Zobrazeno 11 - 20
of 115
pro vyhledávání: '"Schmidt, K. B."'
Autor:
Abramson, L. E., Brammer, G. B., Schmidt, K. B., Treu, T., Morishita, T., Wang, X., Vulcani, B., Henry, A.
We present a catalogue of 22755 objects with slitless, optical, Hubble Space Telescope (HST) spectroscopy from the Grism Lens-Amplified Survey from Space (GLASS). The data cover $\sim$220 sq. arcmin to 7-orbit ($\sim$10 ks) depth in 20 parallel point
Externí odkaz:
http://arxiv.org/abs/1906.00008
Autor:
Hoag, A., Treu, T., Pentericci, L., Amorin, R., Bolzonella, M., Bradač, M., Castellano, M., Cullen, F., Fynbo, J. P. U., Garilli, B., Hathi, N., Henry, A., Jones, T., Mason, C., McLeod, D., McLure, R., Morishita, T., Pozzetti, L., Schaerer, D., Schmidt, K. B., Talia, M., Thomas, R.
We constrain the distribution of spatially offset Lyman-alpha emission (Ly$\alpha$) relative to rest-frame ultraviolet emission in $\sim300$ high redshift ($3
Externí odkaz:
http://arxiv.org/abs/1905.09467
Autor:
Urrutia, T., Wisotzki, L., Kerutt, J., Schmidt, K. B., Herenz, E. C., Klar, J., Saust, R., Werhahn, M., Diener, C., Caruana, J., Krajnović, D., Bacon, R., Boogaard, L., Brinchman, J., Enke, H., Maseda, M., Nanayakkara, T., Richard, J., Steinmetz, M., Weilbacher, P. M.
Publikováno v:
A&A 624, A141 (2019)
We present the MUSE-Wide survey, a blind, 3D spectroscopic survey in the CANDELS/GOODS-S and CANDELS/COSMOS regions. Each MUSE-Wide pointing has a depth of 1 hour and hence targets more extreme and more luminous objects over 10 times the area of the
Externí odkaz:
http://arxiv.org/abs/1811.06549
Autor:
Wisotzki, L., Bacon, R., Brinchmann, J., Cantalupo, S., Richter, P., Schaye, J., Schmidt, K. B., Urrutia, T., Weilbacher, P. M., Akhlaghi, M., Bouche, N., Contini, T., Guiderdoni, B., Herenz, E. C., Inami, H., Kerutt, J., Leclercq, F., Marino, R. A., Maseda, M., Monreal-Ibero, A., Nanayakkara, T., Richard, J., Saust, R., Steinmetz, M., Wendt, M.
Galaxies are surrounded by large reservoirs of gas, mostly hydrogen, fed by inflows from the intergalactic medium and by outflows due to galactic winds. Absorption-line measurements along the sightlines to bright and rare background quasars indicate
Externí odkaz:
http://arxiv.org/abs/1810.00843
Autor:
Morishita, T., Trenti, M., Stiavelli, M., Bradley, L. D., Coe, D., Oesch, P. A., Mason, C. A., Bridge, J. S., Holwerda, B. W., Livermore, R. C., Salmon, B., Schmidt, K. B., Shull, J. M., Treu, T.
We present a full data analysis of the pure-parallel Hubble Space Telescope (HST) imaging observations in the Brightest of Reionizing Galaxies Survey (BoRG[z9]) in Cycle 22. The medium-deep exposures with five HST/WFC3IR+UVIS filter bands from 79 ind
Externí odkaz:
http://arxiv.org/abs/1809.07604
Autor:
Verhamme, A., Garel, T., Ventou, E., Contini, T., Bouché, N., Herenz, E. C., Richard, J., Bacon, R., Schmidt, K. B., Maseda, M., Marino, R. A., Brinchmann, J., Cantalupo, S., Caruana, J., Clément, B., Diener, C., Drake, A. B., Hashimoto, T., Inami, H., Kerutt, J., Kollatschny, W., Leclercq, F., Patrício, V., Schaye, J., Wisotzki, L., Zabl, J.
The Lyman alpha (lya) line of Hydrogen is a prominent feature in the spectra of star-forming galaxies, usually redshifted by a few hundreds of km/s compared to the systemic redshift. This large offset hampers follow-up surveys, galaxy pair statistics
Externí odkaz:
http://arxiv.org/abs/1804.01883
Autor:
Morishita, T., Abramson, L. E., Treu, T., Wang, X., Brammer, G. B., Kelly, P., Stiavelli, M., Jones, T., Schmidt, K. B., Trenti, M., Vulcani, B.
Local massive early-type galaxies are believed to have completed most of their star formation $\sim10$Gyr ago and evolved without having substantial star formation since. If so, their progenitors should have roughly solar stellar metallicities ($Z_*$
Externí odkaz:
http://arxiv.org/abs/1803.01852
Autor:
Patricio, V., Richard, J., Carton, D., Contini, T., Epinat, B., Brinchmann, J., Schmidt, K. B., Krajnovic, D., Bouche, N., Weilbacher, P. M., Pello, R., Caruana, J., Maseda, M., Finley, H., Bauer, F. E., Martinez, J., Mahler, G., Lagattuta, D., Clement, B., Soucail, G., Wisotzki, L.
We analyse a sample of 8 highly magnified galaxies at redshift 0.6
Externí odkaz:
http://arxiv.org/abs/1802.08451
Autor:
Abramson, L. E., Newman, A. B., Treu, T., Huang, K. H., Morishita, T., Wang, X., Hoag, A., Schmidt, K. B., Mason, C. A., Bradač, M., Brammer, G. B., Dressler, A., Poggianti, B. M., Trenti, M., Vulcani, B.
Modern data empower observers to describe galaxies as the spatially and biographically complex objects they are. We illustrate this through case studies of four, $z\sim1.3$ systems based on deep, spatially resolved, 17-band + G102 + G141 Hubble Space
Externí odkaz:
http://arxiv.org/abs/1710.00843
Autor:
Rodney, S. A., Balestra, I., Bradac, M., Brammer, G., Broadhurst, T., Caminha, G. B., Chirivi, G., Diego, J. M., Filippenko, A. V., Foley, R. J., Graur, O., Grillo, C., Hemmati, S., Hjorth, J., Hoag, A., Jauzac, M., Jha, S. W., Kawamata, R., Kelly, P. L., McCully, C., Mobasher, B., Molino, A., Oguri, M., Richard, J., Riess, A. G., Rosati, P., Schmidt, K. B., Selsing, J., Sharon, K., Strolger, L. -G., Suyu, S. H., Treu, T., Weiner, B. J., Williams, L. L. R., Zitrin, A.
A massive galaxy cluster can serve as a magnifying glass for distant stellar populations, with strong gravitational lensing exposing details in the lensed background galaxies that would otherwise be undetectable. The MACS J0416.1-2403 cluster (hereaf
Externí odkaz:
http://arxiv.org/abs/1707.02434