Galactic plane maps, 150 and 100-GHz T difference
Maser hunting in the galactic plane
... Out of the twenty-five 44 GHz masers detected, 23 were re-observed with pointed observations 17 months later. We found that a significant number of the masers varied, 15 (65%) of the masers showed variation in the ...
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Stellar variability near the galactic mid-plane
... periodicity search tool. For this study, Peranso was used primarily to confirm the periods determined by UPSILON. Using the ANOVA period determining method within Peranso, the periods of multiple light curves were ...
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A complete catalogue of dusty supernova remnants in the galactic plane
... Figure 20 . 3.3 Temperature and Mass Maps of Milky Way SNRs The three colour images created out of the Herschel im- ages shown in Section 2.1 and Figure A1 reveal dusty struc- tures and features that appear to be ...
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The IPHAS POSS I proper motion survey of the Galactic plane
... not significant enough). Below about 25 mas/yr it is clear the distribution flattens off and we can say we have no significant population below this mark. We have also compared our results with those in Gould & Kollmeier ...
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Analysis of Galactic molecular cloud polarization maps: a review of the methods
... of maps obtained from the observation of linearly polarized thermal dust emission at submillimeter (submm) wavelengths toward Galactic Molecular Clouds (MCs) and protostellar cores, but the same methods can ...
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The role of environment in the observed Fundamental Plane of radio active galactic nuclei
... 6 C O N C L U S I O N S This short paper considers the environmental dependence on the optical FP of black hole activity. SDSS group catalogues were used to quantify environments around a sample of low-redshift (z < 0.2) ...
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Identification of a Population of X-ray-emitting Massive Stars in the Galactic Plane
... AX J144701–5919 appears to be associated with an unre- solved radio source. Molonglo observed this source in 1994 and 1998, with a measured flux density of 15 ± 5 and 10 ± 5 mJy, respectively. Within these large errors ...
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A Finding List of Faint UV-bright Stars in the Galactic Plane. VI.
... 4. DISCUSSION We discuss some of the more interesting objects found during the course of this portion of the survey analysis. Two sources, Lanning 151 (Paper III) and Lanning 272 (Paper IV), were recovered during the ...
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The VST Photometric Hα Survey of the Southern Galactic Plane and Bulge (VPHAS+)
... An impressive feature of the camera, OmegaCAM, is its potential to deliver remarkably undistorted point-source images all the way across the 1 ◦ field of view. To realize this, it is critical that the VST has an actively ...
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Planck intermediate results XLIV Structure of the Galactic magnetic field from dust polarization maps of the southern Galactic cap
... s. Galactic latitudes to the structure of the ...southern Galactic cap, with a few ...353 GHz dust polarization data over a larger area than the one considered in this ...
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High mass starless clumps in the inner galactic plane: the sample and dust properties
... in Galactic spiral arms and toward the Galactic center and some well- known star-forming ...temperature maps constructed via fi tting far-infrared and submillimeter continuum data to modi fi ed ...
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Diffuse Hard X-ray Sources Discovered with the ASCA Galactic Plane Survey
... In order to estimate the radio flux band for the SN 1006-like SNRs, we tried the spectral fittings with a srcut model (Reynolds et al. 1998; Reynolds & Keohane 1999). The spectral index at 1 GHz was frozen to α = ...
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The IPHAS catalogue of H alpha emission line sources in the northern Galactic plane
... In order to select an appropriate matching radius, and get a handle on the number of spurious matches, we cre- ated a mock catalogue in which all positions in the IPHAS H α emitter catalogue were shifted by 0 . 5 ◦ in ...
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Microlensing optical depth and event rate in the OGLE-IV Galactic plane fields
... However, we can detect microlensing events with source stars fainter than that limit. The overall depth of the survey is I = 21 (Sections 4 and 6 ). The OGLE photometric pipeline is based on the (Woźniak 2000 ) ...
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The XMM-Newton SSC survey of the Galactic plane
... objects, T Tauri and Herbig-Ae stars. In the relatively high galactic latitude fields, due to the lower N H , some sources are identified as extragalactic ...higher Galactic latitudes, as ...
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Neutrino fluxes from the Galactic plane and the ANTARES limit
... Luigi Antonio Fusco 1,2,a on behalf of the ANTARES Collaboration 1 Dipartimento di Fisica e Astronomia dell’Università, Viale Berti-Pichat 6/2, 40127 Bologna, Italy 2 INFN – Sezione di Bologna, Viale Berti-Pichat 6/2, ...
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Creating A Galactic Plane Atlas With Amazon Web Services
... ∗ Corresponding author Abstract This paper describes by example how astronomers can use cloud-computing resources offered by Amazon Web Services (AWS) to create new datasets at scale. We have created from existing ...
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CallPilot 100/150 Upgrade Addendum
... CallPilot 100/150 with new software on a new Feature ...CallPilot 150 to a larger size compact flash memory feature cartridge, for example from 64 MB or 192 MB to 256 ...
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DIFFERENTIAL MAPS, DIFFERENCE MAPS, INTERPOLATED MAPS, AND LONG-TERM PREDICTION
... FIGURE 1 Dependence of the number of accurate iterations on the approximation amplitude, for various pendulum swing amplitudes.. exact, Y(Xap - Xex)2 + (Pap - Pex)2, is calculated.[r] ...
The Difference Between Maps and Globes
... a) “Maps are flat. Globes are round.” b) “Maps let you see all the places in the world at the same time. Globes give you a better picture of what our round planet looks like from space.” c) “Maps and ...
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