for HI and OH absorbers at and , respectively. A…