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Overall properties of the Gaia DR1 reference frame
DOI: 10.1051/0004-6361/201730396 Bibcode: 2017A&A...599A.140L

Liu, N.; Zhu, Z.; Liu, J. -C. +1 more


Aims: The first Gaia data release (Gaia DR1) provides 2191 ICRF2 sources with their positions in the auxiliary quasar solution and five astrometric parameters - positions, parallaxes, and proper motions - for stars in common between the Tycho-2 catalogue and Gaia in the joint Tycho-Gaia astrometric solution (TGAS). We aim to analyze the overa…

2017 Astronomy and Astrophysics
Gaia 4
The calibration of read-out-streak photometry in the XMM-Newton Optical Monitor and the construction of a bright-source catalogue
DOI: 10.1093/mnras/stw3121 Bibcode: 2017MNRAS.466.1061P

Carter, M.; Talavera, A.; Page, M. J. +7 more

The dynamic range of the XMM-Newton Optical Monitor (XMM-OM) is limited at the bright end by coincidence loss, the superposition of multiple photons in the individual frames recorded from its micro-channel-plate (MCP) intensified charge-coupled device (CCD) detector. One way to overcome this limitation is to use photons that arrive during the fram…

2017 Monthly Notices of the Royal Astronomical Society
IUE XMM-Newton eHST 4
Disrupted Asteroid P/2016 G1. II. Follow-up Observations from the Hubble Space Telescope
DOI: 10.3847/1538-3881/aa9893 Bibcode: 2017AJ....154..248M

Moreno, F.; Pinilla-Alonso, N.; Licandro, J. +3 more

After the early observations of the disrupted asteroid P/2016 G1 with the 10.4 m Gran Telescopio Canarias (GTC) and modeling of the dust ejecta, we have performed a follow-up observational campaign of this object using the Hubble Space Telescope (HST) during two epochs (2016 June 28 and July 11). The analysis of these HST images with the same mode…

2017 The Astronomical Journal
eHST 4
Astronomical imaging with the X-ray observatory Hitomi
DOI: 10.1016/j.nima.2017.02.023 Bibcode: 2017NIMPA.873...16N

Nakajima, Hiroshi; Hitomi Collaboration

We report an imaging capability of the Japan-led X-ray observatory Hitomi, formerly known as ASTRO-H. It carries four scientific instruments of Soft X-ray Imager (SXI: CCD camera), Hard X-ray Imager (HXI), Soft X-ray Spectrometer, and Soft Gamma-ray Detector, allowing us to perform a wide-band high-sensitive imaging spectroscopy. We highlight the …

2017 Nuclear Instruments and Methods in Physics Research A
Hitomi 4
Measurement of Solar Neutrons on 05 March 2012, Using a Fiber-Type Neutron Monitor Onboard the Attached Payload to the ISS
DOI: 10.1007/s11207-017-1135-y Bibcode: 2017SoPh..292..115K

Masuda, S.; Muraki, Y.; Kawano, H. +3 more

The solar neutron detector Space Environment Data Acquisition Equipment - Attached Payload (SEDA-FIB) onboard the International Space Station (ISS) detected several events from the solar direction associated with three large solar flares observed on 05 (X1.1), 07 (X5.4), and 09 (M6.3) March 2012. In this study, we focus on the interesting event of…

2017 Solar Physics
SOHO 4
Temporal Variations in Solar Irradiance Since 1947
DOI: 10.1007/s11207-017-1128-x Bibcode: 2017SoPh..292..112T

Tebabal, A.; Damtie, B.; Nigussie, M. +1 more

The study of variations in total solar irradiance (TSI) and spectral irradiance is important for understanding how the Sun affects the Earth's climate. A data-driven approach is used in this article to analyze and model the temporal variation of the TSI and Mg II index back to 1947. In both cases, observed data in the time interval of the satellit…

2017 Solar Physics
SOHO 4
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