output
20092026
most citedJADES. The diverse population of infant Black Holes at 4<z<11: merging, tiny, poor, but mighty

361 citations

Showing 2019Show all

33 papers · 1 filter

astro-ph.SR2019★ 14 cited

VLBI observations of the G25.65+1.05 water maser superburst

R. A. Burns, G. Orosz, O. Bayandina +23

This paper reports observations of a 22 GHz water maser `superburst' in the G25.65+1.05 massive star forming region, conducted in response to an alert from the Maser Monitoring Org…

astro-ph.EP2019★ 32 cited

Kojima-1Lb Is a Mildly Cold Neptune around the Brightest Microlensing Host Star

A. Fukui, D. Suzuki, N. Koshimoto +56

We report the analysis of additional multiband photometry and spectroscopy and new adaptive optics (AO) imaging of the nearby planetary microlensing event TCP J05074264+2447555 (Ko…

astro-ph.CO2019★ 24 cited

Weak Lensing Analysis of CODEX Clusters using Dark Energy Camera Legacy Survey : Mass-Richness Relation

Anirut Phriksee, Eric Jullo, Marceau Limousin +5

We present the weak lensing analysis of 279 CODEX clusters using imaging data from 4200 of the DECam Legacy Survey (DECaLS) Data Release 3. The cluster sample resu…

astro-ph.SR2019★ 19 cited

Near-infrared Monitoring of the Accretion Outburst in the MYSO S255-NIRS3

Mizuho Uchiyama, Takuya Yamashita, Koichiro Sugiyama +10

We followed-up the massive young stellar object (MYSO) S255-NIRS3 (=S255-IRS1b) during its recent accretion outburst event in the Ks band with Kanata/HONIR for four years after its…

astro-ph.SR2019★ 125 cited

The first view of Scuti and Doradus stars with the TESS mission

V. Antoci, M. S. Cunha, D. M. Bowman +63

We present the first asteroseismic results for Scuti and Doradus stars observed in Sectors 1 and 2 of the TESS mission. We utilise the 2-min cadence TESS data for a sample…

astro-ph.GA2019★ 31 cited

Evolution of the Stellar Mass-Metallicity Relation. II. Constraints on Galactic Outflows from the Mg Abundances of Quiescent Galaxies

Nicha Leethochawalit, Evan N. Kirby, Richard S. Ellis +2

We present the stellar mass-[Fe/H] and mass-[Mg/H] relation of quiescent galaxies in two galaxy clusters at and . We derive the age, [Fe/H], and [Mg/Fe] for…

astro-ph.GA2019★ 97 cited

Molecular clouds in the Cosmic Snake normal star-forming galaxy 8 billion years ago

Miroslava Dessauges-Zavadsky, Johan Richard, Françoise Combes +12

The cold molecular gas in contemporary galaxies is structured in discrete cloud complexes. These giant molecular clouds (GMCs), with - solar masses and radii of 5-100 p…

astro-ph.SR2019★ 31 cited

The W-subtype active contact binary PZ UMa with a possible more massive tertiary component

X. Zhou, B. Soonthornthum

Two sets of multiple-color () light curves of PZ UMa were observed in dependently with the 2.4 meter telescope at the Thai National Observatory and the 1 meter tele…

astro-ph.SR2019★ 12 cited

V752 Cen -- A triple-lined spectroscopic contact binary with sudden and continuous period changes

X. Zhou, B. Soonthornthum, S. -B. Qian +2

V752 Cen is a triple-lined spectroscopic contact binary. Its multi-color light curves were obtained in the years 1971 and 2018, independently. Photometric analyses reveal that the…

astro-ph.EP2019★ 37 cited

Optimizing exoplanet atmosphere retrieval using unsupervised machine-learning classification

Joshua J. C. Hayes, E. Kerins, S. Awiphan +6

One of the principal bottlenecks to atmosphere characterisation in the era of all-sky surveys is the availability of fast, autonomous and robust atmospheric retrieval methods. We p…

astro-ph.SR2019★ 59 cited

Discovery of tidally-perturbed pulsations in the eclipsing binary U Gru: a pioneering system for tidal asteroseismology

Dominic M. Bowman, Cole Johnston, Andrew Tkachenko +3

The interior physics of stars is currently not well constrained for early-type stars. This is particularly pertinent for multiple systems as binary interaction becomes more prevale…

astro-ph.GA2019★ 15 cited

MOS spectroscopy of protocluster candidate galaxies at z=6.5

Rosa Calvi, José Miguel Rodríguez Espinosa, José Miguel Mas-Hesse +7

The epoch corresponding to a redshift of z is close to full re-ionisation of the Universe, and early enough to provide an intriguing environment to observe the early sta…

astro-ph.SR2019★ 14 cited

Photometric investigation on the W-subtype contact binary V1197 Her

Xiao Zhou, Boonrucksar Soonthornthum

Multi-color light curves of V1197 Her were obtained with the 2.4 meter optical telescope at Thai National Observatory and the Wilson-Devinney (W-D) program is used to model the obs…

astro-ph.SR2019★ 14 cited

HD 965: An extremely peculiar A star with an extremely long rotation period

G. Mathys, I. I. Romanyuk, S. Hubrig +4

Context. One of the keys to understanding the origin of the Ap stars and their significance in the general context of stellar astrophysics is the consideration of the most extreme…

astro-ph.HE2019★ 8 cited

Signature of stochastic acceleration and cooling processes in an outburst phase of the TeV blazar ON 231

Nibedita Kalita, Utane Sawangwit, Alok C. Gupta +1

We present a detailed spectral and temporal study of the intermediate-type blazar ON 231 during the TeV outburst phase in 2008 June with observations performed by Swift and XMM-New…

astro-ph.SR2019★ 61 cited

Sub-arcsecond (sub)millimeter imaging of the massive protocluster G358.93-0.03: Discovery of 14 new methanol maser lines associated with a hot core

C. L. Brogan, T. R. Hunter, A. P. M. Towner +25

We present (sub)millimeter imaging at 0.5'' resolution of the massive star-forming region G358.93-0.03 acquired in multiple epochs at 2 and 3 months following the recent flaring of…

astro-ph.SR2019★ 9 cited

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.HE2019★ 21 cited

Diagnostics of timing noise in middle aged pulsars

Nakornping Namkham, Phrudth Jaroenjittichai, Simon Johnston

Radio pulsars are often used as clocks in a wide variety of experiments. Imperfections in the clock, known as timing noise, have the potential to reduce the significance of, or eve…

astro-ph.GA2019★ 49 cited

No signs of star formation being regulated in the most luminous quasars at z~2 with ALMA

A. Schulze, J. D. Silverman, E. Daddi +7

We present ALMA Band~7 observations at m of 20 luminous ( [erg s]) unobscured quasars at . We detect continuum emission for 19/20 quas…

astro-ph.EP2019★ 23 cited

KELT-24b: A 5M Planet on a 5.6 day Well-Aligned Orbit around the Young V=8.3 F-star HD 93148

Joseph E. Rodriguez, Jason D. Eastman, George Zhou +76

We present the discovery of KELT-24 b, a massive hot Jupiter orbiting a bright (V=8.3 mag, K=7.2 mag) young F-star with a period of 5.6 days. The host star, KELT-24 (HD 93148), has…

astro-ph.GA2019★ 10 cited

AGN in Dusty Starbursts at Z=2: Feedback Still To Kick In

G. Rodighiero, A. Enia, I. Delvecchio +18

We investigate a sample of 152 dusty sources at 1:5 < z < 2:5 to understand the connection of enhanced Star-Formation-Rate (SFR) and Black-Hole-Accretion-Rate (BHAR). The sources a…

astro-ph.HE2019★ 30 cited

X-ray time lags in AGN: inverse-Compton scattering and spherical corona model

P. Chainakun, A. Watcharangkool, A. J. Young +1

We develop a physically motivated, spherical corona model to investigate the frequency-dependent time lags in AGN. The model includes the effects of Compton up-scattering between t…

hep-ph2019★ 8 cited

Inverse Seesaw and Portal Dark Matter

Chakrit Pongkitivanichkul, Nakorn Thongyoi, Patipan Uttayarat

We study the phenomenology of the inverse seesaw mechanism in the scalar-Higgs portal dark matter model. The model is an extension of the Standard Model including two additional ne…

astro-ph.EP2019★ 45 cited

Extreme Debris Disk Variability -- Exploring the Diverse Outcomes of Large Asteroid Impacts During the Era of Terrestrial Planet Formation

Kate Y. L. Su, Alan P. Jackson, Andras Gaspar +14

The most dramatic phases of terrestrial planet formation are thought to be oligarchic and chaotic growth, on timescales of up to 100-200 Myr, when violent impacts occur between lar…