Search Publications

Reconstruction of the flight and attitude of Rosetta's lander Philae
DOI: 10.1016/j.actaastro.2017.09.017 Bibcode: 2017AcAau.140..509H

Richter, Ingo; Auster, Hans-Ulrich; Heinisch, Philip +14 more

Since Rosetta's lander Philae touched down on comet 67P/Churyumov-Gerasimenko on November 12, 2014, many tools have been applied to reconstruct Philae's flight path and attitude between separation, the touchdowns, collision and the final landing at Abydos. In addition to images from the cameras onboard both orbiter and lander (;OSIRIS;, ;CIVA; and…

2017 Acta Astronautica
Rosetta 4
Detecting periodic oscillations in astronomy data: revisiting wavelet analysis with coloured and white noise
DOI: 10.1093/mnras/stw3349 Bibcode: 2017MNRAS.466.3827X

Xu, Chang

The intrinsic random variability of an astronomical source hampers the detection of possible periodicities that we are interested in. We find that a simple first-order autoregressive [AR(1)] process gives a poor fit to the power decay in the observed spectrum for astrophysical sources and geodetic observations. Thus, appropriate background noise m…

2017 Monthly Notices of the Royal Astronomical Society
XMM-Newton 4
Validation of the CME Geomagnetic Forecast Alerts Under the COMESEP Alert System
DOI: 10.1007/s11207-017-1120-5 Bibcode: 2017SoPh..292...96D

Dumbović, Mateja; Vršnak, Bojan; Rao, Yamini K. +3 more

Under the European Union 7th Framework Programme (EU FP7) project Coronal Mass Ejections and Solar Energetic Particles (COMESEP, http://comesep.aeronomy.be), an automated space weather alert system has been developed to forecast solar energetic particles (SEP) and coronal mass ejection (CME) risk levels at Earth. The COMESEP alert system uses the …

2017 Solar Physics
SOHO 4
Catalogue of Astrometric Positions of Jupiter's Outer Satellites on Photographic Observations in Mao NAS of Ukraine in 1987-1993
DOI: 10.18524/1810-4215.2017.30.114529 Bibcode: 2017OAP....30..201Y

Yizhakevych, O.; Andruk, V.; Pakuliak, L.

The catalog of 33 topocentric positions of Jupiter's moons J6, J7, J8 has been created on photographic observations made in MAO NASU in 1987-1993. Positions are referred to the system of TYCHO-2 using the program package INUX/MIDAS/ROMAFOT. The comparison of observed positions was made online with their theoretical data of IMCCE (www.imcce.fr/sat).

2017 Odessa Astronomical Publications
Hipparcos 4
Future perspectives for abundance measurements in clusters of galaxies with XMM-Newton
DOI: 10.1002/asna.201713346 Bibcode: 2017AN....338..299D

Mernier, F.; de Plaa, J.

The CHEERS (CHEmical enrichment reflection grating spectrometer sample) observations of clusters of galaxies with XMM-Newton have shown to be valuable to constrain the chemical evolution of the universe. The soft X-ray spectrum contains lines of the most abundant metals from N to Ni, which provide relatively accurate abundances that can be compare…

2017 Astronomische Nachrichten
XMM-Newton 4
Kepler Data on KIC 7341653: A Nearby M Dwarf with Monster Flares and a Phase-coherent Variability
DOI: 10.3847/1538-4357/aa7d06 Bibcode: 2017ApJ...845..149M

Makarov, Valeri V.; Goldin, Alexey

KIC 7341653 is one of several late-type M dwarfs observed by the main mission of Kepler with peculiar infrared colors placing them in the domain of suspected young stellar objects (YSO). It is likely associated with a powerful X-ray emitter with X-ray flares. Kepler light curves reveal two distinct types of activity: frequent flares lasting from l…

2017 The Astrophysical Journal
Gaia 4
Proper motions of five OB stars with candidate dusty bow shocks in the Carina Nebula
DOI: 10.1093/mnras/stx607 Bibcode: 2017MNRAS.468.2469K

Smith, Nathan; Bally, John; Reiter, Megan +1 more

We constrain the proper motions of five OB stars associated with candidate stellar wind bow shocks in the Carina Nebula using Hubble Space Telescope ACS imaging over 9-10 yr baselines. These proper motions allow us to directly compare each star's motion to the orientation of its candidate bow shock. Although these stars are saturated in our imagin…

2017 Monthly Notices of the Royal Astronomical Society
Gaia eHST 4
The MEXSAS2 Sample and the Ensemble X-ray Variability of Quasars
DOI: 10.3389/fspas.2017.00021 Bibcode: 2017FrASS...4...21S

Serafinelli, Roberto; Middei, Riccardo; Chiaraluce, Elia +1 more

We present the second Multi-Epoch X-ray Serendipitous AGN Sample (MEXSAS2), extracted from the 6th release of the XMM Serendipitous Source Catalogue release (XMMSSC-DR6), cross-matched with Sloan Digital Sky Survey quasar catalogues DR7Q and DR12Q. Our sample also includes the available measurements for masses, bolometric luminosities, and Eddingt…

2017 Frontiers in Astronomy and Space Sciences
XMM-Newton 4
A New Look at the Integrated Radio/Microwave Continuum Spectrum of Galactic Supernova Remnant IC 443
DOI: 10.3847/1538-3881/153/1/32 Bibcode: 2017AJ....153...32O

Onić, D.; Leahy, D.; Urošević, D.

Recent observations of the microwave sky, by space telescopes such as the Wilkinson Microwave Anisotropy Probe and Planck, have opened a new window into the analysis of continuum emission from supernova remnants (SNRs). In this paper, different emission models that can explain the characteristic shape of currently known integrated radio/microwave …

2017 The Astronomical Journal
Planck 4
X-ray-selected broad absorption line quasi-stellar objects
DOI: 10.1093/mnras/stw2560 Bibcode: 2017MNRAS.464.4586P

Esquej, P.; Streblyanska, A.; Ebrero, J. +11 more

We study a sample of six X-ray-selected broad absorption line (BAL) quasi-stellar objects (QSOs) from the XMM-Newton Wide Angle Survey. All six objects are classified as BALQSOs using the classic balnicity index, and together they form the largest sample of X-ray-selected BALQSOs. We find evidence for absorption in the X-ray spectra of all six obj…

2017 Monthly Notices of the Royal Astronomical Society
XMM-Newton 4