activity
20172026
most citedX-ray bolometric corrections for Compton-thick active galactic nuclei

38 citations · 49 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.EP2026

A Bayesian Search for Planet Engulfment Signatures in Solar Analogs

Zimo Cheng, Sharon Xuesong Wang, Fan Liu +11

We present a systematic Bayesian search for chemical fingerprints of planet engulfment in 113 solar twins and analogs with high-precision abundance measurements, 45 of which host k…

astro-ph.GA2026

The ASKAP-FLASH survey: A first look at the multiwavelength properties and redshift distribution of compact radio sources

W. Roster, E. M. Sadler, E. K. Mahony +15

We present the characterisation, including a photometric redshift (photo-) analysis, of the optical counterparts (CTPs) to over 45 000 bright ( 30 mJy) comp…

astro-ph.IM2025

High-impact Scientific Software in Astronomy and its creators

Johannes Buchner

In the last decades, scientific software has graduated from a hidden side-product to a first-class member of the astrophysics literature. We aim to quantify the activity and impact…

astro-ph.HE2025★ 1 cited

Spin Constraints on 4U 1630-47 via combined Continuum Fitting and Reflection methods: a comparative study using Frequentist and Bayesian statistics

Debtroy Das, Honghui Liu, Zuobin Zhang +5

We present a comprehensive Bayesian spectral analysis of the black hole X-ray binary 4U 1630-47 during its 2022 outburst, using simultaneous NICER and NuSTAR observations. Using th…

astro-ph.EP2025

Short-Period Small Planets with High Mutual Inclinations are more Common around Metal-Rich Stars

Xinyan Hua, Sharon Xuesong Wang, Dongsheng An +7

We present a correlation between the stellar metallicities and the mutual inclinations of multi-planet systems hosting short-period small planets (a/Rs<12, Rp<4Re). We analyzed 89…

astro-ph.HE2024

An Intermediate Mass Black Hole Hidden Behind Thick Obscuration

Peter G. Boorman, Daniel Stern, Roberto J. Assef +12

Recent models suggest approximately half of all accreting supermassive black holes (SMBHs; 10 M) are expected to undergo intense growth phase…

astro-ph.EP2024★ 7 cited

Relative Occurrence Rate Between Hot and Cold Jupiters as an Indicator to Probe Planet Migration

Tianjun Gan, Kangrou Guo, Beibei Liu +4

We propose a second-order statistic parameter , the relative occurrence rate between hot and cold Jupiters (), to probe the migratio…

astro-ph.EP2024★ 1 cited

A revisit of the Mass-Metallicity Trends in Transiting Exoplanets

Qinghui Sun, Sharon Xuesong Wang, Luis Welbanks +2

The two prevailing planet formation scenarios, core-accretion and disk instability, predict distinct planetary mass-metallicity relations. Yet, the detection of this trend remains…

astro-ph.IM2023★ 2 cited

First on-sky results of a FIOS prototype, a Fabry Perot Based Instrument for Oxygen Searches

Surangkhana Rukdee, Sagi Ben-Ami, Mercedes López-Morales +4

The upcoming Extremely Large Telescopes (ELTs) are expected to have the collecting area required to detect potential biosignature gases such as molecular oxygen, , in…

astro-ph.HE2017★ 38 cited

X-ray bolometric corrections for Compton-thick active galactic nuclei

M. Brightman, M. Baloković, D. R. Ballantyne +16

We present X-ray bolometric correction factors, (), for Compton-thick (CT) active galactic nuclei (AGN) with the aim of testing AGN torus models, prob…