J/MNRAS/493/L81          Radio astrometry of MAXI J1820+070        (Atri+, 2020)

A radio parallax to the black hole X-ray binary MAXI J1820+070. Atri P., Miller-Jones J.C.A., Bahramian A., Plotkin R.M., Deller A.T., Jonker P.G., Maccarone T.J., Sivakoff G.R., Soria R., Altamirano D., Belloni T., Fender R., Koerding E., Maitra D., Markoff S., Migliari S., Russell D., Russell T., Sarazin C.L., Tetarenko A.J., Tudose V. <Mon. Not. R. Astron. Soc., 493, L81 (2020)> =2020MNRAS.493L..81A 2020MNRAS.493L..81A (SIMBAD/NED BibCode)
ADC_Keywords: Binaries, X-ray ; Positional data ; Parallaxes, spectroscopic Keywords: astrometry - parallaxes - stars: black holes - radio continuum: transients - X-rays: binaries - high angular resolution Abstract: Using the Very Long Baseline Array and the European Very Long Baseline Interferometry Network, we have made a precise measurement of the radio parallax of the black hole X-ray binary MAXI J1820+070, providing a model-independent distance to the source. Our parallax measurement of (0.348±0.033) mas for MAXI J1820+070 translates to a distance of (2.96±0.33)kpc. This distance implies that the source reached (15±3) per cent of the Eddington luminosity at the peak of its outburst. Further, we use this distance to refine previous estimates of the jet inclination angle, jet velocity, and the mass of the black hole in MAXI J1820+070 to be (63±3)°, (0.89±0.09)c, and (9.2±1.3)M, respectively Description: We monitored MAXI-J1820 (see Table 1) with the Very Long Baseline Array (VLBA), using both the Jet Acceleration and Collimation Probe of Transient X-ray Binaries (JACPOT-XRB) programme, proposal code BM467), and a long-running astrometry programme (proposal code BA130), supplemented with a targeted European VLBI Network (EVN) campaign (proposal code EA062). All observations used a combination of J1821+0549 (J1821 hereon) and J1813+065 (J1813 hereon) as the phase reference and astrometric check sources. The calibrator positions were taken from the Radio Fundamental catalogue (rfc2015a1). Our assumed positions (J2000) were RA = 18:21:27.305837, Dec = 05:49:10.65156 for J1821, and RA = 18:13:33.411619, Dec = 06:15:42.03366 for MAXI J1813. We imaged the calibrated data and determined the target position by fitting a point source in the image plane for every epoch. Objects: ------------------------------------------------------------------------ RA (2000) DE Designation(s) ------------------------------------------------------------------------ 18 20 21.9384568 +07 11 07.001649624 MAXI-J1820+070 = MAXI J1820+070 ------------------------------------------------------------------------ File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 116 11 Summary of the observations of MAXI-J1820+070. table2.dat 118 1 Astrometric details of the black hole X-ray binary MAXI J1820+070 -------------------------------------------------------------------------------- Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 A6 --- Code Project code 9- 16 F8.2 d MJD Date 19- 22 A4 --- Array Array 24- 25 I2 GHz Freq [5/15] Frequency (1) 28- 39 A12 --- Cal Phase calibrator 42- 53 A12 --- Check Check source 55- 56 I2 h RAh Right ascension (J2000) 58- 59 I2 min RAm Right ascension (J2000) 61- 70 F10.7 s RAs Right ascension (J2000) 72- 80 F9.7 s e_RAs rms uncertainty on RA 82- 83 I2 deg DEd Declination (J2000) 85- 86 I2 arcmin DEm Declination (J2000) 88- 96 F9.6 arcsec DEs Declination (J2000) 98-105 F8.6 arcsec e_DEs rms uncertainty on DE 107-111 F5.2 mJy/beam Ipeak Peak intensity in Freq 113-116 F4.2 mJy/beam e_Ipeak Peak intensity in Freq error -------------------------------------------------------------------------------- Note (1): The observing bandwidth was 32MHz for both the VLBA and the EVN. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 14 A14 --- Name Name 16- 17 I2 h RAh Right ascension (J2000) 19- 20 I2 min RAm Right ascension (J2000) 22- 31 F10.7 s RAs Right ascension (J2000) 33- 41 F9.7 s e_RAs Error on RA 43- 44 I2 deg DEd Declination (J2000) 46- 47 I2 arcmin DEm Declination (J2000) 49- 60 F12.9 arcsec DEs Declination (J2000) 62- 71 F10.8 arcsec e_DEs Error on DE (J2000) 72- 77 F6.3 mas/yr pmRA Proper motion along RA 79- 83 F5.3 mas/yr e_pmRA Proper motion along RA error 85- 90 F6.3 mas/yr pmDE Proper motion along DE 92- 96 F5.3 mas/yr e_pmDE Proper motion alond DE error 98-102 F5.3 mas plx Radio_parallax 104-108 F5.3 mas e_plx Error in the radio parallax 110-113 F4.2 kpc Dist Distance of the target from the radio parallax 115-118 F4.2 kpc e_Dist Error on the distance of the target from the radio parallax -------------------------------------------------------------------------------- Acknowledgements: Pikky Atri, pikkyatri23(at)gmail.com
(End) Patricia Vannier [CDS] 28-Sep-2022
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