Search Publications

No excess of bright galaxies around the redshift 7.1 quasar ULAS J1120+0641
DOI: 10.1093/mnras/stu1116 Bibcode: 2014MNRAS.442.3454S

Simpson, Chris; Cantalupo, Sebastiano; Venemans, Bram +5 more

We present optical and near-infrared imaging of the field of the z = 7.0842 quasar ULAS J112001.48+064124.3 taken with the Hubble Space Telescope. We use these data to search for galaxies that may be physically associated with the quasar, using the Lyman break technique, and find three such objects, although the detection of one in Spitzer Space T…

2014 Monthly Notices of the Royal Astronomical Society
eHST 44
Hidden starbursts and active galactic nuclei at 0 < z < 4 from the Herschel-VVDS-CFHTLS-D1 field: Inferences on coevolution and feedback
DOI: 10.1051/0004-6361/201323089 Bibcode: 2014A&A...572A..90L

Le Floc'h, E.; Ilbert, O.; Zamorani, G. +12 more

We investigate of the properties of ~2000 Herschel/SPIRE far-infrared-selected galaxies from 0 <z< 4 in the CFHTLS-D1 field. Using a combination of extensive spectroscopy from the VVDS and ORELSE surveys, deep multiwavelength imaging from CFHT, VLA, Spitzer, XMM-Newton, and Herschel, and well-calibrated spectral energy distribution fitting, …

2014 Astronomy and Astrophysics
Herschel 44
Amazonian mid- to high-latitude glaciation on Mars: Supply-limited ice sources, ice accumulation patterns, and concentric crater fill glacial flow and ice sequestration
DOI: 10.1016/j.pss.2013.12.002 Bibcode: 2014P&SS...91...60F

Head, James W.; Fastook, James L.

Concentric crater fill (CCF) occurs in the interior of impact craters in mid- to high latitudes on Mars and is interpreted to have formed by glacial ice flow and debris covering. We use the characteristics and orientation of deposits comprising CCF, the thickness of pedestal deposits in mid- to high-latitude pedestal craters (Pd), the volumes of t…

2014 Planetary and Space Science
MEx 44
The UBV Color Evolution of Classical Novae. I. Nova-giant Sequence in the Color-Color Diagram
DOI: 10.1088/0004-637X/785/2/97 Bibcode: 2014ApJ...785...97H

Kato, Mariko; Hachisu, Izumi

We identified a general course of classical nova outbursts in the B - V versus U - B color-color diagram. It is reported that novae show spectra similar to those of A-F supergiants near optical light maximum. However, they do not follow the supergiant sequence in the color-color diagram, neither the blackbody nor the main-sequence sequence. Instea…

2014 The Astrophysical Journal
IUE 44
Radiative and mechanical feedback into the molecular gas of NGC 253
DOI: 10.1051/0004-6361/201323109 Bibcode: 2014A&A...564A.126R

van der Werf, P. P.; Güsten, R.; Requena-Torres, M. A. +5 more

Starburst galaxies are galaxies or regions of galaxies undergoing intense periods of star formation. Understanding the heating and cooling mechanisms in these galaxies can give us insight to the driving mechanisms that fuel the starburst. Molecular emission lines play a crucial role in the cooling of the excited gas. With Herschel Spectral and Pho…

2014 Astronomy and Astrophysics
Herschel 44
The Onset of Massive Star Formation: The Evolution of Temperature and Density Structure in an Infrared Dark Cloud
DOI: 10.1088/0004-637X/787/2/113 Bibcode: 2014ApJ...787..113B

Ginsburg, Adam; Battersby, Cara; Bally, John +3 more

We present new NH3 (1, 1), (2, 2), and (4, 4) observations from the Karl G. Jansky Very Large Array compiled with work in the literature to explore the range of conditions observed in young, massive star-forming regions. To sample the effects of evolution independent from those of distance/resolution, abundance, and large-scale environm…

2014 The Astrophysical Journal
Herschel 44
Supernova Remnant W49B and Its Environment
DOI: 10.1088/0004-637X/793/2/95 Bibcode: 2014ApJ...793...95Z

Zhu, H.; Tian, W. W.; Zuo, P.

We study gamma-ray supernova remnant (SNR) W49B and its environment using recent radio and infrared data. Spitzer Infrared Spectrograph low resolution data of W49B shows shocked excitation lines of H2 (0,0) S(0)-S(7) from the SNR-molecular cloud interaction. The H2 gas is composed of two components with temperatures of ~260 K…

2014 The Astrophysical Journal
Herschel 44
Discovery of Time Variation of the Intensity of Molecular Lines in IRC+10216 in the Submillimeter and Far-Infrared Domains
DOI: 10.1088/2041-8205/796/1/L21 Bibcode: 2014ApJ...796L..21C

Teyssier, D.; García-Lario, P.; Barlow, M. J. +12 more

We report on the discovery of strong intensity variations in the high rotational lines of abundant molecular species toward the archetypical circumstellar envelope of IRC+10216. The observations have been carried out with the Heterodyne Instrument for the Far-Infrared (HIFI) instrument on board Herschel and with the IRAM30 m telescope. They cover …

2014 The Astrophysical Journal
Herschel 44
Neutrino constraints: what large-scale structure and CMB data are telling us?
DOI: 10.1088/1475-7516/2014/10/081 Bibcode: 2014JCAP...10..081C

Viel, Matteo; Sartoris, Barbara; Costanzi, Matteo +1 more

We discuss the reliability of neutrino mass constraints, either active or sterile, from the combination of different low redshift Universe probes with measurements of CMB anisotropies. In our analyses we consider WMAP 9-year or Planck Cosmic Microwave Background (CMB) data in combination with Baryonic Acoustic Oscillations (BAO) measurements from …

2014 Journal of Cosmology and Astroparticle Physics
Planck 44
Joint astrometric solution of HIPPARCOS and Gaia. A recipe for the Hundred Thousand Proper Motions project
DOI: 10.1051/0004-6361/201424606 Bibcode: 2014A&A...571A..85M

Michalik, Daniel; Lindegren, Lennart; Hobbs, David +1 more

Context. The first release of astrometric data from Gaia is expected in 2016. It will contain the mean stellar positions and magnitudes from the first year of observations. For more than 100 000 stars in common with the Hipparcos Catalogue it will be possible to compute very accurate proper motions due to the time difference of about 24 years betw…

2014 Astronomy and Astrophysics
Gaia Hipparcos 44