| A correlation between the cosmic microwave background and large-scale structure in the Universe S Boughn, R Crittenden Nature 427 (6969), 45-47, 2004 | 484 | 2004 |
| Combined analysis of the integrated Sachs-Wolfe effect and cosmological implications T Giannantonio, R Scranton, RG Crittenden, RC Nichol, SP Boughn, ... Physical Review D 77 (12), 123520, 2008 | 401 | 2008 |
| Can gravitons be detected? T Rothman, S Boughn Foundations of Physics 36, 1801-1825, 2006 | 204 | 2006 |
| Diffuse light in dense clusters of galaxies. I-R-band observations of Abell 2029 JM Uson, SP Boughn, JR Kuhn Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 369, March 1, 1991, p …, 1991 | 149 | 1991 |
| Dipole and quadrupole anisotropy of the 2.7 K radiation SP Boughn, ES Cheng, DT WILKINsoN Astrophysical Journal, Part 2-Letters to the Editor, vol. 243, Feb. 1, 1981 …, 1981 | 145 | 1981 |
| Galactic emission at 19 GHz A de Oliveira-Costa, M Tegmark, LA Page, SP Boughn The Astrophysical Journal 509 (1), L9, 1998 | 108 | 1998 |
| Cross correlation of the cosmic microwave background with radio sources: constraints on an accelerating universe SP Boughn, RG Crittenden Physical Review Letters 88 (2), 021302, 2001 | 99 | 2001 |
| Correlations between the cosmic X-ray and microwave backgrounds: constraints on a cosmological constant SP Boughn, RG Crittenden, NG Turok arXiv preprint astro-ph/9704043, 1997 | 96 | 1997 |
| Making sense of Bell’s theorem and quantum nonlocality S Boughn Foundations of Physics 47 (5), 640-657, 2017 | 71 | 2017 |
| Observations with a low-temperature, resonant mass, gravitational radiation detector SP Boughn, WM Fairbank, ER Mapoles, MS McAshan, PF Michelson, ... Astrophysical Journal, Part 2-Letters to the Editor, vol. 261, Oct. 1, 1982 …, 1982 | 71 | 1982 |
| Aspects of graviton detection: graviton emission and absorption by atomic hydrogen S Boughn, T Rothman Classical and quantum gravity 23 (20), 5839, 2006 | 70 | 2006 |
| A detection of the integrated Sachs–Wolfe effect SP Boughn, RG Crittenden New Astronomy Reviews 49 (2-6), 75-78, 2005 | 67 | 2005 |
| Radio/X-Ray Luminosity Relation for Advection-dominated Accretion: Implications for Emission-Line Galaxies and the X-Ray Background I Yi, SP Boughn The Astrophysical Journal 499 (1), 198, 1998 | 56 | 1998 |
| The case of the identically accelerated twins SP Boughn Am. J. Phys 57 (9), 791-793, 1989 | 51 | 1989 |
| Limits of Gaussian fluctuations in the cosmic microwave background at 19.2 GHz SP Boughn, ES Cheng, DA Cottingham, DJ Fixsen Astrophysical Journal, Part 2-Letters (ISSN 0004-637X), vol. 391, no. 2 …, 1992 | 50 | 1992 |
| The large-scale structure of the x-ray background and its cosmological implications SP Boughn, RG Crittenden, GP Koehrsen The Astrophysical Journal 580 (2), 672, 2002 | 46 | 2002 |
| The smoothness of the 2.2 micron background-Constraints on models of primeval galaxies SP Boughn, PR Saulson, JM Uson Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 301, Feb. 1, 1986, p …, 1986 | 46 | 1986 |
| Nonquantum gravity S Boughn Foundations of Physics 39, 331-351, 2009 | 38 | 2009 |
| A search for extragalactic background light using the dark cloud L134 SP Boughn, JR Kuhn Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 309, Oct. 1, 1986, p …, 1986 | 36 | 1986 |
| The central galaxy in Abell 2029: an old supergiant JM Uson, SP Boughn, JR Kuhn Science 250 (4980), 539-540, 1990 | 34 | 1990 |
