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173 results on '"Bland-Hawthorn, J"'

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1. First demonstration of OH suppression in a high-efficiency near-infrared spectrograph.

2. The SAMI Galaxy Survey: first detection of a transition in spin orientation with respect to cosmic filaments in the stellar kinematics of galaxies.

3. GALAH Survey: Chemical tagging and disk reconstruction.

4. GALAH SURVEY: CHEMICALLY TAGGING THE THICK DISK.

5. Comparing theoretical models of our galaxy with observations.

6. Comparing theoretical models of our galaxy with observations.

7. FOSSIL IMPRINT OF A POWERFUL FLARE AT THE GALACTIC CENTER ALONG THE MAGELLANIC STREAM.

8. Suppression of the near-infrared OH night-sky lines with fibre Bragg gratings - first results.

9. THE MINIMUM MASS FOR A DWARF GALAXY.

10. The case for OH suppression at near-infrared wavelengths.

11. Galactic winds: a short review.

12. GalaxyCount: ajava calculator of galaxy counts and variances in multiband wide-field surveys to 28 AB mag.

13. New instrument concepts for observational cosmology

14. In search of first light: New technologies and new ideas

15. Optimizing background-limited observing during bright-Moon phases and twilight.

16. Towards a direct detection of warm gas in galactic haloes at cosmological distances.

17. The MAGPI survey: using kinematic asymmetries in stars and gas to dissect drivers of galaxy dynamical evolution.

18. Gaia DR3 data consistent with a short bar connected to a spiral arm.

19. Clues to galaxy formation.

20. KINEMATIC MODELING OF THE MILKY WAY USING THE RAVE AND GCS STELLAR SURVEYS.

21. SAMI Galaxy Survey: physical drivers of stellar-gas kinematic misalignments in the nearby Universe.

22. Modelling the Milky Way with Galaxia and making use of asteroseismology.

23. The GALAH survey: relative throughputs of the 2dF fibre positioner and the HERMES spectrograph from stellar targets.

25. The GALAH survey: scientific motivation.

26. physical connection between central stellar surface density and stellar spin in SAMI and MaNGA nearby galaxies.

27. SAMI Galaxy Survey: the drivers of gas and stellar metallicity differences in galaxies.

28. WARM IONIZED GAS REVEALED IN THE MAGELLANIC BRIDGE TIDAL REMNANT: CONSTRAINING THE BARYON CONTENT AND THE ESCAPING IONIZING PHOTONS AROUND DWARF GALAXIES.

29. Two-phase galaxy evolution: the cosmic star formation histories of spheroids and discs.

30. Galaxy And Mass Assembly (GAMA): in search of Milky Way Magellanic Cloud analogues.

31. Characterization of hexabundles: initial results.

33. The C linewidth distribution for quasars and its implications for broad-line region dynamics and virial mass estimation S. Fine et al. The C linewidth distribution.

34. Lopsided galaxies: the case of NGC 891.

35. Shocks, illumination cones and intrinsic gas structures in the extreme radio galaxy 3C 265.

36. Detection and measurement from narrow-band tunable filter scans.

37. Galaxy destruction and diffuse light in clusters.

38. The SAMI Galaxy Survey: the role of disc fading and progenitor bias in kinematic transitions.

39. A SAMI and MaNGA view on the stellar kinematics of galaxies on the star-forming main sequence.

40. Chronos: A NIR spectroscopic galaxy survey to probe the most fundamental stages of galaxy evolution.

41. The GALAH survey: tracing the Galactic disc with open clusters.

42. Exploring the dust content of galactic haloes with Herschel III. NGC 891.

43. The SAMI Galaxy Survey: Bulge and Disk Stellar Population Properties in Cluster Galaxies.

44. The RAdial Velocity Experiment (RAVE): Parameterisation of RAVE spectra based on convolutional neural networks.

45. The GALAH Survey: non-LTE departure coefficients for large spectroscopic surveys.

46. The SAMI Galaxy Survey: satellite galaxies undergo little structural change during their quenching phase.

47. The SAMI galaxy survey: exploring the gas-phase mass–metallicity relation.

48. The GALAH survey: An abundance, age, and kinematic inventory of the solar neighbourhood made with TGAS.

49. Galaxy and Mass Assembly (GAMA): environmental quenching of centrals and satellites in groups.

50. SAMI Galaxy Survey: observing the environmental quenching of star formation in GAMA groups.

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