Search Publications

Determination of the microbial diversity of spacecraft assembly, testing and launch facilities: First results of the ESA project MiDiv
DOI: 10.1016/j.asr.2006.01.006 Bibcode: 2006AdSpR..38.1260R

Rettberg, P.; Fritze, D.; Verbarg, S. +4 more

In the near future, an increasing number of in situ life detection and sample return missions to planets and other solar system bodies will be launched. The demand to control spacecraft-carried microbial contamination becomes obvious. COSPAR (Committee of Space Research) has defined guidelines and bioburden limits for different types of missions a…

2006 Advances in Space Research
SMART-1 9
Line formation regions of the UV spectrum of CI Cygni
DOI: 10.1051/0004-6361:20052655 Bibcode: 2006A&A...460..191M

Friedjung, M.; Mikołajewska, J.; Quiroga, C.

Aims.They are the interpretation of the emission line formation regions in CI Cygni
Methods: .They involve the examination of radial velocities and fluxes of ultraviolet emission lines at different epochs, deduced from archival IUE and GRHS/HST spectra.
Results: .The line fluxes give electron densities and were in additi…

2006 Astronomy and Astrophysics
IUE eHST 9
Faint U-Band Dropouts in the WFPC2 Parallels of the Hubble Ultra Deep Field
DOI: 10.1086/505747 Bibcode: 2006AJ....132.1023W

Casertano, Stefano; de Mello, Duilia; Wadadekar, Yogesh

We combine data from the extremely deep Hubble Space Telescope U (F300W) image, obtained using WFPC2 as part of the parallel observations of the Hubble Ultra Deep Field campaign, with BVi images from the Great Observatories Origins Deep Survey to identify a sample of Lyman break galaxies in the redshift range 2.0<~z<~3.5. We use recent stell…

2006 The Astronomical Journal
eHST 9
Evidence of standing waves during a Pi2 pulsation event observed on Cluster
DOI: 10.5194/angeo-24-2719-2006 Bibcode: 2006AnGeo..24.2719C

Blomberg, L. G.; Collier, A. B.; Hughes, A. R. W. +1 more

Observations of Pi2 pulsations at middle and low latitudes have been explained in terms of cavity mode resonances, whereas transients associated with field-aligned currents appear to be responsible for the high latitude Pi2 signature. Data from Cluster are used to study a Pi2 event observed at 18:09 UTC on 21 January 2003, when three of the satell…

2006 Annales Geophysicae
Cluster 9
Spitzer observations of red galaxies: Implication for high-redshift star formation
DOI: 10.1016/j.newar.2005.11.023 Bibcode: 2006NewAR..50..134P

Papovich, Casey

My colleagues and I identified distant red galaxies (DRGs) with J - Ks > 2.3 in the southern Great Observatories Origins Deep Surveys (GOODS-S) field. These galaxies reside at z ∼ 1-3.5, (< z> ≃ 2.2) and based on their ACS (0.4-1 µm), ISAAC (1-2.2 µm), and IRAC (3-8 µm) photometry, they typically have stellar …

2006 New Astronomy Reviews
eHST 9
Simulation of the Cluster-Spacecraft Floating Probe Potential
DOI: 10.1109/TPS.2006.883407 Bibcode: 2006ITPS...34.2078T

Escoubet, C. P.; Masson, A.; Laakso, H. +2 more

2006 IEEE Transactions on Plasma Science
Cluster 9
Saturn's Icy Moon Rhea: A Prediction for its Bulk Chemical Composition and Physical Structure at the Time of the Cassini Spacecraft First Flyby
DOI: 10.1071/AS05041 Bibcode: 2006PASA...23....1P

Prentice, Andrew J. R.

I report a model for the formation of Saturn's family of mid-sized icy moons to coincide with the first flypast of Rhea by the Cassini spacecraft on 2005 November 26. It is proposed that the moons had condensed from a concentric family of orbiting gas rings that were shed some 4.6 × 109 yr ago by the proto-Saturnian (hereafter p-Sat) cl…

2006 Publications of the Astronomical Society of Australia
Cassini 9
Shock excitation of the knots of Hen 3-1475
DOI: 10.1051/0004-6361:20053499 Bibcode: 2006A&A...455..203R

Binette, L.; Raga, A. C.; Riera, A.

We present new optical STIS HST spectroscopic observations of the jets of the proto-planetary nebula Hen3-1475. The excitation conditions of the knots of Hen3-1475

are derived from the observed optical spectra, confirming that the knots are shock excited.

The shocked spectra are qualitatively reproduced by simple "3/2"Dbow shock models. …

2006 Astronomy and Astrophysics
eHST 9
APEX blind deconvolution of color Hubble space telescope imagery and other astronomical data
DOI: 10.1117/1.2362579 Bibcode: 2006OptEn..45j7004C

Carasso, Alfred S.

2006 Optical Engineering
eHST 9
Photometric properties of Titan's surface from Cassini VIMS: Relevance to titan's hemispherical albedo dichotomy and surface stability
DOI: 10.1016/j.pss.2006.06.014 Bibcode: 2006P&SS...54.1540N

Sotin, C.; Brown, R. H.; Baines, K. H. +24 more

The Visual and Infrared Mapping Spectrometer (VIMS) instrument on the Cassini Saturn Orbiter returned spectral imaging data as the spacecraft undertook six close encounters with Titan beginning 7 July, 2004. Three of these flybys each produced overlapping coverage of two distinct regions of Titan's surface. Twenty-four points were selected on appr…

2006 Planetary and Space Science
Cassini 9