Search Publications

Evolution of mid-infrared galaxy luminosity functions from the entire AKARI NEP deep field with new CFHT photometry
DOI: 10.1093/mnras/stv1411 Bibcode: 2015MNRAS.452.1684G

Goto, Tomotsugu; Kim, Seong Jin; Burgarella, Denis +22 more

We present infrared (IR) galaxy luminosity functions (LFs) in the AKARI North Ecliptic Pole (NEP) deep field using recently-obtained, wider Canada-France-Hawaii Telescope (CFHT) optical/near-IR images. AKARI has obtained deep images in the mid-infrared (IR), covering 0.6 deg2 of the NEP deep field. However, our previous work was limited…

2015 Monthly Notices of the Royal Astronomical Society
AKARI 18
Do we detect the galactic feedback material in X-ray observations of nearby galaxies? - a case study of NGC 5866
DOI: 10.1093/mnras/stv1701 Bibcode: 2015MNRAS.453.1062L

Li, Jiang-Tao

One of the major sources of the X-ray emitting hot gas around galaxies is the feedback from supernovae (SNe), but most of this metal-enriched feedback material is often not directly detected in X-ray observations. This missing galactic feedback problem is extremely prominent in early-type galaxy bulges, where there is little cool gas to make the T…

2015 Monthly Notices of the Royal Astronomical Society
Suzaku eHST 18
On the diffuse X-ray emission from the Wolf-Rayet bubble NGC 2359
DOI: 10.1093/mnras/stu2163 Bibcode: 2015MNRAS.446.1083T

Gruendl, R. A.; Chu, Y. -H.; Guerrero, M. A. +1 more

A recent XMM-Newton observation has revealed diffuse X-ray emission inside the nebula NGC 2359 around the Wolf-Rayet star WR 7. Taking advantage of an improved point-source rejection and background subtraction, and a detailed comparison of optical and X-ray morphology, we have reanalysed these X-ray observations. Our analysis reveals diffuse X-ray…

2015 Monthly Notices of the Royal Astronomical Society
XMM-Newton 18
The evolution of disc galaxies with and without classical bulges since z ∼ 1
DOI: 10.1093/mnras/stv931 Bibcode: 2015MNRAS.451....2S

Sachdeva, Sonali; Saha, Kanak; Gadotti, Dimitri A. +1 more

Establishing relative role of internally and externally driven mechanisms responsible for disc and bulge growth is essential to understand the evolution of disc galaxies. In this context, we have studied the physical properties of disc galaxies without classical bulges in comparison to those with classical bulges since z ∼ 0.9. Using images from t…

2015 Monthly Notices of the Royal Astronomical Society
eHST 18
The X-ray properties of weak-lensing-selected galaxy clusters
DOI: 10.1093/mnras/stu2679 Bibcode: 2015MNRAS.447.3044G

Birkinshaw, M.; Maughan, B. J.; Massey, R. +4 more

We present the results of an X-ray follow-up campaign targeting 10 weak-lensing (WL)-selected galaxy clusters from a Subaru WL survey. Archival Chandra data exist for two of the clusters, and we obtain dedicated observations of the remaining eight. The WL clusters appear to fit the same scaling relation between X-ray luminosity and temperature as …

2015 Monthly Notices of the Royal Astronomical Society
XMM-Newton 18
New multiwavelength observations of the Of?p star CPD -28° 2561
DOI: 10.1093/mnras/stu2516 Bibcode: 2015MNRAS.447.1885H

Ilyin, I.; Hubrig, S.; Ignace, R. +7 more

A rather strong mean longitudinal magnetic field of the order of a few hundred gauss was detected a few years ago in the Of?p star CPD -28° 2561 using FORS2 (FOcal Reducer low dispersion Spectrograph 2) low-resolution spectropolarimetric observations. In this work, we present additional low-resolution spectropolarimetric observations obtained duri…

2015 Monthly Notices of the Royal Astronomical Society
Suzaku 18
A deep look at the nuclear region of UGC 5101 through high angular resolution mid-IR data with GTC/CanariCam
DOI: 10.1093/mnras/stv2134 Bibcode: 2015MNRAS.454.3577M

Esquej, P.; Hernán-Caballero, A.; Aretxaga, I. +13 more

We present an analysis of the nuclear infrared (IR, 1.6-18 µm) emission of the ultraluminous IR galaxy UGC 5101 to derive the properties of its active galactic nucleus (AGN) and its obscuring material. We use new mid-IR high angular resolution (0.3-0.5 arcsec) imaging using the Si-2 filter (λC = 8.7 µm) and 7.5-13 µm s…

2015 Monthly Notices of the Royal Astronomical Society
eHST 18
Detailed afterglow modelling and host galaxy properties of the dark GRB 111215A
DOI: 10.1093/mnras/stu2407 Bibcode: 2015MNRAS.446.4116V

Kouveliotou, C.; Wijers, R. A. M. J.; Fynbo, J. P. U. +13 more

Gamma-ray burst (GRB) 111215A was bright at X-ray and radio frequencies, but not detected in the optical or near-infrared (nIR) down to deep limits. We have observed the GRB afterglow with the Westerbork Synthesis Radio Telescope and Arcminute Microkelvin Imager at radio frequencies, with the William Herschel Telescope and Nordic Optical Telescope…

2015 Monthly Notices of the Royal Astronomical Society
eHST 18
The local stellar luminosity function and mass-to-light ratio in the near-infrared
DOI: 10.1093/mnras/stv858 Bibcode: 2015MNRAS.451..149J

Rybizki, J.; Dettbarn, C.; Jahreiß, H. +3 more

A new sample of stars, representative of the solar neighbourhood luminosity function (LF), is constructed from the Hipparcos catalogue and the Fifth Catalogue of Nearby Stars. We have cross-matched to sources in the Two Micron All Sky Survey catalogue so that for all stars individually determined near-infrared (NIR) photometry is available on a ho…

2015 Monthly Notices of the Royal Astronomical Society
Hipparcos 18
Dynamical analysis of galaxy cluster merger Abell 2146
DOI: 10.1093/mnras/stv1831 Bibcode: 2015MNRAS.453.2718W

Clowe, D. I.; Fabian, A. C.; McNamara, B. R. +12 more

We present a dynamical analysis of the merging galaxy cluster system Abell 2146 using spectroscopy obtained with the Gemini Multi-Object Spectrograph on the Gemini North telescope. As revealed by the Chandra X-ray Observatory, the system is undergoing a major merger and has a gas structure indicative of a recent first core passage. The system pres…

2015 Monthly Notices of the Royal Astronomical Society
eHST 17