Search Publications

Optical Morphology Evolution of Infrared Luminous Galaxies in GOODS-N
DOI: 10.1086/498019 Bibcode: 2005ApJ...632L..65M

Le Floc'h, E.; Koo, D. C.; Melbourne, J.

We combine optical morphologies and photometry from HST, redshifts from Keck, and mid-infrared luminosities from Spitzer for an optically selected sample of ~800 galaxies in GOODS-N to track the morphology evolution of luminous infrared galaxies (LIRGs) since redshift z=1. We find a 50% decline in the number of LIRGs from z~1 to lower redshift, in…

2005 The Astrophysical Journal
eHST 77
Relationship between X-ray and ultraviolet emission of flares from dMe stars observed by XMM-Newton
DOI: 10.1051/0004-6361:20041201 Bibcode: 2005A&A...431..679M

Raassen, A. J. J.; Mewe, R.; Audard, M. +6 more

We present simultaneous ultraviolet and X-ray observations of the dMe-type flaring stars AT Mic, AU Mic, EV Lac, UV Cet and YZ CMi obtained with the XMM-Newton observatory. During 40 h of simultaneous observation we identify 13 flares which occurred in b…

2005 Astronomy and Astrophysics
XMM-Newton 77
Gamma-Ray Burst-Selected High-Redshift Galaxies: Comparison to Field Galaxy Populations to z ~ 3
DOI: 10.1086/432829 Bibcode: 2005ApJ...633...29C

Kouveliotou, C.; Fruchter, A. S.; Vreeswijk, P. M. +6 more

We study the internal structural properties of 37 long-duration gamma-ray burst (GRB) host galaxies imaged with the Hubble Space Telescope (HST). Our goal is to gain insights in the types of galaxies that give rise to GRBs and the relationship of GRB hosts to high-redshift galaxies selected through more traditional photometric methods. We measure …

2005 The Astrophysical Journal
eHST 77
XMM-Newton observations of three poor clusters: Similarity in dark matter and entropy profiles down to low mass
DOI: 10.1051/0004-6361:20041479 Bibcode: 2005A&A...429..791P

Arnaud, M.; Pratt, G. W.

We present an analysis of the mass and entropy profiles of three poor galaxy clusters (A1991, A2717 and MKW9) observed with XMM-Newton. The clusters have very similar temperatures (kT= 2.65, 2.53 and 2.58 keV), and similar redshifts (0.04 ⪉ z ⪉ 0.06). We trace the surface brightness, temperature, entropy and integrated mass profiles with excellent…

2005 Astronomy and Astrophysics
XMM-Newton 77
The Advanced Camera for Surveys Virgo Cluster Survey. V. Surface Brightness Fluctuation Calibration for Giant and Dwarf Early-Type Galaxies
DOI: 10.1086/429554 Bibcode: 2005ApJ...625..121M

Jordán, Andrés; Tonry, John L.; Côté, Patrick +7 more

As part of the Advanced Camera for Surveys (ACS) Virgo Cluster Survey, we have measured surface brightness fluctuations (SBFs) in a sample of 100 early-type Virgo galaxies. Distances derived from these measurements are needed to explore the three-dimensional structure of the Virgo Cluster, study the intrinsic parameters of globular clusters associ…

2005 The Astrophysical Journal
eHST 77
X-ray absorption lines suggest matter infalling onto the central black-hole of Mrk 509
DOI: 10.1051/0004-6361:20042487 Bibcode: 2005A&A...442..461D

de Rosa, A.; Cappi, M.; Ponti, G. +2 more

Evidence for both red- and blue-shifted absorption lines due to ionized Fe in the X-ray spectrum of the Seyfert 1 galaxy Mrk 509 is reported. These features appear to be transient on time-scales as short as ~20 ks, and have been observed with two different satellites, BeppoSAX and XMM-Newton. The red- and blue-shifted lines are found at E∼5.5 keV …

2005 Astronomy and Astrophysics
XMM-Newton 77
The Three-dimensional Circumstellar Environment of SN 1987A
DOI: 10.1086/430408 Bibcode: 2005ApJS..159...60S

Crotts, Arlin P. S.; Lawrence, Stephen S.; Sugerman, Ben E. K. +2 more

Surrounding SN 1987A is a three-ring nebula attributed to interacting stellar winds, yet no model has successfully reproduced this system. Fortunately, the progenitor's mass-loss history can be reconstructed using light echoes, in which scattered light from the supernova traces the three-dimensional morphology of its circumstellar dust. In this pa…

2005 The Astrophysical Journal Supplement Series
eHST 76
Calculating the Thermal Structure of Solar Active Regions in Three Dimensions
DOI: 10.1086/427739 Bibcode: 2005ApJ...621.1098M

Linker, Jon A.; Mikić, Zoran; Mok, Yung +1 more

We describe a technique to obtain the temperature and density distribution in an active region for a specified plasma heating model. The technique can be applied in general to determine the magnetic field and thermal structure self-consistently. For simplicity, we illustrate the application of this technique in the limit of small plasma β, in whic…

2005 The Astrophysical Journal
SOHO 76
GEMS: Which Galaxies Dominate the z~0.7 Ultraviolet Luminosity Density?
DOI: 10.1086/431659 Bibcode: 2005ApJ...630..771W

Heymans, C.; Wolf, C.; Barden, M. +14 more

We combine high-resolution images from GEMS with redshifts and spectral energy distributions from COMBO-17 to explore the morphological types of galaxies that dominate the z~0.7 UV luminosity density. We analyzed rest-frame 280 nm and V-band luminosities of 1483 galaxies with 0.65<z<0.75, combining these with visual morphological classificat…

2005 The Astrophysical Journal
eHST 76
Asteroid target selection for the new Rosetta mission baseline. 21 Lutetia and 2867 Steins
DOI: 10.1051/0004-6361:20041505 Bibcode: 2005A&A...430..313B

Barbieri, C.; Barucci, M. A.; Fornasier, S. +8 more

The new Rosetta mission baseline to the comet 67P/Churyumov-Gerasimenko includes two asteroid fly-bys. To help in target selection we studied all the candidates of all the possible scenarios. Observations have been carried out at ESO-NTT (La Silla, Chile), TNG (Canaries), and NASA-IRTF (Hawaii) telescopes, in order to determine the taxonomy of all…

2005 Astronomy and Astrophysics
Rosetta 76