Announcements 2013

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id="body"> <div class="row no-page"> <div class="col-md-12"> <div class="archive-search outside"><a href="/public/announcements/search/" class="advanced-search" data-container="body" data-toggle="tooltip" data-placement="left" aria-label="Advanced Search" title="Advanced Search"><span class="fa fa-plus"></span></a><form class="form-inline" role="form" action="/public/announcements/" method="GET"><div class="form-group"><div class="input-group"><input id="id_archivesearch" type="text" value="" placeholder="Search Announcements..." name="search" class="form-control input-sm" /><span class="input-group-btn"><button aria-label="Search" class="btn btn-default btn-sm" type="submit"><span class="fa fa-search"></span></button></span></div></div></form></div> </div> </div> <div class="row no-page"> <div class="col-md-12"> <div class="row"> <div class="col-md-10"> <h1>Announcements 2013 <a href="/public/announcements/feed/" class="listviewrsslink" aria-label="RSS feed"><span class="fa fa-rss"></span></a></h1> </div> <div class="col-md-12 media-categories" style="min-height: 0"> <ul> <li><a href="/public/announcements/">All</a></li> <li><a href="/public/announcements/archive/program/ctio/">Cerro Tololo Inter-American Observatory</a></li> <li><a href="/public/announcements/archive/program/csdc/">Community Science & Data Center</a></li> <li><a href="/public/announcements/archive/program/gemini/">Gemini Observatory</a></li> <li><a href="/public/announcements/archive/program/kpno/">Kitt Peak National Observatory</a></li> <li><a href="/public/announcements/archive/program/noao/">NOAO</a></li> <li><a href="/public/announcements/archive/program/noirlab/">NOIRLab</a></li> <li><a href="/public/announcements/archive/program/noirlab-useltp/">NOIRLab US-ELTP</a></li> <li><a href="/public/announcements/archive/program/useltp/">US Extremely Large Telescope Program</a></li> <li><a href="/public/announcements/archive/program/rubin/">Vera C. Rubin Observatory</a></li> </ul> </div> </div> </div> <div class="col-md-12"> <a href="/public/subscribe/" class="esonews_link">Subscribe to receive news from NOIRLab!</a> <div class="row news-list news-list-overflow"> <div class="col-md-3 col-sm-6 col-xs-12"> <a href="/public/announcements/noaoann13007/"> <div class="news-wrapper"> <div class="news-image"> <img class="img-responsive" src="/public/media/archives/images/thumb350x/noaoann13007a.jpg" alt="KOSMOS has arrived at the Mayall 4-meter"> </div> <div class="news-description"> <div class="news-id" aria-label="noaoann13007 — Announcement ">noaoann13007 — Announcement</div> <div class="news-title" role="heading" aria-level="1" aria-label="KOSMOS has arrived at the Mayall 4-meter ">KOSMOS has arrived at the Mayall 4-meter</div> <div class="news-teaser" aria-label="21 November 2013 The Kitt Peak Ohio State Multi-Object Spectrograph (KOSMOS) and the Cerro Tololo Ohio State Multi-Object Spectrograph (COSMOS) are nearly identical spectrographs being developed simultaneously. The position of the long slit of the spectrograph is shown superimposed on the image of the planetary nebula M 57."><strong>21 November 2013</strong>: The Kitt Peak Ohio State Multi-Object Spectrograph (KOSMOS) and the Cerro Tololo Ohio State Multi-Object Spectrograph (COSMOS) are nearly identical spectrographs being developed simultaneously. The position of the long slit of the spectrograph is shown superimposed on the image of the planetary nebula M 57.</div> </div> <div class="news-readmore" aria-label="Read more">Read more</div> </div>  </a> </div> <div class="col-md-3 col-sm-6 col-xs-12"> <a href="/public/announcements/geminiann13015/"> <div class="news-wrapper"> <div class="news-image"> <img class="img-responsive" src="/public/media/archives/images/thumb350x/geminiann13015a.jpg" alt="Gemini Planet Imager Begins On-sky Integration at Gemini South"> </div> <div class="news-description"> <div class="news-id" aria-label="geminiann13015 — Announcement ">geminiann13015 — Announcement</div> <div class="news-title" role="heading" aria-level="1" aria-label="Gemini Planet Imager Begins On-sky Integration at Gemini South ">Gemini Planet Imager Begins On-sky Integration at Gemini South</div> <div class="news-teaser" aria-label="14 November 2013 Gemini's powerful new instrument for studying planets beyond the Solar System, the Gemini Planet Imager (GPI), has successfully received its first starlight for engineering and testing on the night of November 11-12. On-sky observations are currently ongoing for technical integration with the Gemini South telescope. The GPI team (geminiann13015a) began the 7-night observing run began with a head start, since preliminary pupil and pointing alignments were completed early, due to extensive preparatory work and smooth integration since the instrument arrived at Gemini South in August. “We locked the AO system on the first try with the first star we looked at. Watching the starlight smooth out on the wavefront sensor was amazing,” said GPI Principal Investigator Bruce Macintosh. “GPI is a complex instrument with many subsystems, so integration is a complicated process. For now we’re deep in engineering tests verifying interactions throughout the entire system with real starlight – getting …"><strong>14 November 2013</strong>: Gemini's powerful new instrument for studying planets beyond the Solar System, the Gemini Planet Imager (GPI), has successfully received its first starlight for engineering and testing on the night of November 11-12. On-sky observations are currently ongoing for technical integration with the Gemini South telescope. The GPI team (geminiann13015a) began the 7-night observing run began with a head start, since preliminary pupil and pointing alignments were completed early, due to extensive preparatory work and smooth integration since the instrument arrived at Gemini South in August. “We locked the AO system on the first try with the first star we looked at. Watching the starlight smooth out on the wavefront sensor was amazing,” said GPI Principal Investigator Bruce Macintosh. “GPI is a complex instrument with many subsystems, so integration is a complicated process. For now we’re deep in engineering tests verifying interactions throughout the entire system with real starlight – getting …</div> </div> <div class="news-readmore" aria-label="Read more">Read more</div> </div>  </a> </div> <div class="col-md-3 col-sm-6 col-xs-12"> <a href="/public/announcements/noaoann13006/"> <div class="news-wrapper"> <div class="news-image"> <img class="img-responsive" src="/public/media/archives/images/thumb350x/noaoann13006a.jpg" alt="Planetary Nebula HDW 3"> </div> <div class="news-description"> <div class="news-id" aria-label="noaoann13006 — Announcement ">noaoann13006 — Announcement</div> <div class="news-title" role="heading" aria-level="1" aria-label="Planetary Nebula HDW 3 ">Planetary Nebula HDW 3</div> <div class="news-teaser" aria-label="7 November 2013 This image of Hartl-Dengel-Weinberger 3 (HDW 3) was obtained with the wide-field view of the Mosaic camera on the Mayall 4-meter telescope at Kitt Peak National Observatory. The distinctive braided shape of this large, ancient planetary nebula is the result of the planetary nebula colliding with the interstellar gas around it as the nebula moves through the galaxy."><strong>7 November 2013</strong>: This image of Hartl-Dengel-Weinberger 3 (HDW 3) was obtained with the wide-field view of the Mosaic camera on the Mayall 4-meter telescope at Kitt Peak National Observatory. The distinctive braided shape of this large, ancient planetary nebula is the result of the planetary nebula colliding with the interstellar gas around it as the nebula moves through the galaxy.</div> </div> <div class="news-readmore" aria-label="Read more">Read more</div> </div>  </a> </div> <div class="col-md-3 col-sm-6 col-xs-12"> <a href="/public/announcements/geminiann13014/"> <div class="news-wrapper"> <div class="news-image"> <img class="img-responsive" src="/public/media/archives/images/thumb350x/geminiann13014a.jpg" alt="Bringing the Universe Down-to-Earth in Chile"> </div> <div class="news-description"> <div class="news-id" aria-label="geminiann13014 — Announcement ">geminiann13014 — Announcement</div> <div class="news-title" role="heading" aria-level="1" aria-label="Bringing the Universe Down-to-Earth in Chile ">Bringing the Universe Down-to-Earth in Chile</div> <div class="news-teaser" aria-label="7 October 2013 Gemini’s flagship local outreach program in Chile, Viaje al Universo, blasted off early last week when Gemini South’s Nancy Levenson addressed nearly 800 students at Colegio San Joaquin. The celebration set into motion a week of fun and educational activities for students, teachers and families from across the region of Coquimbo (including the communities of La Serena, Coquimbo and Combarbalá). During the week many hands-on activities engaged students of all ages, from pre-school to senior citizens, with talks on astronomical research done at Gemini and other Chilean observatories, teacher workshops, rocket building and launching, classroom activities and much more. Participants, from students to local community leaders joined in the fun as Gemini’s portable StarLab planetarium wowed audiences with programs on the beautiful dark Chilean skies. Local Almirante Latorre student Alondra Torres had never been inside a portable planetarium before and described it for a national TV station like this, “This …"><strong>7 October 2013</strong>: Gemini’s flagship local outreach program in Chile, Viaje al Universo, blasted off early last week when Gemini South’s Nancy Levenson addressed nearly 800 students at Colegio San Joaquin. The celebration set into motion a week of fun and educational activities for students, teachers and families from across the region of Coquimbo (including the communities of La Serena, Coquimbo and Combarbalá). During the week many hands-on activities engaged students of all ages, from pre-school to senior citizens, with talks on astronomical research done at Gemini and other Chilean observatories, teacher workshops, rocket building and launching, classroom activities and much more. Participants, from students to local community leaders joined in the fun as Gemini’s portable StarLab planetarium wowed audiences with programs on the beautiful dark Chilean skies. Local Almirante Latorre student Alondra Torres had never been inside a portable planetarium before and described it for a national TV station like this, “This …</div> </div> <div class="news-readmore" aria-label="Read more">Read more</div> </div>  </a> </div> </div> <div class="row news-list news-list-overflow"> <div class="col-md-3 col-sm-6 col-xs-12"> <a href="/public/announcements/geminiann13013/"> <div class="news-wrapper"> <div class="news-image"> <img class="img-responsive" src="/public/media/archives/images/thumb350x/geminiann13013a.jpg" alt="Gemini Confirms Lonely Planet Floating in Space"> </div> <div class="news-description"> <div class="news-id" aria-label="geminiann13013 — Announcement ">geminiann13013 — Announcement</div> <div class="news-title" role="heading" aria-level="1" aria-label="Gemini Confirms Lonely Planet Floating in Space ">Gemini Confirms Lonely Planet Floating in Space</div> <div class="news-teaser" aria-label="7 October 2013 Observations using the Gemini Near-Infrared Imager (GNIRS) at the Gemini North telescope have confirmed one of the lowest mass free-floating planet known, perhaps the very lowest. The discovery team, led by the University of Hawaii’s Michael Liu, discovered this reddest known field dwarf using the Pan-STARSSS1 survey telescope on Maui’s Haleakala. The team's follow-up observations on Gemini were made over three nights in late June and early July of this year. From the Gemini (and other observations) the object, known as PSO J318.5-22, appears to have a mass only six times that of Jupiter and likely formed about 12 million years ago at a neighborly distance of about 80 light-years away. In a UH Institute for Astronomy (IfA) press release issued on October 9, 2013, Liu is quoted: "We have never before seen an object free-floating in space that looks like this. It has all the characteristics of young planets …"><strong>7 October 2013</strong>: Observations using the Gemini Near-Infrared Imager (GNIRS) at the Gemini North telescope have confirmed one of the lowest mass free-floating planet known, perhaps the very lowest. The discovery team, led by the University of Hawaii’s Michael Liu, discovered this reddest known field dwarf using the Pan-STARSSS1 survey telescope on Maui’s Haleakala. The team's follow-up observations on Gemini were made over three nights in late June and early July of this year. From the Gemini (and other observations) the object, known as PSO J318.5-22, appears to have a mass only six times that of Jupiter and likely formed about 12 million years ago at a neighborly distance of about 80 light-years away. In a UH Institute for Astronomy (IfA) press release issued on October 9, 2013, Liu is quoted: "We have never before seen an object free-floating in space that looks like this. It has all the characteristics of young planets …</div> </div> <div class="news-readmore" aria-label="Read more">Read more</div> </div>  </a> </div> <div class="col-md-3 col-sm-6 col-xs-12"> <a href="/public/announcements/geminiann13012/"> <div class="news-wrapper"> <div class="news-image"> <img class="img-responsive" src="/public/media/archives/images/thumb350x/geminiann13012a.jpg" alt="Observations Set Limits on Possible Atmosphere Around Distant World"> </div> <div class="news-description"> <div class="news-id" aria-label="geminiann13012 — Announcement ">geminiann13012 — Announcement</div> <div class="news-title" role="heading" aria-level="1" aria-label="Observations Set Limits on Possible Atmosphere Around Distant World ">Observations Set Limits on Possible Atmosphere Around Distant World</div> <div class="news-teaser" aria-label="24 September 2013 Occultations are one of the best ways to determine the size of a Solar System object. The events occur when bodies orbiting the Sun pass between the Earth and a star, blocking out the star’s light for a brief period of time. Since astronomers know the speeds of Solar System bodies very precisely from their orbits, the time that the starlight is blocked directly tells us the size of the occulting object. In addition, an occultation can uncover information about the Solar System body’s atmosphere, if it exists. A rocky body without an atmosphere will very suddenly extinguish the starlight, while one with an atmosphere will create a "fuzzy" event with a slow dimming and eventual blocking of the starlight. For example, one of the reasons we know so much about Pluto, including that it has an atmospheric pressure about a million times lower than the Earth's, is from studies …"><strong>24 September 2013</strong>: Occultations are one of the best ways to determine the size of a Solar System object. The events occur when bodies orbiting the Sun pass between the Earth and a star, blocking out the star’s light for a brief period of time. Since astronomers know the speeds of Solar System bodies very precisely from their orbits, the time that the starlight is blocked directly tells us the size of the occulting object. In addition, an occultation can uncover information about the Solar System body’s atmosphere, if it exists. A rocky body without an atmosphere will very suddenly extinguish the starlight, while one with an atmosphere will create a "fuzzy" event with a slow dimming and eventual blocking of the starlight. For example, one of the reasons we know so much about Pluto, including that it has an atmospheric pressure about a million times lower than the Earth's, is from studies …</div> </div> <div class="news-readmore" aria-label="Read more">Read more</div> </div>  </a> </div> <div class="col-md-3 col-sm-6 col-xs-12"> <a href="/public/announcements/geminiann13011/"> <div class="news-wrapper"> <div class="news-image"> <img class="img-responsive" src="/public/media/archives/images/thumb350x/geminiann13011a.jpg" alt="The Gemini Planet Imager Arrives"> </div> <div class="news-description"> <div class="news-id" aria-label="geminiann13011 — Announcement ">geminiann13011 — Announcement</div> <div class="news-title" role="heading" aria-level="1" aria-label="The Gemini Planet Imager Arrives ">The Gemini Planet Imager Arrives</div> <div class="news-teaser" aria-label="9 September 2013 The Gemini Planet Imager (GPI), Gemini’s next-generation instrument for characterizing new worlds, has seen a frenzy of activity over the past month. In late July the instrument’s cryogenics were warmed up, the instrument’s primary components parsed into shippable pieces (geminiann13011a), and seemingly overnight the instrument arrived at Gemini South (geminiann13011b). “For the past 2.5 years GPI has called the labs at the University of California Santa Cruz home,” said Stephen Goodsell, who manages the project for Gemini. “Now, the fun begins as GPI arrives home and, before the end of this year, gets mounted on the back of the Gemini South telescope and collects light, from real planets!” However, before that can happen the instrument needs to be fully tested and integrated on the Gemini South telescope in Chile. Currently, the instrument is fully assembled in the Gemini South instrument lab on Cerro Pachón in Chile (geminiann13011c). According to the …"><strong>9 September 2013</strong>: The Gemini Planet Imager (GPI), Gemini’s next-generation instrument for characterizing new worlds, has seen a frenzy of activity over the past month. In late July the instrument’s cryogenics were warmed up, the instrument’s primary components parsed into shippable pieces (geminiann13011a), and seemingly overnight the instrument arrived at Gemini South (geminiann13011b). “For the past 2.5 years GPI has called the labs at the University of California Santa Cruz home,” said Stephen Goodsell, who manages the project for Gemini. “Now, the fun begins as GPI arrives home and, before the end of this year, gets mounted on the back of the Gemini South telescope and collects light, from real planets!” However, before that can happen the instrument needs to be fully tested and integrated on the Gemini South telescope in Chile. Currently, the instrument is fully assembled in the Gemini South instrument lab on Cerro Pachón in Chile (geminiann13011c). According to the …</div> </div> <div class="news-readmore" aria-label="Read more">Read more</div> </div>  </a> </div> <div class="col-md-3 col-sm-6 col-xs-12"> <a href="/public/announcements/noaoann13005/"> <div class="news-wrapper"> <div class="news-image"> <img class="img-responsive" src="/public/media/archives/images/thumb350x/noaoann13005a.jpg" alt="September 2013 NOAO Newsletter"> </div> <div class="news-description"> <div class="news-id" aria-label="noaoann13005 — Announcement ">noaoann13005 — Announcement</div> <div class="news-title" role="heading" aria-level="1" aria-label="September 2013 NOAO Newsletter ">September 2013 NOAO Newsletter</div> <div class="news-teaser" aria-label="29 August 2013 The September 2013 NOAO Newsletter is online and ready to download. This issue includes information pertaining to the 2014A Call for Proposals, which are due September 26, 2013. On the Cover The cover image highlights an NOAO large survey program of galaxy clusters, using GMOS on Gemini-South. These clusters were initially identified by the South Pole Telescope (SPT): this spectroscopic survey will measure the growth of the largest structures in the Universe over time. The SPT surveys the cosmic microwave background for potential galaxy clusters, after which the GMOS survey determines velocity dispersion and mass of the clusters. This image shows six typical clusters: SPT significance maps on the left and color images from Magellan-II on the right (Bayliss et al, p.3)"><strong>29 August 2013</strong>: The September 2013 NOAO Newsletter is online and ready to download. This issue includes information pertaining to the 2014A Call for Proposals, which are due September 26, 2013. On the Cover The cover image highlights an NOAO large survey program of galaxy clusters, using GMOS on Gemini-South. These clusters were initially identified by the South Pole Telescope (SPT): this spectroscopic survey will measure the growth of the largest structures in the Universe over time. The SPT surveys the cosmic microwave background for potential galaxy clusters, after which the GMOS survey determines velocity dispersion and mass of the clusters. This image shows six typical clusters: SPT significance maps on the left and color images from Magellan-II on the right (Bayliss et al, p.3)</div> </div> <div class="news-readmore" aria-label="Read more">Read more</div> </div>  </a> </div> </div> <div class="row news-list news-list-overflow"> <div class="col-md-3 col-sm-6 col-xs-12"> <a href="/public/announcements/geminiann13010/"> <div class="news-wrapper"> <div class="news-image"> <img class="img-responsive" src="/public/media/archives/images/thumb350x/geminiann13010a.jpg" alt="First Published Science Result from GeMS: “Young Stars Leave the Nest”"> </div> <div class="news-description"> <div class="news-id" aria-label="geminiann13010 — Announcement ">geminiann13010 — Announcement</div> <div class="news-title" role="heading" aria-level="1" aria-label="First Published Science Result from GeMS: “Young Stars Leave the Nest” ">First Published Science Result from GeMS: “Young Stars Leave the Nest”</div> <div class="news-teaser" aria-label="27 August 2013 The first refereed science paper based on data from the Gemini Multi-conjugate adaptive optics System (GeMS) demonstrates the effective use of young, lower mass stars to determine the age of a star cluster. The work, led by Canada’s Tim Davidge, also brings into focus how young cluster stars “leave the nest” and enter the general population of stars in our galaxy. Recent observations using the powerful new GeMS adaptive optics system at Gemini South catch stars before they settle into their “regular lives” and reveal clues into the past and future of a low-mass star cluster – in this case, Haffner 16 - in our Milky Way Galaxy. The combination of Gemini’s large 8-meter aperture, its infrared sensitivity, and the latest in adaptive optics (which corrects for the blurring effects of the Earth’s atmosphere), provide the key elements for the success of this work. The so-called “pre-main sequence” stars tend …"><strong>27 August 2013</strong>: The first refereed science paper based on data from the Gemini Multi-conjugate adaptive optics System (GeMS) demonstrates the effective use of young, lower mass stars to determine the age of a star cluster. The work, led by Canada’s Tim Davidge, also brings into focus how young cluster stars “leave the nest” and enter the general population of stars in our galaxy. Recent observations using the powerful new GeMS adaptive optics system at Gemini South catch stars before they settle into their “regular lives” and reveal clues into the past and future of a low-mass star cluster – in this case, Haffner 16 - in our Milky Way Galaxy. The combination of Gemini’s large 8-meter aperture, its infrared sensitivity, and the latest in adaptive optics (which corrects for the blurring effects of the Earth’s atmosphere), provide the key elements for the success of this work. The so-called “pre-main sequence” stars tend …</div> </div> <div class="news-readmore" aria-label="Read more">Read more</div> </div>  </a> </div> <div class="col-md-3 col-sm-6 col-xs-12"> <a href="/public/announcements/geminiann13009/"> <div class="news-wrapper"> <div class="news-image"> <img class="img-responsive" src="/public/media/archives/images/thumb350x/geminiann13009a.jpg" alt="Gamma-Ray Burst Illuminates Galaxy in Dark Ages"> </div> <div class="news-description"> <div class="news-id" aria-label="geminiann13009 — Announcement ">geminiann13009 — Announcement</div> <div class="news-title" role="heading" aria-level="1" aria-label="Gamma-Ray Burst Illuminates Galaxy in Dark Ages ">Gamma-Ray Burst Illuminates Galaxy in Dark Ages</div> <div class="news-teaser" aria-label="6 August 2013 Gemini observatory’s rapid-response allows for the detailed study of light from one of the most distant cases of a gamma-ray burst illuminating a galaxy ever observed. Thanks to Gemini’s unparalleled rapid-response capability, and ultra-sensitive nod-and-shuffle spectroscopy, radiation from a distant gamma-ray burst explosion clearly revealed a remarkable event near the edge of the observable universe. The Gemini optical (visible-light) spectrum provided critical evidence that the explosion happened in one of the most distant galaxies ever probed using the illumination provided by a gamma-ray burst (identified as GRB 130606A). This characterization is possible because the high-energy beacon of light from the GRB explosion must pass through interstellar gas within its young host galaxy (shown at left in the figure). The figure also illustrates how the light from the GRB is filtered by billions of light years of intergalactic gas that spans the space between us and the GRB (wide view, at …"><strong>6 August 2013</strong>: Gemini observatory’s rapid-response allows for the detailed study of light from one of the most distant cases of a gamma-ray burst illuminating a galaxy ever observed. Thanks to Gemini’s unparalleled rapid-response capability, and ultra-sensitive nod-and-shuffle spectroscopy, radiation from a distant gamma-ray burst explosion clearly revealed a remarkable event near the edge of the observable universe. The Gemini optical (visible-light) spectrum provided critical evidence that the explosion happened in one of the most distant galaxies ever probed using the illumination provided by a gamma-ray burst (identified as GRB 130606A). This characterization is possible because the high-energy beacon of light from the GRB explosion must pass through interstellar gas within its young host galaxy (shown at left in the figure). The figure also illustrates how the light from the GRB is filtered by billions of light years of intergalactic gas that spans the space between us and the GRB (wide view, at …</div> </div> <div class="news-readmore" aria-label="Read more">Read more</div> </div>  </a> </div> <div class="col-md-3 col-sm-6 col-xs-12"> <a href="/public/announcements/noaoann13004/"> <div class="news-wrapper"> <div class="news-image"> <img class="img-responsive" src="/public/media/archives/images/thumb350x/noaoann13004a.jpg" alt="Fifty Years of Wide Field Studies in the Southern Hemisphere"> </div> <div class="news-description"> <div class="news-id" aria-label="noaoann13004 — Announcement ">noaoann13004 — Announcement</div> <div class="news-title" role="heading" aria-level="1" aria-label="Fifty Years of Wide Field Studies in the Southern Hemisphere ">Fifty Years of Wide Field Studies in the Southern Hemisphere</div> <div class="news-teaser" aria-label="31 May 2013 The CTIO 50th anniversary conference has ended, and was considered a huge success—scientifically diverse and strong, and the historic talks added personality, emotion and pride to the 50th year celebration. We were pleased to have a strong attendance (3 dozen) from the local Chilean Universities, as well as scientists from Europe, Asia, South America and of course the USA. Pictured above are the conference participants."><strong>31 May 2013</strong>: The CTIO 50th anniversary conference has ended, and was considered a huge success—scientifically diverse and strong, and the historic talks added personality, emotion and pride to the 50th year celebration. We were pleased to have a strong attendance (3 dozen) from the local Chilean Universities, as well as scientists from Europe, Asia, South America and of course the USA. Pictured above are the conference participants.</div> </div> <div class="news-readmore" aria-label="Read more">Read more</div> </div>  </a> </div> <div class="col-md-3 col-sm-6 col-xs-12"> <a href="/public/announcements/geminiann13008/"> <div class="news-wrapper"> <div class="news-image"> <img class="img-responsive" src="/public/media/archives/images/thumb350x/geminiann13008a.jpg" alt="Gemini Arrives Early to the Scene of “Shockingly Bright” Gamma-ray Burst"> </div> <div class="news-description"> <div class="news-id" aria-label="geminiann13008 — Announcement ">geminiann13008 — Announcement</div> <div class="news-title" role="heading" aria-level="1" aria-label="Gemini Arrives Early to the Scene of “Shockingly Bright” Gamma-ray Burst ">Gemini Arrives Early to the Scene of “Shockingly Bright” Gamma-ray Burst</div> <div class="news-teaser" aria-label="13 May 2013 Things happened quickly on the night of April 26-27 at the Gemini North control room on Mauna Kea. At 10:45 p.m. an alert arrived for what would later be described in a NASA press release as a “shockingly bright” gamma-ray burst (GRB). Using Gemini’s rapid response Target of Opportunity protocols, the team quickly obtained the first ground-based optical spectrum of the high-energy event. Captured within 90 minutes of detection by both Fermi’s Gamma-ray Burst Monitor (GBM) and NASA’s Swift satellite, Gemini’s spectrum of the GRB’s afterglow surrendered a critical parameter: its distance; the object lies only about 3.6 billion light-years away, which is nearby for a GRB event. Michael Hoenig, who was executing observations with Gemini that night, slewed the telescope to the target almost immediately. “We pretty much dropped everything we were doing at that point,” Hoenig says, “Time is of the essence with GRBs!” Intense flashes of gamma …"><strong>13 May 2013</strong>: Things happened quickly on the night of April 26-27 at the Gemini North control room on Mauna Kea. At 10:45 p.m. an alert arrived for what would later be described in a NASA press release as a “shockingly bright” gamma-ray burst (GRB). Using Gemini’s rapid response Target of Opportunity protocols, the team quickly obtained the first ground-based optical spectrum of the high-energy event. Captured within 90 minutes of detection by both Fermi’s Gamma-ray Burst Monitor (GBM) and NASA’s Swift satellite, Gemini’s spectrum of the GRB’s afterglow surrendered a critical parameter: its distance; the object lies only about 3.6 billion light-years away, which is nearby for a GRB event. Michael Hoenig, who was executing observations with Gemini that night, slewed the telescope to the target almost immediately. “We pretty much dropped everything we were doing at that point,” Hoenig says, “Time is of the essence with GRBs!” Intense flashes of gamma …</div> </div> <div class="news-readmore" aria-label="Read more">Read more</div> </div>  </a> </div> </div> <div class="row news-list news-list-overflow"> <div class="col-md-3 col-sm-6 col-xs-12"> <a href="/public/announcements/geminiann13007/"> <div class="news-wrapper"> <div class="news-image"> <img class="img-responsive" src="/public/media/archives/images/thumb350x/geminiann13007a.jpg" alt="Now Quarterly, April Issue of GeminiFocus Available"> </div> <div class="news-description"> <div class="news-id" aria-label="geminiann13007 — Announcement ">geminiann13007 — Announcement</div> <div class="news-title" role="heading" aria-level="1" aria-label="Now Quarterly, April Issue of GeminiFocus Available ">Now Quarterly, April Issue of GeminiFocus Available</div> <div class="news-teaser" aria-label="9 April 2013 The Gemini Observatory newsletter, GeminiFocus, is now quarterly and available as both a downloadable PDF and in an on-line e-reader format compatible with desktop browsers, tablets, e-readers, and smart phones. Read this issue by visiting: GeminiFocus Each quarterly issue will bring you the latest news about Gemini, its scientific highlights, operations, instrumentation development, and education & outreach. Regular GeminiFocus readers will appreciate the new format's ability to provide more timely information for users while saving resources for Gemini and our planet. In addition, each year, the January issue will provide a year-in-review and be available in a very limited print-run for distribution to libraries and funding agencies. If you would like to be notified of future issues (or receive the annual hard-copy year-in-review issue), please contact us."><strong>9 April 2013</strong>: The Gemini Observatory newsletter, GeminiFocus, is now quarterly and available as both a downloadable PDF and in an on-line e-reader format compatible with desktop browsers, tablets, e-readers, and smart phones. Read this issue by visiting: GeminiFocus Each quarterly issue will bring you the latest news about Gemini, its scientific highlights, operations, instrumentation development, and education & outreach. Regular GeminiFocus readers will appreciate the new format's ability to provide more timely information for users while saving resources for Gemini and our planet. In addition, each year, the January issue will provide a year-in-review and be available in a very limited print-run for distribution to libraries and funding agencies. If you would like to be notified of future issues (or receive the annual hard-copy year-in-review issue), please contact us.</div> </div> <div class="news-readmore" aria-label="Read more">Read more</div> </div>  </a> </div> <div class="col-md-3 col-sm-6 col-xs-12"> <a href="/public/announcements/noaoann13003/"> <div class="news-wrapper"> <div class="news-image"> <img class="img-responsive" src="/public/media/archives/images/thumb350x/noaoann13003a.jpg" alt="Blanco f/8 Secondary Repaired"> </div> <div class="news-description"> <div class="news-id" aria-label="noaoann13003 — Announcement ">noaoann13003 — Announcement</div> <div class="news-title" role="heading" aria-level="1" aria-label="Blanco f/8 Secondary Repaired ">Blanco f/8 Secondary Repaired</div> <div class="news-teaser" aria-label="4 April 2013 The repair of the Blanco telescope’s f/8 secondary has been completed, and the figure of the repaired optic (shown at right) matches the measurement after it was refigured in 1993 (at left). The small circle in the center of the 2013 image represents the diameter of the repair. The repaired mirror will be returned to Chile, where the repairs to the mirror cell are underway. Initial re-integration of the cell on the telescope is scheduled for late June, with first light with the repaired mirror planned for August."><strong>4 April 2013</strong>: The repair of the Blanco telescope’s f/8 secondary has been completed, and the figure of the repaired optic (shown at right) matches the measurement after it was refigured in 1993 (at left). The small circle in the center of the 2013 image represents the diameter of the repair. The repaired mirror will be returned to Chile, where the repairs to the mirror cell are underway. Initial re-integration of the cell on the telescope is scheduled for late June, with first light with the repaired mirror planned for August.</div> </div> <div class="news-readmore" aria-label="Read more">Read more</div> </div>  </a> </div> <div class="col-md-3 col-sm-6 col-xs-12"> <a href="/public/announcements/geminiann13006/"> <div class="news-wrapper"> <div class="news-image"> <img class="img-responsive" src="/public/media/archives/images/thumb350x/geminiann13006a.jpg" alt="Searching for the True Colors of M87's Globular Clusters"> </div> <div class="news-description"> <div class="news-id" aria-label="geminiann13006 — Announcement ">geminiann13006 — Announcement</div> <div class="news-title" role="heading" aria-level="1" aria-label="Searching for the True Colors of M87's Globular Clusters ">Searching for the True Colors of M87's Globular Clusters</div> <div class="news-teaser" aria-label="28 March 2013 Do all globular clusters within a galaxy share a common history? Multiple histories could indicate that different processes drive a galaxy's fundamental development at different times. Juan Carlos Forte (Consejo Nacional de Investigaciones Científicas y Técnicas, Argentina) and colleagues used the Gemini Multi-Object Spectrograph (GMOS) to study over 500 globular clusters in the galaxy M87. Their observations indeed point to such complexity, revealing multiple episodes of star formation. Globular clusters indirectly reveal the star formation history of their host galaxy, and one of their fundamental properties is the metallicity, or abundance of elements more massive than helium. Many globular clusters (GCs) are old, even to the point of challenging other measurements of the age of the universe, but detailed observations can show structure in the distribution of their observed colors. The outstanding question is whether this is evidence of real non-uniformity in the underlying history and metallicity distribution or merely …"><strong>28 March 2013</strong>: Do all globular clusters within a galaxy share a common history? Multiple histories could indicate that different processes drive a galaxy's fundamental development at different times. Juan Carlos Forte (Consejo Nacional de Investigaciones Científicas y Técnicas, Argentina) and colleagues used the Gemini Multi-Object Spectrograph (GMOS) to study over 500 globular clusters in the galaxy M87. Their observations indeed point to such complexity, revealing multiple episodes of star formation. Globular clusters indirectly reveal the star formation history of their host galaxy, and one of their fundamental properties is the metallicity, or abundance of elements more massive than helium. Many globular clusters (GCs) are old, even to the point of challenging other measurements of the age of the universe, but detailed observations can show structure in the distribution of their observed colors. The outstanding question is whether this is evidence of real non-uniformity in the underlying history and metallicity distribution or merely …</div> </div> <div class="news-readmore" aria-label="Read more">Read more</div> </div>  </a> </div> <div class="col-md-3 col-sm-6 col-xs-12"> <a href="/public/announcements/geminiann13005/"> <div class="news-wrapper"> <div class="news-image"> <img class="img-responsive" src="/public/media/archives/images/thumb350x/geminiann13005a.jpg" alt="The Journey Continues…"> </div> <div class="news-description"> <div class="news-id" aria-label="geminiann13005 — Announcement ">geminiann13005 — Announcement</div> <div class="news-title" role="heading" aria-level="1" aria-label="The Journey Continues… ">The Journey Continues…</div> <div class="news-teaser" aria-label="14 March 2013 “Do you think space aliens are real?” Gemini Observatory’s Director Markus Kissler-Patig asks a class of students. His question is part of Gemini’s Journey through the Universe (JttU) program where dozens of scientists and educators share their work and, most importantly, inspire young Hawai‘i Island students. “I think the students in our classrooms today are the ones who will answer the big questions we are asking, such as what, and possibly who, is out there on all of those planets we are only starting to discover now,” says Kissler-Patig. Now in its ninth year, JttU wraps up its annual “Journey Week” on March 15th. During this week Gemini staff joined over 50 other scientists, researchers, and educators in classrooms across East Hawai‘i (see photos in this feature). “The goal of this program is to inspire our keiki,” says the program’s manager and Gemini’s education and outreach leader Janice Harvey. “Even …"><strong>14 March 2013</strong>: “Do you think space aliens are real?” Gemini Observatory’s Director Markus Kissler-Patig asks a class of students. His question is part of Gemini’s Journey through the Universe (JttU) program where dozens of scientists and educators share their work and, most importantly, inspire young Hawai‘i Island students. “I think the students in our classrooms today are the ones who will answer the big questions we are asking, such as what, and possibly who, is out there on all of those planets we are only starting to discover now,” says Kissler-Patig. Now in its ninth year, JttU wraps up its annual “Journey Week” on March 15th. During this week Gemini staff joined over 50 other scientists, researchers, and educators in classrooms across East Hawai‘i (see photos in this feature). “The goal of this program is to inspire our keiki,” says the program’s manager and Gemini’s education and outreach leader Janice Harvey. “Even …</div> </div> <div class="news-readmore" aria-label="Read more">Read more</div> </div>  </a> </div> </div> <div class="row news-list news-list-overflow"> <div class="col-md-3 col-sm-6 col-xs-12"> <a href="/public/announcements/noaoann13002/"> <div class="news-wrapper"> <div class="news-image"> <img class="img-responsive" src="/public/media/archives/images/thumb350x/noaoann13002a.jpg" alt="March 2013 NOAO Newsletter"> </div> <div class="news-description"> <div class="news-id" aria-label="noaoann13002 — Announcement ">noaoann13002 — Announcement</div> <div class="news-title" role="heading" aria-level="1" aria-label="March 2013 NOAO Newsletter ">March 2013 NOAO Newsletter</div> <div class="news-teaser" aria-label="28 February 2013 The March 2013 NOAO Newsletter is online and ready to download. This issue includes information pertaining to the 2013B Call for Proposals, which are due March 28, 2013. On the Cover This cover presents a collage of the past, present, and future of the Cerro Tololo Inter-American Observatory in Chile in celebration of the observatory’s 50th anniversary."><strong>28 February 2013</strong>: The March 2013 NOAO Newsletter is online and ready to download. This issue includes information pertaining to the 2013B Call for Proposals, which are due March 28, 2013. On the Cover This cover presents a collage of the past, present, and future of the Cerro Tololo Inter-American Observatory in Chile in celebration of the observatory’s 50th anniversary.</div> </div> <div class="news-readmore" aria-label="Read more">Read more</div> </div>  </a> </div> <div class="col-md-3 col-sm-6 col-xs-12"> <a href="/public/announcements/geminiann13004/"> <div class="news-wrapper"> <div class="news-image"> <img class="img-responsive" src="/public/media/archives/images/thumb350x/geminiann13004a.jpg" alt="Surprising Results From the Earliest Near-Infrared Spectroscopy of a Type Ia Supernova"> </div> <div class="news-description"> <div class="news-id" aria-label="geminiann13004 — Announcement ">geminiann13004 — Announcement</div> <div class="news-title" role="heading" aria-level="1" aria-label="Surprising Results From the Earliest Near-Infrared Spectroscopy of a Type Ia Supernova ">Surprising Results From the Earliest Near-Infrared Spectroscopy of a Type Ia Supernova</div> <div class="news-teaser" aria-label="14 February 2013 Gemini Near-Infrared Spectrograph (GNIRS) observations lead to surprising results on the nature of Type Ia supernovae (SNe Ia). Time-series near-infrared spectra of SN 2011fe hint that more SNe Ia harbor unprocessed carbon than previously believed, and what we thought was the main driver of the luminosity-decline rate Phillips relation may not be correct. Understanding the true nature of Type Ia supernovae (SNe Ia) is a linchpin of contemporary cosmology. Specifically, these explosions are critical for tracking the expansion history and acceleration of our universe. Commonly called “dark energy,” the discovery of this universal acceleration was the basis for the 2011 Nobel Prize in Physics. Now, researchers using the Gemini Near-Infrared Spectrograph (GNIRS), at the Gemini North telescope on Hawaii’s Mauna Kea, have taken a major leap forward in understanding SNe Ia with the first detection of unprocessed carbon in near-infrared spectra of a normal Type Ia supernova. The supernova (geminiann13004a), …"><strong>14 February 2013</strong>: Gemini Near-Infrared Spectrograph (GNIRS) observations lead to surprising results on the nature of Type Ia supernovae (SNe Ia). Time-series near-infrared spectra of SN 2011fe hint that more SNe Ia harbor unprocessed carbon than previously believed, and what we thought was the main driver of the luminosity-decline rate Phillips relation may not be correct. Understanding the true nature of Type Ia supernovae (SNe Ia) is a linchpin of contemporary cosmology. Specifically, these explosions are critical for tracking the expansion history and acceleration of our universe. Commonly called “dark energy,” the discovery of this universal acceleration was the basis for the 2011 Nobel Prize in Physics. Now, researchers using the Gemini Near-Infrared Spectrograph (GNIRS), at the Gemini North telescope on Hawaii’s Mauna Kea, have taken a major leap forward in understanding SNe Ia with the first detection of unprocessed carbon in near-infrared spectra of a normal Type Ia supernova. The supernova (geminiann13004a), …</div> </div> <div class="news-readmore" aria-label="Read more">Read more</div> </div>  </a> </div> <div class="col-md-3 col-sm-6 col-xs-12"> <a href="/public/announcements/geminiann13003/"> <div class="news-wrapper"> <div class="news-image"> <img class="img-responsive" src="/public/media/archives/images/thumb350x/gemini-ngc7232-final.jpg" alt="Australian Student “Thinks Big” for Imaging Contest"> </div> <div class="news-description"> <div class="news-id" aria-label="geminiann13003 — Announcement ">geminiann13003 — Announcement</div> <div class="news-title" role="heading" aria-level="1" aria-label="Australian Student “Thinks Big” for Imaging Contest ">Australian Student “Thinks Big” for Imaging Contest</div> <div class="news-teaser" aria-label="13 February 2013 On Tuesday, February 12, 2013 Australian High School Senior Ryan Soares had stars in his eyes during a ceremony celebrating his winning selection for the 2012 Australian Gemini Schools Imaging contest. In describing his entry, which features a group of three beautiful galaxies, he said that he chose the grouping because the galaxies, “…had never been imaged as a group by a large professional telescope such as Gemini South.” Ryan was also “thinking big” with this project, by suggesting that the telescope should take not one but two images and “stitch” them together to capture the panorama of the three galaxies. “I thought that if they let me do this, in future other students could propose other big, exciting regions of sky to study,” he said. This approach was challenging due to the limited time available (about one hour total) for the observations. Each of the two images required three …"><strong>13 February 2013</strong>: On Tuesday, February 12, 2013 Australian High School Senior Ryan Soares had stars in his eyes during a ceremony celebrating his winning selection for the 2012 Australian Gemini Schools Imaging contest. In describing his entry, which features a group of three beautiful galaxies, he said that he chose the grouping because the galaxies, “…had never been imaged as a group by a large professional telescope such as Gemini South.” Ryan was also “thinking big” with this project, by suggesting that the telescope should take not one but two images and “stitch” them together to capture the panorama of the three galaxies. “I thought that if they let me do this, in future other students could propose other big, exciting regions of sky to study,” he said. This approach was challenging due to the limited time available (about one hour total) for the observations. Each of the two images required three …</div> </div> <div class="news-readmore" aria-label="Read more">Read more</div> </div>  </a> </div> <div class="col-md-3 col-sm-6 col-xs-12"> <a href="/public/announcements/noaoann13001/"> <div class="news-wrapper"> <div class="news-image"> <img class="img-responsive" src="/public/media/archives/images/thumb350x/noaoann13001a.jpg" alt="Miss Tohono O’odham 2013"> </div> <div class="news-description"> <div class="news-id" aria-label="noaoann13001 — Announcement ">noaoann13001 — Announcement</div> <div class="news-title" role="heading" aria-level="1" aria-label="Miss Tohono O’odham 2013 ">Miss Tohono O’odham 2013</div> <div class="news-teaser" aria-label="11 February 2013 Miss Tohono O’odham 2013 and her court visited the NOAO booth at the 75th Annual Tohono O’odham Rodeo & Fair, Feb 1-3. Shown in the picture: (L2R) Katy Garmany, Lori Allen, 1st Attendant Jaylene Wood, 2nd Attendant Raven Johnson, and Miss Tohono O’odham Nation Hon’mana Sekteoma. Jaylene Wood sang an O’odham traditional song describing an eagle soaring over Kitt Peak. See an article about the Fair in the March NOAO Newsletter."><strong>11 February 2013</strong>: Miss Tohono O’odham 2013 and her court visited the NOAO booth at the 75th Annual Tohono O’odham Rodeo & Fair, Feb 1-3. Shown in the picture: (L2R) Katy Garmany, Lori Allen, 1st Attendant Jaylene Wood, 2nd Attendant Raven Johnson, and Miss Tohono O’odham Nation Hon’mana Sekteoma. Jaylene Wood sang an O’odham traditional song describing an eagle soaring over Kitt Peak. See an article about the Fair in the March NOAO Newsletter.</div> </div> <div class="news-readmore" aria-label="Read more">Read more</div> </div>  </a> </div> </div> <div class="row statusbar"><div class="col-md-3"> Showing 1 to 20 of 22 </div><div class="col-md-6"><div class="text-center"><ul class="pagination"><li class="active"><a href="/public/announcements/archive/year/2013/page/1/">1</a></li><li><a href="/public/announcements/archive/year/2013/page/2/">2</a></li><li><a class="prev-next" href="/public/announcements/archive/year/2013/page/2/">Next</a></li></ul></div></div></div><div class="row"><div class="col-md-12"></div></div> <div class="copyright"> <a href="/public/copyright/">Usage of NOIRLab Images and Videos</a><br /> <a href="/public/subscribe-media/">Are you a journalist? 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Announcements 2013 | NOIRLab