Iras-allsky

History

IRAS and the Founding of IPAC

In 1985, IPAC was established on the campus of the California Institute of Technology as the "Infrared Processing & Analysis Center" for data from IRAS -- the Infrared Astronomical Satellite, joint project of the US, UK and the Netherlands. IPAC has since grown beyond its inaugural name - and is now known simply as "IPAC" - by building upon its experience in infrared data processing and analysis to provide a range of support for more than 20 missions and projects with observatories both in space and on the ground.

 
NED

In 1990, IPAC  built the NASA/IPAC Extragalactic Database (NED), which quickly became an essential tool for extragalactic research. Today, NED is the world's largest database of cross-correlated multiwavelength data for extragalactic objects and services, which spans the entire observed spectrum, from gamma rays to radio frequencies.

IRSA

In the mid-90s, NASA designated IPAC as the US science support center for their infrared  and sub-millimeter projects and missions.  In response, IPAC formed the NASA/IPAC Infrared Science Archive (IRSA)  in order to (1) curate and serve scientific data products, (2) enable optimal scientific exploration of these data sets by astronomers, and (3) support planning for, operation of, and data set generation from NASA missions. Since its founding,  IRSA has evolved to become the data center for a large number of  space missions, including ISO, MSX, Spitzer, WISE/NEOWISE, Herschel, Planck, as well as ground-based telescope facilities such as 2MASS, PTF and ZTF.  IRSA continues to expand to better serve existing and future missions.

Science and Data Center Functions

Already well established as a hub for science data, IPAC continued to expand its expertise to provide multiple mission operations, as well as education and outreach services to NASA and the astronomical community.

IPAC serves as the administrative home of the NASA Exoplanet Science Institute. IPAC provides data and science center functions, and is a partner in several large scale, high-impact missions including the Nancy Grace Roman Space TelescopeEuclidHerschelSpitzerPlanckWISE/NEOWISE, Keck, ISO, IRAS, Rubin, and many more. 

The Future

IPAC continues to seek out missions and projects where the unique range of expertise developed over three decades can be leveraged to optimally support discovery and the advancement of the scientific frontier.  IPAC staff are currently involved in future large and high-priority missions and in mission studies to prepare for follow-on to the US 2020 Astronomy and Astrophysics Decadal Survey. This includes the Ultraviolet Explorer (UVEX) which will undertake a synoptic survey of the entire sky in the near-UV and far-UV. 

IRAS

January 1, 1985

IPAC was established in 1985 on the campus of the California Institute of Technology and originally provided expertise and support for the processing and analysis of data from IRAS. IPAC's role with IRAS continues to this day, with the Infrared Science Archive (IRSA) at IPAC holding the IRAS archive.

NASA Extragalactic Database

January 3, 1990

The NASA/IPAC Extragalactic Database (NED) started service in 1990, and quickly became an essential tool for extragalactic research. NED is the world's largest database of cross-correlated multiwavelength data for extragalactic objects, providing a systematic fusion of information integrated from hundred of large sky surveys and tens of thousands of research publications. The contents and services span the entire observed spectrum from gamma rays through radio frequencies. NED is built around a master list of extragalactic objects for which cross-identifications of names have been established, accurate positions and redshifts entered to the extent possible, and some basic data collected. Bibliographic references relevant to individual objects have been compiled, and abstracts of extragalactic interest are kept on line. Detailed and referenced photometry, position, and redshift data, have been taken from large compilations and from the literature. NED also includes images from 2MASS, from the literature, and from the Digitized Sky Survey. NED's data and references are being continually updated, with revised versions being put on-line every 4-6 months.

IRSA

January 1, 1993

IPAC supports NASA's Astrophysics Archives by operating the NASA/IPAC Infrared Science Archive (IRSA). IRSA is the primary archive for NASA's infrared and submillimeter missions, including Spitzer, (NEO)WISE, 2MASS, IRTF, SOFIA, and IRAS, as well as upcoming missions like SPHEREx and NEOSurveyor. IRSA also serves data from ESA missions with NASA participation, such as Euclid, Planck, and Herschel.

ISO

January 1, 1995

IPAC supported the US community in their use of ISO (1995-98), the first pointed infrared observatory in space. IRSA maintains the ISO Visualizer - a tool for displaying ISO observations on the sky, providing links to the ISO postcard server at Vilspa, Spain and Atlas, which serves a uniform catalog of Short Wavelength Spectrometer (SWS) spectra derived from valid, full-scan, 2.4 - 45.5 micron spectra available in the ISO archive.

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MSX

January 9, 1996

The Midcourse Space Experiment (MSX), a Ballistic Missile Defense Organization (BMDO) sponsored military satellite, was launched in April 1996. MSX offered benefits for both the defense and civilian sectors. Collaborative efforts between the Air Force Research Laboratory and IPAC has resulted in an archive containing images for about 15 percent of the sky, including the entire Galactic Plane, the Large Magellanic Cloud, and regions of the sky not covered by IRAS. The MSX data archive is hosted by IRSA at IPAC.

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2MASS

January 1, 1997

IPAC carried out analysis, processing and archiving for 2MASS (1997-2001), the first high-resolution, all-digital sky survey. IRSA maintains the 2MASS archive with access to images, catalogs and analysis tools.

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Spitzer Science Center

March 1, 1997

The responsibility for the Spitzer Science Center (SSC) was assigned to IPAC in 1997, and Spitzer began science operations in 2003. The SSC was responsible for science operations for the astronomical community including proposal planning, observation planning, observation scheduling, data processing, data archiving, data reduction support, public affairs and education and public outreach. The Spitzer Heritage Archive for science data is hosted by IRSA, also within IPAC. Spitzer was decommissioned on January 30, 2020.

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NExScI

January 1, 2000

The NASA Exoplanet Science Institute (NExScI) was established in 2000. NExScI provides tools and archives for the exoplanet community, co-administers the Hubble Fellowship program and workshops, supports the Keck Interferometer and Large Binocular Telescope Interferometer. NExScI provides administration of NASA Keck telescope time, and additional projects in the Exoplanet Exploration Program. NExScI has also developed and operates the Kepler Science and Analysis System (KSAS), the Keck Observatory Archive, and is the home of NASA's Exoplanet Archive.

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Keck Observatory Archive

September 2, 2004

Keck Observatory Archive is a NASA-funded collaboration between NExScI/IPAC and the W. M. Keck Observatory. KOA’s goal is to provide a long-term archive for all observations acquired at the two 10-m telescopes of the W. M. Keck Observatory on Mauna Kea, Hawaii.

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Palomar Transient Factory

January 1, 2007

The Palomar Transient Factory (PTF) is a fully-automated, wide-field survey aimed at a systematic exploration of the optical transient sky. IPAC is responsible for the data processing and archiving for PTF.

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Planck

January 1, 2009

IPAC is the home of the US Planck Science Data Center, with IPAC engineers and scientists responsible for retrieving mission data from the Planck Data Processing Centers (in Paris, France and Trieste, Italy) and staging data for usage by Planck team members and for archival research. IPAC's responsibilities also included generating the Early Release Compact Source Catalog (ERCSC), which was the first public data product from the mission. Planck was led by the European Space Agency (ESA) with contributions from multiple EU countries and with significant NASA involvement. Planck launched on May 14, 2009 and operated for 4 years.

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Herschel

March 1, 2009

NASA was a partner in the ESA-led Herschel mission, with US participants contributing to the mission; providing mission-enabling instrument technology and sponsoring the NASA Herschel Science Center (NHSC) at IPAC. The NHSC was established to provide the US astronomical community with science and observational support throughout all phases of the Herschel mission. Herschel launched in 2009 with three instruments sensitive to radiation at far infrared and sub-millimeter wavelengths, and remained operational until 2013.

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WISE

June 1, 2009

IPAC is responsible for ingestion of raw WISE / NEOWISE data, data processing to produce the final data products, and archiving mission science and engineering data. IPAC is also responsible for the distribution of WISE data to the community, via the NASA/IPAC Infrared Science Archive (IRSA). The IPAC Communications team also supports WISE and NEOWISE public affairs and public outreach by preparing all of the WISE images for public release into the image gallery. WISE launched in 2009, and completed its primary mission in 2011. After hibernating until late 2013, it was reactivated as the NEOWISE mission to learn more about the population of near-Earth objects and comets that could pose an impact hazard to the Earth. Survey operations were completed on July 31, 2024. The spacecraft was decommissioned on August 8, 2024, and re-entered the Earth's atmosphere on November 1, 2024.

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Thirty Meter Telescope

January 1, 2011

IPAC also supported the TMT Project with a number of business and engineering services, including implementing the TMT Software Test and Integration Laboratory (TMT-STIL). The IPAC Communications and Education team also provided supported for public affairs, education and public outreach activities.

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NASA Exoplanet Archive

December 11, 2011

The NASA Exoplanet Archive, part of NExScI at IPAC, provides data and tools to support community discovery and characterization of exoplanets and their host stars.

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LCOGT

January 1, 2012

IPAC, as part of our role in the scientific collaboration of the Las Cumbres Observatory Global Telescope Network (lcogt.net), serves as the long term data archive for the network of telescopes. The data archive is being designed in concert with the deployment of the 1-m telescopes and will eventually hold data from the 2-m and 0.4-m telescopes as well.

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LSST

January 1, 2014

Since 2006, IPAC has participated in Data Management activities for LSST, and was identified as a key partner for its implementation. In 2014, the LSST Science User Interface and Tools (SUI/T) group was been established at IPAC. IPAC as a part of Caltech is an institutional member of the project, and is developing the web-based Science User Interface, providing the immediate portal for astronomers and the public to the data collected by the LSST on nightly, yearly, and survey-long bases. The data will primarily be in the form of images, from a single CCD to the entire 9 square degree focal plane, and catalogs produced by extracting source information from the images as part of LSST Data Management. The LSST project evolved to become the Vera C. Rubin Observatory.

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Euclid

March 1, 2014

In 2014, NASA established the Euclid NASA Science Center at IPAC (ENSCI) in order to support US-based investigations using Euclid data. ENSCI participates in the Euclid Consortium’s Science Ground Segment, providing algorithm and software development, participating in data quality assurance, and performing data processing. In addition, ENSCI supports the US research community by providing expert insight into the Euclid surveys, data processes, calibration, and products. Euclid was launched on a nominal six-year mission on July 1, 2023.

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WFIRST

January 1, 2015

A major focus of IPAC and STScI in support of pre-formulation was to engage the scientific community in preparing for and helping to define the science mission of WFIRST-AFTA. IPAC and STScI achieved this by organizing and sponsoring science workshops and conferences, maintaining a presence at AAS meetings, establishing a collaborative website with basic information, news, and tools, and providing support to the project in the creation of a WFIRST-AFTA science book. WFIRST subsequently evolved into the Nancy Grace Roman Space Telescope project, projected to launch in 2026.

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ZTF

November 1, 2017

The Zwicky Transient Facility (ZTF) is a time-domain survey with first light at Palomar Observatory in 2017. The Science Data Systems are housed at IPAC. These consist of the data processing pipelines, data archives, infrastructure for long-term curation, and the user services for data retrieval. IPAC also delivers a transient event stream to the science collaboration and project partners to enable rapid follow-up in near real-time.

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SPHEREx

February 13, 2019

SPHEREx is an all-sky spectroscopic survey mission conducting 4 all-sky surveys over 2 years, providing the first near-infrared all-sky spectral survey for the astronomical community with a data pipeline operated at IPAC and a data archive hosted by the NASA IPAC Infrared Science Archive (IRSA). SPHEREx is projected to launch late February 2025.

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NEOSurveyor

January 1, 2020

IPAC will be responsible for NEO Surveyor survey data processing and archiving of the final survey and engineering data products. IPAC will distribute NEO Surveyor image and extracted source data via the NASA/IPAC Infrared Science Archive, and work with the IAU Minor Planet Center and NASA Planetary Data System to release solar system object detections and physical characterizations to the science community. As of 2024, NEO Surveyor is scheduled for launch no later that 2028.

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Rubin

January 6, 2020

The Large Synoptic Survey Telescope is renamed the Vera C. Rubin Observatory. Rubin is one of the next generation of great observatories, designed to conduct a ten- year survey of the dynamic Universe. IPAC is a partner in the Rubin Observatory and is building the Science User Interface and Tools (SUIT) components for the Rubin LSST Science Platform, the environment that will enable the astrophysical community to access and work with Rubin LSST data.

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Roman

May 20, 2020

NASA renamed its next-generation space telescope, the Wide Field Infrared Survey Telescope (WFIRST), in honor of Nancy Grace Roman, NASA’s first chief astronomer, who paved the way for space telescopes focused on the broader universe. IPAC partners with Goddard Space Flight Center and the Space Telescope Science Institute to provide the Science Center functions for the Nancy Grace Roman Space Telescope. In particular, IPAC is responsible for operations for the Coronagraph Instrument (CGI), including commanding and performance monitoring, high-level data processing of the grism and prism data from the Wide Field Instrument (WFI), high-level data processing of the microlensing survey data from WFI, and community engagement for exoplanet science. Roman is schedule to launch no later than May 2027.

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ARIEL/CASE

November 12, 2020

Ariel, the Atmospheric Remote-sensing Infrared Exoplanet Large-survey, was selected as the fourth medium-class mission in ESA’s Cosmic Vision program. NASA-JPL is contributing to the ARIEL Mission with the CASE (Contribution to ARIEL Spectroscopy of Exoplanets, PI Mark Swain) which provides the optical and near-infrared (0.5 - 2 um) science capabilities and fine guidance sensors for ARIEL. IPAC is providing the processing environment and the US Data Archive for all ARIEL data. ARIEL is expected to launch in 2029.

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Lunar Trailblazer

December 2, 2020

Lunar Trailblazer targets one of the most surprising discoveries of the decade: Water on the Moon. IPAC leads the Mission Operation System effort for Lunar Trailblazer, including planning, scheduling, and sequencing of all science, instrument, and spacecraft activities for LTB during the nominal mission [or after lunar orbit injection]. The MOS will include personnel from IPAC and JPL and also students from Caltech and Pasadena City College. IPAC will also be providing facilities in support of Mission Operations for LTB. Lunar Trailblazer is scheduled to launch in 2025.

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Ultraviolet Explorer

February 13, 2024

The Ultraviolet Explorer (UVEX) is targeted to launch in 2030 as NASA’s next Astrophysics Medium-Class Explorer mission. UVEX will undertake a synoptic survey of the entire sky in the near-UV and far-UV. UVEX will study the evolution of low-metallicity, low-mass galaxies. UVEX time-domain surveys will probe the aftermaths of gravitational wave-discovered compact object mergers, discover fast UV transients, and diagnose the early stages of explosive phenomena. IPAC will provide the UVEX Science Data Center (USDC).

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IRAS

NASA Extragalactic Database

IRSA

ISO

MSX

2MASS

Spitzer Science Center

NExScI

Keck Observatory Archive

Palomar Transient Factory

Planck

Herschel

WISE

Thirty Meter Telescope

NASA Exoplanet Archive

LCOGT

LSST

Euclid

WFIRST

ZTF

SPHEREx

NEOSurveyor

Rubin

Roman

ARIEL/CASE

Lunar Trailblazer

Ultraviolet Explorer

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