Search Publications

An Alternative Interpretation of the Relationship between the Inferred Open Solar Flux and the Interplanetary Magnetic Field
DOI: 10.1086/522001 Bibcode: 2007ApJ...667L..97R

Riley, Pete

Photospheric observations at the Wilcox Solar Observatory (WSO) represent an uninterrupted data set of 32 years and are therefore unique for modeling variations in the magnetic structure of the corona and inner heliosphere over three solar cycles. For many years, modelers have applied a latitudinal correction factor to these data, believing that i…

2007 The Astrophysical Journal
SOHO 41
Global Coronal Seismology
DOI: 10.1007/s11207-007-0415-3 Bibcode: 2007SoPh..246..177B

Ballai, I.

Following the observation and analysis of large-scale coronal-wave-like disturbances, we discuss the theoretical progress made in the field of global coronal seismology. Using simple mathematical techniques we determine average values for the magnetic field together with a magnetic map of the quiet Sun. The interaction between global coronal waves…

2007 Solar Physics
SOHO 41
Titan's surface from Cassini RADAR SAR and high resolution radiometry data of the first five flybys
DOI: 10.1016/j.icarus.2007.04.032 Bibcode: 2007Icar..191..211P

Lorenz, R. D.; Janssen, M. A.; Stiles, B. +12 more

The first five Titan flybys with Cassini's Synthetic Aperture RADAR (SAR) and radiometer are examined with emphasis on the calibration and interpretation of the high-resolution radiometry data acquired during the SAR mode (SAR-radiometry). Maps of the 2-cm wavelength brightness temperature are obtained coincident with the SAR swath imaging, with s…

2007 Icarus
Cassini eHST 41
Observation of similar radio signatures at Saturn and Jupiter: Implications for the magnetospheric dynamics
DOI: 10.1029/2007GL030368 Bibcode: 2007GeoRL..3420113L

Gurnett, D. A.; Persoon, A. M.; Hospodarsky, G. B. +13 more

We report on radio signatures observed at Saturn by the Cassini RPWS experiment which are strikingly similar to the Jovian ``energetic events'' observed by Galileo. They consist of sudden intensifications of the auroral radio emission (SKR) followed by the detection of a periodic narrowband radiation which most likely originates from Saturn's plas…

2007 Geophysical Research Letters
Cassini 41
ConvPhot: A profile-matching algorithm for precision photometry
DOI: 10.1016/j.newast.2006.10.004 Bibcode: 2007NewA...12..271D

Santini, P.; Fontana, A.; Grazian, A. +1 more

We describe in this paper a new, public software for accurate "PSF-matched" multiband photometry for images of different resolution and depth, that we have named ConvPhot, of which we analyse performances and limitations. It is designed to work when a high resolution image is available to identify and extract the objects, and colours or variations…

2007 New Astronomy
eHST 41
Differences in the AGN Populations of Groups and Clusters: Clues to AGN Evolution
DOI: 10.1086/511030 Bibcode: 2007ApJ...654L.115S

Shen, Yue; Raychaudhury, Somak; Mulchaey, John S. +2 more

We combine optical and X-ray data for eight low-redshift (z~0.06) poor groups of galaxies from the XI (XMM-IMACS) Groups Project to study the AGN population in the group environment. Among ~140 group members, we identify five AGNs based on their optical emission lines. None of these optically selected AGNs are detected by XMM-Newton. One additiona…

2007 The Astrophysical Journal
XMM-Newton 41
XMM-Newton observation of the persistent Be/neutron star system X Persei at a high-luminosity level
DOI: 10.1051/0004-6361:20077970 Bibcode: 2007A&A...474..137L

Mereghetti, S.; La Palombara, N.

We report on the XMM-Newton observation of the HMXRB X Persei, the prototype of the persistent and low-luminosity Be/neutron star pulsars, which was performed in February 2003. The source was detected at a luminosity level of ~1.4×1035 erg s-1, which is the highest level of the latest three decades. The pulsation period has i…

2007 Astronomy and Astrophysics
XMM-Newton 40
Obscured and unobscured AGN populations in a hard-X-ray selected sample of the XMDS survey
DOI: 10.1051/0004-6361:20066667 Bibcode: 2007A&A...467...73T

Maccagni, D.; Maraschi, L.; Chiappetti, L. +16 more

Aims:Our goal is to probe the populations of obscured and unobscured AGN investigating their optical-IR and X-ray properties as a function of X-ray flux, luminosity and redshift within a hard X-ray selected sample with wide multiwavelength coverage.
Methods: We selected a sample of 136 X-ray sources detected at a significance of ≥3 σ in the 2{…

2007 Astronomy and Astrophysics
XMM-Newton 40
A Spitzer IRAC Census of the Asymptotic Giant Branch Populations in Local Group Dwarfs. I. WLM
DOI: 10.1086/510354 Bibcode: 2007ApJ...656..818J

Skillman, Evan D.; Gehrz, Robert D.; Woodward, Charles E. +2 more

We present Spitzer IRAC observations at 3.6 and 4.5 µm along with optical data from the Local Group Galaxies Survey to investigate the evolved stellar population of the Local Group dwarf irregular galaxy WLM. These observations provide a nearly complete census of the AGB stars. We find that 39% of the infrared-detected AGB stars are not dete…

2007 The Astrophysical Journal
eHST 40
Dressing a Naked Quasar: Star Formation and Active Galactic Nucleus Feedback in HE 0450-2958
DOI: 10.1086/518027 Bibcode: 2007ApJ...662..872F

Feain, Ilana J.; Ekers, Ronald D.; Papadopoulos, Padelis P. +1 more

We present Australia Telescope Compact Array radio continuum observations of the quasar/galaxy system HE 0450-2958. An asymmetric triple linear morphology is observed, with the central radio component coincident with the quasar core and a second radio component associated with a companion galaxy at a projected distance of 7 kpc from the quasar. Th…

2007 The Astrophysical Journal
eHST 40