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11.
Paolo Saracco Sandro D'Odorico Alan Moorwood Jean G. Cuby 《Astrophysics and Space Science》2001,276(2-4):991-998
Deep J- and K
s-band images covering a 5 × 5 arcmin area centred on the NTT Deep Field have been obtained during the Science Verification
of SOFI at the NTT. These images were made available via the Web in early June, 1998. The preliminary results we have obtained
by the analysis of these data are the following: (i) the counts continue to rise with no evidence of a turnover or of a flattening
down to the limits of the survey (K
s = 22.5 and J = 24 mag); (ii) we find a slope d log(N)/dm≈ 0.37, in agreement with most of the faintest surveys but much steeper than the Hawaii survey; (iii) fainter than K
s ≈ 19and J ≈ 20 mag, the median J-K colour of galaxies shows a break in its reddening trend turning toward bluer colours; (iv) faint bluer galaxies also display
a larger compactness index, and a smaller apparent size.
This revised version was published online in July 2006 with corrections to the Cover Date. 相似文献
12.
We report on repeated mid-resolution (R∼2000) spectroscopic observations of Titan, acquired between November 2002 and January 2003 with ISAAC at the ESO/VLT and covering the 4.84-5.05 μm range. These observations, which sample four different positions of Titan around Saturn, clearly indicate a variability of the 5-μm continuum albedo, with Titan's geometric albedo decreasing by ∼40% from Titan's leading side to the trailing side. This Titan 5-μm “lightcurve” appears to be in phase with the other near-infrared lightcurves. This can be understood in terms of a surface model in which water ice coexists in minor and variable proportions (13-25%, if pure) with a second, dark, component. 相似文献
13.
L. Tresse S. J. Maddox O. Le Fèvre J.-G. Cuby 《Monthly notices of the Royal Astronomical Society》2002,337(1):369-383
We describe ISAAC/ESO-VLT observations of the Hαλ6563 Balmer line of 33 field galaxies from the Canada–France Redshift Survey (CFRS) with redshifts selected between 0.5 and 1.1. We detect Hα in emission in 30 galaxies and compare the properties of this sample with the low-redshift sample of CFRS galaxies at z ∼ 0.2 . We find that the Hα luminosity, L (Hα) , is tightly correlated to M ( B AB ) in the same way for both the low- and high-redshift samples. L (Hα) is also correlated to L ([O ii ]λ3727), and again the relation appears to be similar at low and high redshifts. The ratio L (lsqb;O ii ])/ L (Hα) decreases for brighter galaxies by as much as a factor of 2 on average. Derived from the Hα luminosity function, the comoving Hα luminosity density increases by a factor 12 from 〈 z 〉= 0.2 to 〈 z 〉= 1.3 . Our results confirm a strong rise of the star formation rate (SFR) at z < 1.3 , proportional to (1 + z )4.1±0.3 (with H 0 = 50 km s−1 Mpc−1 , q 0 = 0.5 ). We find an average SFR(2800 Å)/SFR (Hα) ratio of 3.2 using the Kennicutt SFR transformations. This corresponds to the dust correction that is required to make the near-ultraviolet data consistent with the reddening-corrected Hα data within the self-contained, I -selected CFRS sample. 相似文献
14.
Jean-Gabriel Bréhéret Micheline Hanzo Abderrazzak El Albani Agnès Iatzoura 《Comptes Rendus Geoscience》2004,336(15):1355-1362
The study of calcareous nodules from four organic-rich black shale series allows us to suggest a prominent part for benthic organisms in creating heterogeneities in the sediment, thus favouring microbially mediated early diagenesis based on organic matter consumption. To cite this article: J.-G. Bréhéret et al., C. R. Geoscience 336 (2004). 相似文献
15.
Agathe Fourmont Jean-Jacques Macaire Jean-Gabriel Brhret Jacqueline Argant Batrice Prat Grard Vernet 《Comptes Rendus Geoscience》2006,338(16):1141-1149
The Sarliève marsh sediments (Massif Central, France) contain two tephras. The first tephra [, ca. 12 000 BP], regionally well known, enables to date the beginning of lacustrine infill to the Lateglacial. The second tephra, the ‘tephra de Sarliève’, the emitting volcano of which is unknown, would be dated to around the Early Subboreal from pollen data. This occurrence, after the discovery of the ‘tephra de Beaunit’, emphasizes that volcanic eruption(s) occurred in the ‘Chaîne des Puys’ or in the volcanic Cézallier more than 1000 years after the last known eruption (Pavin) in the ‘Chaîne des Puys’ at around 6.6/6.7 ka (5800/5900 BP). In the Sarliève piles, these tephras, well preserved in thick and more silicated deposits of deltas, were not observed in carbonated basin sediments where they were altered. The abundance of authigenic zeolites formed during the Lateglacial in restricted depocentre lacustrine waters allows us to detect initial CF1 tephra occurrence. To cite this article: A. Fourmont et al., C. R. Geoscience 338 (2006). 相似文献