| journal=Astronomy & Astrophysics
| journal=Astronomy & Astrophysics
| volume=654 | at=id. A14 | date=October 2021
| volume=654 | at=id. A14 | date=October 2021
| doi=10.1051/0004-6361/202140567 | arxiv=2102.07811
| doi=10.1051/0004-6361/202140567 | =
| bibcode=2021A&A…654A..14D }}
| bibcode=2021A&A…654A..14D }}
| title=Accretion geometry of the black hole binary MAXI J1820+070 probed by frequency-resolved spectroscopy
| last1=Axelsson | first1=Magnus | last2=Veledina | first2=Alexandra
| doi=10.1093/mnras/stab2191 | arxiv=2103.08795
| bibcode=2021MNRAS.507.2744A }}
*{{citation | postscript=.
*{{citation | postscript=.
| title=Measuring fundamental jet properties with multiwavelength fast timing of the black hole X-ray binary MAXI J1820+070
| title=Measuring fundamental jet properties with multiwavelength fast timing of the black hole X-ray binary MAXI J1820+070
| doi=10.1093/mnras/staa564 | doi-access=free
| doi=10.1093/mnras/staa564 | doi-access=free
| arxiv=2002.09691 | bibcode=2020MNRAS.493.5389F }}
| arxiv=2002.09691 | bibcode=2020MNRAS.493.5389F }}
*{{citation | postscript=.
| journal=Monthly Notices of the Royal Astronomical Society: Letters
| volume=493 | issue=1 | pages=L81–L86 | date=March 2020
*{{citation | postscript=.
| title=A Timing Study of MAXI J1820+070 Based on Swift/XRT and NICER Monitoring in 2018/19
| last1=Stiele | first1=H. | last2=Kong | first2=A. K. H.
| journal=The Astrophysical Journal
| volume=889 | issue=2 | at=id. 142 | date=February 2020
| doi=10.3847/1538-4357/ab64ef | doi-access=free
| arxiv=1912.07625 | bibcode=2020ApJ…889..142S }}
*{{citation | postscript=.
*{{citation | postscript=.
| title=Dynamical Confirmation of a Black Hole in MAXI J1820+070
| title=Dynamical Confirmation of a Black Hole in MAXI J1820+070
| doi=10.3847/1538-4357/ab09ff | doi-access=free
| doi=10.3847/1538-4357/ab09ff | doi-access=free
| arxiv=1903.01686 | bibcode=2019ApJ…874..183S }}
| arxiv=1903.01686 | bibcode=2019ApJ…874..183S }}
*{{citation | postscript=.
*{{citation | postscript=.
| title=X-Ray, Optical, and Near-infrared Monitoring of the New X-Ray Transient MAXI J1820+070 in the Low/Hard State
| title=X-Ray, Optical, and Near-infrared Monitoring of the New X-Ray Transient MAXI J1820+070 in the Low/Hard State
 |
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- Example: U Pegasi
X-ray binary in the constellation Pegasus
MAXI J1820+070 is an X-ray binary system in the equatorial constellation of Ophiuchus. The object identifier is from the MAXI telescope mounted on the International Space Station.[2]
- ^ a b c d Vallenari, A.; et al. (Gaia collaboration) (2023), “Gaia Data Release 3. Summary of the content and survey properties”, Astronomy and Astrophysics, 674: A1, arXiv:2208.00211, Bibcode:2023A&A…674A…1G, doi:10.1051/0004-6361/202243940, S2CID 244398875.
Gaia DR3 record for this source at VizieR. - ^ Matsuoka, Masaru; et al. (October 2009), “The MAXI Mission on the ISS: Science and Instruments for Monitoring All-Sky X-Ray Images”, Publications of the Astronomical Society of Japan, 61 (5): 999–1010, arXiv:0906.0631, Bibcode:2009PASJ…61..999M, doi:10.1093/pasj/61.5.999.
- Bright, Joe S.; et al. (August 2025), “The accretion–ejection connection in the black hole X-ray binary MAXI J1820+070”, Monthly Notices of the Royal Astronomical Society, 541 (2): 1851–1865, arXiv:2507.11303, Bibcode:2025MNRAS.541.1851B, doi:10.1093/mnras/staf1098.
- Banerjee, Srimanta; et al. (April 2024), “A Multiwavelength Study of the Hard and Soft States of MAXI J1820+070 During Its 2018 Outburst”, The Astrophysical Journal, 964 (2), id. 189, arXiv:2402.08237, Bibcode:2024ApJ…964..189B, doi:10.3847/1538-4357/ad24ef.
- Koljonen, K. I. I.; et al. (May 2023), “The origin of optical emission lines in the soft state of X-ray binary outbursts: the case of MAXI J1820+070”, Monthly Notices of the Royal Astronomical Society, 521 (3): 4190–4206, arXiv:2303.09242, Bibcode:2023MNRAS.521.4190K, doi:10.1093/mnras/stad809.
- Cangemi, F.; et al. (January 2023), “INTEGRAL study of MAXI J1535−571, MAXI J1820+070, and MAXI J1348 − 630 outbursts. I. Detection and polarization properties of the high-energy emission”, Astronomy & Astrophysics, 669, id. A65, arXiv:2210.08561, Bibcode:2023A&A…669A..65C, doi:10.1051/0004-6361/202243564.
- Zdziarski, Andrzej A.; et al. (February 2022), “Jet Parameters in the Black Hole X-Ray Binary MAXI J1820+070”, The Astrophysical Journal, 925 (2), id. 189, arXiv:2108.10929, Bibcode:2022ApJ…925..189Z, doi:10.3847/1538-4357/ac38a9.
- Thomas, Jessymol K.; et al. (January 2022), “Large optical modulations during 2018 outburst of MAXI J1820 + 070 reveal evolution of warped accretion disc through X-ray state change”, Monthly Notices of the Royal Astronomical Society, 509 (1): 1062–1074, arXiv:2108.05447, Bibcode:2022MNRAS.509.1062T, doi:10.1093/mnras/stab3033.
- De Marco, B.; et al. (October 2021), “The inner flow geometry in MAXI J1820+070 during hard and hard-intermediate states”, Astronomy & Astrophysics, 654, id. A14, arXiv:2102.07811, Bibcode:2021A&A…654A..14D, doi:10.1051/0004-6361/202140567.
- Axelsson, Magnus; Veledina, Alexandra (October 2021), “Accretion geometry of the black hole binary MAXI J1820+070 probed by frequency-resolved spectroscopy”, Monthly Notices of the Royal Astronomical Society, 507 (2): 2744–2754, arXiv:2103.08795, Bibcode:2021MNRAS.507.2744A, doi:10.1093/mnras/stab2191.
{{citation}}: CS1 maint: unflagged free DOI (link) - Tetarenko, A. J.; et al. (July 2021), “Measuring fundamental jet properties with multiwavelength fast timing of the black hole X-ray binary MAXI J1820+070”, Monthly Notices of the Royal Astronomical Society, 504 (3): 3862–3883, arXiv:2103.09318, Bibcode:2021MNRAS.504.3862T, doi:10.1093/mnras/stab820.
- Rodi, J.; et al. (March 2021), “A Broadband View on Microquasar MAXI J1820+070 during the 2018 Outburst”, The Astrophysical Journal, 910 (1), id. 21, arXiv:2101.10767, Bibcode:2021ApJ…910…21R, doi:10.3847/1538-4357/abdfd0.
- Chakraborty, Sudip; et al. (November 2020), “A spectral study of the black hole X-ray binary MAXI J1820+070 with AstroSat and NuSTAR”, Monthly Notices of the Royal Astronomical Society, 498 (4): 5873–5884, arXiv:2009.02465, Bibcode:2020MNRAS.498.5873C, doi:10.1093/mnras/staa2711.
- Xu, Yanjun; et al. (April 2020), “Evidence for Disk Truncation at Low Accretion States of the Black Hole Binary MAXI J1820+070 Observed by NuSTAR and XMM-Newton”, The Astrophysical Journal, 893 (1), id. 42, arXiv:2003.01778, Bibcode:2020ApJ…893…42X, doi:10.3847/1538-4357/ab7cdb.
- Fabian, A. C.; et al. (April 2020), “The soft state of the black hole transient source MAXI J1820+070: emission from the edge of the plunge region?”, Monthly Notices of the Royal Astronomical Society, 493 (4): 5389–5396, arXiv:2002.09691, Bibcode:2020MNRAS.493.5389F, doi:10.1093/mnras/staa564.
- Atri, P.; et al. (March 2020), “A radio parallax to the black hole X-ray binary MAXI J1820+070”, Monthly Notices of the Royal Astronomical Society: Letters, 493 (1): L81 – L86, arXiv:1912.04525, Bibcode:2020MNRAS.493L..81A, doi:10.1093/mnrasl/slaa010.
- Stiele, H.; Kong, A. K. H. (February 2020), “A Timing Study of MAXI J1820+070 Based on Swift/XRT and NICER Monitoring in 2018/19”, The Astrophysical Journal, 889 (2), id. 142, arXiv:1912.07625, Bibcode:2020ApJ…889..142S, doi:10.3847/1538-4357/ab64ef.
- Torres, M. A. P.; et al. (September 2019), “Dynamical Confirmation of a Black Hole in MAXI J1820+070”, The Astrophysical Journal Letters, 882 (2), id. L21, arXiv:1907.00938, Bibcode:2019ApJ…882L..21T, doi:10.3847/2041-8213/ab39df.
- Veledina, Alexandra; et al. (March 2019), “Evolving optical polarisation of the black hole X-ray binary MAXI J1820+070”, Astronomy & Astrophysics, 623, id. A75, arXiv:1808.09002, Bibcode:2019A&A…623A..75V, doi:10.1051/0004-6361/201834140.
- Shidatsu, Megumi; et al. (April 2019), “X-Ray and Optical Monitoring of State Transitions in MAXI J1820+070”, The Astrophysical Journal, 874 (2), id. 183, arXiv:1903.01686, Bibcode:2019ApJ…874..183S, doi:10.3847/1538-4357/ab09ff.
- Shidatsu, Megumi; et al. (November 2018), “X-Ray, Optical, and Near-infrared Monitoring of the New X-Ray Transient MAXI J1820+070 in the Low/Hard State”, The Astrophysical Journal, 868 (1), id. 54, arXiv:1810.11222, Bibcode:2018ApJ…868…54S, doi:10.3847/1538-4357/aae929.
