Search Publications

Testing the Unification Model for Active Galactic Nuclei in the Infrared: Are the Obscuring Tori of Type 1 and 2 Seyferts Different?
DOI: 10.1088/0004-637X/731/2/92 Bibcode: 2011ApJ...731...92R

Pérez García, A. M.; Díaz-Santos, T.; Packham, C. +7 more

We present new mid-infrared imaging data for three Type-1 Seyfert galaxies obtained with T-ReCS on the Gemini-South Telescope at subarcsecond resolution. Our aim is to enlarge the sample studied in a previous work to compare the properties of Type-1 and Type-2 Seyfert tori using clumpy torus models and a Bayesian approach to fit the infrared (IR) …

2011 The Astrophysical Journal
eHST 188
Planck early results. XX. New light on anomalous microwave emission from spinning dust grains
DOI: 10.1051/0004-6361/201116470 Bibcode: 2011A&A...536A..20P

Kneissl, R.; Miville-Deschênes, M. -A.; Boulanger, F. +213 more

Anomalous microwave emission (AME) has been observed by numerous experiments in the frequency range ~10-60 GHz. Using Planck maps and multi-frequency ancillary data, we have constructed spectra for two known AME regions: the Perseus and ρ Ophiuchi molecular clouds. The spectra are well fitted by a combination of free-free radiation, cosmic microwa…

2011 Astronomy and Astrophysics
Planck 184
The Spin of the Supermassive Black Hole in NGC 3783
DOI: 10.1088/0004-637X/736/2/103 Bibcode: 2011ApJ...736..103B

Nandra, K.; Iwasawa, K.; Fabian, A. C. +9 more

The Suzaku AGN Spin Survey is designed to determine the supermassive black hole spin in six nearby active galactic nuclei (AGNs) via deep Suzaku stares, thereby giving us our first glimpse of the local black hole spin distribution. Here, we present an analysis of the first target to be studied under the auspices of this Key Project, the Seyfert ga…

2011 The Astrophysical Journal
Suzaku 183
The Relationships among Compact Stellar Systems: A Fresh View of Ultracompact Dwarfs
DOI: 10.1088/0004-6256/142/6/199 Bibcode: 2011AJ....142..199B

Forbes, Duncan A.; Romanowsky, Aaron J.; Brodie, Jean P. +1 more

We use a combined imaging and spectroscopic survey of the nearby central cluster galaxy, M87, to assemble a sample of 34 confirmed ultracompact dwarfs (UCDs) with half-light radii of gsim10 pc measured from Hubble Space Telescope images. This doubles the existing sample in M87, making it the largest such sample for any galaxy, while extending the …

2011 The Astronomical Journal
eHST 183
Pan-STARRS1 Discovery of Two Ultraluminous Supernovae at z ≈ 0.9
DOI: 10.1088/0004-637X/743/2/114 Bibcode: 2011ApJ...743..114C

Price, P. A.; Berger, E.; Kirshner, R. P. +29 more

We present the discovery of two ultraluminous supernovae (SNe) at z ≈ 0.9 with the Pan-STARRS1 Medium Deep Survey. These SNe, PS1-10ky and PS1-10awh, are among the most luminous SNe ever discovered, comparable to the unusual transients SN 2005ap and SCP 06F6. Like SN 2005ap and SCP 06F6, they show characteristic high luminosities (M bol

2011 The Astrophysical Journal
eHST 180
Astrometry and Photometry with HST WFC3. II. Improved Geometric-Distortion Corrections for 10 Filters of the UVIS Channel
DOI: 10.1086/659878 Bibcode: 2011PASP..123..622B

Anderson, J.; Bedin, L. R.; Bellini, A.

We present an improved geometric-distortion solution for the Hubble Space Telescope UVIS channel of Wide Field Camera 3 for 10 broadband filters. The solution is made up of three parts: (1) a third-order polynomial to deal with the general optical distortion, (2) a table of residuals that accounts for both chip-related anomalies and fine-structure…

2011 Publications of the Astronomical Society of the Pacific
eHST 179
The Impact of Galaxy Interactions on Active Galactic Nucleus Activity in zCOSMOS
DOI: 10.1088/0004-637X/743/1/2 Bibcode: 2011ApJ...743....2S

Finoguenov, A.; Jahnke, K.; Silverman, J. D. +52 more

Close encounters between galaxies are expected to be a viable mechanism, as predicted by numerical simulations, by which accretion onto supermassive black holes can be initiated. To test this scenario, we construct a sample of 562 galaxies (M * > 2.5 × 1010 M ) in kinematic pairs over the redshift range 0.25 &l…

2011 The Astrophysical Journal
eHST 177
Quasar Accretion Disks are Strongly Inhomogeneous
DOI: 10.1088/2041-8205/727/1/L24 Bibcode: 2011ApJ...727L..24D

Agol, Eric; Dexter, Jason

Active galactic nuclei have been observed to vary stochastically with 10%-20% rms amplitudes over a range of optical wavelengths where the emission arises in an accretion disk. Since the accretion disk is unlikely to vary coherently, local fluctuations may be significantly larger than the global rms variability. We investigate toy models of quasar…

2011 The Astrophysical Journal
eHST 177
Search for brown-dwarf companions of stars
DOI: 10.1051/0004-6361/201015427 Bibcode: 2011A&A...525A..95S

Zucker, S.; Queloz, D.; Sahlmann, J. +7 more

Context. The frequency of brown-dwarf companions in close orbit around Sun-like stars is low compared to the frequency of planetary and stellar companions. There is presently no comprehensive explanation of this lack of brown-dwarf companions.
Aims: By combining the orbital solutions obtained from stellar radial-velocity curves and Hipparcos …

2011 Astronomy and Astrophysics
Hipparcos 176
Gas Clumping in the Outskirts of ΛCDM Clusters
DOI: 10.1088/2041-8205/731/1/L10 Bibcode: 2011ApJ...731L..10N

Nagai, Daisuke; Lau, Erwin T.

Recent Suzaku X-ray observations revealed that the observed entropy profile of the intracluster medium (ICM) deviates significantly from the prediction of hydrodynamical simulations of galaxy clusters. In this work, we show that gas clumping introduces significant biases in X-ray measurements of the ICM profiles in the outskirts of galaxy clusters…

2011 The Astrophysical Journal
Suzaku 176