Search Publications

Hinode/XRT and STEREO Observations of a Diffuse Coronal "Wave"-Coronal Mass Ejection-Dimming Event
DOI: 10.1088/0004-637X/704/2/1296 Bibcode: 2009ApJ...704.1296A

Testa, Paola; Attrill, Gemma D. R.; Engell, Alexander J. +2 more

We report on observations of the first diffuse coronal wave detected by Hinode/XRT. The event occurred near the west solar limb on 2007 May 23, originating from active region (AR) 10956 and was associated with a coronal mass ejection (CME) and coronal dimmings. The bright emission forming the coronal wave expanded predominantly to the east and sou…

2009 The Astrophysical Journal
Hinode SOHO 50
Ultradeep Near-Infrared Observations of Goods 850-5
DOI: 10.1088/0004-637X/690/1/319 Bibcode: 2009ApJ...690..319W

Wang, Wei-Hao; Cowie, Lennox L.; Barger, Amy J.

GOODS 850-5 is a hyperluminous radio-faint submillimeter source in the Great Observatories Origins Deep Survey-North. Although it is generally agreed that GOODS 850-5 is at a high redshift, z gsim 4, its exact redshift is unknown. While its stellar spectral energy distribution (SED) suggests z ~ 6, its radio/far-IR (FIR) SED suggests a lower redsh…

2009 The Astrophysical Journal
eHST 50
Spitzer Observations of Extended Lyman-α Clouds in the SSA22 Field
DOI: 10.1088/0004-637X/692/2/1561 Bibcode: 2009ApJ...692.1561W

Egami, E.; Yamada, T.; Matsuda, Y. +5 more

We present the results of a Spitzer IRAC and MIPS 24 µm study of extended Lyman-α clouds (or Lyman-α Blobs, LABs) within the SSA22 filamentary structure at z = 3.09. We detect 6/26 LABs in all IRAC filters, four of which are also detected at 24 µm, and find good correspondence with the 850 µm measurements of Geach et al. An analy…

2009 The Astrophysical Journal
XMM-Newton 50
Bright Strongly Lensed Galaxies at Redshift z ~ 6-7 behind the Clusters Abell 1703 and CL0024+16
DOI: 10.1088/0004-637X/697/2/1907 Bibcode: 2009ApJ...697.1907Z

Ford, H. C.; Infante, L.; Zheng, W. +10 more

We report on the discovery of three bright, strongly lensed objects behind Abell 1703 and CL0024+16 from a dropout search over 25 arcmin2 of deep NICMOS data, with deep ACS optical coverage. They are undetected in the deep ACS images below 8500 Å and have clear detections in the J and H bands. Fits to the ACS, NICMOS, and IRAC data yiel…

2009 The Astrophysical Journal
eHST 50
X-ray Insights into the Physics of Mini-BAL Quasar Outflows
DOI: 10.1088/0004-637X/696/1/924 Bibcode: 2009ApJ...696..924G

Brandt, W. N.; Schneider, Donald P.; Gallagher, S. C. +1 more

We examine the ultraviolet and X-ray properties of 256 radio-quiet Sloan Digital Sky Survey quasars (QSOs) observed in X-rays with Chandra and/or XMM-Newton in order to study the relationship between QSOs with broad C IV absorption lines (BALs; width >2000 km s-1) and those with C IV mini-BALs (here defined to have widths of 1000-200…

2009 The Astrophysical Journal
XMM-Newton 50
The Nature of Optically Dull Active Galactic Nuclei in COSMOS
DOI: 10.1088/0004-637X/706/1/797 Bibcode: 2009ApJ...706..797T

Kartaltepe, Jeyhan S.; Koekemoer, Anton M.; Trump, Jonathan R. +17 more

We present infrared, optical, and X-ray data of 48 X-ray bright, optically dull active galactic nuclei (AGNs) in the COSMOS field. These objects exhibit the X-ray luminosity of an AGN but lack broad and narrow emission lines in their optical spectrum. We show that despite the lack of optical emission lines, most of these optically dull AGNs are no…

2009 The Astrophysical Journal
eHST 50
The 5.25 and 5.7 µm Astronomical Polycyclic Aromatic Hydrocarbon Emission Features
DOI: 10.1088/0004-637X/690/2/1208 Bibcode: 2009ApJ...690.1208B

Tielens, A. G. G. M.; Boersma, C.; Allamandola, L. J. +3 more

Astronomical mid-IR spectra show two minor polycyclic aromatic hydrocarbon (PAH) features at 5.25 and 5.7 µm (1905 and 1754 cm-1) that hitherto have been little studied, but contain information about the astronomical PAH population that complements that of the major emission bands. Here, we report a study involving both laboratory…

2009 The Astrophysical Journal
ISO 50
Implosion in a Coronal Eruption
DOI: 10.1088/0004-637X/696/1/121 Bibcode: 2009ApJ...696..121L

Wang, Haimin; Liu, Rui; Alexander, David

We present the observations of the contraction of the extreme-ultraviolet coronal loops overlying the flaring region during the preheating as well as the early impulsive phase of a GOES class C8.9 flare. During the relatively long, 6 minutes, preheating phase, hard X-ray (HXR) count rates at lower energies (below 25 keV) as well as soft X-ray flux…

2009 The Astrophysical Journal
SOHO 50
Asymmetric Eruptive Filaments
DOI: 10.1088/0004-637X/691/2/1079 Bibcode: 2009ApJ...691.1079L

Liu, Rui; Alexander, David; Gilbert, Holly R.

Filaments are often observed to erupt asymmetrically, during which one leg is fixed to the photosphere (referred to as the anchored leg) while the other undertakes most of the dynamic motions (referred to as the active leg) during the eruptive process. In this paper, we present observations of a group of asymmetric eruptive filaments, in which two…

2009 The Astrophysical Journal
SOHO 50
First Direct Metallicity Measurement Of a Lensed Star-Forming Galaxy at z = 1.7
DOI: 10.1088/0004-637X/699/2/L161 Bibcode: 2009ApJ...699L.161Y

Yuan, T. -T.; Kewley, L. J.

We present the rest-frame optical spectrum of a strongly lensed galaxy at redshift z = 1.7 behind the cluster Abell 1689. We detect the temperature sensitive auroral line [O III] λ4363, which allows the first direct metallicity measurement for galaxies at z > 1. Our high signal-to-noise spectrum indicates that the target is an extremely low met…

2009 The Astrophysical Journal
eHST 50