activity
20092026
most citedThick gas discs in faint dwarf galaxies

398 citations · 1.9k across the 38 of their papers we have counts for

collaborators

37 papers

astro-ph.GA2026

From Atomic Gas to Star Formation

Erik Rosolowsky, Eric Koch, Sambit Roychowdhury +9

Since the 2015 SKA Chapters, the advent of panchromatic observations of nearby galaxies, capable of resolving the interstellar medium (ISM) into individual star-forming regions and…

astro-ph.GA2025★ 2 cited

Pearls on a string: Dark and bright galaxies on a strikingly straight and narrow filament

Maryam Arabsalmani, Sambit Roychowdhury, Benjamin Schneider +11

We identify a chain of galaxies along an almost straight line in the nearby Universe with a projected length of ~5 Mpc. The galaxies are distributed within projected distances of o…

astro-ph.GA2024★ 6 cited

The Smallest Scale of Hierarchy Survey (SSH) III. Dwarf-dwarf satellite merging phenomena in the low-mass regime

Elena Sacchi, Michele Bellazzini, Francesca Annibali +13

We present new deep, wide-field Large Binocular Telescope (LBT) and imaging data from the Smallest Scale of Hierarchy Survey (SSH) revealing previously undetected tidal fea…

astro-ph.GA2024

DEVILS/MIGHTEE/GAMA/DINGO: The Impact of SFR Timescales on the SFR-Radio Luminosity Correlation

Robin H. W. Cook, Luke J. M. Davies, Jonghwan Rhee +20

The tight relationship between infrared luminosity (L) and 1.4 GHz radio continuum luminosity (L) has proven useful for understanding star formatio…

astro-ph.GA2024

MIGHTEE-HI: HI galaxy properties in the large scale structure environment at z~0.37 from a stacking experiment

Francesco Sinigaglia, Giulia Rodighiero, Ed Elson +20

We present the first measurement of HI mass of star-forming galaxies in different large scale structure environments from a blind survey at . In particular, we carry ou…

astro-ph.CO2023★ 12 cited

Galaxy And Mass Assembly (GAMA): The group HI mass as a function of halo mass

Ajay Dev, Simon P. Driver, Martin Meyer +11

We determine the atomic hydrogen (HI) to halo mass relation (HIHM) using Arecibo Legacy Fast ALFA survey HI data at the location of optically selected groups from the Galaxy and Ma…

astro-ph.GA2022★ 33 cited

The resolved scaling relations in DustPedia: Zooming in on the local Universe

Viviana Casasola, Simone Bianchi, Laura Magrini +18

We perform a homogeneous analysis of an unprecedented set of spatially resolved scaling relations (SRs) between ISM components and other properties in the range of scales 0.3-3.4 k…

astro-ph.GA2022★ 30 cited

Deep Investigation of Neutral Gas Origins (DINGO): HI stacking experiments with early science data

Jonghwan Rhee, Martin Meyer, Attila Popping +19

We present early science results from Deep Investigation of Neutral Gas Origins (DINGO), an HI survey using the Australian Square Kilometre Array Pathfinder (ASKAP). Using ASKAP su…

astro-ph.GA2022★ 9 cited

Probing galaxy evolution through HI 21-cm emission and absorption: current status and prospects with the Square Kilometre Array

Rajeshwari Dutta, Sushma Kurapati, J. N. H. S. Aditya +8

One of the major science goals of the Square Kilometre Array (SKA) is to understand the role played by atomic hydrogen (HI) gas in the evolution of galaxies throughout cosmic time.…

astro-ph.GA2022★ 6 cited

Unusual gas structure in an otherwise normal spiral galaxy hosting GRB 171205A / SN 2017iuk

M. Arabsalmani, S. Roychowdhury, F. Renaud +4

We study the structure of atomic hydrogen (HI) in the host galaxy of GRB 171205A / SN 2017iuk at z=0.037 through HI 21cm emission line observations with the Karl G. Jansky Very Lar…

astro-ph.GA2022★ 20 cited

ALMA/ACA CO Survey of the IC 1459 and NGC 4636 Groups: Environmental Effects on the Molecular Gas of Group Galaxies

Bumhyun Lee, Jing Wang, Aeree Chung +30

We present new results of a 12CO(J=1-0) imaging survey using the Atacama Compact Array (ACA) for 31 HI detected galaxies in the IC 1459 and NGC 4636 groups. This is the first CO im…

astro-ph.GA2022★ 7 cited

The variation of the gas content of galaxy groups and pairs compared to isolated galaxies

Sambit Roychowdhury, Martin J. Meyer, Jonghwan Rhee +17

We measure how the atomic gas (HI) fraction () of groups and pairs taken as single units vary with average stellar mass ($\langle {\rm M_*} \rang…

astro-ph.GA2021★ 17 cited

WALLABY pre-pilot survey: Two dark clouds in the vicinity of NGC 1395

O. Ivy Wong, A. R. H. Stevens, B. -Q. For +34

We present the Australian Square Kilometre Array Pathfinder (ASKAP) WALLABY pre-pilot observations of two `dark' HI sources (with HI masses of a few times 10^8 Msol and no known st…

astro-ph.IM2021★ 32 cited

The BINGO Project II: Instrument Description

Carlos A. Wuensche, Thyrso Villela, Elcio Abdalla +41

The measurement of diffuse 21-cm radiation from the hyperfine transition of neutral hydrogen (HI signal) in different redshifts is an important tool for modern cosmology. However,…

astro-ph.CO2021★ 61 cited

The BINGO Project I: Baryon Acoustic Oscillations from Integrated Neutral Gas Observations

Elcio Abdalla, Elisa G. M. Ferreira, Ricardo G. Landim +43

Observations of the redshifted 21-cm line of neutral hydrogen (HI) are a new and powerful window of observation that offers us the possibility to map the spatial distribution of co…

astro-ph.GA2021★ 118 cited

A Nearby Galaxy Perspective on Dust Evolution. Scaling relations and constraints on the dust build-up in galaxies with the DustPedia and DGS samples

Frédéric Galliano, Angelos Nersesian, Simone Bianchi +14

Methods. We have modelled a sample of ~800 nearby galaxies, spanning a wide range of metallicity, gas fraction, specific star formation rate and Hubble stage. We have derived the d…

astro-ph.GA2020★ 7 cited

Local starburst conditions and formation of GRB 980425 / SN 1998bw within a collisional ring

M. Arabsalmani, F. Renaud, S. Roychowdhury +9

We present the first spatially resolved study of molecular gas in the vicinity of a Gamma Ray Burst, using CO(2-1) emission line observations with the Atacama Large Millimetre Arra…

astro-ph.CO2019★ 2 cited

A first quantification of the effects of absorption for HI Intensity Mapping experiments

Sambit Roychowdhury, Clive Dickinson, Ian W. A. Browne

HI Intensity Mapping (IM) will be used to do precision cosmology using many existing and upcoming radio observatories. The signal will be contaminated due to absorption, the larges…

astro-ph.GA2019★ 12 cited

A superluminous supernova in high surface density molecular gas within the bar of a metal-rich galaxy

M. Arabsalmani, S. Roychowdhury, F. Renaud +8

We report the Atacama Large Millimeter/submillimeter Array (ALMA) observations of the metal rich host galaxy of superluminous supernova (SLSN) PTF10tpz, a barred spiral galaxy at z…

astro-ph.GA2019★ 25 cited

The host galaxy of GRB 980425 / SN1998bw: a collisional ring galaxy

M. Arabsalmani, S. Roychowdhury, T. K. Starkenburg +8

We report Giant Metrewave Radio Telescope (GMRT) , Very Large Telescope (VLT) and Spitzer Space Telescope observations of ESO 184G82, the host galaxy of GRB 980425/SN 1998bw, th…

astro-ph.HE2019★ 24 cited

HI 21cm mapping of the host galaxy of AT2018cow: a fast-evolving luminous transient within a ring of high column density gas

Sambit Roychowdhury, Maryam Arabsalmani, Nissim Kanekar

We report Giant Metrewave Radio Telescope (GMRT) HI 21cm imaging of CGCG 137-068, the host galaxy of the fast-evolving luminous transient (FELT) AT2018cow. This is the first study…

astro-ph.GA2019★ 217 cited

A systematic metallicity study of DustPedia galaxies reveals evolution in the dust-to-metal ratios

P. De Vis, A. Jones, S. Viaene +17

Observations of evolution in the dust-to-metal ratio allow us to constrain the dominant dust processing mechanisms. In this work, we present a study of the dust-to-metal and dust-t…

astro-ph.CO2018★ 309 cited

Cosmology with Phase 1 of the Square Kilometre Array; Red Book 2018: Technical specifications and performance forecasts

Square Kilometre Array Cosmology Science Working Group, David J. Bacon, Richard A. Battye +44

We present a detailed overview of the cosmological surveys that will be carried out with Phase 1 of the Square Kilometre Array (SKA1), and the science that they will enable. We hig…

astro-ph.CO2017★ 51 cited

Impact of Simulated 1/f Noise for HI Intensity Mapping Experiments

Stuart Harper, Clive Dickinson, Richard Battye +5

Cosmology has entered an era where the experimental limitations are not due to instrumental sensitivity but instead due to inherent systematic uncertainties in the instrumentation…