activity
20082026
most citedHXMT Identification of a non-thermal X-ray burst from SGR J1935+2154 and with FRB 200428

274 citations · 1.4k across the 41 of their papers we have counts for

collaborators

43 papers

astro-ph.GA2026

Photometric redshifts for active galactic nuclei with LePHARE for the Vera C. Rubin Observatory

R. Shirley, M. Salvato, J. Cohen-Tanugi +31

Active Galactic Nuclei (AGN) play a crucial role in galaxy evolution, but they are a minority of extragalactic sources with diverse Spectral Energy Distributions (SEDs), which depe…

astro-ph.HE2026

Fast Radio Bursts in the Era of the Vera C. Rubin Observatory's Legacy Survey of Space and Time

C. W. James, B. Smith, K. Dage +12

Identifying the host galaxies of fast radio bursts (FRBs), and comparing their redshifts and dispersion measures, has unlocked a new probe of the cosmological distribution of ionis…

astro-ph.CO2025

Cosmic Shear constraints from HSC Year 3 with clustering calibration of the tomographic redshift distributions from DESI

J. Choppin de Janvry, B. Dai, S. Gontcho A Gontcho +2

We reanalyze cosmological constraints from Hyper Suprime-Cam (HSC) Y3 shear-shear correlation function using new calibration of the tomographic redshift distribution via the cluste…

astro-ph.CO2025

Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI

J. Choppin de Janvry, S. Gontcho A Gontcho, U. Seljak +53

The calibration of tomographic redshift distributions is essential for cosmological analysis of weak lensing data. In this work, we calibrate all four tomographic bins of the Hyper…

astro-ph.IM2025★ 1 cited

Photometric Redshift Estimation for Rubin Observatory Data Preview 1 with Redshift Assessment Infrastructure Layers (RAIL)

T. Zhang, E. Charles, J. F. Crenshaw +87

We present the first systematic analysis of photometric redshifts (photo-z) estimated from the Rubin Observatory Data Preview 1 (DP1) data taken with the Legacy Survey of Space and…

astro-ph.IM2025

Demonstrating the velocity response of a table-top EPR Speedmeter

S. L. Kranzhoff, S. L. Danilishin, S. Steinlechner +3

The sensitivity of gravitational-wave interferometers is fundamentally limited by quantum noise, as dictated by the Heisenberg uncertainty principle, due to their continuous positi…

astro-ph.CO2025

Lensing Without Borders: Measurements of galaxy-galaxy lensing and projected galaxy clustering in DESI DR1

S. Heydenreich, A. Leauthaud, C. Blake +64

We present Galaxy-Galaxy Lensing measurements obtained by cross-correlating spectroscopically observed galaxies from the first data release of the Dark Energy Spectroscopic Instrum…

astro-ph.CO2025★ 12 cited

OpenUniverse2024: A shared, simulated view of the sky for the next generation of cosmological surveys

OpenUniverse, The LSST Dark Energy Science Collaboration, The Roman HLIS Project Infrastructure Team +58

The OpenUniverse2024 simulation suite is a cross-collaboration effort to produce matched simulated imaging for multiple surveys as they would observe a common simulated sky. Both t…

astro-ph.IM2022★ 27 cited

A Joint Roman Space Telescope and Rubin Observatory Synthetic Wide-Field Imaging Survey

M. A. Troxel, C. Lin, A. Park +22

We present and validate 20 deg of overlapping synthetic imaging surveys representing the full depth of the Nancy Grace Roman Space Telescope High-Latitude Imaging Survey (HLIS)…

astro-ph.IM2022★ 26 cited

ETpathfinder: a cryogenic testbed for interferometric gravitational-wave detectors

A. Utina, A. Amato, J. Arends +112

The third-generation of gravitational wave observatories, such as the Einstein Telescope (ET) and Cosmic Explorer (CE), aim for an improvement in sensitivity of at least a factor o…

astro-ph.HE2022

SN 2020wnt: a slow-evolving carbon-rich superluminous supernova with no O II lines and a bumpy light curve

C. P. Gutiérrez, A. Pastorello, M. Bersten +29

We present the analysis of SN 2020wnt, an unusual hydrogen-poor super-luminous supernova (SLSN-I), at a redshift of 0.032. The light curves of SN 2020wnt are characterised by an ea…

astro-ph.HE2021★ 54 cited

Circumstellar Interaction Powers the Light Curves of Luminous Rapidly Evolving Optical Transients

C. Pellegrino, D. A. Howell, J. Vinkó +16

Rapidly evolving transients, or objects that rise and fade in brightness on timescales two to three times shorter than those of typical Type Ia or Type II supernovae (SNe), have un…

astro-ph.HE2021★ 10 cited

The optical properties of three type II supernovae: 2014cx, 2014cy and 2015cz

R. Dastidar, K. Misra, M. Singh +19

We present the photometric and spectroscopic analysis of three Type II SNe: 2014cx, 2014cy and 2015cz. SN 2014cx is a conventional Type IIP with a shallow slope (0.2 mag/50d) and a…

astro-ph.HE2020★ 14 cited

Insight-HXMT observations of Swift J0243.6+6124: the evolution of RMS pulse fractions at super-Eddington luminosity

P. J. Wang, L. D. Kong, S. Zhang +116

Based on Insight-HXMT data, we report on the pulse fraction evolution during the 2017-2018 outburst of the newly discovered first Galactic ultraluminous X-ray source (ULX) Swift J0…

astro-ph.HE2020★ 22 cited

Insight-HXMT firm detection of the highest energy fundamental cyclotron resonance scattering feature in the spectrum of GRO J1008-57

M. Y. Ge, L. Ji, S. N. Zhang +118

We report on the observation of the accreting pulsar GRO J1008-57 performed by Insight-HXMT at the peak of the source's 2017 outburst. Pulsations are detected with a spin period of…

astro-ph.HE2020★ 274 cited

HXMT Identification of a non-thermal X-ray burst from SGR J1935+2154 and with FRB 200428

C. K. Li, L. Lin, S. L. Xiong +117

Fast radio bursts (FRBs) are short pulses observed in radio band from cosmological distances. One class of models invoke soft gamma-ray repeaters (SGRs), or magnetars, as the sourc…

astro-ph.HE2020★ 3 cited

Insight-HXMT insight into switch of the accretion mode: the case of the X-ray pulsar 4U 1901+03

Y. L. Tuo, L. Ji, S. S. Tsygankov +116

We use the In data collected during the 2019 outburst from X-ray pulsar 4U 1901+03 to complement the orbital parameters reported by Fermi/GBM. Using the Insight-HXMT, we examine th…

astro-ph.HE2020★ 34 cited

The evolution of the broadband temporal features observed in the black-hole transient MAXI J1820+070 with Insight-HXMT

Yanan Wang, Long Ji, S. N. Zhang +117

We study the evolution of the temporal properties of MAXI 1820+070 during the 2018 outburst in its hard state from MJD 58190 to 58289 with Insight-HXMT in a broad energy band 1-150…

astro-ph.HE2020★ 19 cited

Discovery of delayed spin-up behavior following two large glitches in the Crab pulsar, and the statistics of such processes

M. Y. Ge, S. N. Zhang, F. J. Lu +130

Glitches correspond to sudden jumps of rotation frequency () and its derivative () of pulsars, the origin of which remains not well understood yet, partly because the jum…

astro-ph.HE2020★ 98 cited

GRANDMA Observations of Advanced LIGO's and Advanced Virgo's Third Observational Campaign

S. Antier, S. Agayeva, M. Almualla +55

GRANDMA is a network of 25 telescopes of different sizes, including both photometric and spectroscopic facilities. The network aims to coordinate follow-up observations of gravitat…

astro-ph.HE2020★ 30 cited

A search for prompt gamma-ray counterparts to fast radio bursts in the Insight-HXMT data

C. Guidorzi, M. Marongiu, R. Martone +118

No robust detection of prompt electromagnetic counterparts to fast radio bursts (FRBs) has yet been obtained, in spite of several multi-wavelength searches carried out so far. Spec…

astro-ph.HE2020★ 13 cited

Switches between accretion structures during flares in 4U 1901+03

L. Ji, L. Ducci, A. Santangelo +120

We report on our analysis of the 2019 outburst of the X-ray accreting pulsar 4U 1901+03 observed with Insight-HXMT and NICER. Both spectra and pulse profiles evolve significantly i…

astro-ph.HE2020

Joint Analysis of Energy and RMS Spectra from MAXI J1535-571 with Insight-HXMT

L. D. Kong, S. Zhang, Y. P. Chen +115

A new black hole X-ray binary (BHXRB) MAXI J1535-571 was discovered by MAXI during its outburst in 2017. Using observations taken by the first Chinese X-ray satellite, the Hard X-r…

astro-ph.HE2019

Diagnostic of the spectral properties of Aquila X-1 by Insight-HXMT snapshots during the early propeller phase

C. Güngör, M. Y. Ge, S. Zhang +108

We study the 2018 outburst of Aql X-1 via the monitor of all sky X-ray image (MAXI) data. We show that the outburst starting in February 2018 is a member of short-low class in the…