Zobrazeno 1 - 10
of 315
pro vyhledávání: '"Koprowski, M."'
Autor:
Postigo, A. de Ugarte, Michalowski, M., Thoene, C. C., Martin, S., Ashok, A., Fernandez, J. F. Agui, Bremer, M., Misra, K., Perley, D. A., Heintz, K. E., Cherukuri, S. V., Dimitrov, W., Geron, T., Ghosh, A., Izzo, L., Kann, D. A., Koprowski, M. P., Lesniewska, A., Leung, J. K., Levan, A., Omar, A., Oszkiewicz, D., Polinska, M., Resmi, L., Schulze, S.
GRBs produced by the collapse of massive stars are usually found near the most prominent star-forming regions of star-forming galaxies. GRB 171205A happened in the outskirts of a spiral galaxy, a peculiar location in an atypical GRB host. In this pap
Externí odkaz:
http://arxiv.org/abs/2406.16726
Autor:
Gao, Zhen-Kai, Lim, Chen-Fatt, Wang, Wei-Hao, Chen, Chian-Chou, Smail, Ian, Chapman, Scott C., Zheng, Xian Zhong, Shim, Hyunjin, Kodama, Tadayuki, Ao, Yiping, Chang, Siou-Yu, Clements, David L., Dunlop, James S., Ho, Luis C., Hsu, Yun-Hsin, Hwang, Chorng-Yuan, Hwang, Ho Seong, Koprowski, M. P., Scott, Douglas, Serjeant, Stephen, Toba, Yoshiki, Urquhart, Sheona A.
We present confusion-limited SCUBA-2 450-$\mu$m observations in the COSMOS-CANDELS region as part of the JCMT Large Program, SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES). Our maps at 450 and 850 $\mu$m cover an area of 450 arcmin$^2$. We achieved
Externí odkaz:
http://arxiv.org/abs/2405.20616
Autor:
Koprowski, M. P., Wijesekera, J. V., Dunlop, J. S., McLeod, D. J., Michałowski, M. J., Lisiecki, K., McLure, R. J.
Publikováno v:
A&A 691, A164 (2024)
We present a new determination of the star-forming main sequence (MS), obtained through stacking 100k K-band-selected galaxies in the far-infrared (FIR) Herschel and James Clerk Maxwell Telescope (JCMT) imaging. By fitting the dust emission curve to
Externí odkaz:
http://arxiv.org/abs/2403.06575
Autor:
Michałowski, Michał J., Gall, C., Hjorth, J., Frayer, D. T., Tsai, A. -L., Rowlands, K., Takeuchi, T. T., Leśniewska, A., Behrendt, D., Bourne, N., Hughes, D. H., Koprowski, M. P., Nadolny, J., Ryzhov, O., Solar, M., Spring, E., Zavala, J., Bartczak, P.
Publikováno v:
2024, ApJ, 964, 129
Understanding how galaxies quench their star formation is crucial for studies of galaxy evolution. Quenching is related to the cold gas decrease. In the first paper we showed that the dust removal timescale in early-type galaxies (ETGs) is about 2.5
Externí odkaz:
http://arxiv.org/abs/2401.04774
Autor:
Dunlop, J. S., McLure, R. J., Biggs, A. D., Geach, J. E., Michałowski, M. J., Ivison, R. J., Rujopakarn, W., van Kampen, E., Kirkpatrick, A., Pope, A., Scott, D., Swinbank, A. M., Targett, T. A., Aretxaga, I., Austermann, J. E., Best, P. N., Bruce, V. A., Chapin, E. L., Charlot, S., Cirasuolo, M., Coppin, K., Ellis, R. S., Finkelstein, S. L., Hayward, C. C., Hughes, D. H., Ibar, E., Jagannathan, P., Khochfar, S., Koprowski, M. P., Narayanan, D., Nyland, K., Papovich, C., Peacock, J. A., Rieke, G. H., Robertson, B., Vernstrom, T., Werf, P. P. van der, Wilson, G. W., Yun, M.
We present the results of the first, deep Atacama Large Millimeter Array ( ALMA) imaging covering the full similar or equal to 4.5 arcmin(2) of the Hubble Ultra Deep Field ( HUDF) imaged with Wide Field Camera 3/IR on HST. Using a 45-pointing mosaic,
Externí odkaz:
http://hdl.handle.net/10150/623849
http://arizona.openrepository.com/arizona/handle/10150/623849
http://arizona.openrepository.com/arizona/handle/10150/623849
Autor:
Le, N., Karska, A., Figueira, M., Sewiło, M., Mirocha, A., Fischer, Ch., Kaźmierczak-Barthel, M., Klein, R., Gawroński, M., Koprowski, M., Kowalczyk, K., Fischer, W. J., Menten, K. M., Wyrowski, F., König, C., Kristensen, L. E.
Publikováno v:
A&A 674, A64 (2023)
(abridged) Far-infrared (FIR) line emission provides key information about the gas cooling and heating due to shocks and UV radiation associated with the early stages of star formation. Gas cooling via FIR lines might, however, depend on metallicity.
Externí odkaz:
http://arxiv.org/abs/2304.08127
Autor:
Garratt, T. K., Geach, J. E., Tamura, Y., Coppin, K. E. K., Franco, M., Ao, Y., Chen, C. -C., Cheng, C., Clements, D. L., Dai, Y. S., Dannerbauer, H., Greve, T. R., Hatsukade, B., Hwang, H. S., Jiang, L., Kohno, K., Koprowski, M. P., Michalowski, M. J., Sawicki, M., Scott, D., Shim, H., Takeuchi, T. T., Wang, W. -H., Xue, Y. Q., Yang, C.
We present 850um imaging of the XMM-LSS field observed for 170 hours as part of the James Clerk Maxwell Telescope SCUBA-2 Large eXtragalactic Survey (S2LXS). S2LXS XMM-LSS maps an area of 9 square degrees, reaching a moderate depth of 1-sigma ~ 4 mJy
Externí odkaz:
http://arxiv.org/abs/2301.10801
Autor:
Shim, H., Lee, D., Kim, Y., Scott, D., Serjeant, S., Ao, Y., Barrufet, L., Chapman, S. C., Clements, D., Conselice, C. J., Goto, T., Greve, T. R., Hwang, H. S., Im, M., Jeong, W. -S., Kim, H. K., Kim, M., Kim, S. J., Kong, A. K. H., Koprowski, M. P., Malkan, M. A., Michalowski, M., Pearson, C., Seo, H., Takagi, T., Toba, Y., White, G. J., Woo, J. -H.
We present the multi-wavelength counterparts of 850-$\mu$m selected submillimetre sources over a 2-deg$^2$ field centred on the North Ecliptic Pole. In order to overcome the large beam size (15 arcsec) of the 850-$\mu$m images, deep optical to near-i
Externí odkaz:
http://arxiv.org/abs/2204.11392
Autor:
Leśniewska, Aleksandra, Michałowski, M. J., Kamphuis, P., Dziadura, K., Baes, M., Cerón, J. M. Castro, Gentile, G., Hjorth, J., Hunt, L. K., Jespersen, C. K., Koprowski, M. P., Floc'h, E. Le, Miraghaei, H., Guelbenzu, A. Nicuesa, Oszkiewicz, D., Palazzi, E., Polińska, M., Rasmussen, J., Schady, P., Watson, D.
Long ($>2$ s) gamma ray bursts (GRBs) are associated with explosions of massive stars, although in three instances, supernovae (SNe) have not been detected, despite deep observations. With new HI line and archival optical integral field spectroscopy
Externí odkaz:
http://arxiv.org/abs/2202.01188
Autor:
Garratt, T. K., Coppin, K. E. K., Geach, J. E., Almaini, O., Hartley, W. G., Maltby, D. T., Simpson, C. J., Wilkinson, A., Conselice, C. J., Franco, M., Ivison, R. J., Koprowski, M. P., Lovell, C. C., Pope, A., Scott, D., van der Werf, P.
We present new empirical constraints on the evolution of $\rho_{\rm H_2}$, the cosmological mass density of molecular hydrogen, back to $z\approx2.5$. We employ a statistical approach measuring the average observed $850\mu{\rm m}$ flux density of nea
Externí odkaz:
http://arxiv.org/abs/2103.08613