Search Publications

Millimeter and submillimeter excess emission in M 33 revealed by Planck and LABOCA
DOI: 10.1051/0004-6361/201525816 Bibcode: 2016A&A...590A..56H

Boquien, M.; Kramer, C.; Relaño, M. +6 more

Context. Previous studies have shown the existence of an excess of emission at submillimeter (submm) and millimeter (mm) wavelengths in the spectral energy distribution (SED) of many low-metallicity galaxies. The so-called "submm excess", whose origin remains unknown, challenges our understanding of the dust properties in low-metallicity environme…

2016 Astronomy and Astrophysics
Herschel Planck 26
H II Region Ionization of the Interstellar Medium: A Case Study of NGC 7538
DOI: 10.3847/0004-637X/824/2/125 Bibcode: 2016ApJ...824..125L

Anderson, L. D.; Bania, T. M.; Balser, Dana S. +2 more

Using data from the Green Bank Telescope, we analyze the radio continuum (free-free) and radio recombination line (RRL) emission of the compact H II region NGC 7538 (Sharpless 158). We detect extended radio continuum and hydrogen RRL emission beyond the photodissociation region (PDR) toward the north and east, but a sharp decrease in emission towa…

2016 The Astrophysical Journal
Herschel 26
Cross-correlation between X-Ray and Optical/Near-infrared Background Intensity Fluctuations
DOI: 10.3847/0004-637X/832/2/104 Bibcode: 2016ApJ...832..104M

Luo, Bin; Xue, Yongquan; Koekemoer, Anton +3 more

Angular power spectra of optical and infrared background anisotropies at wavelengths between 0.5 and 5 µm are a useful probe of faint sources present during reionization, in addition to faint galaxies and diffuse signals at low redshift. The cross-correlation of these fluctuations with backgrounds at other wavelengths can be used to separate…

2016 The Astrophysical Journal
eHST 26
Relativistic Fe Kα line study in Seyfert 1 galaxies observed with Suzaku
DOI: 10.1093/mnras/stw596 Bibcode: 2016MNRAS.458.4198M

Nandra, K.; Ponti, G.; Mantovani, G.

We present an analysis of a sample of Seyfert 1 galaxies observed with Suzaku. The aim of this work is to examine critically the evidence for a relativistic Fe Kα line in the X-ray spectra of these active galactic nuclei. The sample was compiled from those sources in which a relativistic component was missing in at least one XMM-Newton observation…

2016 Monthly Notices of the Royal Astronomical Society
Suzaku 26
The SOPHIE search for northern extrasolar planets. XI. Three new companions and an orbit update: Giant planets in the habitable zone
DOI: 10.1051/0004-6361/201628331 Bibcode: 2016A&A...591A.146D

Bouchy, F.; Deleuil, M.; Moutou, C. +25 more

We report the discovery of three new substellar companions to solar-type stars, HD 191806, HD 214823, and HD 221585, based on radial velocity measurements obtained at the Haute-Provence Observatory. Data from the SOPHIE spectrograph are combined with observations acquired with its predecessor, ELODIE, to detect and characterise the orbital paramet…

2016 Astronomy and Astrophysics
Hipparcos 25
An alternative validation strategy for the Planck cluster catalogue and y-distortion maps
DOI: 10.1051/0004-6361/201526479 Bibcode: 2016A&A...592A..48K

Khatri, Rishi

We present an all-sky map of the y-type distortion calculated from the full mission Planck High Frequency Instrument (HFI) data using the recently proposed approach to component separation, which is based on parametric model fitting and model selection. This simple model-selection approach enables us to distinguish between carbon monoxide (CO) lin…

2016 Astronomy and Astrophysics
Planck 25
Discovery of Molecular Hydrogen in SN 1987A
DOI: 10.3847/2041-8205/821/1/L5 Bibcode: 2016ApJ...821L...5F

Fransson, Claes; Leibundgut, Bruno; Spyromilio, Jason +3 more

Both CO and SiO have been observed at early and late phases in SN 1987A. H2 was predicted to form at roughly the same time as these molecules, but was not detected at early epochs. Here, we report the detection of NIR lines from H2 at 2.12 and 2.40 µ {{m}} in VLT/SINFONI spectra obtained between days 6489 and 10,120. Th…

2016 The Astrophysical Journal
eHST 25
The variable spin-down rate of the transient magnetar XTE J1810-197
DOI: 10.1093/mnras/stw351 Bibcode: 2016MNRAS.458.2088P

Pintore, Fabio; Mereghetti, Sandro; Esposito, Paolo +7 more

We have analysed XMM-Newton and Chandra observations of the transient magnetar XTE J1810-197 spanning more than 11 yr, from the initial phases of the 2003 outburst to the current quiescent level. We investigated the evolution of the pulsar spin period and we found evidence for two distinct regimes: during the outburst decay, dot{ν } was highly var…

2016 Monthly Notices of the Royal Astronomical Society
XMM-Newton 25
The CDF Archive: Herschel PACS and SPIRE Spectroscopic Data Pipeline and Products for Protostars and Young Stellar Objects
DOI: 10.3847/0004-6256/151/3/75 Bibcode: 2016AJ....151...75G

Larson, Rebecca L.; Lee, Jeong-Eun; Bouwman, Jeroen +6 more

We present the COPS-DIGIT-FOOSH (CDF) Herschel spectroscopy data product archive, and related ancillary data products, along with data fidelity assessments, and a user-created archive in collaboration with the Herschel-PACS and SPIRE ICC groups. Our products include datacubes, contour maps, automated line fitting results, and best 1D spectra produ…

2016 The Astronomical Journal
Herschel 25
Solo dwarfs I: survey introduction and first results for the Sagittarius dwarf irregular galaxy
DOI: 10.1093/mnras/stw257 Bibcode: 2016MNRAS.458.1678H

Côté, P.; Battaglia, G.; Lewis, G. F. +6 more

We introduce the Solitary Local dwarfs survey (Solo), a wide-field photometric study targeting every isolated dwarf galaxy within 3 Mpc of the Milky Way. Solo is based on (u)gi multiband imaging from Canada-France-Hawaii Telescope/MegaCam for northern targets, and Magellan/Megacam for southern targets. All galaxies fainter than MV ≃ -18…

2016 Monthly Notices of the Royal Astronomical Society
eHST 25