Slide 1Lab #4 The Hubble Law Slide 2 Slide 3 - means that the spectra are easy to identify Links to the Galaxy Images Links to the Galaxy Spectra Slide 4 Example: NGC 1357…
Slide 1Data Release 6 Access to DR6 and SEGUE Catalog Data SDSS Data Release 6 Access to DR6 and SEGUE Catalog Data Ani Thakar Alex Szalay, Maria Nieto-Santisteban, Nolan…
1. UV Visi NI FIRMIR Russell Johnston Collaborators: MattiaVaccari, Matt Jarvis, Mat Smith, Matt Prescott, Elodie Giovannoli The evolving relation between SFR and M* in the…
Slide 1Galaxy surveys: from controlling systematics to new physics Ofer Lahav (UCL) CLASH MACS1206 1 Slide 2 Outline Which surveys, what science, what methods Systematics:…
GRB Physics: an Overview Bing Zhang University of Nevada Las Vegas Kavli Institute of Astronomy and Astrophysics & Astronomy Department, Peking University Nov. 8, 2012,…
J. Sánchez Almeida, J. A. L. Aguerri, C. Muñoz-Tuñón, A. de Vicente @IAC Automatic Unsupervised Spectral Classification of Galaxies for GTC Motivation Uses within…
Russell Johnston Dept of Physics and Astronomy University of Glasgow Edwin Hubble Hubble measured the shift in colour, or wavelength, of the light from distant galaxies.…
Slide 1 EXPANDING UNIVERSE OLBERS PARADOX âThe night sky is dark.â This statement is called Olbersâ paradox, after astronomer who discussed the subject back in 1823. Why…