Search Publications

Three New Cool Brown Dwarfs Discovered with the Wide-field Infrared Survey Explorer (WISE) and an Improved Spectrum of the Y0 Dwarf WISE J041022.71+150248.4
DOI: 10.1088/0004-6256/147/5/113 Bibcode: 2014AJ....147..113C

Gould, Andrew; Cushing, Michael C.; Kirkpatrick, J. Davy +3 more

As part of a larger search of Wide-field Infrared Survey Explorer (WISE) data for cool brown dwarfs with effective temperatures less than 1000 K, we present the discovery of three new cool brown dwarfs with spectral types later than T7. Using low-resolution, near-infrared spectra obtained with the NASA Infrared Telescope Facility and the Hubble Sp…

2014 The Astronomical Journal
eHST 56
Water in star-forming regions with Herschel (WISH). V. The physical conditions in low-mass protostellar outflows revealed by multi-transition water observations
DOI: 10.1051/0004-6361/201424267 Bibcode: 2014A&A...572A..21M

Liseau, R.; van Dishoeck, E. F.; Bergin, E. A. +17 more

Context. Outflows are an important part of the star formation process as both the result of ongoing active accretion and one of the main sources of mechanical feedback on small scales. Water is the ideal tracer of these effects because it is present in high abundance for the conditions expected in various parts of the protostar, particularly the o…

2014 Astronomy and Astrophysics
Herschel 56
Whistler mode waves at magnetotail dipolarization fronts
DOI: 10.1002/2014JA019892 Bibcode: 2014JGRA..119.2605V

André, M.; Vaivads, A.; Khotyaintsev, Yu. V. +3 more

We report the statistics of whistler mode waves observed in relation to dipolarization fronts (DFs) in Earth's magnetotail using data from the four Cluster spacecraft spanning a period of 9 years, 2001-2009. We show that whistler mode waves are common in a vicinity of DFs: between 30 and 60% of all DFs are associated with whistlers. Whistlers are …

2014 Journal of Geophysical Research (Space Physics)
Cluster 56
Constraints on the merging channel of massive galaxies since z ∼ 1
DOI: 10.1093/mnras/stu1425 Bibcode: 2014MNRAS.444..906F

Hernán-Caballero, A.; Cava, A.; Pérez-González, P. G. +8 more

We probe the merging channel of massive galaxies over the z = 0.3-1.3 redshift window by studying close pairs in a sample of 238 galaxies with stellar mass ≳1011 M, from the SHARDS (Survey for High-z Absorption Red and Dead Sources) survey. SHARDS provides medium-band photometry equivalent to low-resolution optical spectra (…

2014 Monthly Notices of the Royal Astronomical Society
eHST 56
Two estimates of the distance to the Galactic Centre
DOI: 10.1093/mnras/stu631 Bibcode: 2014MNRAS.441.1105F

Francis, Charles; Anderson, Erik

We use recently updated globular cluster distances to estimate the distance to the Galactic Centre, finding 7.4 ± 0.2|stat ± 0.2|sys kpc from symmetry considerations, including a trough at the Galactic Centre and peaks denoting the position of the bar. We recalibrate the red clump magnitude from Hipparcos stars, finding a ske…

2014 Monthly Notices of the Royal Astronomical Society
Hipparcos 56
The Distribution of Polarized Radio Sources >15 µJy in GOODS-N
DOI: 10.1088/0004-637X/785/1/45 Bibcode: 2014ApJ...785...45R

Owen, F. N.; Rudnick, L.

We present deep Very Large Array observations of the polarization of radio sources in the GOODS-N field at 1.4 GHz at resolutions of 1.''6 and 10''. At 1.''6, we find that the peak flux cumulative number count distribution is N(> p) ~ 45*(p/30 µJy)-0.6 per square degree above a detection threshold of 14.5 µJy. This repres…

2014 The Astrophysical Journal
eHST 56
Hubble Space Telescope Grism Spectroscopy of Extreme Starbursts across Cosmic Time: The Role of Dwarf Galaxies in the Star Formation History of the Universe
DOI: 10.1088/0004-637X/789/2/96 Bibcode: 2014ApJ...789...96A

Martin, Crystal L.; Teplitz, Harry I.; Bunker, Andrew J. +15 more

Near infrared slitless spectroscopy with the Wide Field Camera 3, on board the Hubble Space Telescope, offers a unique opportunity to study low-mass galaxy populations at high redshift (z ~ 1-2). While most high-z surveys are biased toward massive galaxies, we are able to select sources via their emission lines that have very faint continua. We in…

2014 The Astrophysical Journal
eHST 56
Gas inflows towards the nucleus of the active galaxy NGC 7213
DOI: 10.1093/mnras/stt2440 Bibcode: 2014MNRAS.438.3322S

Schnorr-Müller, Allan; Storchi-Bergmann, Thaisa; Nagar, Neil M. +1 more

We present two-dimensional stellar and gaseous kinematics of the inner 0.8 × 1.1 kpc2 of the LINER/Seyfert 1 galaxy NGC 7213, from optical spectra obtained with the Gemini Multi-Object Spectrograph integral field spectrograph on the Gemini South telescope at a spatial resolution of ≈ 60 pc. The stellar kinematics shows an average veloci…

2014 Monthly Notices of the Royal Astronomical Society
eHST 56
ALMA Observations of a Candidate Molecular Outflow in an Obscured Quasar
DOI: 10.1088/0004-637X/790/2/160 Bibcode: 2014ApJ...790..160S

Greene, Jenny E.; Zakamska, Nadia L.; Nesvadba, Nicole P. H. +1 more

We present Atacama Large Millimeter/Submillimeter Array CO (1-0) and CO (3-2) observations of SDSS J135646.10+102609.0, an obscured quasar and ultra-luminous infrared galaxy with two merging nuclei and a known 20 kpc scale ionized outflow. The total molecular gas mass is M_{mol}\approx 9^{+19}_{-6}\times 10^8 M , mostly distributed in …

2014 The Astrophysical Journal
Herschel eHST 56
Planck 2013 results. IV. Low Frequency Instrument beams and window functions
DOI: 10.1051/0004-6361/201321544 Bibcode: 2014A&A...571A...4P

Bernard, J. -P.; Planck Collaboration; Aghanim, N. +207 more

This paper presents the characterization of the in-flight beams, the beam window functions, and the associated uncertainties for the Planck Low Frequency Instrument (LFI). Knowledge of the beam profiles is necessary for determining the transfer function to go from the observed to the actual sky anisotropy power spectrum. The main beam distortions …

2014 Astronomy and Astrophysics
Planck 56