Search Publications

Quasi Periodic Oscillations in Blazars
DOI: 10.1007/s12036-014-9219-7 Bibcode: 2014JApA...35..307G

Gupta, Alok C.

Here we report our recent discoveries of Quasi-Periodic Oscillations (QPOs) in blazars time series data in X-ray and optical electromagnetic bands. Any such detection can give important clue of the location and nature of the processes of emission mechanism. In the case of radio-quiet AGN, the detected QPOs are very likely to be associated with the…

2014 Journal of Astrophysics and Astronomy
XMM-Newton 31
Archival legacy investigations of circumstellar environments: overview and first results
DOI: 10.1117/12.2056672 Bibcode: 2014SPIE.9143E..57C

Schneider, Glenn; Hines, Dean C.; Perrin, Marshall D. +12 more

We are currently conducting a comprehensive and consistent re-processing of archival HST-NICMOS coronagraphic surveys using advanced PSF subtraction methods, entitled the Archival Legacy Investigations of Circumstellar Environments program (ALICE, HST/AR 12652). This virtual campaign of about 400 targets has already produced numerous new detection…

2014 Space Telescopes and Instrumentation 2014: Optical, Infrared, and Millimeter Wave
eHST 31
Drainage systems of Lonar Crater, India: Contributions to Lonar Lake hydrology and crater degradation
DOI: 10.1016/j.pss.2013.05.011 Bibcode: 2014P&SS...95...45K

Sekine, Yasuhito; Matsui, Takafumi; Komatsu, Goro +3 more

Lonar, a 1.8-km-diameter impact crater in India, is a rare example of terrestrial impact craters formed in basaltic bedrock. The estimated age of the crater ranges widely from less than 12 ka to over 600 ka, but the crater preserves a relatively pristine morphology. We conducted a study of various drainage systems of Lonar Crater. The crater floor…

2014 Planetary and Space Science
MEx 31
Modeling the microphysics of CO2 ice clouds within wave-induced cold pockets in the martian mesosphere
DOI: 10.1016/j.icarus.2014.04.022 Bibcode: 2014Icar..237..239L

Montmessin, F.; Spiga, A.; Lefèvre, F. +2 more

Mesospheric CO2 ice clouds on Mars are simulated with a 1D microphysical model, which includes a crystal growth rate adapted to high supersaturations encountered in the martian mesosphere. Observational constraints (crystal radius and opacity) exist for these clouds observed during the day around the equator at ∼60-80 km altitude. Night…

2014 Icarus
MEx 31
Halo Mass Dependence of H I and O VI Absorption: Evidence for Differential Kinematics
DOI: 10.1088/0004-637X/792/2/128 Bibcode: 2014ApJ...792..128M

Kacprzak, Glenn G.; Churchill, Christopher W.; Nielsen, Nikole M. +4 more

We studied a sample of 14 galaxies (0.1 < z < 0.7) using HST/WFPC2 imaging and high-resolution HST/COS or HST/STIS quasar spectroscopy of Lyα, Lyβ, and O VI λλ1031, 1037 absorption. The galaxies, having 10.8 <= log (M h/M ) <= 12.2, lie within D = 300 kpc of quasar sightlines, probing out to D/R vir =…

2014 The Astrophysical Journal
eHST 31
The pointing system of the Herschel space observatory. Description, Calibration, Performance and improvements
DOI: 10.1007/s10686-014-9396-z Bibcode: 2014ExA....37..453S

Marston, Anthony; Linz, Hendrik; Merín, Bruno +13 more

We present the activities carried out to calibrate and characterise the performance of the elements of attitude control and measurement on board the Herschel spacecraft. The main calibration parameters and the evolution of the indicators of the pointing performance are described, from the initial values derived from the observations carried out in…

2014 Experimental Astronomy
Herschel 31
HerMES: Spectral Energy Distributions of Submillimeter Galaxies at z > 4
DOI: 10.1088/0004-637X/784/1/52 Bibcode: 2014ApJ...784...52H

Bock, J. J.; Clements, D. L.; Burgarella, D. +20 more

We present a study of the infrared properties for a sample of seven spectroscopically confirmed submillimeter galaxies (SMGs) at z > 4.0. By combining ground-based near-infrared, Spitzer IRAC and MIPS, Herschel SPIRE, and ground-based submillimeter/millimeter photometry, we construct their spectral energy distributions (SEDs) and a composite mo…

2014 The Astrophysical Journal
Herschel 31
The NUV-r versus Mr Plane as a Tracer of Early-type Galaxy Evolution in the USGC U376 and LGG 225 Groups
DOI: 10.1088/0004-637X/782/1/53 Bibcode: 2014ApJ...782...53M

Mazzei, Paola; Rampazzo, Roberto; Marino, Antonietta

With the aim of tracing back the evolution of galaxies in nearby groups, we use smooth particle hydrodynamical (SPH) simulations with chemo-photometric implementation. Here, we focus on the evolution of the early-type members (Es and S0s; ETGs hereafter) in two groups, USGC U376 and LGG 225, both in the Leo cloud. We use the near-UV (NUV)-optical …

2014 The Astrophysical Journal
AKARI 31
Fermi-LAT Observations of Supernova Remnants Kesteven 79
DOI: 10.1088/0004-637X/783/1/32 Bibcode: 2014ApJ...783...32A

Auchettl, Katie; Slane, Patrick; Castro, Daniel

In this paper, we report on the detection of γ-ray emission coincident with the Galactic supernova remnant (SNR) Kesteven 79 (Kes 79). We analyzed approximately 52 months of data obtained with the Large Area Telescope on board the Fermi Gamma-ray Space Telescope. Kes 79 is thought to be interacting with adjacent molecular clouds, based on the pres…

2014 The Astrophysical Journal
XMM-Newton 31
Accounting for Cosmic Variance in Studies of Gravitationally Lensed High-redshift Galaxies in the Hubble Frontier Field Clusters
DOI: 10.1088/2041-8205/796/2/L27 Bibcode: 2014ApJ...796L..27R

Ellis, Richard S.; Robertson, Brant E.; Dunlop, James S. +3 more

Strong gravitational lensing provides a powerful means for studying faint galaxies in the distant universe. By magnifying the apparent brightness of background sources, massive clusters enable the detection of galaxies fainter than the usual sensitivity limit for blank fields. However, this gain in effective sensitivity comes at the cost of a redu…

2014 The Astrophysical Journal
eHST 31