papers

Publications (13)

astro-ph.SR2024

J0526+5934: a peculiar ultra-short period double white dwarf

Alberto Rebassa-Mansergas, Mark Hollands, Steven G. Parsons +6

Ultra-short period compact binaries are important sources of gravitational waves, which include e.g. the progenitors of type Ia supernovae or the progenitors of merger episodes tha…

astro-ph.SR2022

Doubling of minute-long Quasi-Periodic Pulsations from super-flares on a low mass star

J. Gerry Doyle, Puji Irawati, Dmitrii Y. Kolotkov +5

Using the ULTRASPEC instrument mounted on the 2.4-m Thai National Telescope, we observed two large flares, each with a total energy close to 10^34 erg with sub-second cadence. A co…

astro-ph.SR2016

PTF1 J082340.04+081936.5: A hot subdwarf B star with a low mass white dwarf companion in an 87 minute orbit

Thomas Kupfer, Jan van Roestel, Jared Brooks +19

We present the discovery of the hot subdwarf B star (sdB) binary PTF1 J082340.04+081936.5. The system has an orbital period P min (0.060761584(10) days), ma…

astro-ph.SR2016

Hunting For Eclipses: High Speed Observations of Cataclysmic Variables

Liam K Hardy, Martin J McAllister, Vik S Dhillon +12

We present new time-resolved photometry of 74 cataclysmic variables (CVs), 47 of which are eclipsing. 13 of these eclipsing systems are newly discovered. For all 47 eclipsing syste…

astro-ph.GA2016

A multiwavelength investigation of the HII region S311: Young stellar population and star formation

Ram Kesh Yadav, A. K. Pandey, Saurabh Sharma +9

We present a multiwavelength investigation of the young stellar population and star formation activities around the \hii region Sharpless 311. Using our deep near-infrared observat…

astro-ph.HE2025

Further evidence for natal kick segregation by spectral type in high-mass X-ray binaries

Pornisara Nuchvanichakul, Poshak Gandhi, Christian Knigge +4

High-mass X-ray binaries (HMXBs) are systems in which a neutron star or black hole accretes material from a massive companion. HMXBs are expected to have experienced a supernova in…

astro-ph.SR2025

Characterisation of H spectra from EXO 051910+3737.7 X-rays binaries

Pornisara Nuchvanichakul, Puji Irawati, Pakakaew Rittipruk +4

We investigate the spectral characteristics of the Be/X-ray binary system, EXO 051910+3737.7, in which Be/X-ray systems are the largest sub-class of high-mass X-ray binaries. Spect…

astro-ph.IM2024

AstroInformatics: Recommendations for Global Cooperation

Ashish Mahabal, Pranav Sharma, Rana Adhikari +45

Policy Brief on "AstroInformatics, Recommendations for Global Collaboration", distilled from panel discussions during S20 Policy Webinar on Astroinformatics for Sustainable Develop…

astro-ph.SR2023

Post-outburst evolution of bonafide FUor V2493 Cyg: A Spectro-photometric monitoring

Arpan Ghosh, Saurabh Sharma, Joe P. Ninan +11

We present here the results of eight years of our near-simultaneous optical/near-infrared spectro-photometric monitoring of bonafide FUor candidate `V2493 Cyg' starting from 2013 S…

astro-ph.SR2020

An extremely hot white dwarf with a rapidly rotating K-type subgiant companion: UCAC2 46706450

Klaus Werner, Nicole Reindl, Lisa Löbling +5

UCAC2 46706450 is a late-type star with an ultraviolet (UV) excess. It was considered a candidate to establish a sample of FGK stars with white dwarf (WD) companions that can be us…

astro-ph.SR2019

Short period variable stars in young open cluster Stock 8

Sneh Lata, Anil. K. Pandey, Ram Kesh Yadav +5

We present time series photometry in the field of Stock 8 and identified 130 short period variable stars. Twenty eight main-sequence and 23 pre-main-sequence variables are found to…

astro-ph.IM2024

Workforce Development in Astronomy and Astroinformatics

Kartik Sheth, Kevin Govender, Vanessa McBride +8

Policy Brief on "Workforce Development in Astronomy and Astroinformatics", distilled from the corresponding panel that was part of the discussions during S20 Policy Webinar on Astr…

astro-ph.IM2020

Machine Learning for Transient Recognition in Difference Imaging With Minimum Sampling Effort

Yik-Lun Mong, Kendall Ackley, Duncan Galloway +45

The amount of observational data produced by time-domain astronomy is exponentially in-creasing. Human inspection alone is not an effective way to identify genuine transients fromt…