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pro vyhledávání: '"Bond N"'
Autor:
Boada, Steven, Tilvi, V., Papovich, C., Quadri, R. F., Hilton, M., Finkelstein, S., Guo, Yicheng, Bond, N., Conselice, C., Dekel, A., Ferguson, H., Giavalisco, M., Grogin, N. A., Kocevski, D. D., Koekemoer, A. M., Koo, D. C.
We use data from the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey to study how the spatial variation in the stellar populations of galaxies relate to the formation of galaxies at $1.5 < z < 3.5$. We use the Internal Color Dispersion
Externí odkaz:
http://arxiv.org/abs/1503.00722
Akademický článek
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Autor:
Fleuren, S., Sutherland, W., Dunne, L., Smith, D. J. B., Maddox, S. J., González-Nuevo, J., Findlay, J., Auld, R., Baes, M., Bond, N. A., Bonfield, D. G., Bourne, N., Cooray, A., Buttiglione, S., Cava, A., Dariush, A., De Zotti, G., Driver, S. P., Dye, S., Eales, S., Fritz, J., Gunawardhana, M. L. P., Hopwood, R., Ibar, E., Ivison, R. J., Jarvis, M. J., Kelvin, L., Lapi, A., Liske, J., Michalowski, M. J., Negrello, M., Pascale, E., Pohlen, M., Prescott, M., Rigby, E. E., Robotham, A., Scott, D., Temi, P., Thompson, M. A., Valiante, E., van der Werf, P.
We identify near-infrared Ks band counterparts to Herschel-ATLAS sub-mm sources, using a preliminary object catalogue from the VISTA VIKING survey. The sub-mm sources are selected from the H-ATLAS Phase 1 catalogue of the GAMA 9h field, which include
Externí odkaz:
http://arxiv.org/abs/1202.3891
We present the results of a comparative study of the rest-frame optical and rest-frame ultraviolet morphological properties of 117 star-forming galaxies (SFGs), including BX, BzK, and Lyman break galaxies with B<24.5, and 15 passive galaxies in the r
Externí odkaz:
http://arxiv.org/abs/1010.1525
Lyman-Alpha-Emitting Galaxies at z = 2.1 in ECDF-S: Building Blocks of Typical Present-day Galaxies?
Autor:
Guaita, L., Gawiser, E., Padilla, N., Francke, H., Bond, N. A., Gronwall, C., Ciardullo, R., Feldmeier, J. J., Sinawa, S., Blanc, G. A., Virani, S.
Publikováno v:
Astrophys.J.714:255-269,2010
We discovered a sample of 250 Ly-Alpha emitting (LAE) galaxies at z=2.1 in an ultra-deep 3727 A narrow-band MUSYC image of the Extended Chandra Deep Field-South. LAEs were selected to have rest-frame equivalent widths (EW) > 20 A and emission line fl
Externí odkaz:
http://arxiv.org/abs/0910.2244
Publikováno v:
Astrophys.J.716:1-29,2010
We study Milky Way kinematics using a sample of 18.8 million main-sequence stars with r<20 and proper-motion measurements derived from SDSS and POSS astrometry, including ~170,000 stars with radial-velocity measurements from the SDSS spectroscopic su
Externí odkaz:
http://arxiv.org/abs/0909.0013
Publikováno v:
Astrophys.J.705:639-649,2009
We present a rest-frame ultraviolet analysis of ~120 z~3.1 Lyman Alpha Emitters (LAEs) in the Extended Chandra Deep Field South (ECDF-S). Using Hubble Space Telescope (HST) images taken as part of the Galaxy Evolution From Morphology and SEDS (GEMS)
Externí odkaz:
http://arxiv.org/abs/0907.2235
Autor:
Ivezic, Z., Bond, N., Juric, M., Munn, J. A., Lupton, R. H., Pier, J. R., Hennessy, G. S., Knapp, G. R., Gunn, J. E., Rockosi, C. M., Quinn, T.
Publikováno v:
2005, ASP Conf. Series, Vol. 338, p.201
We discuss several results made possible by accurate SDSS astrometric measurements in a large sky area, with emphasis on asteroids and stellar proper motions obtained by comparing POSS and SDSS. SDSS has observed over 200,000 moving objects in five p
Externí odkaz:
http://arxiv.org/abs/astro-ph/0701502
Autor:
Ivezic, Z., Schlegel, D., Uomoto, A., Bond, N., Beers, T., Prieto, C. Allende, Wilhelm, R., Lee, Y. Sun, Sivarani, T., Juric, M., Lupton, R., Rockosi, C., Knapp, G., Gunn, J., Yanny, B., Jester, S., Kent, S., Pier, J., Munn, J., Richards, G., Newberg, H., Blanton, M., Eisenstein, D., Hawley, S., Anderson, S., Harris, H., Kiuchi, F., Chen, A., Bushong, J., Sohi, H., Haggard, D., Kimball, A., Barentine, J., Brewington, H., Harvanek, M., Kleinman, S., Krzesinski, J., Long, D., Nitta, A., Snedden, S.
Publikováno v:
Mem.Soc.Ast.It.77:1057,2006
In addition to optical photometry of unprecedented quality, the Sloan Digital Sky Survey (SDSS) is also producing a massive spectroscopic database. We discuss determination of stellar parameters, such as effective temperature, gravity and metallicity
Externí odkaz:
http://arxiv.org/abs/astro-ph/0701509
Autor:
Ivezic, Z., Smith, J. A., Miknaitis, G., Lin, H., Tucker, D., Lupton, R., Knapp, G., Gunn, J., Strauss, M., Holtzman, J., Kent, S., Yanny, B., Schlegel, D., Finkbeiner, D., Padmanabhan, N., Rockosi, C., Juric, M., Bond, N., Lee, B., Jester, S., Harris, H., Harding, P., Brinkmann, J., York, D.
Publikováno v:
ASP Conf.Ser.364:165,2007
We compare Stetson's photometric standards with measurements listed in a standard star catalog constructed using repeated SDSS imaging observations. The SDSS catalog includes over 700,000 candidate standard stars from the equatorial stripe 82 (|Dec|<
Externí odkaz:
http://arxiv.org/abs/astro-ph/0701508