     explanation:
       goals: 'This page aims to give background to the scientific motivation behind the project for a more technical audience.'
       data: 'You may be looking for data - public Galaxy Zoo data is available in a range of formats <a href="http://data.galaxyzoo.org">here</a>.'
-      papers: 'Alternatively, you can browse a list of papers published by the team <a href="http://www.zooniverse.org/publications?project=hubble">here</a>.'
+      papers: 'Alternatively, you can browse a list of papers published by the team <a href="https://www.zooniverse.org/#/about/publications">here</a>.'
     
     morphology:
       heading: 'Why is galaxy morphology important?'

    candels_2epoch: 'CANDELS 2-epoch'
    ukidss: 'UKIDSS'
    sdss_singleband: 'Single-band images'
    ferengi: 'Artificially redshifted images'
    dr8: 'Data Release 8'
    sdss_id: 'SDSS ObjectID'

    p5: "Along the way, we added more detailed images from an area of the survey known as 'Stripe 82', but it was soon time to look at the more distant Universe. The site’s third incarnation, Galaxy Zoo : Hubble drew from surveys conducted by the Hubble Space Telescope to view earlier epochs of galaxy formation. In these surveys, which involve many, many days of dedicated observing time, we can see light from galaxies which has taken billions of years to reach us. The idea behind Galaxy Zoo : Hubble was to be able to compare galaxies then to galaxies now, giving us a clear understanding of what factors influence their growth, whether through mergers, active black holes or simply star formation."
    p6: '''The present day Galaxy Zoo combines new imaging from Sloan, giving us our best ever view of the local Universe, with the most distant images yet from Hubble's CANDELS survey. The <a href="http://candels.ucolick.org" target="_blank">CANDELS survey</a> makes use of the new Wide Field Camera 3 - installed during the final shuttle mission to Hubble - to take ultra-deep images of the Universe, so who knows what's out there to be found?'''
    p7: 'The site also includes images taken with the United Kingdom Infrared Telescope (UKIRT), in Hawaii, for the recently-completed UKIDSS project (http://www.ukidss.org). UKIDSS is the largest, deepest survey of the sky at infrared wavelengths. The UKIDSS infrared-light pictures and the SDSS visible-light pictures are different for two reasons. Firstly, older stars are brighter in infrared wavelengths (while in visible-light we see younger stars), and secondly, infrared light, like a foglight, can penetrate the dust and smoke in the centres of galaxies. Examining the UKIDSS images in Galaxy Zoo will therefore enable us to see how old and young stars are arranged differently in the galaxies, and will reveal more of the structure in the inner parts of galaxies.'
    p8: '''The data sets being put into Galaxy Zoo change quickly, thanks to the dedicated work of volunteers and the "retirement" of images that have already been completed. One of the new sets of images to be classified comes from the Dark Energy Camera Legacy Survey (DECaLS), a survey which uses DECam, one of the most sensitive and widest-area cameras ever built and a key tool in our search to measure and understand dark energy. The camera, mounted on the 4-m Blanco telescope at CTIO in Chile, images the sky at similar wavelengths to SDSS, but with much better resolution and with the ability to detect fainter galaxies. These images are extending the reach of the science we began with Galaxy Zoo 2 and SDSS. Finally, the site also has Galaxy Zoo's first-ever images of fully simulated galaxies; these are images that have been created entirely on a computer, using sophisticated simulations of the Universe starting just after the Big Bang and then watching as dark matter, gas, and stars evolve to form the galaxies we see today. Classification of these images, which come from the Illustris project, are a vital test of the physics that go into these simulations.'''
  
  
  team:
