OzDES multi-object fibre spectroscopy for the Dark Energy Survey: Results and second data release. (arXiv:2006.00449v1 [astro-ph.CO])
<a href="http://arxiv.org/find/astro-ph/1/au:+Lidman_C/0/1/0/all/0/1">C. Lidman</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Tucker_B/0/1/0/all/0/1">B. E. Tucker</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Davis_T/0/1/0/all/0/1">T. M. Davis</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Uddin_S/0/1/0/all/0/1">S. A. Uddin</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Asorey_J/0/1/0/all/0/1">J. Asorey</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bolejko_K/0/1/0/all/0/1">K. Bolejko</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Brout_D/0/1/0/all/0/1">D. Brout</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Calcino_J/0/1/0/all/0/1">J. Calcino</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Carollo_D/0/1/0/all/0/1">D. Carollo</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Carr_A/0/1/0/all/0/1">A. Carr</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Childress_M/0/1/0/all/0/1">M. Childress</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Hoormann_J/0/1/0/all/0/1">J. K. Hoormann</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Foley_R/0/1/0/all/0/1">R. J. Foley</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Galbany_L/0/1/0/all/0/1">L. Galbany</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Glazebrook_K/0/1/0/all/0/1">K. Glazebrook</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Hinton_S/0/1/0/all/0/1">S. R. Hinton</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Kessler_R/0/1/0/all/0/1">R. Kessler</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Kim_A/0/1/0/all/0/1">A. G. Kim</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+King_A/0/1/0/all/0/1">A. King</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Kremin_A/0/1/0/all/0/1">A. Kremin</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Kuehn_K/0/1/0/all/0/1">K. Kuehn</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Lagattuta_D/0/1/0/all/0/1">D. Lagattuta</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Lewis_G/0/1/0/all/0/1">G. F. Lewis</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Macaulay_E/0/1/0/all/0/1">E. Macaulay</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Malik_U/0/1/0/all/0/1">U. Malik</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+March_M/0/1/0/all/0/1">M. March</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Martini_P/0/1/0/all/0/1">P. Martini</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Moller_A/0/1/0/all/0/1">A. M&#xf6;ller</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Mudd_D/0/1/0/all/0/1">D. Mudd</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Nichol_R/0/1/0/all/0/1">R. C. Nichol</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Panther_F/0/1/0/all/0/1">F. Panther</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Parkinson_D/0/1/0/all/0/1">D. Parkinson</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Pursiainen_M/0/1/0/all/0/1">M. Pursiainen</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Sako_M/0/1/0/all/0/1">M. Sako</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Swann_E/0/1/0/all/0/1">E. Swann</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Scalzo_R/0/1/0/all/0/1">R. Scalzo</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Scolnic_D/0/1/0/all/0/1">D. Scolnic</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Sharp_R/0/1/0/all/0/1">R. Sharp</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Smith_M/0/1/0/all/0/1">M. Smith</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Sommer_N/0/1/0/all/0/1">N. E. Sommer</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Sullivan_M/0/1/0/all/0/1">M. Sullivan</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Webb_S/0/1/0/all/0/1">S. Webb</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Wiseman_P/0/1/0/all/0/1">P. Wiseman</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Yu_Z/0/1/0/all/0/1">Z. Yu</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Yuan_F/0/1/0/all/0/1">F. Yuan</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Zhang_B/0/1/0/all/0/1">B. Zhang</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Abbott_T/0/1/0/all/0/1">T. M. C. Abbott</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Aguena_M/0/1/0/all/0/1">M. Aguena</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Allam_S/0/1/0/all/0/1">S. Allam</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Annis_J/0/1/0/all/0/1">J. Annis</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Avila_S/0/1/0/all/0/1">S. Avila</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bertin_E/0/1/0/all/0/1">E. Bertin</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bhargava_S/0/1/0/all/0/1">S. Bhargava</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Brooks_D/0/1/0/all/0/1">D. Brooks</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Rosell_A/0/1/0/all/0/1">A. Carnero Rosell</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Kind_M/0/1/0/all/0/1">M. Carrasco Kind</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Carretero_J/0/1/0/all/0/1">J. Carretero</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Castander_F/0/1/0/all/0/1">F. J. Castander</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Costanzi_M/0/1/0/all/0/1">M. Costanzi</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Costa_L/0/1/0/all/0/1">L. N. da Costa</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Vicente_J/0/1/0/all/0/1">J. De Vicente</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Doel_P/0/1/0/all/0/1">P. Doel</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Eifler_T/0/1/0/all/0/1">T. F. Eifler</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Everett_S/0/1/0/all/0/1">S. Everett</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Fosalba_P/0/1/0/all/0/1">P. Fosalba</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Frieman_J/0/1/0/all/0/1">J. Frieman</a>, et al. (38 additional authors not shown)

We present a description of the Australian Dark Energy Survey (OzDES) and
summarise the results from its six years of operations. Using the 2dF fibre
positioner and AAOmega spectrograph on the 3.9-metre Anglo-Australian
Telescope, OzDES has monitored 771 AGN, classified hundreds of supernovae, and
obtained redshifts for thousands of galaxies that hosted a transient within the
10 deep fields of the Dark Energy Survey. We also present the second OzDES data
release, containing the redshifts of almost 30,000 sources, some as faint as
$r_{mathrm AB}=24$ mag, and 375,000 individual spectra. These data, in
combination with the time-series photometry from the Dark Energy Survey, will
be used to measure the expansion history of the Universe out to $zsim1.2$ and
the masses of hundreds of black holes out to $zsim4$. OzDES is a template for
future surveys that combine simultaneous monitoring of targets with wide-field
imaging cameras and wide-field multi-object spectrographs.

We present a description of the Australian Dark Energy Survey (OzDES) and
summarise the results from its six years of operations. Using the 2dF fibre
positioner and AAOmega spectrograph on the 3.9-metre Anglo-Australian
Telescope, OzDES has monitored 771 AGN, classified hundreds of supernovae, and
obtained redshifts for thousands of galaxies that hosted a transient within the
10 deep fields of the Dark Energy Survey. We also present the second OzDES data
release, containing the redshifts of almost 30,000 sources, some as faint as
$r_{mathrm AB}=24$ mag, and 375,000 individual spectra. These data, in
combination with the time-series photometry from the Dark Energy Survey, will
be used to measure the expansion history of the Universe out to $zsim1.2$ and
the masses of hundreds of black holes out to $zsim4$. OzDES is a template for
future surveys that combine simultaneous monitoring of targets with wide-field
imaging cameras and wide-field multi-object spectrographs.

http://arxiv.org/icons/sfx.gif