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Data reduction pipeline for the Hi-GAL survey
DOI: 10.1111/j.1365-2966.2011.19244.x Bibcode: 2011MNRAS.416.2932T

Natoli, P.; Piacentini, F.; Polenta, G. +13 more

We present the data reduction pipeline for the Herschel Infrared Galactic Plane survey (Hi-GAL). Hi-GAL is a key project of the Herschel satellite, which is mapping the inner part of the Galactic plane (|l| ≤ 70° and |b| ≤ 1°), using two Photodetector Array Camera and Spectrometer (PACS) and three Spectral and Photometric Imaging Receiver (SPIRE) …

2011 Monthly Notices of the Royal Astronomical Society
Herschel 114
Heavy ion escape from Mars, influence from solar wind conditions and crustal magnetic fields
DOI: 10.1016/j.icarus.2011.08.003 Bibcode: 2011Icar..215..475N

Barabash, Stas; Lundin, Rickard; Nilsson, Hans +5 more

We have used more than 4 years of Mars Express ion data to estimate the escape of heavy ions ( O+,O2+ and CO2+) from Mars. To take the limited field of view of the instrument into account, the data has been binned into spatial bins and angular bins to create average distribution functions for different positions in the near Mars space. …

2011 Icarus
MEx 114
Reflection in Seyfert galaxies and the unified model of AGN
DOI: 10.1051/0004-6361/201016409 Bibcode: 2011A&A...532A.102R

Paltani, S.; Walter, R.; Ricci, C. +1 more

We present a deep study of the average hard X-ray spectra of Seyfert galaxies. We aim to test the unified model of active galactic nuclei, and constrain differences and similarities between different classes of objects. We analyzed all public INTEGRAL IBIS/ISGRI data available on all the 165 Seyfert galaxies detected at z < 0.2. Our final sampl…

2011 Astronomy and Astrophysics
INTEGRAL 114
The emission line properties of gravitationally lensed 1.5 < z < 5 galaxies
DOI: 10.1111/j.1365-2966.2010.18161.x Bibcode: 2011MNRAS.413..643R

Richard, Johan; Ellis, Richard; Stark, Daniel P. +3 more

We present and analyse near-infrared spectroscopy for a sample of 28 gravitationally lensed star-forming galaxies in the redshift range 1.5 < z < 5, observed mostly with the Keck II telescope. With typical magnifications of ≃1.5-4 mag, our survey provides a valuable census of star formation rates, gas-phase metallicities and dynamical masses…

2011 Monthly Notices of the Royal Astronomical Society
eHST 114
First Results from the 3D-HST Survey: The Striking Diversity of Massive Galaxies at z > 1
DOI: 10.1088/2041-8205/743/1/L15 Bibcode: 2011ApJ...743L..15V

Schmidt, Kasper B.; van Dokkum, Pieter G.; Franx, Marijn +26 more

We present first results from the 3D-HST program, a near-IR spectroscopic survey performed with the Wide Field Camera 3 (WFC3) on the HST. We have used 3D-HST spectra to measure redshifts and Hα equivalent widths (EW) for a complete, stellar mass-limited sample of 34 galaxies at 1 < z < 1.5 with M star > 1011<…

2011 The Astrophysical Journal
eHST 114
Corona, Jet, and Relativistic Line Models for Suzaku/RXTE/Chandra-HETG Observations of the Cygnus X-1 Hard State
DOI: 10.1088/0004-637X/728/1/13 Bibcode: 2011ApJ...728...13N

Pottschmidt, Katja; Wilms, Jörn; Tramper, Frank +7 more

Using Suzaku and the Rossi X-ray Timing Explorer (RXTE), we have conducted a series of four simultaneous observations of the galactic black hole candidate Cyg X-1 in what were historically faint and spectrally hard "low states." Additionally, all of these observations occurred near superior conjunction with our line of sight to the X-ray source pa…

2011 The Astrophysical Journal
Suzaku 114
Cross-calibration of the X-ray instruments onboard the Chandra, INTEGRAL, RXTE, Suzaku, Swift, and XMM-Newton observatories using G21.5-0.9
DOI: 10.1051/0004-6361/201015597 Bibcode: 2011A&A...525A..25T

Read, A. M.; Guainazzi, M.; Tsujimoto, M. +7 more

Context. For many years, X-ray astronomy missions have used the Crab nebula as a celestial calibration source for the X-ray flux and spectral shape. However, the object is often too bright for current and future missions equipped with instruments with improved sensitivity.
Aims: We use G21.5-0.9, a pulsar-wind nebula with a time-constant powe…

2011 Astronomy and Astrophysics
INTEGRAL Suzaku XMM-Newton 114
Herschel Measurements of Molecular Oxygen in Orion
DOI: 10.1088/0004-637X/737/2/96 Bibcode: 2011ApJ...737...96G

Caselli, Paola; Li, Di; Viti, Serena +32 more

We report observations of three rotational transitions of molecular oxygen (O2) in emission from the H2 Peak 1 position of vibrationally excited molecular hydrogen in Orion. We observed the 487 GHz, 774 GHz, and 1121 GHz lines using the Heterodyne Instrument for the Far Infrared on the Herschel Space Observatory, having veloc…

2011 The Astrophysical Journal
Herschel 113
The DEEP3 Galaxy Redshift Survey: Keck/DEIMOS Spectroscopy in the GOODS-N Field
DOI: 10.1088/0067-0049/193/1/14 Bibcode: 2011ApJS..193...14C

Nandra, Kirpal; Davis, Marc; Juneau, Stéphanie +8 more

We present the results of spectroscopic observations in the GOODS-N field completed using DEIMOS on the Keck II telescope as part of the DEEP3 Galaxy Redshift Survey. Observations of 370 unique targets down to a limiting magnitude of R AB = 24.4 yielded 156 secure redshifts. In addition to redshift information, we provide sky-subtracted…

2011 The Astrophysical Journal Supplement Series
eHST 113
The Be Star Spectra (BeSS) Database
DOI: 10.1088/0004-6256/142/5/149 Bibcode: 2011AJ....142..149N

Neiner, C.; Floquet, M.; de Batz, B. +3 more

Be stars vary on many timescales, from hours to decades. A long time base of observations to analyze certain phenomena in these stars is therefore necessary. Collecting all existing and future Be star spectra into one database has thus emerged as an important tool for the Be star community. Moreover, for statistical studies, it is useful to have c…

2011 The Astronomical Journal
IUE 113