papers

Publications (31)

astro-ph.SR2020

ALMA Survey of Orion Planck Galactic Cold Clumps (ALMASOP): I. Detection of New Hot Corinos with ACA

Shih-Ying Hsu, Sheng-Yuan Liu, Tie Liu +29

We report the detection of four new hot corino sources, G211.47-19.27S, G208.68-19.20N1, G210.49-19.79W and G192.12-11.10 from a survey study of Planck Galactic Cold Clumps in the…

astro-ph.GA2018

A holistic perspective on the dynamics of G035.39-00.33: the interplay between gas and magnetic fields

Tie Liu, Pak Shing Li, Mika Juvela +54

Magnetic field is one of the key agents that play a crucial role in shaping molecular clouds and regulating star formation, yet the complete information on the magnetic field is no…

astro-ph.GA2019

Cloud G074.11+00.11: a stellar cluster in formation

Mika Saajasto, Jorma Harju, Mika Juvela +9

We present molecular line and dust continuum observations of a Planck-detected cold cloud, G074.11+00.11. The cloud consists of a system of curved filaments and a central star-form…

astro-ph.GA2017

The TOP-SCOPE survey of Planck Galactic Cold Clumps: Survey overview and results of an exemplar source, PGCC G26.53+0.17

Tie Liu, Kee-Tae Kim, Mika Juvela +11

The low dust temperatures (<14 K) of Planck Galactic Cold Clumps (PGCCs) make them ideal targets to probe the initial conditions and very early phase of star formation. TOP-SCOPE i…

astro-ph.SR2013

Protoplanetary Disk Masses from Stars to Brown Dwarfs

Subhanjoy Mohanty, Jane Greaves, Daniel Mortlock +6

We present SCUBA-2 850um observations for 7 very low mass stars (VLMS) and brown dwarfs (BDs): 3 in Taurus, 4 in the TWA, and all classical T Tauri (cTT) analogs. We detect 2 of th…

astro-ph.GA2012

H2D+ in the high mass star-forming Region Cygnus-X

Thushara Pillai, Paola Caselli, Jens Kauffmann +3

H2D+ is a primary ion which dominates the gas-phase chemistry of cold dense gas. Therefore it is hailed as a unique tool in probing the earliest, prestellar phase of star formation…

astro-ph.IM2024

AtLAST Science Overview Report

Mark Booth, Pamela Klaassen, Claudia Cicone +81

Submillimeter and millimeter wavelengths provide a unique view of the Universe, from the gas and dust that fills and surrounds galaxies to the chromosphere of our own Sun. Current…

astro-ph.CO2012

The Infrared Properties of Sources Matched in the WISE all-sky and Herschel-ATLAS Surveys

Nicholas A. Bond, Dominic J. Benford, Jonathan P. Gardner +34

We describe the infrared properties of sources detected over ~36 deg^2 of sky in the GAMA 15-hr equatorial field, using data from both the Herschel Astrophysical Terahertz Large-Ar…

astro-ph.GA2011

The G305 star-forming complex: the central star clusters Danks 1 and Danks 2

Ben Davies, J. S. Clark, Christine Trombley +7

The G305 HII complex (G305.4+0.1) is one of the most massive star forming structures yet identified within the Galaxy. It is host to many massive stars at all stages of formation a…

q-bio.GN2014

Structuring research methods and data with the Research Object model: genomics workflows as a case study

Kristina M. Hettne, Harish Dharuri, Jun Zhao +16

One of the main challenges for biomedical research lies in the computer-assisted integrative study of large and increasingly complex combinations of data in order to understand mol…

astro-ph.GA2016

Astrochemical Properties of Planck Cold Clumps

Ken'ichi Tatematsu, Tie Liu, Satoshi Ohashi +25

We observed thirteen Planck cold clumps with the James Clerk Maxwell Telescope/SCUBA-2 and with the Nobeyama 45 m radio telescope. The NH distribution obtained with the Nob…

astro-ph.GA2018

Planck Cold Clumps in the Orionis complex. II. Environmental effects on core formation

Hee-Weon Yi, Jeong-Eun Lee, Tie Liu +27

Based on the 850 m dust continuum data from SCUBA-2 at James Clerk Maxwell Telescope (JCMT), we compare overall properties of Planck Galactic Cold Clumps (PGCCs) in the Or…

astro-ph.GA2026

Determination of kinematic distances of WISE & SMGPS H II regions in the Galactic plane using SEDIGISM cloud association

Moses Langa, Mark Thompson, Andrew Rigby +7

The paper presents a method to assign kinematic distances to H II regions by associating them with molecular clouds from the SEDIGISM 13CO survey, producing a catalog of distances…

#h ii regions#kinematic distance#molecular clouds#galactic structure
cs.CV2025

LCS: An AI-based Low-Complexity Scaler for Power-Efficient Super-Resolution of Game Content

Simon Pochinda, Momen K. Tageldeen, Mark Thompson +5

The increasing complexity of content rendering in modern games has led to a problematic growth in the workload of the GPU. In this paper, we propose an AI-based low-complexity scal…

astro-ph.GA2018

Massive outflows associated with ATLASGAL clumps

Aiyuan Yang, Mark Thompson, James Urquhart +1

We have undertaken the largest survey for outflows within the Galactic Plane using simultaneously observed 13CO and C18O data. 325 out of a total of 919 ATLASGAL clumps have data s…

astro-ph.GA2014

The ionised, radical and molecular Milky Way: spectroscopic surveys with the SKA

Mark Thompson, Henrik Beuther, Clive Dickinson +6

The bandwith, sensitivity and sheer survey speed of the SKA offers unique potential for deep spectroscopic surveys of the Milky Way. Within the frequency bands available to the SKA…

astro-ph.SR2014

The impact of the SKA on Galactic Radioastronomy: continuum observations

Grazia Umana, Corrado Trigilio, Luciano Cerrigone +11

The SKA will be a state of the art radiotelescope optimized for both large area surveys as well as for deep pointed observations. In this paper we analyze the impact that the SKA w…

astro-ph.GA2013

The G305 star-forming complex: radio continuum and molecular line observations

Luke Hindson, Mark Thompson, James Urquhart +4

We present 109-115 GHz (3 mm) wide-field spectral line observations of 12^CO, 13^CO and C^18O J=1-0 molecular emission and 5.5 and 8.8 GHz (6 and 3 cm) radio continuum emission tow…

cs.HC2020

Cyber-Human System for Remote Collaborators

Srikanth Jonnada, Ram Dantu, Ishan Ranasinghe +3

With the increasing ubiquity of technology in our daily lives, the complexity of our environment and the mechanisms required to function have also increased exponentially. Failure…

astro-ph.GA2017

Herschel and SCUBA-2 observations of dust emission in a sample of Planck cold clumps

Mika Juvela, Jinhua He, Katherine Pattle +26

Analysis of all-sky Planck submillimetre observations and the IRAS 100um data has led to the detection of a population of Galactic cold clumps. The clumps can be used to study star…

astro-ph.CO2010

A Pilot Study for the SCUBA-2 'All-Sky' Survey

Todd Mackenzie, Filiberto G. Braglia, Andy G. Gibb +30

We have carried out a pilot study for the SCUBA-2 'All-Sky' Survey, SASSy, a wide and shallow mapping project at 850 microns, designed to find rare objects, both Galactic and extra…

astro-ph.IM2012

Future Science Prospects for AMI

Keith Grainge, Paul Alexander, Richard Battye +72

The Arcminute Microkelvin Imager (AMI) is a telescope specifically designed for high sensitivity measurements of low-surface-brightness features at cm-wavelength and has unique, im…

astro-ph.GA2017

The SCUBA-2 Ambitious Sky Survey: a catalogue of beam-sized sources in the Galactic longitude range 120 to 140

Will Nettke, Douglas Scott, Andy Gibb +13

The SCUBA-2 Ambitious Sky Survey (SASSy) is composed of shallow 850-$\umu$m imaging using the Sub-millimetre Common-User Bolometer Array 2 (SCUBA-2) on the James Clerk Maxwell Tele…

astro-ph.GA2020

A population of hypercompact HII regions identified from young HII regions

Aiyuan Yang, James Urquhart, Mark Thompson +8

Context. The derived physical parameters for young HII regions are normally determined assuming the emission region to be optically thin. However, this assumption is unlikely to ho…

astro-ph.GA2019

Galactic continuum surveys with the new 850 micron MKID camera at the EAO/JCMT 15-m telescope

Tie Liu, Di Li, David Eden +24

This white paper gives a brief summary of Galactic continuum surveys with the next generation 850 micron camera at the James Clerk Maxwell Telescope (JCMT) in the next decade. This…

math.AP2014

Existence theory for a Poisson-Nernst-Planck model of electrophoresis

Luciano Bedin, Mark Thompson

A system modeling the electrophoretic motion of a charged rigid macromolecule immersed in a incompressible ionized fluid is considered. The ionic concentration is governing by the…

cs.CV2025

Improved Allergy Wheal Detection for the Skin Prick Automated Test Device

Rembert Daems, Sven Seys, Valérie Hox +21

Background: The skin prick test (SPT) is the gold standard for diagnosing sensitization to inhalant allergies. The Skin Prick Automated Test (SPAT) device was designed for increase…

astro-ph.GA2015

Planck cold clumps in the Orionis complex: I. Discovery of an extremely young Class 0 protostellar object and a proto-brown dwarf candidate in a bright rimmed clump PGCC G192.32-11.88

Tie Liu, Qizhou Zhang, Kee-Tae Kim +37

We are performing a series of observations with ground-based telescopes toward Planck Galactic cold clumps (PGCCs) in the Orionis complex in order to systematically investigat…

astro-ph.CO2010

The Herschel-SPIRE Legacy Survey (HSLS): the scientific goals of a shallow and wide submillimeter imaging survey with SPIRE

Asantha Cooray, Steve Eales, Scott Chapman +247

A large sub-mm survey with Herschel will enable many exciting science opportunities, especially in an era of wide-field optical and radio surveys and high resolution cosmic microwa…

cs.DL2014

Aca 2.0: Questions and Answers

Raphael Poss, Sebastian Altmeyer, Mark Thompson +1

"Academia 2.0" is a proposal to organize scientific publishing around true peer-to-peer distributed dissemination channels and eliminate the traditional role of the academic publis…

astro-ph.SR2014

Tomography of Galactic star-forming regions and spiral arms with the Square Kilometer Array

Laurent Loinard, Mark Thompson, Melvin Hoare +12

Very Long Baseline Interferometry (VLBI) at radio wavelengths can provide astrometry accurate to 10 micro-arcseconds or better (i.e. better than the target GAIA accuracy) without b…