Search Publications

Near-infrared Emission Spectrum of WASP-103b Using Hubble Space Telescope/Wide Field Camera 3
DOI: 10.3847/1538-3881/153/1/34 Bibcode: 2017AJ....153...34C

Knutson, Heather; Stassun, Keivan G.; Wright, Jason T. +8 more

We present here our observations and analysis of the dayside emission spectrum of the hot Jupiter WASP-103b. We observed WASP-103b during secondary eclipse using two visits of the Hubble Space Telescope with the G141 grism on Wide Field Camera 3 in spatial scan mode. We generated secondary eclipse light curves of the planet in both blended white-l…

2017 The Astronomical Journal
eHST 41
37 GHz observations of narrow-line Seyfert 1 galaxies
DOI: 10.1051/0004-6361/201630257 Bibcode: 2017A&A...603A.100L

Harrison, D. L.; Lähteenmäki, A.; López-Caniego, M. +12 more

Observations performed at Metsähovi Radio Observatory at 37 GHz are presented for a sample of 78 radio-loud and radio-quiet narrow-line Seyfert 1 (NLS1) galaxies, together with additional lower and higher frequency radio data from RATAN-600, Owens Valley Radio Observatory, and the Planck satellite. Most of the data have been gathered between Febru…

2017 Astronomy and Astrophysics
Planck 41
Simultaneous X-ray and radio observations of the radio-mode-switching pulsar PSR B1822-09
DOI: 10.1093/mnras/stw3135 Bibcode: 2017MNRAS.466.1688H

Kuiper, L.; Hermsen, W.; Hessels, J. W. T. +7 more

We report on simultaneous X-ray and radio observations of the radio-mode-switching pulsar PSR B1822-09 with ESA's XMM-Newton and the Westerbork Synthesis Radio Telescope, Giant Metrewave Radio Telescope and Lovell radio telescopes. PSR B1822-09 switches between a radio-bright and radio-quiet mode, and we discovered a relationship between the durat…

2017 Monthly Notices of the Royal Astronomical Society
XMM-Newton 40
The AGN-Star Formation Connection: Future Prospects with JWST
DOI: 10.3847/1538-4357/aa911d Bibcode: 2017ApJ...849..111K

Barro, Guillermo; Santini, Paola; Grogin, Norman A. +13 more

The bulk of the stellar growth over cosmic time is dominated by IR-luminous galaxies at cosmic noon (z=1{--}2), many of which harbor a hidden active galactic nucleus (AGN). We use state-of-the-art infrared color diagnostics, combining Spitzer and Herschel observations, to separate dust-obscured AGNs from dusty star-forming galaxies (SFGs) in the C…

2017 The Astrophysical Journal
Herschel 40
SOHO comets: 20 years and 3000 objects later
DOI: 10.1098/rsta.2016.0257 Bibcode: 2017RSPTA.37560257B

Knight, Matthew M.; Battams, Karl

We present a summary of the more than 3000 sungrazing and near-Sun comets discovered in coronagraph images returned by the Solar and Heliospheric Observatory (SOHO), since its launch in December 1995. We address each of the four main populations of objects observed by SOHO: Kreutz (sungrazing) group, Meyer group, Marsden and Kracht (96P-family) gr…

2017 Philosophical Transactions of the Royal Society of London Series A
Rosetta SOHO 40
Characterization of star-forming dwarf galaxies at 0.1 ≲z ≲ 0.9 in VUDS: probing the low-mass end of the mass-metallicity relation
DOI: 10.1051/0004-6361/201629762 Bibcode: 2017A&A...601A..95C

Maccagni, D.; Schaerer, D.; Castellano, M. +19 more

Context. The study of statistically significant samples of star-forming dwarf galaxies (SFDGs) at different cosmic epochs is essential for the detailed understanding of galaxy assembly and chemical evolution. However, the main properties of this large population of galaxies at intermediate redshift are still poorly known.
Aims: We present the…

2017 Astronomy and Astrophysics
eHST 40
Modeling solar energetic particle events using ENLIL heliosphere simulations
DOI: 10.1002/2017SW001617 Bibcode: 2017SpWea..15..934L

Futaana, Y.; Luhmann, J. G.; Odstrcil, D. +9 more

Solar energetic particle (SEP) event modeling has gained renewed attention in part because of the availability of a decade of multipoint measurements from STEREO and L1 spacecraft at 1 AU. These observations are coupled with improving simulations of the geometry and strength of heliospheric shocks obtained by using coronagraph images to send erupt…

2017 Space Weather
SOHO 40
Cosmic microwave background constraints for global strings and global monopoles
DOI: 10.1088/1475-7516/2017/07/026 Bibcode: 2017JCAP...07..026L

Lizarraga, Joanes; Urrestilla, Jon; Hindmarsh, Mark +1 more

We present the first cosmic microwave background (CMB) power spectra from numerical simulations of the global O(N) linear σ-model, with N=2,3, which have global strings and monopoles as topological defects. In order to compute the CMB power spectra we compute the unequal time correlators (UETCs) of the energy-momentum tensor, showing that they fal…

2017 Journal of Cosmology and Astroparticle Physics
Planck 40
Flares, wind and nebulae: the 2015 December mini-outburst of V404 Cygni
DOI: 10.1093/mnrasl/slw222 Bibcode: 2017MNRAS.465L.124M

Ponti, G.; Dhillon, V. S.; Charles, P. A. +22 more

After more than 26 years in quiescence, the black hole transient V404 Cyg went into a luminous outburst in 2015 June, and additional activity was detected in late December of the same year. Here, we present an optical spectroscopic follow-up of the December mini-outburst, together with X-ray, optical and radio monitoring that spanned more than a m…

2017 Monthly Notices of the Royal Astronomical Society
INTEGRAL 40
Characterizing the Transition from Diffuse Atomic to Dense Molecular Clouds in the Magellanic Clouds with [C II], [C I], and CO
DOI: 10.3847/1538-4357/aa683a Bibcode: 2017ApJ...839..107P

Ott, Jürgen; Hughes, Annie; Wong, Tony +8 more

We present and analyze deep Herschel/HIFI observations of the [C II] 158 µm, [C I] 609 µm, and [C I] 370 µm lines toward 54 lines of sight in the Large Magellanic Cloud (LMC) and Small Magellanic Cloud (SMC). These observations are used to determine the physical conditions of the line-emitting gas, which we use to study the trans…

2017 The Astrophysical Journal
Herschel 40