Zobrazeno 1 - 10
of 49
pro vyhledávání: '"Karczewski, O. Ł."'
Autor:
Schirm, M. R. P., Wilson, C. D., Kamenetzky, J., Parkin, T. J., Glenn, J., Maloney, P., Rangwala, N., Spinoglio, L., Baes, M., Boselli, A., Cooray, A., De Looze, I., Fernández-Ontiveros, J. A., Karczewski, O. Ł., Wu, R.
We present Herschel Spectral and Photometric Imaging Receiver (SPIRE)-Fourier Transform Spectrometer (FTS) intermediate-sampled mapping observations of the central similar to 8 kpc (similar to 150 arcsec) of M51, with a spatial resolution of 40 arcse
Externí odkaz:
http://hdl.handle.net/10150/625734
http://arizona.openrepository.com/arizona/handle/10150/625734
http://arizona.openrepository.com/arizona/handle/10150/625734
Autor:
White, N. E., Bauer, F. E., Baumgartner, W., Bautz, M., Berger, E., Cenko, S. B., Chang, T. -C., Falcone, A., Fausey, H., Feldman, C., Fox, D., Fox, O., Fruchter, A., Fryer, C., Ghirlanda, G., Gorski, K., Grant, K., Guiriec, S., Hart, M., Hartmann, D., Hennawi, J., Kann, D. A., Kaplan, D., Kennea, A., Kocevski, D., Kouveliotou, C., Lawrence, C., Levan, A. J., Lidz, A., Lien, A., Littenberg, T. B., Mas-Ribas, L., Moss, M., O'Brien, P., O'Meara, J., Palmer, D. M., Pasham, D., Racusin, J., Remillard, R., Roberts, O. J., Roming, P., Rud, M., Salvaterra, R., Sambruna, R., Seiffert, M., Sun, G., Tanvir, N. R., Terrile, R., Thomas, N., van der Horst, A., Verstrand, W. T., Willems, P., Wilson-Hodge, C., Young, E. T., Amati, L., Bozzo, E., Karczewski, O. Ł., Hernandez-Monteagudo, C., Lopez, R. Rebolo, Genova-Santos, R., Rubino-Martin, J. A., Granot, J., Bemiamini, P., Gill, R., Burns, E.
Publikováno v:
Proc. SPIE 11821, UV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XXII, 1182109 (24 August 2021)
The Gamow Explorer will use Gamma Ray Bursts (GRBs) to: 1) probe the high redshift universe (z > 6) when the first stars were born, galaxies formed and Hydrogen was reionized; and 2) enable multi-messenger astrophysics by rapidly identifying Electro-
Externí odkaz:
http://arxiv.org/abs/2111.06497
Autor:
Polles, F. L., Madden, S. C., Lebouteiller, V., Cormier, D., Abel, N., Galliano, F., Hony, S., Karczewski, O. L., Lee, M. -Y., Chevance, M., Galametz, M., Lianou, S.
Publikováno v:
A&A 622, A119 (2019)
Our objective is to investigate the physical properties of the ionised gas of the low-metallicity dwarf galaxy, IC 10, at various spatial scales: from individual HII regions to the entire galaxy scale and examine whether diagnostics for integrated me
Externí odkaz:
http://arxiv.org/abs/1810.03633
Autor:
Hughes, T. M., Baes, M., Schirm, M. R. P., Parkin, T. J., Wu, R., De Looze, I., Wilson, C. D., Viaene, S., Bendo, G. J., Boselli, A., Cormier, D., Ibar, E., Karczewski, O. Ł., Lu, N., Spinoglio, L.
Publikováno v:
A&A 587, A45 (2016)
A correlation between the 24 {\mu}m continuum and the [NII] 205 {\mu}m line emission may arise if both quantities trace the star formation activity on spatially-resolved scales within a galaxy, yet has so far only been observed in the nearby edge-on
Externí odkaz:
http://arxiv.org/abs/1601.01317
Autor:
Viaene, S., Baes, M., Bendo, G., Boquien, M., Boselli, A., Ciesla, L., Cortese, L., De Looze, I., Eales, S., Fritz, J., Karczewski, O. Ł., Madden, S., Smith, M. W. L., Spinoglio, L.
Publikováno v:
A&A 586, A13 (2016)
The dust in nearby galaxies absorbs a fraction of the UV-optical-near-infrared radiation produced by stars. This energy is consequently re-emitted in the infrared. We investigate the portion of the stellar radiation absorbed by spiral galaxies from t
Externí odkaz:
http://arxiv.org/abs/1511.07430
Autor:
Rémy-Ruyer, A., Madden, S. C., Galliano, F., Lebouteiller, V., Baes, M., Bendo, G. J., Boselli, A., Ciesla, L., Cormier, D., Cooray, A., Cortese, L., De Looze, I., Doublier-Pritchard, V., Galametz, M., Jones, A. P., Karczewski, O. Ł., Lu, N., Spinoglio, L.
Publikováno v:
A&A 582, A121 (2015)
In this work, we aim at providing a consistent analysis of the dust properties from metal-poor to metal-rich environments by linking them to fundamental galactic parameters. We consider two samples of galaxies: the Dwarf Galaxy Survey (DGS) and KINGF
Externí odkaz:
http://arxiv.org/abs/1507.05432
Autor:
Cormier, D., Madden, S. C., Lebouteiller, V., Abel, N., Hony, S., Galliano, F., Remy-Ruyer, A., Bigiel, F., Baes, M., Boselli, A., Chevance, M., Cooray, A., De Looze, I., Doublier, V., Galametz, M., Hugues, T., Karczewski, O. L., Lee, M. -Y., Lu, N., Spinoglio, L.
Publikováno v:
A&A 578, A53 (2015)
The far-infrared (FIR) lines are key tracers of the physical conditions of the interstellar medium (ISM) and are becoming workhorse diagnostics for galaxies throughout the universe. Our goal is to explain the differences and trends observed in the FI
Externí odkaz:
http://arxiv.org/abs/1502.03131
Insights into gas heating and cooling in the disc of NGC 891 from Herschel far-infrared spectroscopy
Autor:
Hughes, T. M., Foyle, K., Schirm, M. R. P., Parkin, T. J., De Looze, I., Wilson, C. D., Bendo, G. J., Baes, M., Fritz, J., Boselli, A., Cooray, A., Cormier, D., Karczewski, O. Ł., Lebouteiller, V., Lu, N., Madden, S. C., Spinoglio, L., Viaene, S.
Publikováno v:
A&A 575, A17 (2015)
We present Herschel PACS and SPIRE spectroscopy of the most important far-infrared cooling lines in the nearby edge-on spiral galaxy, NGC 891: [CII] 158 $\mu$m, [NII] 122, 205 $\mu$m, [OI] 63, 145 $\mu$m, and [OIII] 88 $\mu$m. We find that the photoe
Externí odkaz:
http://arxiv.org/abs/1410.6156
Autor:
Parkin, T. J., Wilson, C. D., Schirm, M. R. P., Baes, M., Boquien, M., Boselli, A., Cormier, D., Galametz, M., Karczewski, O. Ł., Lebouteiller, V., De Looze, I., Madden, S. C., Roussel, H., Smith, M. W. L., Spinoglio, L.
We search for variations in the disk of Centaurus A of the emission from atomic fine structure lines using Herschel PACS and SPIRE spectroscopy. In particular we observe the [C II](158 $\mu$m), [N II](122 and 205 $\mu$m), [O I](63 and 145 $\mu$m) and
Externí odkaz:
http://arxiv.org/abs/1404.0403
Autor:
Viaene, S., Fritz, J., Baes, M., Bendo, G. J., Blommaert, J. A. D. L., Boquien, M., Boselli, A., Ciesla, L., Cortese, L., De Looze, I., Gear, W. K., Gentile, G., Hughes, T. M., Jarrett, T., Karczewski, O. Ł., Smith, M. W. L., Spinoglio, L., Tamm, A., Tempel, E., Thilker, D., Verstappen, J.
Publikováno v:
A&A 567, A71 (2014)
The imprints of dust-starlight interactions are visible in scaling relations between stellar characteristics, star formation parameters and dust properties. We aim to examine dust scaling relations on a sub-kpc resolution in the Andromeda galaxy (M31
Externí odkaz:
http://arxiv.org/abs/1403.4272