Search Publications

An X-Ray Flare from 47 Cas
DOI: 10.1088/0004-6256/149/2/47 Bibcode: 2015AJ....149...47P

Karmakar, Subhajeet; Pandey, Jeewan C.

Using XMM-Newton observations, we investigate properties of a flare from the very active but poorly known stellar system 47 Cas. The luminosity at the peak of the flare is found to be 3.54 × 1030 erg {{s}-1}, which is ∼2 times higher than that at a quiescent state. The quiescent state corona of 47 Cas can be represented by tw…

2015 The Astronomical Journal
XMM-Newton 11
A Search for Population III Galaxies in CLASH. I. Singly-imaged Candidates at High Redshift
DOI: 10.1088/0004-637X/804/1/13 Bibcode: 2015ApJ...804...13R

Östlin, Göran; Melinder, Jens; Zitrin, Adi +6 more

Population III (Pop III) galaxies are predicted to exist at high redshifts and may be rendered sufficiently bright for detection with current telescopes when gravitationally lensed by a foreground galaxy cluster. Pop III galaxies that exhibit strong Lyα emission should furthermore be identifiable from broadband photometry because of their unusual …

2015 The Astrophysical Journal
eHST 11
Broadband X-Ray Spectral Investigations of Magnetars, 4U 0142+61, 1E 1841-045,1E 2259+586, AND 1E 1048.1-5937
DOI: 10.1088/0004-637X/815/1/15 Bibcode: 2015ApJ...815...15W

Göğüş, Ersin; Weng, Shan-Shan

We have generated an extended version of a rather simplified but physically oriented three-dimensional magnetar emission model, STEMS3D, to allow spectral investigations up to 100 keV. We then applied our model to the broadband spectra of four magnetars: 4U 0142+61, 1E 1841-045, 1E 2259+586, and 1E 1048.1-5937, using data collected with Swift/XRT …

2015 The Astrophysical Journal
XMM-Newton 11
Exploration of quasars with the Gaia mission
DOI: 10.1051/0004-6361/201323280 Bibcode: 2015A&A...574A..46P

Wambsganss, Joachim; Proft, Svea

We analyze the opportunities in and limits to investigating quasars with the Gaia satellite by studying Gaia's low- and high-resolution quasar spectra, with consideration of their signal-to-noise ratios. Furthermore, we explore bright quasars from the Sloan Digital Sky Survey with broad emission lines (BELs) redshifted into the spectral range of G…

2015 Astronomy and Astrophysics
Gaia 11
Dynamic SEP event probability forecasts
DOI: 10.1002/2015SW001222 Bibcode: 2015SpWea..13..665K

Kahler, S. W.; Ling, A.

The forecasting of solar energetic particle (SEP) event probabilities at Earth has been based primarily on the estimates of magnetic free energy in active regions and on the observations of peak fluxes and fluences of large (≥ M2) solar X-ray flares. These forecasts are typically issued for the next 24 h or with no definite expiration time, which …

2015 Space Weather
SOHO 11
Magnesium-rich Ejecta in the SNR G284.3-1.8 Around the High-mass Gamma-Ray Binary 1FGL J1018.6-5856
DOI: 10.1088/2041-8205/808/1/L19 Bibcode: 2015ApJ...808L..19W

Pavlov, George G.; Kargaltsev, Oleg; Rangelov, Blagoy +1 more

We present results from two Chandra observations of the 16.6 day X-ray/γ-ray high-mass binary 1FGL J1018.6-5856 located at the center of the supernova remnant (SNR) G284.3-1.8. The binary spectra, separated by 0.25 in binary phase, are fit with an absorbed power-law model with {{Γ }}≈ 1.7-1.8 for both observations (the flux during the second obser…

2015 The Astrophysical Journal
XMM-Newton 11
Herschel-PACS observations of discs in the η Chamaeleontis association
DOI: 10.1051/0004-6361/201526584 Bibcode: 2015A&A...584A..22R

Dent, W. R. F.; Kamp, I.; Montesinos, B. +6 more

Context. Protoplanetary discs are the birthplace of planets. Studying protoplanetary discs is the key to constraining theories of planet formation. By observing dust and gas in associations at different ages we can study the evolution of these discs, their clearing timescales, and their physical and geometrical properties.The stellar association η…

2015 Astronomy and Astrophysics
AKARI Herschel 11
Two Populations of Old Star Clusters in the Spiral Galaxy M101 Based on HST/ACS Observations
DOI: 10.1088/0004-637X/805/2/160 Bibcode: 2015ApJ...805..160S

Whitmore, Bradley C.; Chandar, Rupali; Simanton, Lesley A.

We present a new photometric catalog of 326 candidate globular clusters (GCs) in the nearby spiral galaxy M101, selected from B, V, and I Hubble Space Telescope Advanced Camera for Surveys images. The luminosity function (LF) of these clusters has an unusually large number of faint sources compared with GCLFs in many other spiral galaxies. Accordi…

2015 The Astrophysical Journal
eHST 11
Total mass of six quiescent prominences estimated from their multi-spectral observations
DOI: 10.1051/0004-6361/201423513 Bibcode: 2015A&A...574A..62S

Heinzel, P.; Golub, L.; Schwartz, P. +4 more

Context. Total masses of six solar prominences were estimated using prominence multi-spectral observations (in EUV, X-rays, Hα, and Ca ii H). The observations were made during the observing campaign from April through June 2011.
Aims: The aim of the work was to apply a complex method for the prominence mass estimations that can be used later …

2015 Astronomy and Astrophysics
Hinode 11
The Atacama Cosmology Telescope: The LABOCA/ACT Survey of Clusters at All Redshifts
DOI: 10.1088/0004-637X/803/2/79 Bibcode: 2015ApJ...803...79L

Hilton, Matt; Sifón, Cristóbal; Bond, J. Richard +24 more

We present a multi-wavelength analysis of 11 Sunyaev-Zel’dovich effect (SZE)-selected galaxy clusters (10 with new data) from the Atacama Cosmology Telescope (ACT) southern survey. We have obtained new imaging from the Large APEX Bolometer Camera (345 GHz; LABOCA) on the Atacama Pathfinder EXperiment (APEX) telescope, the Australia Telescope Compa…

2015 The Astrophysical Journal
Herschel Planck 11