The spin measurement of MAXI J1348-630 using the Insight-HXMT data
arXiv:2309.05232 · doi:10.1093/mnras/stad3166
Abstract
We report the results of fitting Insight-HXMT data to the black hole X-ray binary MAXI J1348-430, which was discovered on January 26th, 2019, with the Gas Slit Camera (GSC) on-board MAXI. Several observations at the beginning of the first burst were selected, with a total of 10 spectra. From the residuals of fits using disk plus power law models, X-ray reflection signatures were clearly visible in some of these observations. We use the state-of the-art relxill series reflection model to fit six spectra with distinct reflection signatures and a joint fit to these spectra. In particular, we focus on the results for the black hole spin values. Assuming Rin = RISCO, the spin parameter is constrained to be 0.82+0.04-0.03 with 90% confidence level (statistical only).
arXiv commentAccepted for publication in MNRAS
References in corpus (58)
- On the Absorption of X-rays in the Interstellar Medium
- X-ray Properties of Black-Hole Binaries
- The Nuclear Spectroscopic Telescope Array (NuSTAR) Mission
- Atomic Data for Astrophysics. II. New Analytic Fits for Photoionization Cross Sections of Atoms and Ions
- The MAXI Mission on the ISS: Science and Instruments for Monitoring All Sky X-Ray Images
- Broad-band gamma-ray and X-ray spectra of NGC 4151 and their implications for physical processes and geometry
- Improved Reflection Models of Black-Hole Accretion Disks: Treating the Angular Distribution of X-rays
- The May 1989 outburst of the Soft X-ray Transient GS 2023+338 (V404 Cyg)
- Broad iron lines in Active Galactic Nuclei
- Spectral Properties of Accretion Disks Around Galactic and Extragalactic Black Holes
- Black Hole Spin in X-Ray Binaries: Observational Consequences
- Correlations in the QPO Frequencies of Low Mass X-Ray Binaries and the Relativistic Precession Model
- The evolution of black hole states
- Relativistic X-ray Lines from the Inner Accretion Disks Around Black Holes
- Estimating the Spin of Stellar-Mass Black Holes via Spectral Fitting of the X-ray Continuum
- X-ray reflected spectra from accretion disk models. I. Constant density atmospheres
- Black Hole Spin via Continuum Fitting and the Role of Spin in Powering Transient Jets
- Overview to the Hard X-ray Modulation Telescope (Insight-HXMT) Satellite
- The Constant Inner-Disk Radius of LMC X-3: A Basis for Measuring Black Hole Spin
- Stellar-mass Black Hole Spin Constraints from Disk Reflection and Continuum Modeling
- The Spin of the Black Hole Microquasar XTE J1550-564 via the Continuum-Fitting and Fe-Line Methods
- The Medium Energy (ME) X-ray telescope onboard the Insight-HXMT astronomy satellite
- A Determination of the Spin of the Black Hole Primary in LMC X-1
- Confirmation Via the Continuum-Fitting Method that the Spin of the Black Hole in Cygnus X-1 is Extreme
- NuSTAR Spectroscopy of GRS 1915+105: Disk Reflection, Spin, and Connections to Jets
- Alternative explanations for extreme supersolar iron abundances inferred from the energy spectrum of Cygnus X-1
- NuSTAR and Suzaku observations of the hard state in Cygnus X-1: locating the inner accretion disk
- Testing Comptonization models using BeppoSAX observations of Seyfert 1 galaxies
- A Prominent Accretion Disk in the Low-Hard State of the Black Hole Candidate SWIFT J1753.5-0127
- NuSTAR and Swift observations of the very high state in GX 339-4: Weighing the black hole with X-rays
- The Disk Wind in the Rapidly Spinning Stellar-Mass Black Hole 4U 1630-472 Observed with NuSTAR
- A catalogue of high-mass X-ray binaries in the Galaxy: from the INTEGRAL to the Gaia era
- Self-Consistent Black Hole Accretion Spectral Models and the Forgotten Role of Coronal Comptonization of Reflection Emission
- Limits on spin determination from disc spectral fitting in GX 339-4
- The Low-Spin Black Hole in LMC X-3
- A Global Study of the Behaviour of Black Hole X-ray Binary Discs
- NICER observations reveal that the X-ray transient MAXI J1348-630 is a Black Hole X-ray binary
- Estimating the black hole spin for the X-ray binary MAXI J1820+070
- AstroSat view of GRS 1915+105 during the Soft State: Detection of HFQPOs and estimation of Mass and Spin
- Discovery of the black hole X-ray binary transient MAXIJ1348-630
- Measuring the distance to the black hole candidate X-ray binary MAXI J1348-630 using HI absorption
- Why is IGR J17091-3624 so faint? Constraints on distance, mass, and spin from `phase-resolved' spectroscopy of the `heartbeat' oscillations
- Detailed analysis on the reflection component for the black hole candidate MAXI J1348-630
- NuSTAR monitoring of MAXI J1348-630: evidence of high density disc reflection
- Stronger Reflection from Black Hole Accretion Disks in Soft X-ray States
- AstroSat and Chandra view of the high soft state of 4U 1630-47 (4U 1630-472): evidence of the disk wind and a rapidly spinning black hole
- The Galactic LMXB Population and the Galactic Centre Region
- Spectral Index as a Function of Mass Accretion Rate in Black Hole Sources. Monte-Carlo Simulations and an Analytical Description
- Power-law Tails from Dynamical Comptonization in Converging Flows
- The reflection component in the average and heartbeat spectra of the black-hole candidate IGR J17091-3642 during the 2016 outburst
- Peculiar disk behaviors of the black hole candidate MAXI J1348-630 in the hard state observed by Insight-HXMT and Swift
- AstroSat and MAXI view of Cygnus X-1: Signature of an `extreme' soft nature
- NuSTAR and Swift Observations of the Extragalactic Black Hole X-ray Binaries
- A detailed study on the reflection component for the Black Hole Candidate MAXI J1836-194
- MAXI~J1348--630: Estimating the black hole mass and binary inclination using a scaling technique
- A retrograde spin of the black hole in MAXI J1659--152
- Estimating the spin of the black hole candidate MAXI J1659-152 with the X-ray continuum-fitting method
- Broadband Spectral properties of MAXI J1348--630 using AstroSat Observations