[1] |
J.H. Oort, 1932 The force exerted by the stellar system in the direction perpendicular to the galactic plane and some related problems Bull Astron. Inst. Neth.6 249 · Zbl 0005.12805 |
[2] |
F. Zwicky, 1937 On the Masses of Nebulae and of Clusters of Nebulae, https://doi.org/10.1086/143864 Astrophys. J.86 217 · Zbl 0017.28802 · doi:10.1086/143864 |
[3] |
V.C. Rubin, W.K. Ford Jr. and N. Thonnard, 1978 Extended rotation curves of high-luminosity spiral galaxies. IV. Systematic dynamical properties, Sa through Sc, https://doi.org/10.1086/182804 Astrophys. J. Lett.225 L107 · doi:10.1086/182804 |
[4] |
V.C. Rubin, W.K. Ford Jr. and N. Thonnard, 1980 Rotational properties of 21 SC galaxies with a large range of luminosities and radii, from NGC 4605 (R = 4 kpc) to UGC 2885 (R = 122 kpc), https://doi.org/10.1086/158003 Astrophys. J.238 471 · doi:10.1086/158003 |
[5] |
J. Tyson, G.P. Kochanski and I.P. Dell’Antonio, 1998 Detailed mass map of CL0024+1654 from strong lensing, https://doi.org/10.1086/311314 Astrophys. J. Lett.498L107 [astro-ph/9801193] · doi:10.1086/311314 |
[6] |
M. Hasselfield et al., 2013 The Atacama Cosmology Telescope: Sunyaev-Zel’dovich selected galaxyclusters at 148 GHz from three seasons of data J. Cosmol. Astropart. Phys.2013 07 008 [1301.0816] |
[7] |
K. Osato, S. Flender, D. Nagai, M. Shirasaki and N. Yoshida, 2018 Investigating cluster astrophysics and cosmology with cross-correlation of the thermal Sunyaev-Zel’dovich effect and weak lensing, https://doi.org/10.1093/mnras/stx3215 Mon. Not. Roy. Astron. Soc.475 532 [1706.08972] · doi:10.1093/mnras/stx3215 |
[8] |
Planck collaboration, 2016 Planck 2015 results. XXIV. Cosmology from Sunyaev-Zeldovich cluster counts, https://doi.org/10.1051/0004-6361/201525833 Astron. Astrophys.594 A24 [1502.01597] · doi:10.1051/0004-6361/201525833 |
[9] |
T. Sakamoto, M. Chiba and T.C. Beers, 2003 The Mass of the Milky Way: Limits from a newly assembled set of halo objects, https://doi.org/10.1051/0004-6361:20021499 Astron. Astrophys.397 899 [astro-ph/0210508] · doi:10.1051/0004-6361:20021499 |
[10] |
SDSS collaboration, 2008 The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ∼2400 SDSS Blue Horizontal Branch Stars, https://doi.org/10.1086/589500 Astrophys. J.684 1143 [0801.1232] · doi:10.1086/589500 |
[11] |
P.R. Kafle, S. Sharma, G.F. Lewis and J. Bland-Hawthorn, 2014 On the Shoulders of Giants: Properties of the Stellar Halo and the Milky Way Mass Distribution, https://doi.org/10.1088/0004-637X/794/1/59 Astrophys. J.794 59 [1408.1787] · doi:10.1088/0004-637X/794/1/59 |
[12] |
F. Iocco, M. Pato and G. Bertone, 2015 Evidence for dark matter in the inner Milky Way, https://doi.org/10.1038/nphys3237 Nature Phys.11 245 [1502.03821] · doi:10.1038/nphys3237 |
[13] |
D.M. Scolnic et al., 2018 The Complete Light-curve Sample of Spectroscopically Confirmed SNe Ia from Pan-STARRS1 and Cosmological Constraints from the Combined Pantheon Sample, https://doi.org/10.3847/1538-4357/aab9bb Astrophys. J.859 101 [1710.00845] · doi:10.3847/1538-4357/aab9bb |
[14] |
Planck collaboration, Planck 2018 results. VI. Cosmological parameters, [1807.06209] |
[15] |
A.J. Ross, L. Samushia, C. Howlett, W.J. Percival, A. Burden and M. Manera, 2015 The clustering of the SDSS DR7 main Galaxy sample — I. A 4 per cent distance measure at z = 0.15, https://doi.org/10.1093/mnras/stv154 Mon. Not. Roy. Astron. Soc.449 835 [1409.3242] · doi:10.1093/mnras/stv154 |
[16] |
BOSS collaboration, 2017 The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample, https://doi.org/10.1093/mnras/stx721 Mon. Not. Roy. Astron. Soc.470 2617 [1607.03155] · doi:10.1093/mnras/stx721 |
[17] |
DES collaboration, 2019 Dark Energy Survey Year 1 Results: Measurement of the Baryon Acoustic Oscillation scale in the distribution of galaxies to redshift 1, https://doi.org/10.1093/mnras/sty3351 Mon. Not. Roy. Astron. Soc.483 4866 [1712.06209] · doi:10.1093/mnras/sty3351 |
[18] |
S.E. Nuza et al., 2013 The clustering of galaxies at z∼ 0.5 in the SDSS-III Data Release 9 BOSS-CMASS sample: a test for the LCDM cosmology, https://doi.org/10.1093/mnras/stt513 Mon. Not. Roy. Astron. Soc.432 743 [1202.6057] · doi:10.1093/mnras/stt513 |
[19] |
M. Schumann, 2019 Direct Detection of WIMP Dark Matter: Concepts and Status, https://doi.org/10.1088/1361-6471/ab2ea5 J. Phys. G46 103003 [1903.03026] · doi:10.1088/1361-6471/ab2ea5 |
[20] |
M. Milgrom, 1983 A Modification of the Newtonian dynamics as a possible alternative to the hidden mass hypothesis, https://doi.org/10.1086/161130 Astrophys. J.270 365 · doi:10.1086/161130 |
[21] |
J.D. Bekenstein, 2004 Relativistic gravitation theory for the MOND paradigm, https://doi.org/10.1103/PhysRevD.70.083509 Phys. Rev. D70 083509 [Erratum ibid 71 (2005) 069901] [astro-ph/0403694] · doi:10.1103/PhysRevD.70.083509 |
[22] |
D. Clowe et al., 2006 A direct empirical proof of the existence of dark matter, https://doi.org/10.1086/508162 Astrophys. J. Lett.648L109 [astro-ph/0608407] · doi:10.1086/508162 |
[23] |
J.W. Moffat, 2006 Scalar-tensor-vector gravity theory J. Cosmol. Astropart. Phys.2006 03 004 [gr-qc/0506021] · Zbl 1236.83047 |
[24] |
J.W. Moffat and V.T. Toth, 2008 Testing modified gravity with globular cluster velocity dispersions, https://doi.org/10.1086/587926 Astrophys. J.680 1158 [0708.1935] · doi:10.1086/587926 |
[25] |
J.W. Moffat and S. Rahvar, 2014 The MOG weak field approximation — II. Observational test of Chandra X-ray clusters, https://doi.org/10.1093/mnras/stu855 Mon. Not. Roy. Astron. Soc.441 3724 [1309.5077] · doi:10.1093/mnras/stu855 |
[26] |
J.W. Moffat and M.H. Zhoolideh Haghighi, 2017 Modified gravity (MOG) and the Abell 1689 cluster acceleration data, https://doi.org/10.1140/epjp/i2017-11684-4 Eur. Phys. J. Plus132 417 [1611.05382] · doi:10.1140/epjp/i2017-11684-4 |
[27] |
J.W. Moffat and S. Rahvar, 2013 The MOG weak field approximation and observational test of galaxy rotation curves, https://doi.org/10.1093/mnras/stt1670 Mon. Not. Roy. Astron. Soc.436 1439 [1306.6383] · doi:10.1093/mnras/stt1670 |
[28] |
M.H. Zhoolideh Haghighi and S. Rahvar, 2017 Testing MOG, Non-Local Gravity and MOND with rotation curves of dwarf galaxies, https://doi.org/10.1093/mnras/stx692 Mon. Not. Roy. Astron. Soc.468 4048 [1609.07851] · doi:10.1093/mnras/stx692 |
[29] |
C. Negrelli, M. Benito, S. Landau, F. Iocco and L. Kraiselburd, 2018 Testing modified gravity theory in the Milky Way, https://doi.org/10.1103/PhysRevD.98.104061 Phys. Rev. D98 104061 [1810.07200] · doi:10.1103/PhysRevD.98.104061 |
[30] |
D. Clowe et al., 2006 A direct empirical proof of the existence of dark matter, https://doi.org/10.1086/508162 Astrophys. J. Lett.648L109 [astro-ph/0608407] · doi:10.1086/508162 |
[31] |
J.R. Brownstein and J.W. Moffat, 2007 The Bullet Cluster 1E0657-558 evidence shows Modified Gravity in the absence of Dark Matter, https://doi.org/10.1111/j.1365-2966.2007.12275.x Mon. Not. Roy. Astron. Soc.382 29 [astro-ph/0702146] · doi:10.1111/j.1365-2966.2007.12275.x |
[32] |
N.S. Israel and J.W. Moffat, 2018 The Train Wreck Cluster Abell 520 and the Bullet Cluster 1E0657-558 in a Generalized Theory of Gravitation, https://doi.org/10.3390/galaxies6020041 Galaxies6 41 [1606.09128] · doi:10.3390/galaxies6020041 |
[33] |
T.M. Nieuwenhuizen, A. Morandi and M. Limousin, 2018 Modified Gravity and its test on galaxy clusters, https://doi.org/10.1093/mnras/sty380 Mon. Not. Roy. Astron. Soc.476 3393 [1802.04891] · doi:10.1093/mnras/sty380 |
[34] |
S. Boran, S. Desai, E.O. Kahya and R.P. Woodard, 2018 GW170817 Falsifies Dark Matter Emulators, https://doi.org/10.1103/PhysRevD.97.041501 Phys. Rev. D97 041501 [1710.06168] · doi:10.1103/PhysRevD.97.041501 |
[35] |
M.A. Green, J.W. Moffat and V.T. Toth, 2018 Modified Gravity (MOG), the speed of gravitational radiation and the event GW170817/GRB170817A, https://doi.org/10.1016/j.physletb.2018.03.015 Phys. Lett. B780 300 [1710.11177] · Zbl 1390.83280 · doi:10.1016/j.physletb.2018.03.015 |
[36] |
Supernova Search Team collaboration, 1998 The High Z supernova search: Measuring cosmic deceleration and global curvature of the universe using type-IA supernovae, https://doi.org/10.1086/306308 Astrophys. J.507 46 [astro-ph/9805200] · doi:10.1086/306308 |
[37] |
S. Tsujikawa, 2011 Dark energy: investigation and modeling, in https://doi.org/10.1007/978-90-481-8685-3_8 Astrophysics and Space Science Library370 Springer, Dordrecht The Netherlands [1004.1493] · Zbl 1213.83011 · doi:10.1007/978-90-481-8685-3_8 |
[38] |
A. De Felice and S. Tsujikawa, 2010 f(R) theories, https://doi.org/10.12942/lrr-2010-3 Living Rev. Rel.13 3 [1002.4928] · Zbl 1215.83005 · doi:10.12942/lrr-2010-3 |
[39] |
J.W. Moffat and V.T. Toth, 2009 Fundamental parameter-free solutions in modified gravity, https://doi.org/10.1088/0264-9381/26/8/085002 Class. Quant. Grav.26 085002 [0712.1796] · Zbl 1161.83414 · doi:10.1088/0264-9381/26/8/085002 |
[40] |
J.W. Moffat and V.T. Toth, Modified Gravity: Cosmology without dark matter or Einstein’s cosmological constant, [0710.0364] |
[41] |
J.W. Moffat and V.T. Toth, 2013 Cosmological observations in a modified theory of gravity (MOG), https://doi.org/10.3390/galaxies1010065 Galaxies1 65 [1104.2957] · doi:10.3390/galaxies1010065 |
[42] |
V.T. Toth, Cosmological consequences of Modified Gravity (MOG), in proceedings of the International Conference on Two Cosmological Models, Mexico City, Mexico, 17-19 November 2010, [1011.5174] |
[43] |
S. Jamali and M. Roshan, 2016 The phase space analysis of modified gravity (MOG), https://doi.org/10.1140/epjc/s10052-016-4336-x Eur. Phys. J. C76 490 [1608.06251] · doi:10.1140/epjc/s10052-016-4336-x |
[44] |
S. Jamali, M. Roshan and L. Amendola, 2020 Linear cosmological perturbations in Scalar-tensor-vector gravity, https://doi.org/10.1016/j.physletb.2020.135238 Phys. Lett. B802 135238 [1811.04445] · Zbl 1435.83129 · doi:10.1016/j.physletb.2020.135238 |
[45] |
R. Jimenez and A. Loeb, 2002 Constraining cosmological parameters based on relative galaxy ages, https://doi.org/10.1086/340549 Astrophys. J.573 37 [astro-ph/0106145] · doi:10.1086/340549 |
[46] |
J. Simon, L. Verde and R. Jimenez, 2005 Constraints on the redshift dependence of the dark energy potential, https://doi.org/10.1103/PhysRevD.71.123001 Phys. Rev. D71 123001 [astro-ph/0412269] · doi:10.1103/PhysRevD.71.123001 |
[47] |
R.G. Abraham et al., 2004 The Gemini Deep Deep Survey. 1. Introduction to the survey, catalogs and composite spectra, https://doi.org/10.1086/383557 Astron. J.127 2455 [astro-ph/0402436] · doi:10.1086/383557 |
[48] |
J. Dunlop et al., 1996 A 3.5-Gyr-old galaxy at redshift 1.55, https://doi.org/10.1038/381581a0 Nature381 581 · doi:10.1038/381581a0 |
[49] |
L.A. Nolan, J.S. Dunlop, R. Jimenez and A.F. Heavens, 2003 F stars, metallicity and the ages of red galaxies at z > 1, https://doi.org/10.1046/j.1365-8711.2003.06398.x Mon. Not. Roy. Astron. Soc.341 464 [astro-ph/0103450] · doi:10.1046/j.1365-8711.2003.06398.x |
[50] |
H. Spinrad et al., 1997 LBDS 53W091: an old, red galaxy at z=1.552, https://doi.org/10.1086/304381 Astrophys. J.484 581 [astro-ph/9702233] · doi:10.1086/304381 |
[51] |
T. Treu, M. Stiavelli, S. Casertano, P. Moller and G. Bertin, 1999 The properties of field elliptical galaxies at intermediate redshift. I: empirical scaling laws, https://doi.org/10.1046/j.1365-8711.1999.02794.x Mon. Not. Roy. Astron. Soc.308 1037 [astro-ph/9904327] · doi:10.1046/j.1365-8711.1999.02794.x |
[52] |
T. Treu, M. Stiavelli, P. Moller, S. Casertano and G. Bertin, 2001 The properties of field elliptical galaxies at intermediate redshift. 2. Photometry and spectroscopy of an HST selected sample, https://doi.org/10.1046/j.1365-8711.2001.04593.x Mon. Not. Roy. Astron. Soc.326 221 [astro-ph/0104177] · doi:10.1046/j.1365-8711.2001.04593.x |
[53] |
T. Treu, M. Stiavelli, S. Casertano, P. Moller and G. Bertin, 2002 The evolution of field early-type galaxies to z∼ 0.7, https://doi.org/10.1086/338790 Astrophys. J. Lett.564L13 [astro-ph/0111504] · doi:10.1086/338790 |
[54] |
D. Stern, R. Jimenez, L. Verde, M. Kamionkowski and S. Stanford, 2010 Cosmic Chronometers: Constraining the Equation of State of Dark Energy. I: H(z) Measurements J. Cosmol. Astropart. Phys.2010 02 008 [0907.3149] |
[55] |
D. Stern et al., 2001 First results from the spices survey, in https://doi.org/10.1007/10854354_14 Deep Fields, proceedings of the ESO Workshop, Garching, Germany, 9-12 October 2000, S. Cristiani, A. Renzini and R.E. Williams eds., Springer , pp. 76-80 [astro-ph/0012146] · doi:10.1007/10854354_14 |
[56] |
O. Le Fèvre et al., 2005 First epoch VVDS-deep survey: 11 564 spectra with 17.5 ≤ I_AB ≤ 24 and the redshift distribution over 0 ≤ z ≤ 5, https://doi.org/10.1051/0004-6361:20041960 Astron. Astrophys.439 845 [astro-ph/0409133] · doi:10.1051/0004-6361:20041960 |
[57] |
M. Moresco et al., 2012 Improved constraints on the expansion rate of the Universe up to z∼ 1.1 from the spectroscopic evolution of cosmic chronometers J. Cosmol. Astropart. Phys.2012 08 006 [1201.3609] |
[58] |
A. Cimatti et al., 2002 The K 20 survey. 4. The Redshift distribution of K_s < 20 galaxies: A Test of galaxy formation models, https://doi.org/10.1051/0004-6361:20021012 Astron. Astrophys.391 L1 [astro-ph/0207191] · doi:10.1051/0004-6361:20021012 |
[59] |
R. Demarco et al., 2010 Star Formation Histories in a Cluster Environment at z∼ 0.84, https://doi.org/10.1088/0004-637X/725/1/1252 Astrophys. J.725 1252 [1009.3986] · doi:10.1088/0004-637X/725/1/1252 |
[60] |
SDSS collaboration, 2001 Spectroscopic target selection for the Sloan Digital Sky Survey: The Luminous red galaxy sample, https://doi.org/10.1086/323717 Astron. J.122 2267 [astro-ph/0108153] · doi:10.1086/323717 |
[61] |
D. Le Borgne et al., 2006 Gemini Deep Deep Survey. 6. Massive post-starburst galaxies at z=1, https://doi.org/10.1086/500005 Astrophys. J.642 48 [astro-ph/0503401] · doi:10.1086/500005 |
[62] |
S.J. Lilly et al., 2009 The zCOSMOS 10 k-Bright Spectroscopic Sample, https://doi.org/10.1088/0067-0049/184/2/218 Astrophys. J. Suppl. Ser.184 218 · doi:10.1088/0067-0049/184/2/218 |
[63] |
M. Onodera et al., 2010 A z=1.82 Analog of Local Ultra-massive Elliptical Galaxies, https://doi.org/10.1088/2041-8205/715/1/L6 Astrophys. J. Lett.715 L6 [1004.2120] · doi:10.1088/2041-8205/715/1/L6 |
[64] |
P. Rosati et al., 2009 Multi-wavelength study of XMMU J2235.3-2557: the most massive galaxy cluster at z > 1, https://doi.org/10.1051/0004-6361/200913099 Astron. Astrophys.508 583 [0910.1716] · doi:10.1051/0004-6361/200913099 |
[65] |
SDSS collaboration, 2002 Spectroscopic Target Selection in the Sloan Digital Sky Survey: The Main Galaxy Sample, https://doi.org/10.1086/342343 Astron. J.124 1810 [astro-ph/0206225] · doi:10.1086/342343 |
[66] |
GOODS collaboration, 2008 The Great Observatories Origins Deep Survey. VLT/FORS2 Spectroscopy in the GOODS-South Field. 3, https://doi.org/10.1051/0004-6361:20078332 Astron. Astrophys.478 83 [0711.0850] · doi:10.1051/0004-6361:20078332 |
[67] |
C. Zhang, H. Zhang, S. Yuan, T.-J. Zhang and Y.-C. Sun, 2014 Four new observational H(z) data from luminous red galaxies in the Sloan Digital Sky Survey data release seven, https://doi.org/10.1088/1674-4527/14/10/002 Res. Astron. Astrophys.14 1221 [1207.4541] · doi:10.1088/1674-4527/14/10/002 |
[68] |
SDSS collaboration, 2009 The Seventh Data Release of the Sloan Digital Sky Survey, https://doi.org/10.1088/0067-0049/182/2/543 Astrophys. J. Suppl.182 543 [0812.0649] · doi:10.1088/0067-0049/182/2/543 |
[69] |
M. Moresco, 2015 Raising the bar: new constraints on the Hubble parameter with cosmic chronometers at z ∼ 2, https://doi.org/10.1093/mnrasl/slv037 Mon. Not. Roy. Astron. Soc.450 L16 [1503.01116] · doi:10.1093/mnrasl/slv037 |
[70] |
R. Gobat et al., 2013 WFC3 GRISM Confirmation of the Distant Cluster Cl J1449+0856 at ⟨ z ⟩ = 2.00: Quiescent and Star-forming Galaxy Populations, https://doi.org/10.1088/0004-637X/776/1/9 Astrophys. J.776 9 [1305.3576] · doi:10.1088/0004-637X/776/1/9 |
[71] |
M. Kriek et al., 2009 An ultra-deep near-infrared spectrum of a compact quiescent galaxy at z=2.2, https://doi.org/10.1088/0004-637X/700/1/221 Astrophys. J.700 221 [0905.1692] · doi:10.1088/0004-637X/700/1/221 |
[72] |
J.-K. Krogager, A.W. Zirm, S. Toft, A. Man and G. Brammer, 2014 A spectroscopic sample of massive, quiescent z ∼ 2 galaxies: Implications for the evolution of the mass-size relation, https://doi.org/10.1088/0004-637X/797/1/17 Astrophys. J.797 17 [1309.6316] · doi:10.1088/0004-637X/797/1/17 |
[73] |
M. Onodera et al., 2012 Deep near-infrared spectroscopy of passively evolving galaxies at z > 1.4, https://doi.org/10.1088/0004-637X/755/1/26 Astrophys. J.755 26 [1206.1540] · doi:10.1088/0004-637X/755/1/26 |
[74] |
P. Saracco et al., 2005 The Density of very massive evolved galaxies to z ∼ 1.7, https://doi.org/10.1111/j.1745-3933.2005.00014.x Mon. Not. Roy. Astron. Soc. Lett.357 L40 [astro-ph/0412020] · doi:10.1111/j.1745-3933.2005.00014.x |
[75] |
M. Moresco et al., 2016 A 6 evidence of the epoch of cosmic re-acceleration J. Cosmol. Astropart. Phys.2016 05 014 [1601.01701] |
[76] |
BOSS collaboration, 2013 The Baryon Oscillation Spectroscopic Survey of SDSS-III, https://doi.org/10.1088/0004-6256/145/1/10 Astron. J.145 10 [1208.0022] · doi:10.1088/0004-6256/145/1/10 |
[77] |
SDSS collaboration, 2011 SDSS-III: Massive Spectroscopic Surveys of the Distant Universe, the Milky Way Galaxy and Extra-Solar Planetary Systems, https://doi.org/10.1088/0004-6256/142/3/72 Astron. J.142 72 [1101.1529] · doi:10.1088/0004-6256/142/3/72 |
[78] |
F. Beutler et al., 2011 The 6dF Galaxy Survey: Baryon Acoustic Oscillations and the Local Hubble Constant, https://doi.org/10.1111/j.1365-2966.2011.19250.x Mon. Not. Roy. Astron. Soc.416 3017 [1106.3366] · doi:10.1111/j.1365-2966.2011.19250.x |
[79] |
E.A. Kazin et al., 2014 The WiggleZ Dark Energy Survey: improved distance measurements to z = 1 with reconstruction of the baryonic acoustic feature, https://doi.org/10.1093/mnras/stu778 Mon. Not. Roy. Astron. Soc.441 3524 [1401.0358] · doi:10.1093/mnras/stu778 |
[80] |
M. Ata et al., 2018 The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: first measurement of baryon acoustic oscillations between redshift 0.8 and 2.2, https://doi.org/10.1093/mnras/stx2630 Mon. Not. Roy. Astron. Soc.473 4773 [1705.06373] · doi:10.1093/mnras/stx2630 |
[81] |
J.E. Bautista et al., 2017 Measurement of baryon acoustic oscillation correlations at z=2.3 with SDSS DR12 Lyα-Forests, https://doi.org/10.1051/0004-6361/201730533 Astron. Astrophys.603 A12 [1702.00176] · doi:10.1051/0004-6361/201730533 |
[82] |
H. du Mas des Bourboux et al., 2017 Baryon acoustic oscillations from the complete SDSS-III Lyα-quasar cross-correlation function at z=2.4, https://doi.org/10.1051/0004-6361/201731731 Astron. Astrophys.608 A130 [1708.02225] · doi:10.1051/0004-6361/201731731 |
[83] |
A.G. Riess et al., 2018 New Parallaxes of Galactic Cepheids from Spatially Scanning the Hubble Space Telescope: Implications for the Hubble Constant, https://doi.org/10.3847/1538-4357/aaadb7 Astrophys. J.855 136 [1801.01120] · doi:10.3847/1538-4357/aaadb7 |