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Prof. Offner received her bachelor's degrees in physics and mathematics from Wellesley College in 2003 and completed a Ph.D. in physics at the University of California at Berkeley in 2009. From 2009-2012 she was an NSF Astronomy & Astrophysics prize postdoctoral fellow at the Harvard-Smithsonian Center for Astrophysics and a NASA Hubble prize postdoctoral fellow at Yale from 2012-2014. Before joining the astronomy faculty at UT Austin in 2017, she was an assistant professor at the University of Massachusetts Amherst. Prof. Offner's research focuses on understanding how stars like the Sun form by combining numerical simulations, observations and observational modeling. She is also intesested in applying statistical techniques and machine learning to parse data and identify the physical characteristics of forming stars.
Flexible Image Transport System (FITS) was initially developed by astronomers in the USA and Europe in the late 1970s to serve the interchange of data between observatories and was brought under the auspices of the International Astronomical Union in 1982. In 2012, FITS is still in widespread use as a data interchange and archiving format by astronomers. FITS is a fileformat designed to store, transmit, and manipulate scientific images and associated data. The term "image" in the standard's name is loosely applied and FITS files often contain only non-image data. Astronomers view their images as data for analysis rather than simply as pictures to look at. From its beginning, FITS was seen as a transport format for more than a still image intended for printing or viewing in two dimensions. FITS was designed to facilitate the unambiguous transmission of n-dimensional regularly spaced data arrays, an n-cube. These multi-dimensional arrays may be 1-D spectra, 2-D images or data cubes of three or more dimensions. Two-dimensional tables containing rows and columns of data can also be stored in a FITS file. The substantial use of FITS for data that even astronomers would not class as image data led to consideration to change the full name for the FITS format, but the proposal was rejected. For the same reason, in this resource, FITS is categorized primarily as a dataset format, with use for image data as secondary.
FITS was designed with an eye towards long-term archival use, and the maxim "once FITS, forever FITS" (or "once FITS, always FITS") has guided the IAU to ensure that the format is backwards compatible as new features are added. Version 3 (published in 2012 and distinguished in this format resource as FITS_3) documented several features approved since the previous edition of the full specification: support for 64-bit integers (from an earlier maximum of 32 bits) in images and tables; tables with variable-length arrays; and adopted new World Coordinate Systems (WCS) conventions to map an element in a data array to standard physical coordinates on the sky. WCS conventions also exist to define mappings for a spectral coordinate into a standard frame of reference, allowing spectral shifts due to the Doppler effect and/or cosmic expansion to be accounted for. The WCS conventions are implemented through an extensive set of reserved keywords and values to be used in headers associated with image arrays. A WCS convention for specifying time and relative dimensions in space is in preparation as of early 2013.
The FITS format is primarily for use with astronomy images and/or data; it is not a format for raster images in general. Many FITS files have no image data, containing, for example a catalog of celestial objects. A useful description of FITS for an audience interested in the applicability of FITS for storing scanned images of cultural heritage materials, such as manuscripts, was given by Lucio Chiappetti at the 2012 European Week of Astronomy and Space Science [ _EWASS2012.pdf] at a special session on long-term preservation of digital cultural resources.
The FITS data format was developed in the late 1970s for interchange of astronomical image data between observatories. In 1981, the FITS specification was published in Astronomy and Astrophysics Supplement, Vol. 44, pp. 363-370. By then, FITS had become the de facto standard interchange format for astronomy data. In the 1990s several versions of the specification were published by NOST (NASA Office of Science and Technology): NOST 100-1.0 (June 1993); NOST 100-1.1 (September 29 1995); NOST 100-1.2 (April 1998); and NOST 100-2.0 (March 1999). FITS Version 2.1b was published in December 2005. Version 3.0 was approved in July 2008, and formally published in 2010. Version 4.0 was adopted in July 2016, and formally released in August 2018 after editing for language, not substance. All versions since 1993 are available at _standard.html.
MAJOR RENOVATIONS TIMELINE:1988 - Became Dan Law Field, lighting system installed, first night game ever played.1990 - Formerly an all grass field saw installation of Astro Turf 8 to Dan Law Field infield.1992 - Concession stand, ticket booth, restrooms installed.1993 - Message board added to scoreboard structure.1994 - Original locker rooms built on first and third base side.1996 - 14 luxury skyboxes installed.1999 - New infield turf installed.2001 - Addition of a new clubhouse, outfield fence complete with major-league style bullpens, an interior brick facade and new exterior fence.2004 - LED Video Board (15' X 20') installed.2007 - FieldTurf installed.2009 - Clubhouse renovations that include 67-inch, high definition television along with theater style seating, wireless Internet, individual seating at each locker and game tables.2011 - Announced plans for a $5 million renovation with a new press box and suites and addition of a club level with outdoor seating. A new shading structure will cover the area in the center portion of the grandstand and will rise above the new suites and press box. Shading structure will be directly overhead 1,154 individual chair-back seats that will be installed at Dan Law Field for the first time in the history of the stadium.2011 - Announced stadium name change to Dan Law Field at Rip Griffin Park.2012 - Began play at the renovated Dan Law Field at Rip Griffin Park.2015 - Installed a new FieldTurf surface and replaced video board with an updated version that previously occupied Jones AT&T Stadium.2016 - Installed a new outfield padded fence, keeping the dimensions to the walls the same and dropping the height of the fence to 7'6".
The UCSC major in astrophysics is administered by the Physics Department and combines a core physics major with advanced electives in astrophysics, an astrophysics laboratory course, and senior thesis work on a topic in astrophysics. It is a rigorous program designed to prepare students for a broad range of technical careers or for entry into graduate or professional programs. A full description of the major can be found in the physics section of this catalog.
In 2012, the skeuomorphic look of Frutiger Aero (i.e. Windows 7) started to fade in favor of the Flat Design look (i.e. Windows 10). Sometimes, companies like Windows 8 and LG webOS 1.0-3.6 have switched to Frutiger Metro, and then to Flat Design. By 2013, Frutiger Aero was fully overtaken by Flat Design with the release of iOS 7. In 2017, another minimalist Web/tech aesthetic appeared, known as Corporate Memphis.
* As part of the 2011-2012 McCain Performance Series, Pilobolus Dance Theatre will perform at 7:30 p.m. Tuesday, April 24, at McCain Auditorium. A highly unusual dance company, Pilobolus is creative, expressive and athletic. The group is known for its humor, stunning imagery and acrobatic skill. Tickets cost $12.50-$36, plus applicable taxes and fees. Drop by the McCain Auditorium box office to get tickets or call 785-532-6428. Tickets also can be purchased online at -state.edu/mccain. 2ff7e9595c
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