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Herschel -ATLAS: revealing dust build-up and decline across gas, dust and stellar mass selected samples - I. Scaling relations
DOI: 10.1093/mnras/stw2501 Bibcode: 2017MNRAS.464.4680D

Ivison, R. J.; Baes, M.; Baker, A. J. +19 more

We present a study of the dust, stars and atomic gas (H I) in an H I-selected sample of local galaxies (z < 0.035) in the Herschel Astrophysical Terahertz Large Area Survey fields. This H I-selected sample reveals a population of very high gas fraction (>80 per cent), low stellar mass sources that appear to be in the earliest stages of their…

2017 Monthly Notices of the Royal Astronomical Society
Herschel 53
Signatures of Nitrogen Chemistry in Hot Jupiter Atmospheres
DOI: 10.3847/2041-8213/aa97d4 Bibcode: 2017ApJ...850L..15M

Madhusudhan, Nikku; MacDonald, Ryan J.

Inferences of molecular compositions of exoplanetary atmospheres have generally focused on carbon, hydrogen, and oxygen-bearing molecules. Recently, additional absorption in Hubble Space Telescope Wide Field Camera 3 (WFC3) transmission spectra around 1.55 µm has been attributed to nitrogen-bearing chemical species: NH3 or HCN. Th…

2017 The Astrophysical Journal
eHST 53
Surface Gravities for 228 M, L, and T Dwarfs in the NIRSPEC Brown Dwarf Spectroscopic Survey
DOI: 10.3847/1538-4357/aa6338 Bibcode: 2017ApJ...838...73M

Kirkpatrick, J. Davy; Burgasser, Adam J.; Logsdon, Sarah E. +6 more

We combine 131 new medium-resolution (R ∼ 2000) J-band spectra of M, L, and T dwarfs from the Keck NIRSPEC Brown Dwarf Spectroscopic Survey (BDSS) with 97 previously published BDSS spectra to study surface-gravity-sensitive indices for 228 low-mass stars and brown dwarfs spanning spectral types M5-T9. Specifically, we use an established set of spe…

2017 The Astrophysical Journal
Gaia 53
Detection of nanoflare-heated plasma in the solar corona by the FOXSI-2 sounding rocket
DOI: 10.1038/s41550-017-0269-z Bibcode: 2017NatAs...1..771I

Krucker, Säm; Narukage, Noriyuki; Glesener, Lindsay +4 more

The processes that heat the solar and stellar coronae to several million kelvins, compared with the much cooler photosphere (5,800 K for the Sun), are still not well known1. One proposed mechanism is heating via a large number of small, unresolved, impulsive heating events called nanoflares2. Each event would heat and cool qu…

2017 Nature Astronomy
Hinode 53
An Updated 2017 Astrometric Solution for Betelgeuse
DOI: 10.3847/1538-3881/aa6ff9 Bibcode: 2017AJ....154...11H

Kervella, P.; Decin, L.; Richards, A. M. S. +4 more

We provide an update for the astrometric solution for the Type II supernova progenitor Betelgeuse using the revised Hipparcos Intermediate Astrometric Data (HIAD) of van Leeuwen, combined with existing VLA and new e-MERLIN and ALMA positions. The 2007 Hipparcos refined abscissa measurements required the addition of so-called Cosmic Noise of 2.4 ma…

2017 The Astronomical Journal
Hipparcos 52
Gaia16apd - a link between fast and slowly declining type I superluminous supernovae
DOI: 10.1093/mnras/stx833 Bibcode: 2017MNRAS.469.1246K

Lundqvist, P.; Wyrzykowski, Ł.; Kankare, E. +18 more

We present ultraviolet (UV), optical and infrared photometry and optical spectroscopy of the type Ic superluminous supernova (SLSN) Gaia16apd (=SN 2016eay), covering its evolution from 26 d before the g-band peak to 234.1 d after the peak. Gaia16apd was followed as a part of the NOT Unbiased Transient Survey (NUTS). It is one of the closest SLSNe …

2017 Monthly Notices of the Royal Astronomical Society
eHST 52
Assessing distances and consistency of kinematics in Gaia/TGAS
DOI: 10.1093/mnras/stx2189 Bibcode: 2017MNRAS.472.3979S

Schönrich, Ralph; Aumer, Michael

We apply the statistical methods by Schönrich, Binney & Asplund to assess the quality of distances and kinematics in the Radial Velocity Experiment (RAVE)-Tycho-Gaia Astrometric Solution (TGAS) and Large Sky Area Multiobject Fiber Spectroscopic Telescope (LAMOST)-TGAS samples of Solar neighbourhood stars. These methods yield a nominal distance…

2017 Monthly Notices of the Royal Astronomical Society
Gaia 52
Cosmological constraints from thermal Sunyaev-Zeldovich power spectrum revisited
DOI: 10.1093/mnras/stx766 Bibcode: 2017MNRAS.469..394H

Seljak, U.; Horowitz, B.

Thermal Sunyaev-Zeldovich (tSZ) power spectrum is one of the most sensitive methods to constrain cosmological parameters, scaling as the amplitude σ _8^8. It is determined by the integral over the halo mass function multiplied by the total pressure content of clusters and further convolved by the cluster gas pressure profile. It has been shown tha…

2017 Monthly Notices of the Royal Astronomical Society
Planck 52
The Great Observatories All-Sky LIRG Survey: Herschel Image Atlas and Aperture Photometry
DOI: 10.3847/1538-4365/aa5d15 Bibcode: 2017ApJS..229...25C

Sanders, D. B.; Frayer, D. T.; Kim, D. -C. +24 more

Far-infrared images and photometry are presented for 201 Luminous and Ultraluminous Infrared Galaxies [LIRGs: log ({L}{IR}/{L})=11.00{--}11.99, ULIRGs: log ({L}{IR}/{L})=12.00{--}12.99], in the Great Observatories All-Sky LIRG Survey (GOALS), based on observations with the Herschel Space Observatory …

2017 The Astrophysical Journal Supplement Series
Herschel 52
Molecular gas properties of a lensed star-forming galaxy at z 3.6: a case study
DOI: 10.1051/0004-6361/201628513 Bibcode: 2017A&A...605A..81D

Kneib, J. -P.; Schaerer, D.; Rujopakarn, W. +12 more

We report on the galaxy MACSJ0032-arc at zCO = 3.6314 discovered during the Herschel Lensing snapshot Survey of massive galaxy clusters, and strongly lensed by the cluster MACS J0032.1+1808. The successful detections of its rest-frame ultraviolet (UV), optical, far-infrared (FIR), millimeter, and radio continua, and of its CO emission e…

2017 Astronomy and Astrophysics
Herschel eHST 52