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19912026
most citedSciPy 1.0--Fundamental Algorithms for Scientific Computing in Python

40.2k citations

Showing 2022 · astro-ph.GAShow all

40 papers · 2 filters

astro-ph.GA2022★ 13 cited

A Polarimetric Study of 9 PG Quasars with the VLA

Janhavi Baghel, P. Kharb, Silpa S. +2

We present polarization images of 9 radio-loud (RL) quasars from the VLA B-array at 6 GHz. These quasars belong to the Palomar-Green (PG) "blazar" sample comprising 16 RL quasars a…

astro-ph.GA2022★ 27 cited

Atomic Gas Scaling Relations of Star-forming Galaxies at

Aditya Chowdhury, Nissim Kanekar, Jayaram Chengalur

We use the Giant Metrewave Radio Telescope (GMRT) Cold-HI AT (CAT) survey, a 510 hr HI 21cm emission survey of galaxies at , to report the first measur…

astro-ph.GA2022★ 16 cited

Ultraviolet imaging observations of three jellyfish galaxies: Star formation suppression in the centre and ongoing star formation in stripped tails

Koshy George, B. M. Poggianti, Neven Tomičić +13

Spiral galaxies undergo strong ram-pressure effects when they fall into the galaxy cluster potential. As a consequence, their gas is stripped to form extended tails within which st…

astro-ph.GA2022★ 45 cited

Stellar Escape from Globular Clusters. I. Escape Mechanisms and Properties at Ejection

Newlin C. Weatherford, Fulya Kıroğlu, Giacomo Fragione +3

The theory of stellar escape from globular clusters (GCs) dates back nearly a century, especially the gradual evaporation of GCs via two-body relaxation coupled with external tides…

astro-ph.GA2022★ 22 cited

The HI mass function of star-forming galaxies at

Apurba Bera, Nissim Kanekar, Jayaram N. Chengalur +1

The neutral atomic hydrogen (HI) mass function (HIMF) describes the distribution of the HI content of galaxies at any epoch; its evolution provides an important probe of models of…

astro-ph.GA2022★ 8 cited

Emission line star catalogues post-Gaia DR3: A validation of Gaia DR3 data using LAMOST OBA emission catalogue

B. Shridharan, Blesson Mathew, Suman Bhattacharyya +9

Gaia DR3 and further releases have the potential to identify and categorise new emission-line stars in the Galaxy. We perform a comprehensive validation of astrophysical parameters…

astro-ph.GA2022★ 29 cited

Extension of HOPS Out to 500 ParSecs (eHOPS). I. Identification and Modeling of Protostars in the Aquila Molecular Clouds

Riwaj Pokhrel, S. Thomas Megeath, Robert A. Gutermuth +14

We present a Spitzer/Herschel focused survey of the Aquila molecular clouds (~pc) as part of the eHOPS (extension of HOPS Out to 500 ParSecs) census of nearby protostar…

astro-ph.GA2022★ 31 cited

The need for obscured supermassive black hole growth to explain quasar proximity zones in the epoch of reionization

Sindhu Satyavolu, Girish Kulkarni, Laura C. Keating +1

Proximity zones of high-redshift quasars are unique probes of supermassive black hole formation, but simultaneously explaining proximity zone sizes and black hole masses has proved…

astro-ph.GA2022★ 3 cited

Fragmented atomic shell around S187 HII region and its interaction with molecular and ionized gas

Petr Zemlyanukha, Igor I. Zinchenko, Evgeny Dombek +6

The environment of S187, a nearby H II region (1.40.3 kpc), is analyzed. A surrounding shell has been studied in the H I line, molecular lines, and also in infrared and radio…

astro-ph.GA2022★ 25 cited

Atomic Gas Dominates the Baryonic Mass of Star-forming Galaxies at

Aditya Chowdhury, Nissim Kanekar, Jayaram N. Chengalur

We present a comparison between the average atomic gas mass, (including HI and He), the average molecular gas mass, , and the aver…

astro-ph.GA2022★ 1 cited

Investigating star-formation activity towards the southern HII region RCW 42

Vipin Kumar, S. Vig, V. S. Veena +4

The star-forming activity in the HII region RCW 42 is investigated using multiple wavebands, from near-infrared to radio wavelengths. Located at a distance of 5.8 kpc, this souther…

astro-ph.GA2022★ 18 cited

High-resolution, High-sensitivity, Low-frequency uGMRT View of Coma Cluster of Galaxies

D. V. Lal, N. Lyskova, C. Zhang +12

We present high-resolution, high-sensitivity upgraded Giant Metrewave Radio Telescope observations of the Coma cluster (A1656) at 250-500 MHz and 550-850 MHz. At 250-500 MHz, 135 s…

astro-ph.GA2022★ 7 cited

Revealing the dust grain polarization properties as a function of extinction and distance towards NGC 1893

N. Bijas, Chakali Eswaraiah, Jia-Wei Wang +5

Dust polarization observations at optical wavelengths help to understand the dust grain properties and trace the plane-of-the-sky component of the magnetic field. In this study, we…

astro-ph.GA2022★ 24 cited

The Giant Metrewave Radio Telescope Cold-HI AT Survey

Aditya Chowdhury, Nissim Kanekar, Jayaram N. Chengalur

We describe the design, data analysis, and basic results of the Giant Metrewave Radio Telescope Cold-HI AT (GMRT-CAT1) survey, a 510-hour upgraded GMRT HI 21 cm emis…

astro-ph.GA2022

Investigating the origin of X-ray jets: A case study of four hybrid morphology MOJAVE blazars

Biny Sebastian, Preeti Kharb, Matthew L. Lister +3

We have carried out Chandra, HST, and VLA observations of four MOJAVE blazars that have been previously classified as 'hybrid' (FR I/II) blazars in terms of radio morphology but no…

astro-ph.GA2022★ 8 cited

Jansky Very Large Array detections of CO(1-0) emission in HI-absorption-selected galaxies at

Balpreet Kaur, Nissim Kanekar, Marc Rafelski +3

We report a Karl G. Jansky Very Large Array search for redshifted CO(1-0) emission from three HI-absorption-selected galaxies at , identified earlier in their CO(3-2)…

astro-ph.GA2022★ 9 cited

A Massive, Dusty HI-Absorption-Selected Galaxy at Identified in a CO Emission Survey

Balpreet Kaur, Nissim Kanekar, Mitchell Revalski +4

We report a NOrthern Extended Millimeter Array (NOEMA) and Atacama Large Millimeter/submillimeter Array (ALMA) search for redshifted CO emission from the galaxies associated with s…

astro-ph.GA2022★ 13 cited

A Green Pea starburst arising from a galaxy-galaxy merger

S. Purkayastha, N. Kanekar, J. N. Chengalur +3

Green Pea galaxies are low-redshift starburst dwarf galaxies, with properties similar to those of the high-redshift galaxies that reionized the Universe. We report the first mappin…

astro-ph.GA2022★ 3 cited

Stellar populations of the globular cluster NGC 5053 investigated using AstroSat-Ultra Violet Imaging Telescope

K. J. Nikitha, S. Vig, S. K. Ghosh

Globular clusters being old and densely packed serve as ideal laboratories to test stellar evolution theories. Although there is enormous literature on globular clusters in optical…

astro-ph.GA2022★ 9 cited

A recent update of gas-phase chemical reactions and molecular lines in CLOUDY: its effects on millimeter and sub-millimeter molecular line predictions

Gargi Shaw, G. J. Ferland, M. Chatzikos

Here we present our current updates of the gas-phase chemical reaction rates and molecular lines in the spectral synthesis code CLOUDY, and its implications in spectroscopic modell…

astro-ph.GA2022★ 17 cited

A multiwavelength study of the W33 Main ultracompact HII region

Sarwar Khan, Jagadheep D. Pandian, Dharam V. Lal +7

The dynamics of ionized gas around the W33 Main ultracompact HII region is studied using observations of hydrogen radio recombination lines and a detailed multiwavelength character…

astro-ph.GA2022★ 5 cited

Host galaxy magnitude of OJ 287 from its colours at minimum light

Mauri J. Valtonen, Lankeswar Dey, S. Zola +54

OJ 287 is a BL Lacertae type quasar in which the active galactic nucleus (AGN) outshines the host galaxy by an order of magnitude. The only exception to this may be at minimum ligh…

astro-ph.GA2022★ 1 cited

Detecting PAHs in high-z galaxies in proxy: Modelling physical conditions in an extremely strong damped Lyman-alpha absorber towards QSO SDSS J1143+1420 at z=2.323

Gargi Shaw, A. Ranjan

We explore indirect methods to detect Polycyclic Aromatic Hydrocarbons (PAHs) in gas-rich, absorption-selected galaxies at high redshift. We look at the optical VLT/X-shooter obser…

astro-ph.GA2022★ 13 cited

Insufficient Gas Accretion Caused the Decline in Cosmic Star-Formation Activity 8 Billion Years Ago

Aditya Chowdhury, Nissim Kanekar, Jayaram N. Chengalur

Measurements of the atomic hydrogen (HI) properties of high-redshift galaxies are critical to understanding the decline in the star-formation rate (SFR) density of the Universe aft…