Zobrazeno 1 - 10
of 94
pro vyhledávání: '"Zabl, J."'
Autor:
Heintz, K. E., Fynbo, J. P. U., Møller, P., Milvang-Jensen, B., Zabl, J., Maddox, N., Krogager, J.-K., Geier, S., Vestergaard, M., Noterdaeme, P., Ledoux, C.
The sub-population of quasars reddened by intrinsic or intervening clouds of dust are known to be underrepresented in optical quasar surveys. By defining a complete parent sample of the brightest and spatially unresolved quasars in the COSMOS field,
Externí odkaz:
http://hdl.handle.net/10150/622443
http://arizona.openrepository.com/arizona/handle/10150/622443
http://arizona.openrepository.com/arizona/handle/10150/622443
Autor:
Langan, I., Zabl, J., Bouche, N. F., Ginolfi, M., Popping, G., Schroetter, I., Wendt, M., Schaye, J., Boogaard, L., Freundlich, J., Richard, J., Matthee, J., Mercier, W., Contini, T., Guo, Y., Cherrey, M.
We study the link between gas flow events and key galaxy scaling relations: the relations between star formation rate (SFR) and stellar mass (the main sequence, MS), gas metallicity and stellar mass (the mass-metallicity relation, MZR) and gas metall
Externí odkaz:
http://arxiv.org/abs/2301.10779
Autor:
Ciesla, L., Béthermin, M., Daddi, E., Richard, J., Diaz-Santos, T., Sargent, M. T., Elbaz, D., Boquien, M., Wang, T., Schreiber, C., Yang, C., Zabl, J., Fraser, M., Aravena, M., Assef, R. J., Baker, A. J., Beelen, A., Boselli, A., Bournaud, F., Burgarella, D., Charmandaris, V., Côté, P., Epinat, B., Ferrarese, L., Gobat, R., Ilbert, O.
Publikováno v:
A&A 635, A27 (2020)
[Abridged] We discovered in the Herschel Reference Survey an extremely bright IR source with $S_{500}$~120mJy (Red Virgo 4 - RV4). Based on IRAM/EMIR and IRAM/NOEMA detections of the CO(5-4), CO(4-3), and [CI] lines, RV4 is located at z=4.724, yieldi
Externí odkaz:
http://arxiv.org/abs/2001.03641
Autor:
Tilvi, V., Malhotra, S., Rhoads, J. E., Coughlin, A., Zheng, Z., Finkelstein, S. L., Veilleux, S., Mobasher, B., Wang, J., Probst, R., Swaters, R., Hibon, P., Joshi, B., Zabl, J., Jiang, T., Pharo, J., Yang, H.
While most of the inter-galactic medium (IGM) today is permeated by ionized hydrogen, it was largely filled with neutral hydrogen for the first 700 million years after the Big Bang. The process that ionized the IGM (cosmic reionization) is expected t
Externí odkaz:
http://arxiv.org/abs/2001.00873
Autor:
de La Vieuville, G., Bina, D., Pello, R., Mahler, G., Richard, J., Drake, A. B., Herenz, E. C., Bauer, F. E., Clément, B., Lagattuta, D., Laporte, N., Martinez, J., Patriìcio, V., Wisotzki, L., Zabl, J., Bouwens, R. J., Contini, T., Garel, T., Guiderdoni, B., Marino, R. A., Maseda, M. V., Matthee, J., Schaye, J., Soucail, G.
Publikováno v:
A&A 628, A3 (2019)
We present the results obtained with VLT/MUSE on the faint-end of the Lyman-alpha luminosity function (LF) based on deep observations of four lensing clusters. The precise aim of the present study is to further constrain the abundance of Lyman-alpha
Externí odkaz:
http://arxiv.org/abs/1905.13696
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
Publikováno v:
Ebeling H. et al., 2018, ApJ, 852, L7
We report the discovery of eMACSJ1341-QG-1, a quiescent galaxy at $z=1.594$ located behind the massive galaxy cluster eMACSJ1341.9$-$2442 ($z=0.835$). The system was identified as a gravitationally lensed triple image in Hubble Space Telescope images
Externí odkaz:
http://arxiv.org/abs/1802.00133
Autor:
Tanvir, N. R., Laskar, T., Levan, A. J., Perley, D. A., Zabl, J., Fynbo, J. P. U., Rhoads, J., Cenko, S. B., Greiner, J., Wiersema, K., Hjorth, J., Cucchiara, A., Berger, E., Bremer, M. N., Cano, Z., Cobb, B. E., Covino, S., D'Elia, V., Fong, W., Fruchter, A. S., Goldoni, P., Hammer, F., Heintz, K. E., Jakobsson, P., Kann, D. A., Kaper, L., Klose, S., Knust, F., Kruehler, T., Malesani, D., Misra, K., Guelbenzu, A. Nicuesa, Pugliese, G., Sanchez-Ramirez, R., Schulze, S., Stanway, E. R., Postigo, A. de Ugarte, Watson, D., Wijers, R. A. M. J., Xu, D.
Gamma-ray bursts (GRBs) are powerful probes of early stars and galaxies, during and potentially even before the era of reionization. Although the number of GRBs identified at z>6 remains small, they provide a unique window on typical star-forming gal
Externí odkaz:
http://arxiv.org/abs/1703.09052
Autor:
Laigle, C., McCracken, H. J., Ilbert, O., Hsieh, B. C., Davidzon, I., Capak, P., Hasinger, G., Silverman, J. D., Pichon, C., Coupon, J., Aussel, H., Borgne, D. Le, Caputi, K., Cassata, P., Chang, Y. -Y., Civano, F., Dunlop, J., Fynbo, J., kartaltepe, J. S., Koekemoer, A., Fevre, O. Le, Floc'h, E. Le, Leauthaud, A., Lilly, S., Lin, L., Marchesi, S., Milvang-Jensen, B., Salvato, M., Sanders, D. B., Scoville, N., Smolcic, V., Stockmann, M., Taniguchi, Y., Tasca, L., Toft, S., Vaccari, M., Zabl, J.
We present the COSMOS2015 catalog which contains precise photometric redshifts and stellar masses for more than half a million objects over the 2deg$^{2}$ COSMOS field. Including new $YJHK_{\rm s}$ images from the UltraVISTA-DR2 survey, $Y$-band from
Externí odkaz:
http://arxiv.org/abs/1604.02350
Autor:
Zabl, J., Freudling, W., Møller, P., Milvang-Jensen, B., Nilsson, K. K., Fynbo, J. P. U., Fèvre, O. Le, Tasca, L. A. M.
Publikováno v:
A&A 590, A66 (2016)
High redshift star-forming galaxies are discovered routinely through a flux excess in narrowband filters (NB) caused by an emission line. In most cases, the width of such filters is broad compared to typical line widths, and the throughput of the fil
Externí odkaz:
http://arxiv.org/abs/1602.06304