Hintze Centre for Astrophysical Surveys: publications

SUPERNOVA 2009kf: AN ULTRAVIOLET BRIGHT TYPE IIP SUPERNOVA DISCOVERED WITH PAN-STARRS 1 AND GALEX

The Astrophysical Journal Letters American Astronomical Society 717:1 (2010) l52-l56

Authors:

MT Botticella, C Trundle, A Pastorello, S Rodney, A Rest, S Gezari, SJ Smartt, G Narayan, ME Huber, JL Tonry, D Young, K Smith, F Bresolin, S Valenti, R Kotak, S Mattila, E Kankare, WM Wood-Vasey, A Riess, JD Neill, K Forster, DC Martin, CW Stubbs, WS Burgett, KC Chambers, T Dombeck, H Flewelling, T Grav, JN Heasley, KW Hodapp, N Kaiser, R Kudritzki, G Luppino, RH Lupton, EA Magnier, DG Monet, JS Morgan, PM Onaka, PA Price, PH Rhoads, WA Siegmund, WE Sweeney, RJ Wainscoat, C Waters, MF Waterson, CG Wynn-Williams

An excess of star-forming galaxies in the fields of high-redshift QSOs

\mnras 405 (2010) 2623-2638-2623-2638

Authors:

JA Stevens, MJ Jarvis, KEK Coppin, MJ Page, TR Greve, FJ Carrera, RJ Ivison

The VLT-FLAMES Tarantula survey

Proceedings of the International Astronomical Union Cambridge University Press (CUP) 6:S272 (2010) 296-297

Authors:

Daniel J Lennon, Christopher J Evans, Nate Bastian, Yuri Beletsky, Ines Brott, Matteo Cantiello, Giovanni Carraro, J Simon Clark, Paul A Crowther, Alex de Koter, Selma E de Mink, Philip L Dufton, Paul Dunstall, Mark Gieles, Goetz Gräfener, Vincent Hénault-Brunet, Artemio Herrero, Ian D Howarth, Norbert Langer, Jesus Maíz Apellániz, Nevena Markova, F Paco Najarro, Joachim Puls, Hugues Sana, Sergio Simón-Díaz, Stephen J Smartt, Vanessa E Stroud, William D Taylor, Jacco T van Loon, Jorick S Vink, Nolan R Walborn

Measuring the low mass end of the Mbh - sigma relation

AIP Conference Proceedings AIP Publishing 1240 (2010) 215

Authors:

D Krajnovic, Rm McDermid, Michele Cappellari, Roger Davies

Abstract:

We show that high quality laser guide star (LGS) adaptive optics (AO) observations of nearby early-type galaxies are possible when the tip-tilt correction is done by guiding on nuclei while the focus compensation due to the changing distance to the sodium layer is made 'open loop'. We achieve corrections such that 40% of flux comes from R<0.2 arcsec. To measure a black hole mass (Mbh) one needs integral field observations of both high spatial resolution and large field of view. With these data it is possible to determine the lower limit to Mbh even if the spatial resolution of the observations are up to a few times larger than the sphere of influence of the black hole.

Formation of Slowly Rotating Elliptical Galaxies in Major Mergers. A Resolution 51��

AIP Conference Proceedings AIP Publishing 1240:1 (2010) 405-406

Authors:

M Bois, F Bournaud, E Emsellem, K Alatalo, L Blitz, M Bureau, M Cappellari, RL Davies, TA Davis, PT de Zeeuw, J Falcón-Barroso, S Khochfar, D Krajnović, H Kuntschner, P-Y Lablanche, RM McDermid, R Morganti, T Naab, M Sarzi, N Scott, P Serra, RCE van den Bosch, G van de Ven, A Weijmans, LM Young, Victor P Debattista, CC Popescu

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