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63 results on '"Riebel, D."'

51. Big Bear Bakery

Author

Riebel, D and Riebel, D

Abstract

3 story $34,000 building originally built by D.W. McGrath for the Clarke Baking Co

Published
1919

53. Miller House

Author

Miller, William A, RIEBEL D AND SONS, Miller, William A, and RIEBEL D AND SONS

Abstract

located on the site of the Hare Orphan's Home; Ohio State Journal 1/30/1867 p.5; Ohio State Journal 2/14/1867 p.5; Ohio State Journal 6/6/1867 p.5. The building permit printed 6/23/1907 later Glenmont Home for Christian Scientists; Columbus Dispatch 5/10/1942 p.C-3 Columbus Press Post 6/23/1907 p.8 photo; Columbus Dispatch 10/4/1908 p.1 (sect.2); 1/17/1909 p. 4 (Local) Photo; Columbus Dispatch, 9/18/1988, page I-1; Columbus Neighborhoods, R 977.13 C72 B565c, page 167

Published
1908

56. St John the Baptist Church

Author

Marrapese, Casto, RIEBEL D, Marrapese, Casto, and RIEBEL D

Abstract

Late Gothic Revival style. Sisters of the Sick Poor Convent to be demolished; Columbus Dispatch 10/5/1996 p.h-10. church seating for 480. The Italian Cultural Center was built next door in 1989.

Published
1898

57. Lane Avenue Elementary

Author

Riebel, D and Riebel, D

Abstract

Lane Avenue Elementary was known as Lisle Avenue Elementary when it was built in 1911. It was closed c1937 and OSU bought it on 1/26/1940 and has used it for storage

Published
1922

58. Constraints on Λ CDM extensions from the SPT-3G 2018 E E and T E power spectra

Author

Balkenhol, L., Dutcher, D., Ade, P. A. R., Ahmed, Z., Anderes, E., Anderson, A. J., Archipley, M., Avva, J. S., Aylor, K., Barry, P. S., Basu Thakur, R., Benabed, K., Bender, A. N., Benson, B. A., Bianchini, F., Bleem, L. E., Bouchet, F. R., Bryant, L., Byrum, K., Carlstrom, J. E., Carter, F. W., Cecil, T. W., Chang, C. L., Chaubal, P., Chen, G., Cho, H.-M., Chou, T.-L., Cliche, J.-F., Crawford, T. M., Cukierman, A., Daley, C., de Haan, T., Denison, E. V., Dibert, K., Ding, J., Dobbs, M. A., Everett, W., Feng, C., Ferguson, K. R., Foster, A., Fu, J., Galli, S., Gambrel, A. E., Gardner, R. W., Goeckner-Wald, N., Gualtieri, R., Guns, S., Gupta, N., Guyser, R., Halverson, N. W., Harke-Hosemann, A. H., Harrington, N. L., Henning, J. W., Hilton, G. C., Hivon, E., Holder, G. P., Holzapfel, W. L., Hood, J. C., Howe, D., Huang, N., Irwin, K. D., Jeong, O. B., Jonas, M., Jones, A., Khaire, T. S., Knox, L., Kofman, A. M., Korman, M., Kubik, D. L., Kuhlmann, S., Kuo, C.-L., Lee, A. T., Leitch, E. M., Lowitz, A. E., Lu, C., Meyer, S. S., Michalik, D., Millea, M., Montgomery, J., Nadolski, A., Natoli, T., Nguyen, H., Noble, G. I., Novosad, V., Omori, Y., Padin, S., Pan, Z., Paschos, P., Pearson, J., Posada, C. M., Prabhu, K., Quan, W., Rahlin, A., Reichardt, C. L., Riebel, D., Riedel, B., Rouble, M., Ruhl, J. E., Sayre, J. T., Schiappucci, E., Shirokoff, E., Smecher, G., Sobrin, J. A., Stark, A. A., Stephen, J., Story, K. T., Suzuki, A., Thompson, K. L., Thorne, B., Tucker, C., Umilta, C., Vale, L. R., Vanderlinde, K., Vieira, J. D., Wang, G., Whitehorn, N., Wu, W. L. K., Yefremenko, V., Yoon, K. W., and Young, M. R.

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60. Oxygen-rich dust production in IC 10

Author

Lebouteiller, V., Sloan, G. C., Groenewegen, M. A. T., Matsuura, M., Riebel, D., Whelan, D. G., Bernard-Salas, J., Massey, P., Bayet, E., Lebouteiller, V., Sloan, G. C., Groenewegen, M. A. T., Matsuura, M., Riebel, D., Whelan, D. G., Bernard-Salas, J., Massey, P., and Bayet, E.

Abstract

Context We report the detection of oxygen-rich circumstellar envelopes in stars of the nearby (700 kpc) starburst galaxy IC 10. The star formation history and the chemical environment of this galaxy makes it an ideal target to observe dust production by high-mass stars in a low-metallicity environment. Aims The goal of this study is to identify oxygen-rich stars in IC 10 and to constrain their nature between asymptotic giant branch stars (AGBs), red supergiants (RSGs), and other infrared bright sources. We examine the mass-loss rate of the stars and compare to results obtained for the Magellanic Clouds. Our objectives are to (1) assess whether RSGs can be significant dust producers in IC 10, and (2), solve the discrepancy between the star formation history of IC 10 and the relatively low number of RSGs detected in the optical. Methods We search for silicate dust in emission by using the spectral map observed with the Infrared Spectrograph on board the Spitzer Space Telescope. The optical (UBVRI) and infrared (JHK, Spitzer/IRAC and Spitzer/MIPS) photometry is used to assert the membership of the stars to IC 10 and disentangle between AGBs and RSGs. Radiative models are used to infer mass-loss rates and stellar luminosities. Results The luminosity and colors of at least 9 silicate emission sources are consistent with stars within IC 10. Furthermore, the photometry of 2 of these sources is consistent with RSGs. We derive dust mass-loss rates similar to the values found in the Magellanic Clouds. Accounting for the sample completeness, RSGs are not important contributors to the dust mass budget in IC 10.

61. Particle physics with the cosmic microwave background with SPT-3G

Author

Avva, S. J., Ade, P.A.R, Ahmed, Z, Anderson, A.J, Aylor, K, Basu Thakur, B, Bender, A.N, Benson, B.A, Bleem, L.E, Bocquet, S, Bryant, L, Carlstrom, J.E, Carter, F.W, Cecil, T.W, Chang, C.L, Crawford, T.M, Cukierman, A, de Haan, T, Ding, J, Dobbs, M.A, Dodelson, S, Dutcher, D, Everett, W, Ferguson, K.R, Foster, A, Gallicchio, J, Gambrel, A.E, Gardner, R.W, Groh, J.C, Guns, S, Halverson, N.W, Harke-Hosemann, A.H, Harrington, N.L, Henning, J.W, Holder, G.P, Holzapfel, W.L, Howe, D, Huang, N, Irwin, K.D, Jeong, O.B, Jonas, M, Jones, A, Khaire, T.S, Knox, L, Kofman, A.M, Korman, M, Kubik, D.L, Kuhlmann, S, Kuo, C.-L, Lee, A.T, Lowitz, A.E, Meyer, S.S, Michalik, D, Montgomery, J, Nadolski, A, Natoli, T, Nguyen, H, Noble, G.I, Novosad, V, Padin, S, Pan, Z, Paschos, P, Pearson, J, Posada, C.M, Quan, W, Raghunathan, S, Rahlin, A, Reichardt, C.L, Riebel, D, Ruhl, J.E, Sayre, J.T, Shirokoff, E, Smecher, G, Sobrin, J.A, Stark, A.A, Stephen, J, Story, K.T, Suzuki, A, Thompson, K.L, Tucker, C, Vanderlinde, K, Viera, J.D, Wang, G, Whitehorn, N, Wu, W.L.K, Yefremenko, V, Yoon, K.W, Young, M.R, Avva, S. J., Ade, P.A.R, Ahmed, Z, Anderson, A.J, Aylor, K, Basu Thakur, B, Bender, A.N, Benson, B.A, Bleem, L.E, Bocquet, S, Bryant, L, Carlstrom, J.E, Carter, F.W, Cecil, T.W, Chang, C.L, Crawford, T.M, Cukierman, A, de Haan, T, Ding, J, Dobbs, M.A, Dodelson, S, Dutcher, D, Everett, W, Ferguson, K.R, Foster, A, Gallicchio, J, Gambrel, A.E, Gardner, R.W, Groh, J.C, Guns, S, Halverson, N.W, Harke-Hosemann, A.H, Harrington, N.L, Henning, J.W, Holder, G.P, Holzapfel, W.L, Howe, D, Huang, N, Irwin, K.D, Jeong, O.B, Jonas, M, Jones, A, Khaire, T.S, Knox, L, Kofman, A.M, Korman, M, Kubik, D.L, Kuhlmann, S, Kuo, C.-L, Lee, A.T, Lowitz, A.E, Meyer, S.S, Michalik, D, Montgomery, J, Nadolski, A, Natoli, T, Nguyen, H, Noble, G.I, Novosad, V, Padin, S, Pan, Z, Paschos, P, Pearson, J, Posada, C.M, Quan, W, Raghunathan, S, Rahlin, A, Reichardt, C.L, Riebel, D, Ruhl, J.E, Sayre, J.T, Shirokoff, E, Smecher, G, Sobrin, J.A, Stark, A.A, Stephen, J, Story, K.T, Suzuki, A, Thompson, K.L, Tucker, C, Vanderlinde, K, Viera, J.D, Wang, G, Whitehorn, N, Wu, W.L.K, Yefremenko, V, Yoon, K.W, and Young, M.R

Abstract

The cosmic microwave background (CMB) encodes information about the content and evolution of the universe. The presence of light, weakly interacting particles impacts the expansion history of the early universe, which alters the temperature and polarization anisotropies of the CMB. In this way, current measurements of the CMB place interesting constraints on the neutrino energy density and mass, as well as on the abundance of other possible light relativistic particle species. We present the status of an on-going 1500 sq. deg. survey with the SPT-3G receiver, a new mm-wavelength camera on the 10-m diameter South Pole Telescope (SPT). The SPT-3G camera consists of 16,000 superconducting transition edge sensors, a 10x increase over the previous generation camera, which allows it to map the CMB with an unprecedented combination of sensitivity and angular resolution. We highlight projected constraints on the abundance of sterile neutrinos and the sum of the neutrino masses for the SPT-3G survey, which could help determine the neutrino mass hierarchy....

63. Comparison between the reactivities of fresh, preserved at 4 degrees C and cryopreserved abdominal aortae of the rabbit.

Author

Skowron O, Descotes JL, Stanke F, Baudot A, Riebel D, Bessard G, Egelhoffer H, Mazuer J, and Odin J

Subjects
Acetylcholine pharmacology, Animals, Cold Temperature, Cryoprotective Agents, Endothelium, Vascular physiology, Male, Muscle Contraction drug effects, Organ Preservation Solutions, Rabbits, Aorta, Abdominal drug effects, Aorta, Abdominal physiology, Cryopreservation methods, Muscle Contraction physiology, Muscle, Smooth, Vascular drug effects, Muscle, Smooth, Vascular physiology, Organ Preservation methods
Published
1998
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