Zobrazeno 1 - 10
of 192
pro vyhledávání: '"Woody, D"'
Autor:
Chung, D. T., Breysse, P. C., Cleary, K. A., Dunne, D. A., Lunde, J. G. S., Padmanabhan, H., Stutzer, N. -O., Tolgay, D., Bond, J. R., Church, S. E., Eriksen, H. K., Gaier, T., Gundersen, J. O., Harper, S. E., Harris, A. I., Hobbs, R., Ihle, H. T., Kim, J., Lamb, J. W., Lawrence, C. R., Murray, N., Pearson, T. J., Philip, L., Readhead, A. C. S., Rennie, T. J., Wehus, I. K., Woody, D. P.
The Carbon monOxide Mapping Array Project (COMAP) Pathfinder survey continues to demonstrate the feasibility of line-intensity mapping using high-redshift carbon monoxide (CO) line emission traced at cosmological scales. The latest COMAP Pathfinder p
Externí odkaz:
http://arxiv.org/abs/2406.07512
Autor:
Stutzer, N. -O., Lunde, J. G. S., Breysse, P. C., Chung, D. T., Cleary, K. A., Dunne, D. A., Eriksen, H. K., Ihle, H. T., Padmanabhan, H., Tolgay, D., Wehus, I. K., Bond, J. R., Church, S. E., Gaier, T., Gundersen, J. O., Harris, A. I., Harper, S. E., Hobbs, R., Kim, J., Lamb, J. W., Lawrence, C. R., Murray, N., Pearson, T. J., Philip, L., Readhead, A. C. S., Rennie, T. J., Woody, D. P.
We present updated constraints on the cosmological 3D power spectrum of carbon monoxide CO(1-0) emission in the redshift range $2.4$-$3.4$. The constraints are derived from the two first seasons of Carbon monOxide Mapping Array Project (COMAP) Pathfi
Externí odkaz:
http://arxiv.org/abs/2406.07511
Autor:
Lunde, J. G. S., Stutzer, N. -O., Breysse, P. C., Chung, D. T., Cleary, K. A., Dunne, D. A., Eriksen, H. K., Harper, S. E., Ihle, H. T., Lamb, J. W., Pearson, T. J., Philip, L., Wehus, I. K., Woody, D. P., Bond, J. R., Church, S. E., Gaier, T., Gundersen, J. O., Harris, A. I., Hobbs, R., Kim, J., Lawrence, C. R., Murray, N., Padmanabhan, H., Readhead, A. C. S., Rennie, T. J., Tolgay, D.
The CO Mapping Array Project (COMAP) Pathfinder is performing line intensity mapping of CO emission to trace the distribution of unresolved galaxies at redshift $z \sim 3$. We present an improved version of the COMAP data processing pipeline and appl
Externí odkaz:
http://arxiv.org/abs/2406.07510
Autor:
Law, C. J., Sharma, K., Ravi, V., Chen, G., Catha, M., Connor, L., Faber, J. T., Hallinan, G., Harnach, C., Hellbourg, G., Hobbs, R., Hodge, D., Hodges, M., Lamb, J. W., Rasmussen, P., Sherman, M. B., Shi, J., Simard, D., Squillace, R., Weinreb, S., Woody, D. P., Yadlapalli, N.
Fast Radio Bursts (FRBs) are a powerful and mysterious new class of transient that are luminous enough to be detected at cosmological distances. By associating FRBs to host galaxies, we can measure intrinsic and environmental properties that test FRB
Externí odkaz:
http://arxiv.org/abs/2307.03344
Autor:
Hallinan, G., Ravi, V., Weinreb, S., Kocz, J., Huang, Y., Woody, D. P., Lamb, J., D'Addario, L., Catha, M., Shi, J., Law, C., Kulkarni, S. R., Phinney, E. S., Eastwood, M. W., Bouman, K. L., McLaughlin, M. A., Ransom, S. M., Siemens, X., Cordes, J. M., Lynch, R. S., Kaplan, D. L., Chatterjee, S., Lazio, J., Brazier, A., Bhatnagar, S., Myers, S. T., Walter, F., Gaensler, B. M.
We present the DSA-2000: a world-leading radio survey telescope and multi-messenger discovery engine for the next decade. The array will be the first true radio camera, outputting science-ready image data over the 0.7 - 2 GHz frequency range with a s
Externí odkaz:
http://arxiv.org/abs/1907.07648
Autor:
Ravi, V., Catha, M., D'Addario, L., Djorgovski, S. G., Hallinan, G., Hobbs, R., Kocz, J., Kulkarni, S. R., Shi, J., Vedantham, H. K., Weinreb, S., Woody, D. P.
Intense, millisecond-duration bursts of radio waves have been detected from beyond the Milky Way [1]. Their extragalactic origins are evidenced by their large dispersion measures, which are greater than expected for propagation through the Milky Way
Externí odkaz:
http://arxiv.org/abs/1907.01542
Autor:
Kocz, J., Ravi, V., Catha, M., D'Addario, L., Hallinan, G., Hobbs, R., Kulkarni, S., Shi, J., Vedantham, H., Weinreb, S., Woody, D.
The Deep Synoptic Array 10 dish prototype is an instrument designed to detect and localise fast radio bursts with arcsecond accuracy in real time. Deployed at Owens Valley Radio Observatory, it consists of ten 4.5m diameter dishes, equipped with a 25
Externí odkaz:
http://arxiv.org/abs/1906.08699
Autor:
Price, D. C., Greenhill, L. J., Fialkov, A., Bernardi, G., Garsden, H., Barsdell, B. R., Kocz, J., Anderson, M. M., Bourke, S. A., Craig, J., Dexter, M. R., Dowell, J., Eastwood, M. W., Eftekhari, T., Ellingson, S. W., Hallinan, G., Hartman, J. M., Kimberk, R., Lazio, T. J. W., Leiker, S., MacMahon, D., Monroe, R., Schinzel, F., Taylor, G. B., Tong, E., Werthimer, D., Woody, D. P.
The Large-Aperture Experiment to Detect the Dark Age (LEDA) was designed to detect the predicted O(100)mK sky-averaged absorption of the Cosmic Microwave Background by Hydrogen in the neutral pre- and intergalactic medium just after the cosmological
Externí odkaz:
http://arxiv.org/abs/1709.09313
Autor:
Frayer, D. T., Maddalena, Ronald J., Meijer, M., Hough, L., White, S., Norrod, R., Watts, G., Stennes, M., Simon, R., Woody, D., Srikanth, S., Pospieszalski, M., Bryerton, E., Whitehead, M., Ford, P., Mello, M., Bloss, M.
We present a 67--93.6 GHz spectral line survey of Orion-KL with the new 4 mm Receiver on the Green Bank Telescope (GBT). The survey reaches unprecedented depths and covers the low-frequency end of the 3 mm atmospheric window which has been relatively
Externí odkaz:
http://arxiv.org/abs/1502.01280
Autor:
Plambeck, R. L., Bolatto, A. D., Carpenter, J. M., Eisner, J. A., Lamb, J. W., Leitch, E. M., Marrone, D. P., Muchovej, S. J., Perez, L. M., Pound, M. W., Teuben, P. J., Volgenau, N. H., Woody, D. P., Wright, M. C. H., Zauderer, B. A.
The 229 GHz (lambda 1.3mm) radio emission from Orion-KL was mapped with up to 0.14" angular resolution with CARMA, allowing measurements of the flux densities of Source I ('SrcI') and the Becklin-Neugebauer Object (BN), the 2 most massive stars in th
Externí odkaz:
http://arxiv.org/abs/1211.0085