Detection of the gravitational redshift in the orbit of the star S2 near the Galactic centre massive black hole
Open accessAbstract
The highly elliptical, 16-year-period orbit of the star S2 around the massive black hole candidate Sgr A ✻ is a sensitive probe of the gravitational field in the Galactic centre. Near pericentre at 120 AU ≈ 1400 Schwarzschild radii, the star has an orbital speed of ≈7650 km s −1 , such that the first-order effects of Special and General Relativity have now become detectable with current capabilities. Over the past 26 years, we have monitored the radial velocity and motion on the sky of S2, mainly with the SINFONI and NACO adaptive optics instruments on the ESO Very Large Telescope, and since 2016 and leading up to the pericentre approach in May 2018, with the four-telescope interferometric beam-combiner instrument GRAVITY. From data up to and including pericentre, we robustly detect the combined gravitational redshift and relativistic transverse Doppler effect for S2 of z = Δ λ / λ ≈ 200 km s −1 / c with different statistical analysis methods. When parameterising the post-Newtonian contribution from these effects by a factor f , with f = 0 and f = 1 corresponding to the Newtonian and general relativistic limits, respectively, we find from posterior fitting with different weighting schemes f = 0.90 ± 0.09| stat ± 0.15| sys . The S2 data are inconsistent with pure Newtonian dynamics.
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Integrity signals
Registry
Cites
Statistics
Claims the paper makes
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Claims other papers make about this one
Each is checked against this paper’s own text: does it say what the citing paper says it does?
R⊙ = 8.122 ± 0.031 kpc.
“which we take as R ⊙ = 8 . 122 ± 0 . 031 kpc (Gravity Collaboration et al. 2018)”
From The milky way total mass profile as inferred from Gaia DR2 (2020) · cites this paper as Gravity Collaboration et al. 2018
Self-check
Percentages, sums and reported differences re-computed from the paper’s own numbers.
The self-check needs the paper’s full text.
Cites
Observation of Gravitational Waves from a Binary Black Hole Merger
Abbott, B. P., Abbott, R., Abbott, T. D., Abernathy, M. R., Acernese, F., Ackley, K., Adams, C., Adams, T., Addesso, P., Adhikari, R. X., et al. (2016) · Physical Review Letters · doi:10.1103/physrevlett.116.061102 · Cited by 14,251 · see citing works
The Confrontation between General Relativity and Experiment
Will, C. M. (2014) · Living Reviews in Relativity · doi:10.12942/lrr-2014-4 · Cited by 3,996 · see citing works
Die Grundlage der allgemeinen Relativitätstheorie
Einstein, A. (1916) · Annalen der Physik · doi:10.1002/andp.19163540702 · Cited by 3,468 · see citing works
GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence
Abbott, B. P., Abbott, R., Abbott, T. D., et al. (2016) · Physical Review Letters · doi:10.1103/physrevlett.116.241103 · Cited by 3,457 · see citing works
MONITORING STELLAR ORBITS AROUND THE MASSIVE BLACK HOLE IN THE GALACTIC CENTER
Gillessen, S., Eisenhauer, F., Trippe, S., Alexander, T., Genzel, R., Martins, F., & Ott, T. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/692/2/1075 · Cited by 1,779 · see citing works
Self-citationGhez, A. M., Salim, S., Weinberg, N. N., Lu, J. R., Do, T., Dunn, J. K., Matthews, K., Morris, M. R., Yelda, S., Becklin, E. E., et al. (2008) · The Astrophysical Journal · doi:10.1086/592738 · Cited by 1,577 · see citing works
The Galactic Center massive black hole and nuclear star cluster
Genzel, R., Eisenhauer, F., & Gillessen, S. (2010) · Reviews of Modern Physics · doi:10.1103/revmodphys.82.3121 · Cited by 1,236 · see citing works
Self-citationA star in a 15.2-year orbit around the supermassive black hole at the centre of the Milky Way
Schödel, R., Ott, T., Genzel, R., Hofmann, R., Lehnert, M., Eckart, A., Mouawad, N., Alexander, T., Reid, M. J., Lenzen, R., et al. (2002) · Nature · doi:10.1038/nature01121 · Cited by 1,166 · see citing works
Self-citationViewing the Shadow of the Black Hole at the Galactic Center
Falcke, H. D., Melia, F., & Agol, E. (2000) · The Astrophysical Journal · doi:10.1086/312423 · Cited by 1,101 · see citing works
Tests of General Relativity from Timing the Double Pulsar
Krämer, M., Stairs, I. H., Manchester, R. N., et al. (2006) · Science · doi:10.1126/science.1132305 · Cited by 1,098 · see citing works
Tanaka, Y., Nandra, K., Fabian, A. C., Inoue, H., Otani, C., Dotani, T., Hayashida, K., Iwasawa, K., Kii, T., Kunieda, H., et al. (1995) · Nature · doi:10.1038/375659a0 · Cited by 1,033 · see citing works
The Lense-Thirring Effect and Accretion Disks around Kerr Black Holes
Bardeen, J. M., & Petterson, J. A. (1975) · The Astrophysical Journal · doi:10.1086/181711 · Cited by 887 · see citing works
Event-horizon-scale structure in the supermassive black hole candidate at the Galactic Centre
Doeleman, S. S., Weintroub, J., Rogers, A. E. E., Plambeck, R. L., Freund, R. W., Tilanus, R. P. J., Friberg, P., Ziurys, L. M., Moran, J. M., Corey, B. E., et al. (2008) · Nature · doi:10.1038/nature07245 · Cited by 836 · see citing works
ASTROPHYSICAL IMPLICATIONS OF THE BINARY BLACK HOLE MERGER GW150914
Abbott, B. P., Abbott, R., Abbott, T. D., et al. (2016) · The Astrophysical Journal Letters · doi:10.3847/2041-8205/818/2/l22 · Cited by 816 · see citing works
A new test of general relativity - Gravitational radiation and the binary pulsar PSR 1913+16
Taylor, J. H., & Weisberg, J. M. (1982) · The Astrophysical Journal · doi:10.1086/159690 · Cited by 805 · see citing works
The Proper Motion of Sagittarius A*. II. The Mass of Sagittarius A*
Reid, M. J., & Brunthaler, A. (2004) · The Astrophysical Journal · doi:10.1086/424960 · Cited by 791 · see citing works
Ghez, A. M., Duchêne, G., Matthews, K., Hornstein, S. D., Tanner, A., Larkin, J., Morris, M., Becklin, E. E., Salim, S., Kremenek, T., et al. (2003) · The Astrophysical Journal · doi:10.1086/374804 · Cited by 717 · see citing works
SINFONI in the Galactic Center: Young Stars and Infrared Flares in the Central Light‐Month
Eisenhauer, F., Genzel, R., Tal Alexander, A., Abuter, R., Paumard, T., Ott, T., Gilbert, A., Gillessen, S., Horrobin, M., Trippe, S., et al. (2005) · The Astrophysical Journal · doi:10.1086/430667 · Cited by 662 · see citing works
Self-citationThe Stellar Cusp around the Supermassive Black Hole in the Galactic Center
Genzel, R., Schödel, R., Ott, T., Eisenhauer, F., Hofmann, R., Lehnert, M. D., Eckart, A., Tal Alexander, A., Sternberg, A., Lenzen, R., et al. (2003) · The Astrophysical Journal · doi:10.1086/377127 · Cited by 587 · see citing works
Self-citationAbuter, R., Accardo, M., Amorim, A., Anugu, N., Ávila, G., Azouaoui, N., Benisty, M., Berger, J.-P., Blind, N., Bonnet, H., et al. (2017) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201730838 · Cited by 586 · see citing works
Self-citationBroad Iron Lines in Active Galactic Nuclei
Fabian, A. C., Iwasawa, K., Reynolds, C. S., et al. (2000) · Publications of the Astronomical Society of the Pacific · doi:10.1086/316610 · Cited by 547 · see citing works
An Update on Monitoring Stellar Orbits in the Galactic Center
Gillessen, S., Plewa, P. M., Eisenhauer, F., Sari, R., Waisberg, I., Habibi, M., Pfuhl, O., George, E., Dexter, J., von Fellenberg, S. D., et al. (2017) · The Astrophysical Journal · doi:10.3847/1538-4357/aa5c41 · Cited by 503 · see citing works
Self-citationTHE ORBIT OF THE STAR S2 AROUND SGR A* FROM VERY LARGE TELESCOPE AND KECK DATA
Gillessen, S., Eisenhauer, F., Fritz, T. K., Bartko, H., Dodds-Eden, K., Pfuhl, O., Ott, T., & Genzel, R. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/707/2/l114 · Cited by 467 · see citing works
Self-citationGravitational Red-Shift in Nuclear Resonance
Pound, R. V., & Rebka, G. A. (1959) · Physical Review Letters · doi:10.1103/physrevlett.3.439 · Cited by 389 · see citing works
SINFONI - Integral field spectroscopy at 50 milli-arcsecond resolution with the ESO VLT
Eisenhauer, F., Abuter, R., Bickert, K., Biancat-Marchet, F., Bonnet, H., Brynnel, J., Conzelmann, R. D., Delabre, B., Donaldson, R., Farinato, J., et al. (2003) · Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE · doi:10.1117/12.459468 · Cited by 377 · see citing works
Self-citationA Geometric Determination of the Distance to the Galactic Center
Eisenhauer, F., Schdel, R., Genzel, R., Ott, T., Tecza, M., Abuter, R., Eckart, A., & Alexander, T. (2003) · The Astrophysical Journal · doi:10.1086/380188 · Cited by 354 · see citing works
Self-citationStellar processes near the massive black hole in the Galactic center
Alexander, T. (2005) · Physics Reports · doi:10.1016/j.physrep.2005.08.002 · Cited by 302 · see citing works
AN IMPROVED DISTANCE AND MASS ESTIMATE FOR SGR A* FROM A MULTISTAR ORBIT ANALYSIS
Boehle, A., Ghez, A. M., Schödel, R., Meyer, L., Yelda, S., Albers, S., Martinez, G. D., Becklin, E. E., Do, T., Lu, J. R., et al. (2016) · The Astrophysical Journal · doi:10.3847/0004-637x/830/1/17 · Cited by 293 · see citing works
Interferometric data reduction with AMBER/VLTI. Principle, estimators, and illustration
Tatulli, E., Millour, F., Chelli, A., et al. (2007) · Astronomy and Astrophysics · doi:10.1051/0004-6361:20064799 · Cited by 282 · see citing works
The nuclear star cluster of the Milky Way: proper motions and mass
Schödel, R., Merritt, D. R., & Eckart, A. (2009) · Astronomy and Astrophysics · doi:10.1051/0004-6361/200810922 · Cited by 275 · see citing works
Self-citationWill, C. M. (2008) · The Astrophysical Journal · doi:10.1086/528847 · Cited by 271 · see citing works
Hees, A., Do, T., Ghez, A. M., Martinez, G. D., Naoz, S., Becklin, E. E., Boehle, A., Chappell, S., Chu, D. S., Dehghanfar, A., et al. (2017) · Physical Review Letters · doi:10.1103/physrevlett.118.211101 · Cited by 265 · see citing works
The Shortest-Known–Period Star Orbiting Our Galaxy’s Supermassive Black Hole
Meyer, L., Ghez, A. M., Schödel, R., Yelda, S., Boehle, A., Lu, J. R., Do, T., Morris, M., Becklin, E. E., & Matthews, K. (2012) · Science · doi:10.1126/science.1225506 · Cited by 227 · see citing works
Testing properties of the Galactic center black hole using stellar orbits
Merritt, D. R., Tal Alexander, A., Mikkola, S., & Will, C. M. (2010) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.81.062002 · Cited by 197 · see citing works
Dos and don'ts of reduced chi-squaredPreprint
Andrae, R., Schulze-Hartung, T., & Melchior, P. (2010) · arXiv (Cornell University) · doi:10.48550/arxiv.1012.3754 · Cited by 178 · see citing works
Imaging a boson star at the Galactic center
Vincent, F. H., Méliani, Z., Grandclément, P., et al. (2016) · Classical and Quantum Gravity · doi:10.1088/0264-9381/33/10/105015 · Cited by 165 · see citing works
Self-citationToward the event horizon—the supermassive black hole in the Galactic Center
Falcke, H., & Markoff, S. (2013) · Classical and Quantum Gravity · doi:10.1088/0264-9381/30/24/244003 · Cited by 164 · see citing works
CONICA: the high-resolution near-infrared camera for the ESO VLT
Lenzen, R., Hofmann, R., Bizenberger, P., & Tusche, A. (1998) · Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE · doi:10.1117/12.317287 · Cited by 139 · see citing works
Self-citationProbing Post-Newtonian Physics near the Galactic Black Hole with Stellar Redshift Measurements
Zucker, S., Tal Alexander, A., Gillessen, S., Eisenhauer, F., & Genzel, R. (2006) · The Astrophysical Journal · doi:10.1086/501436 · Cited by 127 · see citing works
Self-citationHubble Space Telescope spectroscopy of the Balmer lines in Sirius B★
Barstow, M. A., Bond, H. E., Holberg, J. B., Burleigh, M. R., Hubeny, I., & Koester, D. (2005) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2005.09359.x · Cited by 112 · see citing works
Habibi, M., Gillessen, S., Martins, F., Eisenhauer, F., Plewa, P., Pfuhl, O., George, E., Dexter, J., Waisberg, I., Ott, T., et al. (2017) · The Astrophysical Journal · doi:10.3847/1538-4357/aa876f · Cited by 105 · see citing works
Self-citationParsa, M., Eckart, A., Shahzamanian, B., Karas, V., Zajaček, M., Zensus, J. A., & Straubmeier, C. (2017) · The Astrophysical Journal · doi:10.3847/1538-4357/aa7bf0 · Cited by 102 · see citing works
Self-citationPERTURBATIONS OF INTERMEDIATE-MASS BLACK HOLES ON STELLAR ORBITS IN THE GALACTIC CENTER
Gualandris, A., & Merritt, D. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/705/1/361 · Cited by 99 · see citing works
The distribution of stars around the Milky Way’s central black hole
Gallego-Cano, E., Schödel, R., Dong, H., Nogueras-Lara, F., Gallego-Calvente, A. T., Amaro‐Seoane, P., & Baumgardt, H. (2017) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201730451 · Cited by 99 · see citing works
MIRA: an effective imaging algorithm for optical interferometry
Thiébaut, É. (2008) · Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE · doi:10.1117/12.788822 · Cited by 98 · see citing works
THE NUCLEAR CLUSTER OF THE MILKY WAY: TOTAL MASS AND LUMINOSITY*
Fritz, T. K., Chatzopoulos, S., Gerhard, O., Gillessen, S., Genzel, R., Pfuhl, O., Tacchella, S., Eisenhauer, F., & Ott, T. (2016) · The Astrophysical Journal · doi:10.3847/0004-637x/821/1/44 · Cited by 98 · see citing works
Self-citationOn the Nature of the Fast-Moving Star S2 in the Galactic Center
Martins, F., Gillessen, S., Eisenhauer, F., Genzel, R., Ott, T., & Trippe, S. (2007) · The Astrophysical Journal · doi:10.1086/526768 · Cited by 97 · see citing works
Self-citationThe Position of Sagittarius A*. III. Motion of the Stellar Cusp
Reid, M. J., Menten, K. M., Trippe, S., et al. (2007) · The Astrophysical Journal · doi:10.1086/511744 · Cited by 85 · see citing works
General relativistic effects on the orbit of the S2 star with GRAVITY
Grould, M., Vincent, F. H., Paumard, T., et al. (2017) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201731148 · Cited by 77 · see citing works
Self-citationGalactic center research: manifestations of the central black hole
Morris, M., Meyer, L., & Ghez, A. M. (2012) · Research in Astronomy and Astrophysics · doi:10.1088/1674-4527/12/8/007 · Cited by 74 · see citing works
Pinpointing the near-infrared location of Sgr A* by correcting optical distortion in the NACO imager
Plewa, P. M., Gillessen, S., Eisenhauer, F., Ott, T., Pfuhl, O., George, E. M., Dexter, J., Habibi, M., Genzel, R., Reid, M. J., et al. (2015) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stv1910 · Cited by 72 · see citing works
Self-citationDynamical Imaging with Interferometry
Johnson, M. D., Bouman, K. L., Blackburn, L., Chael, A., Rosen, J., Shiokawa, H., Roelofs, F., Akiyama, K., Fish, V. L., & Doeleman, S. S. (2017) · The Astrophysical Journal · doi:10.3847/1538-4357/aa97dd · Cited by 68 · see citing works
Chu, D. S., Do, T., Hees, A., Ghez, A. M., Naoz, S., Witzel, G., Sakai, S., Chappell, S., Gautam, A. K., Lu, J. R., et al. (2018) · The Astrophysical Journal · doi:10.3847/1538-4357/aaa3eb · Cited by 67 · see citing works
IS THERE A SUPERMASSIVE BLACK HOLE AT THE CENTER OF THE MILKY WAY?
Reid, M. J. (2009) · International Journal of Modern Physics D · doi:10.1142/s0218271809014820 · Cited by 65 · see citing works
Design of the Nasmyth adaptive optics system (NAOS) of the VLT
Rousset, G., Lacombe, F., Puget, P., Hubin, N., Gendron, E., Conan, J., Kern, P. Y., Madec, P. Y., Rabaud, D., Mouillet, D., et al. (1998) · Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE · doi:10.1117/12.321686 · Cited by 61 · see citing works
Self-citationEffective Temperature, Radius, and Gravitational Redshift of Sirius B
Greenstein, J. L., Oke, J. B., & Shipman, H. L. (1971) · The Astrophysical Journal · doi:10.1086/151174 · Cited by 61 · see citing works
Sch\"odel, R., Gallego-Cano, E., Dong, H., Nogueras-Lara, F., Gallego-Calvente, A. T., Amaro‐Seoane, P., & Baumgardt, H. (2017) · arXiv (Cornell University) · doi:10.1051/0004-6361/201730452 · Cited by 57 · see citing works
The S-star cluster at the center of the Milky Way
Sabha, N. B., Eckart, A., Merritt, D. R., Zamaninasab, M., Witzel, G., García-Marín, M., Jalali, B., Valencia-S., M., Yazıcı, Ş., Buchholz, R., et al. (2012) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201219203 · Cited by 52 · see citing works
Self-citationThe Galactic Centre star S2 as a dynamical probe for intermediate-mass black holes
Gualandris, A., Gillessen, S., & Merritt, D. R. (2010) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2010.17373.x · Cited by 51 · see citing works
Self-citationWaisberg, I., Dexter, J., Gillessen, S., Pfuhl, O., Eisenhauer, F., Plewa, P. M., Bauböck, M., Jiménez-Rosales, A., Habibi, M., Ott, T., et al. (2018) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sty476 · Cited by 41 · see citing works
Self-citationLachaume, R., & Berger, J.-P. (2013) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stt1462 · Cited by 13 · see citing works
Self-citationMethods for multiple-telescope beam imaging and guiding in the near-infrared
Anugu, N., Amorim, A., Gordo, P. R., et al. (2018) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sty223 · Cited by 12 · see citing works
Self-citationUnrecognized astrometric confusion in the Galactic Centre
Plewa, P. M., & Sari, R. (2018) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sty512 · Cited by 11 · see citing works
Self-citationHigh resolution K-band images of the galactic centre
Hofmann, R., Eckart, A., Genzel, R., et al. (1993) · Astrophysics and Space Science · doi:10.1007/bf00657949 · Cited by 11 · see citing works
Self-citationCIAO: wavefront sensors for GRAVITY
Scheithauer, S., Brandner, W., Deen, C. P., et al. (2016) · Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE · doi:10.1117/12.2232997 · Cited by 8 · see citing works
Self-citationHsiao, H.-K., Winick, K. A., Monnier, J. D., et al. (2010) · Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE · doi:10.1117/12.858295 · Cited by 3 · see citing works
Flagged first, then by citations
Research works printed but not linked: 71
- Abbott, B. P., Abbott, R., Abbott, T. D., et al. 2016a, ApJ, 818, L22 · DOI
- Abbott, B. P., Abbott, R., Abbott, T. D., et al. 2016b, Phys. Rev. Lett., 116, 241103 · DOI
- Abbott, B. P., Abbott, R., Abbott, T. D., et al. 2016c, Phys. Rev. Lett., 116, 061102 · DOI
- Alexander, T. 2005, Phys. Rep., 419, 65 · DOI
- Anugu, N., Amorim, A., Gordo, P., et al. 2018, MNRAS, 476, 459 · DOI
- Bardeen, J. M., & Petterson, J. A. 1975, ApJ, 195, L65 · DOI
- Baron, F., Monnier, J. D., & Kloppenborg, B. 2010, in Optical and Infrared Interferometry II, Proc. SPIE, 7734, 77342I · DOI
- Barstow, M. A., Bond, H. E., Holberg, J. B., et al. 2005, MNRAS, 362, 1134 · DOI
- Boehle, A., Ghez, A. M., Schödel, R., et al. 2016, ApJ, 830, 17 · DOI
- Bonnet, H., Abuter, R., Baker, A., et al. 2004, The Messenger, 117, 17 · DOI
- Chu, D. S., Do, T., Hees, A., et al. 2018, ApJ, 854, 12 · DOI
- Doeleman, S. S., Weintroub, J., Rogers, A. E. E., et al. 2008, Nature, 455, 78 · DOI
- Einstein, A. 1916, Ann. Phys., 354, 769 · DOI
- Eisenhauer, F., Abuter, R., Bickert, K., et al. 2003a, in Instrument Design and Performance for Optical/Infrared Ground-based Telescopes, eds. M. Iye, & A. F. M. Moorwood, Proc. SPIE, 4841, 1548 · DOI
- Eisenhauer, F., Schödel, R., Genzel, R., et al. 2003b, ApJ, 597, L121 · DOI
- Eisenhauer, F., Genzel, R., Alexander, T., et al. 2005, ApJ, 628, 246 · DOI
- Fabian, A. C., Iwasawa, K., Reynolds, C. S., & Young, A. J. 2000, PASP, 112, 1145 · DOI
- Falcke, H., & Markoff, S. B. 2013, Class. Quant. Grav., 30, 244003 · DOI
- Falcke, H., Melia, F., & Agol, E. 2000, ApJ, 528, L13 · DOI
- Fritz, T. K., Chatzopoulos, S., Gerhard, O., et al. 2016, ApJ, 821, 44 · DOI
- Gallego-Cano, E., Schödel, R., Dong, H., et al. 2018, A&A, 609, A26 · DOI
- Genzel, R., Schödel, R., Ott, T., et al. 2003, ApJ, 594, 812 · DOI
- Genzel, R., Eisenhauer, F., & Gillessen, S. 2010, Rev. Mod. Phys., 82, 3121 · DOI
- Ghez, A. M., Duchêne, G., Matthews, K., et al. 2003, ApJ, 586, L127 · DOI
- Ghez, A. M., Salim, S., Weinberg, N. N., et al. 2008, ApJ, 689, 1044 · DOI
- Gillessen, S., Eisenhauer, F., Fritz, T. K., et al. 2009a, ApJ, 707, L114 · DOI
- Gillessen, S., Eisenhauer, F., Trippe, S., et al. 2009b, ApJ, 692, 1075 · DOI
- Gillessen, S., Plewa, P. M., Eisenhauer, F., et al. 2017, ApJ, 837, 30 · DOI
- GRAVITY Collaboration (Abuter, R., et al.) 2017, A&A, 602, A94 · DOI
- Greenstein, J. L., Oke, J. B., & Shipman, H. L. 1971, ApJ, 169, 563 · DOI
- Greisen, E. W. 2003, in Information Handling in Astronomy -Historical Vistas, ed. A. Heck, Astrophysics and Space Science Library, 285, 109 · DOI
- Grould, M., Vincent, F. H., Paumard, T., & Perrin, G. 2017, A&A, 608, A60 · DOI
- Gualandris, A., Gillessen, S., & Merritt, D. 2010, MNRAS, 409, 1146 · DOI
- Gualandris, A., & Merritt, D. 2009, ApJ, 705, 361 · DOI
- Habibi, M., Gillessen, S., Martins, F., et al. 2017, ApJ, 847, 120 · DOI
- Hees, A., Do, T., Ghez, A. M., et al. 2017, Phys. Rev. Lett., 118, 211101 · DOI
- Hofmann, R., Eckart, A., Genzel, R., & Drapatz, S. 1993, Ap&SS, 205, 1 · DOI
- Högbom, J. A. 1974, A&AS, 15, 417 · DOI
- Johnson, M. D., Bouman, K. L., Blackburn, L., et al. 2017, ApJ, 850, 172 · DOI
- Kramer, M., Stairs, I. H., Manchester, R. N., et al. 2006, Science, 314, 97 · DOI
- Lachaume, R., & Berger, J.-P. 2013, MNRAS, 435, 2501 · DOI
- Lapeyrere, V., Kervella, P., Lacour, S., et al. 2014, in Optical and Infrared Interferometry IV, Proc. SPIE, 9146, 91462D · DOI
- Lenzen, R., Hofmann, R., Bizenberger, P., & Tusche, A. 1998, in Infrared Astronomical Instrumentation, ed. A. M. Fowler, Proc. SPIE, 3354, 606 · DOI
- Mackay, D. J. C. 2003, Information Theory, Inference and Learning Algorithms, 640 · DOI
- Martins, F., Gillessen, S., Eisenhauer, F., et al. 2008, ApJ, 672, L119 · DOI
- Merritt, D., Alexander, T., Mikkola, S., & Will, C. M. 2010, Phys. Rev. D, 81, 062002 · DOI
- Meyer, L., Ghez, A. M., Schödel, R., et al. 2012, Science, 338, 84 · DOI
- Misner, C. W., Thorne, K. S., & Wheeler, J. A. 1973, Gravitation Morris, M. R., Meyer, L., & Ghez, A. M. 2012, Res. Astron. Astrophys., 12, 995 · DOI
- Parsa, M., Eckart, A., Shahzamanian, B., et al. 2017, ApJ, 845, 22 · DOI
- Plewa, P. M., Gillessen, S., Eisenhauer, F., et al. 2015, MNRAS, 453, 3234 · DOI
- Plewa, P. M., & Sari, R. 2018, MNRAS, 476, 4372 · DOI
- Pound, R. V., & Rebka, G. A. 1959, Phys. Rev. Lett., 3, 439 · DOI
- Psaltis, D. 2004, in X-ray Timing 2003: Rossi and Beyond, eds. P. Kaaret, F. K. Lamb, & J. H. Swank, American Institute of Physics Conference Series, 714, 29 · DOI
- Reid, M. J. 2009, Int. J. Mod. Phys. D, 18, 889 · DOI
- Reid, M. J., & Brunthaler, A. 2004, ApJ, 616, 872 · DOI
- Reid, M. J., Menten, K. M., Trippe, S., Ott, T., & Genzel, R. 2007, ApJ, 659, 378 · DOI
- Rousset, G., Lacombe, F., Puget, P., et al. 1998, in Adaptive Optical System Technologies, eds. D. Bonaccini, & R. K. Tyson, Proc. SPIE, 3353, 508 · DOI
- Sabha, N., Eckart, A., Merritt, D., et al. 2012, A&A, 545, A70 · DOI
- Scheithauer, S., Brandner, W., Deen, C., et al. 2016, in Adaptive Optics Systems V, Proc. SPIE, 9909, 99092L · DOI
- Schödel, R., Ott, T., Genzel, R., et al. 2002, Nature, 419, 694 · DOI
- Schödel, R., Merritt, D., & Eckart, A. 2009, A&A, 502, 91 · DOI
- Schödel, R., Gallego-Cano, E., Dong, H., et al. 2018, A&A, 609, A27 · DOI
- Tanaka, Y., Nandra, K., Fabian, A. C., et al. 1995, Nature, 375, 659 · DOI
- Tatulli, E., Millour, F., Chelli, A., et al. 2007, A&A, 464, 29 · DOI
- Taylor, J. H., & Weisberg, J. M. 1982, ApJ, 253, 908 · DOI
- Thiébaut, E. 2008, in Optical and Infrared Interferometry, Proc. SPIE, 7013, 70131I · DOI
- Vincent, F. H., Meliani, Z., Grandclément, P., Gourgoulhon, E., & Straub, O. 2016, Class. Quant. Grav., 33, 105015 · DOI
- Waisberg, I., Dexter, J., Gillessen, S., et al. 2018, MNRAS, 476, 3600 · DOI
- Will, C. M. 2008, ApJ, 674, L25 · DOI
- Will, C. M. 2014, Liv. Rev. Rel., 17, 4 · DOI
- Zucker, S., Alexander, T., Gillessen, S., Eisenhauer, F., & Genzel, R. 2006, ApJ, 639, L21 · DOI
Cited by
Sorted by citations
A geometric distance measurement to the Galactic center black hole with 0.3% uncertainty
The GRAVITY Collaboration, Abuter, R., Amorim, A., Bauböck, M., Berger, J. P., Bonnet, H., Brandner, W., Clénet, Y., Coudé du Foresto, V., de Zeeuw, P. T., et al. (2019) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201935656 · Cited by 827 · see citing works
Self-citationEvent Horizon Telescope Collaboration, Akiyama, K., Alberdi, A., Alef, W., Algaba, J. C., Anantua, R., Asada, K., Azulay, R., Bach, U., Baczko, A.-K., et al. (2022) · The Astrophysical Journal Letters · doi:10.3847/2041-8213/ac6429 · Cited by 449 · see citing works
Self-citationThe Circular Velocity Curve of the Milky Way from 5 to 25 kpc
Eilers, A.-C., Hogg, D. W., Rix, H.-W., & Ness, M. K. (2019) · The Astrophysical Journal · doi:10.3847/1538-4357/aaf648 · Cited by 404 · see citing works
The milky way total mass profile as inferred from Gaia DR2
Cautun, M., Benítez-Llambay, A., Deason, A. J., Frenk, C. S., Fattahi, A., Gómez, F. A., Grand, R. J. J., Oman, K. A., Navarro, J. F., & Simpson, C. M. (2020) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/staa1017 · Cited by 332 · see citing works
The Milky Way total mass profile as inferred from Gaia DR2
Cautun, M., Benitez-Llambay, A., Deason, A. J., Frenk, C. S., Fattahi, A., Gómez, F. A., Grand, R. J. J., Oman, K. A., Navarro, J. F., & Simpson, C. M. (2019) · arXiv · doi:10.48550/arxiv.1911.04557 · Cited by 335
On the estimation of the local dark matter density using the rotation curve of the Milky Way
de Salas, P. F., Malhan, K., Freese, K., Hattori, K., & Valluri, M. (2019) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2019/10/037 · Cited by 176 · see citing works
Millimeter Light Curves of Sagittarius A* Observed during the 2017 Event Horizon Telescope Campaign
Wielgus, M., Marchili, N., Martí-Vidal, I., Keating, G. K., Ramakrishnan, V., Tiede, P., Fomalont, E., Issaoun, S., Neilsen, J., Nowak, M. A., et al. (2025) · The Astrophysical Journal Letters · doi:10.3847/2041-8213/ac6428 · Cited by 112 · see citing works
Self-citationKoposov, S. E., Erkal, D., Li, T. S., Da Costa, G. S., Cullinane, L. R., Ji, A. P., Kuehn, K., Lewis, G. F., Pace, A. B., Shipp, N., et al. (2023) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stad551 · Cited by 109 · see citing works
The Scattering and Intrinsic Structure of Sagittarius A* at Radio Wavelengths
Johnson, M. D., Narayan, R., Psaltis, D., Blackburn, L., Kovalev, Y. Y., Gwinn, C. R., Zhao, G.-Y., Bower, G. C., Moran, J. M., Kino, M., et al. (2018) · The Astrophysical Journal · doi:10.3847/1538-4357/aadcff · Cited by 105 · see citing works
Self-citationDetection of the LMC-induced sloshing of the Galactic halo
Erkal, D., Deason, A. J., Belokurov, V., Xue, X.-X., Koposov, S. E., Bird, S. A., Liu, C., Simion, I. T., Yang, C., Zhang, L., et al. (2021) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stab1828 · Cited by 101 · see citing works
The Circular Velocity Curve of the Milky Way from 5–25 kpc Using Luminous Red Giant Branch Stars
Zhou, Y., Li, X., Huang, Y., & Zhang, H. (2023) · The Astrophysical Journal · doi:10.3847/1538-4357/acadd9 · Cited by 85 · see citing works
Koop, O., Antoja, T., Helmi, A., Callingham, T. M., & Laporte, C. F. P. (2024) · Astronomy & Astrophysics · doi:10.1051/0004-6361/202450911 · Cited by 14 · see citing works
MICROSCOPE’s view at gravitation
Bergé, J. (2023) · Reports on Progress in Physics · doi:10.1088/1361-6633/acd203 · Cited by 12 · see citing works
- Authors
- GRAVITY Collaboration, Abuter, R., Amorim, A., Anugu, N., Bauböck, M., Benisty, M., Berger, J. P., Blind, N., Bonnet, H., Brandner, W., Buron, A., Collin, C., Chapron, F., Clénet, Y., dCoudé u Foresto, V., de Zeeuw, P. T., Deen, C., Delplancke-Ströbele, F., Dembet, R., Dexter, J., Duvert, G., Eckart, A., Eisenhauer, F., Finger, G., Förster Schreiber, N. M., Fédou, P., Garcia, P., Garcia Lopez, R., Gao, F., Gendron, E., Genzel, R., Gillessen, S., Gordo, P., Habibi, M., Haubois, X., Haug, M., Haußmann, F., Henning, T., Hippler, S., Horrobin, M., Hubert, Z., Hubin, N., Jimenez Rosales, A., Jochum, L., Jocou, L., Kaufer, A., Kellner, S., Kendrew, S., Kervella, P., Kok, Y., Kulas, M., Lacour, S., Lapeyrère, V., Lazareff, B., Le Bouquin, J.-B., Léna, P., Lippa, M., Lenzen, R., Mérand, A., Müler, E., Neumann, U., Ott, T., Palanca, L., Paumard, T., Pasquini, L., Perraut, K., Perrin, G., Pfuhl, O., Plewa, P. M., Rabien, S., Ramírez, A., Ramos, J., Rau, C., Rodríguez-Coira, G., Rohloff, R.-R., Rousset, G., Sanchez-Bermudez, J., Scheithauer, S., Schöller, M., Schuler, N., Spyromilio, J., Straub, O., Straubmeier, C., Sturm, E., Tacconi, L. J., Tristram, K. R. W., Vincent, F., von Fellenberg, S., Wank, I., Waisberg, I., Widmann, F., Wieprecht, E., Wiest, M., Wiezorrek, E., Woillez, J., Yazici, S., Ziegler, D., & Zins, G.
- Affiliations
- European Southern Observatory (DE)
- University of Lisbon (PT)
- Universidade do Porto (PT)
- Max Planck Institute for Extraterrestrial Physics (DE)
- Centre National de la Recherche Scientifique (FR)
- University of Geneva (CH)
- Max Planck Institute for Astronomy (DE)
- University of Cologne (DE)
- European Southern Observatory (CL)
- Max Planck Institute for Radio Astronomy (DE)
- Space Telescope Science Institute (US)
- ORCID
- Amorim, A.
- Bauböck, M.
- Benisty, M.
- Blind, N.
- Brandner, W.
- Clénet, Y.
- Dexter, J.
- Duvert, G.
- Eckart, A.
- Gendron, E.
- Genzel, R.
- Haubois, X.
- Horrobin, M.
- Jocou, L.
- Kaufer, A.
- Kervella, P.
- Lacour, S.
- Lapeyrère, V.
- Mérand, A.
- Ott, T.
- Paumard, T.
- Perraut, K.
- Perrin, G.
- Scheithauer, S.
- Straub, O.
- Straubmeier, C.
- Vincent, F.
- Woillez, J.
- Zins, G.
- Venue
- Astronomy & Astrophysics
- Publisher
- EDP Sciences
- Published
- 2018-07
- Volume
- 615
- Pages
- L15
- ISSN
- 0004-6361 (ISSN-L)
- 1432-0746
- OpenAlex
- W2884375320
- Cited by
- 946
- References
- 66
- Citations by year
- 2026: 70 · 2025: 106 · 2024: 107 · 2023: 121 · 2022: 104 · 2021: 132 · 2020: 131 · 2019: 143 · 2018: 30 · 2017: 1 · 2014: 1
- FWCI
- 58.42
- Type
- journal article
- Language
- en
- Open access
- bronze
- doi.org
- Locations
- Astronomy and Astrophysics (publishedVersion)
- Kölner Universitäts PublikationsServer (Universität zu Köln) (publishedVersion)
- Open Research Exeter (University of Exeter) (acceptedVersion)
- arXiv (Cornell University) (submittedVersion)
- HAL (submittedVersion, other-oa)
- HAL (submittedVersion)
- MPG.PuRe (Max Planck Society) (submittedVersion)
- arXiv (Cornell University)
- Funders
- Deutsche Forschungsgemeinschaft
- Bundesministerium für Bildung und Forschung
- Max-Planck-Gesellschaft
- Centre National de la Recherche Scientifique
- Observatoire de Paris, Université de Recherche Paris Sciences et Lettres
- FP7 Ideas: European Research Council (610058, 306311)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astrophysical Phenomena and Observations
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Pulsars and Gravitational Waves Research
- Keywords
- gravitational redshift, S2 star, Sgr A*, Galactic Center, massive black holes, relativistic Doppler effect, post-Newtonian effects, tests of general relativity, stellar orbits, GRAVITY interferometer, adaptive optics, radial velocity
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
What counts as a claim ›How we measure confidence ›How we check this ›
Are you an author, or do you see a problem with this page? Request a review