This week’s SDSS tweeter is Jonathan Bird, current the VIDA (Vanderbilt Inititative in Intensive Data Astrophysics) postdoctoral fellow at Vanderbilt University, and Co-Chair of the Disk Science Working Group for APOGEE.
Jonathan received his PhD in 2012 from the Ohio State University. His thesis focused on using numerical simulations to look for patterns in the dynamics and chemistry of the stars in disk galaxies which can be linked to specific evolution and formation mechanisms. He has used both APOGEE and SEGUE data to search for such signatures in our own Milky Way Galaxy.
Jonathan is currently working on generating mock APOGEE catalogs from simulated disk galaxies. Of the SDSS surveys, he is most connected with APOGEE, where he is co-chair of the disk science working group, but he is also hoping to get more involved with MaNGA soon.
Jonathan regularly tweets as @galaxyhistorian and has been working on some awesome visualisations of the APOGEE and SEGUE data sets, so keep your fingers cross for a sneak peek this week.
This week the Sloan Foundation 2.5m telescope at Apache Point Observatory will reopen and start observing for the new season. Did you know that all SDSS Collaboration members can sign up for nightly notifications of what the telescope has been observing?
The tweeter for this exciting week in the annual life of SDSS will be Isabelle Paris from the Osservatorio astronomico di Trieste (Astronomical Observatory of Trieste, Italy). Isabelle has been an SDSS member since she started working on her PhD with Patrick Petitjean at the IAP (Institut d’Astrophysique de Paris, France). The topic of her thesis was the cosmological evolution of the opacity of the intergalactic medium, which Isabelle studied using SDSS-DR7 and BOSS data. Following this Isabelle has a 2 year postdoc at the Universidad de Chile, and is now an External Participant of the SDSS Collaboration based in Trieste.
Isabelle is the Chair of the (SDSS-III) quasar science working-group and is also in charge of generating the quasar catalogues for SDSS. So I think we can expect to hear a lot about supermassive black holes and very high redshift sources this week.
Above, Isabelle is pictured in July 2010 attending a BOSS Lyman-alpha Forest and Quasar Working Groups meeting in Pittsburgh.
This week the SDSS is preparing for our telescope at Apache Point Observatory to come out of its usual 4 week summer
vacation shutdown and get back to observing.
This period of shutdown is a very busy one for SDSS operations when a lot of essential maintenance happens. For example this year the primary mirror of the telescope has been given a new reflective coating. The timing of the shut down is set to coincide with the monsoon season in the South West of the USA – a period when the weather is often not good for observing anyway.
As part of the process of re-opening, SDSS Operations Software Guru John Parejko (who is usually based at Yale University in New Haven, CT) will travel out to APO. John has agreed to tweet what’s going on for us as our “Tweep of the week” while the telescope gets ready to start observing again.
John got his PhD in physics in 2010 from Drexel University where he used SDSS data to study the topic of Low Luminosity Active Galaxies (ie. how supermassive black holes which are only accreting a little bit work). Following this he was a postdoc at Yale University working on the BOSS (Baryon Acoustic Oscillation Spectrosopice Survey) data, before taking over responsibility for the SDSS telescope operations software two years ago.
John’s an example of someone whose been in the SDSS family for a while!
Over 150 scientists from institutions in 13 countries in Europe, Asia, North America and South America recently traveled to Park City, Utah for the SDSS Collaboration meetings. First SDSS-IV got underway. The start of SDSS-IV observations on July 1, 2014 meant that this meeting was much less anticipatory and much more participatory than the SDSS-IV meeting last year. For the second half of the week, the SDSS-III collaboration, data all taken, was focused on the interesting science results coming out of this very successful 6-year survey. The overlap between the membership of the SDSS-IV and SDSS-III collaborations is quite large, so expect to see many of the faces in the photo from the SDSS-III half of the meeting in the future as well! Our enthusiastic thanks to the University of Utah for playing host to such a fabulous set of meetings.
A Storify of tweets from the recent collaboration meeting with the hashtag #sdss2014.
This week is the 2014 SDSS Collaboration Meeting which is happening in Park City, Utah. The @SDSSurveys twitter account will be “taken over” this week by Dr. Karen Masters from the Institute of Cosmology and Gravitation at the University of Portsmouth.
Karen is the first ever “SDSS Tweep of the Week” – a new idea to give the SDSS Twitter account over to collaboration members for week long stints. We don’t expect to fill every week this way, but look out on the blog for introductions to future “Tweeps” from the more than 200 scientists involved in SDSS from all over the world.
As our SDSS Director of Education and Public Engagement, Karen is the ideal guinea pig for this plan. Karen is also a science team member of the @MangaSurvey part of SDSS so expect to hear a lot from MaNGA parallel sessions during this week.
If you’re a SDSS Collaboration Member reading this and interested to sign up for a week please visit the Twitter Schedule on the Wiki (password protected site).
The Alfred P. Sloan Foundation is now accepting nominations for Sloan Research Fellowships in eight fields: chemistry, computational and evolutionary molecular biology, computer science, economics, mathematics, neuroscience, ocean sciences, and physics. These two-year, $50,000 fellowships are awarded annually to 126 early-career faculty in recognition of their distinguished performance and exceptional potential as researchers. Candidates must be nominated by a department head or other senior researcher. For more information, please visit this site:
With the start of SDSS-IV this July, the Sloan Digital Sky Survey is entering a new and exciting phase of exploring the Universe. We’ve imaged 1/3 of the sky and taken over 3 million spectra, but we haven’t explored beyond the centers of nearby galaxies, haven’t mapped the Universe between 3 and 7 billion years after the Big Bang, and haven’t studied the part of the Milky Way that is only visible from the Southern Hemisphere. Well, that all changes starting now! We have a press release today featuring the science of SDSS-IV and including a fantastic video by John Parejko illustrating how SDSS takes all that data (hint: it starts with a lot of work in the daytime and continues with a lot of work in the nighttime).
As part of the transition from SDSS-III to SDSS-IV we have just launched a revamped version of the sdss.org website.
The site is redesigned to represent the entire SDSS, from the beginning through today. We hope that it provides a good balance between presenting our amazing results so far and our exciting future.
Congratulations to the web team on the successful transition of the sites.
Tonight marks the official start of the fourth phase of the Sloan Digital Sky Surveys (SDSS-IV), and the end of SDSS-III.
SDSS-III ran from 2008-2014 and made a major upgrade of the SDSS spectrographs. SDSS-III contained four interweaved surveys: BOSS focussed on mapping the clustering of galaxies and intergalactic gas in the distant universe; SEGUE-2 and APOGEE surveyed the dynamics and chemical evolution of the Milky Way; and MARVELS observed the population of extra-solar giant planets. Over the full survey, SDSS-III took more than 2 million spectra, all of which will be released in a final SDSS-III Data Release (DR12 for the SDSS) in January 2015.
SDSS-IV will run from 2014-2020, comprising three surveys, eBOSS, APOGEE-2 and MaNGA. eBOSS will work to extend precision cosmological measurements to a critical early phase of cosmic history; APOGEE-2 will expand the survey of the Galaxy across both the northern and southern hemispheres, and MaNGA will for the first time using the Sloan spectrographs to make spatially resolved maps of individual galaxies.
We’d like to take this chance to congratulate the SDSS-III collaboration on a successful set of surveys, and wish SDSS-IV all the best for the future.
The 2014 Shaw Prize in Astronomy has been awarded to Daniel Eisenstein, John Peacock, and Shaun Cole “for their contributions to the measurements of features in the large-scale structure of galaxies used to constrain the cosmological model including baryon acoustic oscillations and redshift-space distortions.” For more details on the Shaw Prize see http://www.shawprize.org/en/
Daniel Eisenstein, the director of SDSS-III, remarks that “although this is a tremendously gratifying personal recognition, it is also a wonderful recognition of the SDSS/BOSS and 2dFGRS collaborations that have created these exquisite surveys and pushed forward the science of large-scale structure. It is a great honor for our field and our teams!”
Shaun Cole and John Peacock were key members of the 2dF Galaxy Redshift Survey (2dFGRS) which together with the work of Daniel Eisenstein and his SDSS collaborators made the first detections of the baryon acoustic oscillation pattern in the distribution of galaxies in the Universe. Baryon acoustic oscillations are an imprint from fluctuations of matter and light in the early Universe. By measuring the apparent size of this pattern at different cosmic eras, astronomers are studying the nature and amount of dark matter and dark energy that govern our expanding Universe.
SDSS congratulates all of the winners of this year’s Shaw Prize in Astronomy!
A post by Garrett Ebelke, Telescope Operation Specialist and APOGEE Hardware Development and Training Coordinator at Apache Point Observatory. Translated into Spanish by Loreto Barcos and Guillermo Damke (University of Virginia), with help from Veronica Motta (Universidad de Valparaíso, Chile).
Publicado por Garret Ebelke, Especialista de Operaciones del Telescopio y Coordinador de Desarrollo y Entrenamiento del Instrumento de APOGEE del Observatorio Apache Point. Traducido al Español por Loreto Barcos-Muñoz y Guillermo Damke (Universidad de Virginia, con ayuda de Veronica Motta (Universidad de Valparaíso, Chile).
Durante la segunda mitad de Abril, los ingenieros Daniel Garrido y Mario Cáceres viajaron desde Chile al Observatorio Apache Point (APO, por sus siglas en inglés), en Nuevo México, como parte del proyecto QUIMAL de la Universidad de La Serena. El objetivo de su viaje fue conocer en profundidad la infraestructura del instrumento de APOGEE para adquirir un conocimiento más acabado de sus numerosos subsistemas. Estos serán replicados en el proyecto APOGEE-2 e instalados en el telescopio du Pont de 2.5 m ubicado en el Observatorio Las Campanas (LCO, por sus siglas en inglés).
During the second half of April, Daniel Garrido and Mario Caceres, both engineers from Chile, travelled to Apache Point Observatory in New Mexico as part of the QUIMAL project at the Universidad de La Serena. The purpose of their trip was to delve deep into the APOGEE infrastructure hardware to gain a better understanding of the numerous hardware sub-systems. These systems will be replicated for the APOGEE-2 project and installed at the du Pont 100-inch Telescope at Las Campanas Observatory.
[For more on the plans for APOGEE observing at Las Campanas see this blog post.]
While at APO, they were introduced to the daily task of plugging fiber optics into spectrographic plug plates, all contained within cartridges. They became very familiar with mounting these cartridges to the telescope, and how much care must be taken when handling the cartridges. A similar cartridge design will be used at LCO and Daniel will be heavily involved in assembling and populating the cartridges with fiber optics. Daniel was very eager to explore the internal configuration of the cartridges and quickly got his hands dirty once we opened a cartridge.
Durante su visita a APO, se les inició en la tarea diaria de conectar fibras ópticas a placas espectrográficas, cada una contenida en distintos cartuchos. Daniel y Mario también aprendieron a montar estos cartuchos en el telescopio y entendieron la delicadeza de este proceso. Los cartuchos que se utilizarán en el LCO tendrán un diseño similar. Daniel además estará involucrado en el montaje e instalación de las fibras ópticas en los cartuchos en el LCO. Daniel mostró mucho entusiasmo en explorar la configuración interna de los cartuchos y no tuvo inconvenientes en “ensuciarse las manos” para estudiarlos por sí mismo.
No pudimos dejarlos marcharse de APO sin antes llevarlos a disfrutar del lado oscuro de las operaciones, donde pasaron varias noches familiarizándose con las operaciones nocturnas. Una parte importante de las observaciones es el aprendizaje del software usado para controlar el telescopio y el instrumento de APOGEE.
We couldn’t let them leave APO without letting them join the dark side of operations, where they spent several nights being introduced to nightly operations. A major part of observing is learning the software used to interface with the telescope and the APOGEE instrument.
This was an excellent start to incorporating some Chilean participants to the APOGEE-2 project, the hardware designs, operational processes and forge an excellent working relationship that will last throughout the entire project.
Esta fue una gran oportunidad para comenzar a incorporar participantes chilenos al proyecto APOGEE-2, al diseño del instrumento, los procesos operacionales, y para forjar una excelente relación de trabajo que durará a lo largo de todo el proyecto.
All photos were taken using Daniel Garrido’s camera, there are many more photos at Mario’s web gallery.
A post by Anne-Marie Weijmans, the MaNGA Lead Observer:
Last month MaNGA (Mapping Nearby Galaxies at APO) had its first commissioning run at Apache Point Observatory, with its first installed cartridge. MaNGA is part of SDSS-IV and scheduled to start observing in July of this year, but it now already has its first galaxies in hand!
MaNGA is an integral-field spectroscopy survey, which will map the motions and properties of stars and gas in 10,000 galaxies. By grouping fibers together into integral-field units, MaNGA obtains spectra not just of the centre of the galaxy, but also its outskirts, covering the whole galaxy. This means that we can measure properties of stars, such as age and metallicity, over a large surface area in the galaxy, and based on that, figure out how these galaxies were assembled. We also are able to measure the velocities of the stars, which in turn tells us about the structure of the galaxy, and how much dark matter is present. From the gas, we learn about the radiation present in the galaxy: is the gas energized by young stars (indicating that there is on-going star formation), by an active black hole, or both? Combining all these different sets of information, we form a picture of how different galaxies form, and evolve over time.
MaNGA instrument scientist Niv Drory (UT at Austin) and chief engineer Nick MacDonald (UW) prepared the cartridge, carefully adding the MaNGA integral-field units and making sure that the surfaces of the fibers were clean to optimize their light throughput. The observers at APO, together with MaNGA lead observer Anne-Marie Weijmans and several other members of the MaNGA team took various test-observations of sky and stars, before turning their attention to galaxies. MaNGA can observe 17 galaxies in one go, and with two plates completed this resulted in 34 galaxies.
Right now, two more cartridges are being prepared for MaNGA to start observing this summer, and in the Fall, three more cartridges will follow. And at the same time, MaNGA lead data scientist David Law (Toronto) and survey scientist Renbin Yan (Kentucky) with many other members of the MaNGA team are working hard to analyze the results of these first 34 galaxies. Only 9,966 more to go!
To keep in touch with MaNGA and see what we are up to, follow us on Twitter @MaNGASurvey.
A few more pictures:
The SDSS is delighted, and feel this is a well a deserved recognition testament to Daniel’s scientific accomplishments and leadership.
Daniel wants to emphasize that he feels this recognition is also a recognition of the impressive scientific scope of the Sloan Digital Sky Survey, in all its iterations, which has been the context for key aspects of Daniel’s scientific and leadership accomplishments.
So congratulations to the SDSS-III Director and also to all those who have helped make all phases and surveys of the SDSS a success over the past decades.
Please join us in congratulating all four astronomers on this honor and accomplishment!