Zobrazeno 1 - 10
of 10
pro vyhledávání: '"Gim, H. B."'
Autor:
Polletta, M., Frye, B. L., Garuda, N., Willner, S. P., Berta, S., Kneissl, R., Dole, H., Jansen, R. A., Lehnert, M. D., Cohen, S. H., Summers, J., Windhorst, R. A., D'Silva, J. C. J., Koekemoer, A. M., Coe, D., Conselice, C. J., Driver, S. P., Grogin, N. A., Marshall, M. A., Nonino, M., Ortiz III, R., Pirzkal, N., Robotham, A., Ryan, Jr., R. E., Willmer, C. N. A., Yan, H., Arumugam, V., Cheng, C., Gim, H. B., Hathi, N. P., Holwerda, B., Kamieneski, P., Keel, W. C., Li, J., Pascale, M., Rottgering, H., Smith, B. M., Yun, M. S.
Dusty star-forming galaxies (DSFGs) contribute significantly to the stellar buildup at cosmic noon. Major mergers and gas accretion are often invoked to explain DSFGs' prodigious star-formation rates (SFRs) and large stellar masses. We conducted a sp
Externí odkaz:
http://arxiv.org/abs/2405.07986
Autor:
O'Brien, Rosalia, Jansen, Rolf A., Grogin, Norman A., Cohen, Seth H., Smith, Brent M., Silver, Ross M., Maksym III, W. P., Windhorst, Rogier A., Carleton, Timothy, Koekemoer, Anton M., Hathi, Nimish P., Willmer, Christopher N. A., Frye, Brenda L., Alpaslan, M., Ashby, M. L. N., Ashcraft, T. A., Bonoli, S., Brisken, W., Cappelluti, N., Civano, F., Conselice, C. J., Dhillon, V. S., Driver, S. P., Duncan, K. J., Dupke, R., Elvis, M., Fazio, G. G., Finkelstein, S. L., Gim, H. B., Griffiths, A., Hammel, H. B., Hyun, M., Im, M., Jones, V. R., Kim, D., Ladjelate, B., Larson, R. L., Malhotra, S., Marshall, M. A., Milam, S. N., Pierel, J. D. R., Rhoads, J. E., Rodney, S. A., Röttgering, H. J. A., Rutkowski, M. J., Ryan, Jr., R. E., Ward, M. J., White, C. W., van Weeren, R. J., Zhao, X., Summers, J., D'Silva, J. C. J., Ortiz III, R., Robotham, A. S. G., Coe, D., Nonino, M., Pirzkal, N., Yan, H., Acharya, T.
The JWST North Ecliptic Pole (NEP) Time Domain Field (TDF) is a $>$14 arcmin diameter field optimized for multi-wavelength time-domain science with JWST. It has been observed across the electromagnetic spectrum both from the ground and from space, in
Externí odkaz:
http://arxiv.org/abs/2401.04944
Autor:
Willner, S. P., Gim, H. B., Polletta, M. del Carmen, Cohen, S. H., Willmer, C. N. A., Zhao, X., D'Silva, J. C. J., Jansen, R. A., Koekemoer, A. M., Summers, J., Windhorst, R. A., Coe, D., Conselice, C. J., Driver, S. P., Frye, B., Grogin, N. A., Marshall, M. A., Nonino, M., Ortiz III, R., Pirzkal, N., Robotham, A., Rutkowski, M. J., Ryan, Jr., R. E., Tompkins, S., Yan, H., Hammel, H. B., Milam, S. N., Adams, N. J., Beacom, J. F., Bhatawdekar, R., Cheng, C., Civano, F., Cotton, W., Hyun, M., Kikuta, S., Nyland, K. E., Peters, W. M., Petric, A., Röttgering, H. J. A., Shimwell, T., Yun, M. S.
The Time Domain Field (TDF) near the North Ecliptic Pole in JWST's continuous-viewing zone will become a premier "blank field" for extragalactic science. JWST/NIRCam data in a 16 arcmin$^2$ portion of the TDF identify 4.4 $\mu$m counterparts for 62 o
Externí odkaz:
http://arxiv.org/abs/2309.13008
Autor:
Dodson, R., Momjian, E., Pisano, D. J., Luber, N., Bird, J. Blue, Rozgonyi, K., Smith, E. T., van Gorkom, J. H., Lucero, D., Hess, K. M., Yun, M., Rhee, J., van der Hulst, J. M., Vinsen, K., Meyer, M., Fernandez, X., Gim, H. B., Popping, A., Wilcots, E.
Radio Astronomy is undergoing a renaissance, as the next-generation of instruments provides a massive leap forward in collecting area and therefore raw sensitivity. However, to achieve this theoretical level of sensitivity in the science data product
Externí odkaz:
http://arxiv.org/abs/2112.06488
Autor:
Bird, J. Blue, Davis, J., Luber, N., van Gorkom, J. H., Wilcots, E., Pisano, D. J., Gim, H. B., Momjian, E., Fernandez, X., Hess, K. M., Lucero, D., Dodson, R., Vinsen, K., Popping, A., Chung, A., Kreckel, K., van der Hulst, J. M., Yun, M.
We present neutral hydrogen (HI) and ionized hydrogen (H${\alpha}$) observations of ten galaxies out to a redshift of 0.1. The HI observations are from the first epoch (178 hours) of the COSMOS HI Large Extragalactic Survey (CHILES). Our sample is HI
Externí odkaz:
http://arxiv.org/abs/1912.01062
Autor:
Yun, Min S., Aretxaga, I., Gurwell, M. A., Hughes, D. H., Montaña, A., Narayanan, G., González, D. Rosa, Sánchez-Argüelles, D., Schloerb, F. P., Snell, R. L., Vega, O., Wilson, G. W., Zeballos, M., Chavez, M., Cybulski, J. R., Díaz-Santos, T., De la Luz, V., Erickson, N., Ferrusca, D., Gim, H. B., Heyer, M. H., Iono, D., Pope, A., Rogstad, S. M., Scott, K. S., Souccar, K., Terlevich, E., Terlevich, R., Wilner, D., Zavala, J. A.
Measuring redshifted CO line emission is an unambiguous method for obtaining an accurate redshift and total cold gas content of optically faint, dusty starburst systems. Here, we report the first successful spectroscopic redshift determination of AzT
Externí odkaz:
http://arxiv.org/abs/1508.05425
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
Blue Bird, J, Davis, J, Luber, N, van Gorkom, J H, Wilcots, E, Pisano, D J, Gim, H B, Momjian, E, Fernandez, X, Hess, K M, Lucero, D, Dodson, R, Vinsen, K, Popping, A, Chung, A, Kreckel, K, van der Hulst, J M, Yun, M
Publikováno v:
Monthly Notices of the Royal Astronomical Society; Feb2020, Vol. 492 Issue 1, p153-176, 24p
Autor:
Yun, Min S., Aretxaga, I., Gurwell, M. A., Hughes, D. H., Montaña, A., Narayanan, G., González, D. Rosa, Sánchez-Argüelles, D., Schloerb, F. P., Snell, R. L., Vega, O., Wilson, G. W., Zeballos, M., Chavez, M., Cybulski, R., Díaz-Santos, T., De la Luz, V., Erickson, N., Ferrusca, D., Gim, H. B.
Publikováno v:
Monthly Notices of the Royal Astronomical Society; 12/21/2015, Vol. 454 Issue 4, p3485-3499, 15p