[PDF] Top 20 The SAMI Galaxy Survey : Early Data Release

... The reported per-pixel S/N of the extracted stellar spectra is typically in the range 20–50, with some observations reaching as high as 80. As the uncertainty is propagated through the telluric correction process, its ... See full document

... with SAMI data cubes refer- enced to ancillary data ...the SAMI Galaxy Survey Early Data Release by Allen et ... See full document

... The Galaxy And Mass Assembly (GAMA) survey is one of the largest contemporary spectro- scopic surveys of low redshift ...five survey regions) down to a limiting magnitude of r < ...imaging ... See full document

... Spectroscopic Survey (BOSS), part of the Sloan Digital Sky Survey (SDSS) III project, has provided the largest survey of galaxy redshifts available to date, in terms of both the number of ... See full document

... IFS data to the quality of typical (KROSS) z ≈ 1 obser- vations, we must bear in mind that this is not the same as asking what one might observe were the z ≈ 0 galaxy pop- ulation to be figuratively placed ... See full document

... Area Survey ( CALIFA, Sánchez et ...( SAMI, Croom et ...Sky Survey ( SDSS-IV ) , the MaNGA project bundles single fi bers from the Baryon Oscillation Spectroscopic Survey ( BOSS ) spectrograph ... See full document

... deep galaxy number-count data from the  Galaxy And Mass Assembly, COSMOS / G10, Hubble Space Telescope ( HST ) Early Release Science, HST UVUDF, and various near-, mid-, and far-IR ... See full document

... a galaxy than single-fibre or long-slit spectroscopy, the nature of a large-scale hexabundle integral field spectroscopy survey presents us with some ...the SAMI instrument con- sists of hexabundles ... See full document

... GALAH survey joins a vibrant and exciting landscape of Galactic spectroscopic surveys that are highly complementary in scale and ...Gaia-ESO Survey on the VLT (Gilmore et ...APOGEE survey (Abolfathi ... See full document

... This DMU identifies the cosmic web of large-scale structure within the GAMA equatorial survey regions by classifying the geometric environment of each point in space as either a void, a sheet, a fil- ament, or a ... See full document

... our data set in a meaningful way we develop in this paper a classification of the galaxies based upon their observed ...astronomical data, there are different approaches for analysing galaxy spectra ... See full document

... Figure 4, sorted by observed stellar velocity dispersion. The stack was created after smoothing with a five pixel wide box filter and resampling each spectrum to a common grid rang- ing from 3690 A ˚ to 5100 A ˚ in ... See full document

... Stars have long been known to vary in brightness, and photometric studies over the past centuries have revealed many classes of stars exhibiting a variety of variability (Pickering 1881). With interest in stellar ... See full document

... be small focus drifts and small detector movements due to instrument flexure. These give a slight, additional broadening to the LSF. Since we often take flats and arcs both at the beginning and the end of the exposure ... See full document

... Doubling the S / N would result in a sample size smaller by a factor of 4. A sample size of 2500  galaxies would be too small to meet our requirements. For example, if we want to study the dependence of a galaxy ... See full document

... Pilot Survey spin parameters with those measured here and fi nd a mean difference l R fid ( SGS - Pilot ) = ...N data in the maps of Fogarty et ...Pilot Survey galaxies that meet our selection ... See full document

... on data taken from the Sloan Digital Sky Survey and the UKIRT Infrared Deep Sky ...independent survey programmes including GALEX MIS, VST KiDS, VISTA VIKING, WISE, Herschel-ATLAS, GMRT and ASKAP ... See full document

... of SAMI galaxies to the global SFMS. We sum the SFR maps for each galaxy to obtain the total SFR and use the total stellar masses from the GAMA ...(2016). SAMI galaxies visually classified as ‘late ... See full document

... the SAMI instrument + AAOmega spectrograph + AAT telescope, excluding atmospheric losses (solid lines) and including losses from the atmosphere (dashed ...original SAMI-I before the new hexabundles and ... See full document

... The mass and angular momentum of a galaxy are most directly probed by its kinematic state. A galaxy’s accretion and merger his- tory is central to defining its character, and aspects of this history are encoded in ... See full document