View source for Near Infrared Camera and Multi-Object Spectrometer

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| caption1  = The [[gas giant]] Uranus showing cloud bands, rings, and moons of the Uranian system, taken with NICMOS in 1998

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| caption2  = [[Pistol Star]] and [[Pistol Nebula]], taken by NICMOS in 1997

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| caption3  = NICMOS's [[Hubble Ultra Deep Field]]. The instrument provided near-infrared views of the HUDF, extending the data available for that area.
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The '''Near Infrared Camera and Multi-Object Spectrometer''' ('''NICMOS''') is a [[Measuring instrument|scientific instrument]] for [[infrared astronomy]], installed on the [[Hubble Space Telescope]] (HST), operating from 1997 to 1999, and from 2002 to 2008. Images produced by NICMOS contain data from the near-infrared part of the light spectrum.

NICMOS was conceived and designed by the NICMOS Instrument Definition Team centered at [[Steward Observatory]], [[University of Arizona]], USA. NICMOS is an imager and [[Multi-Object Spectrometer|multi-object spectrometer]] built by [[Ball Aerospace & Technologies Corp.]] that allows the HST to observe [[infrared light]], with [[wavelength]]s between 0.8 and 2.4 micrometers, providing imaging and slitless spectrophotometric capabilities. NICMOS contains three near-infrared detectors in three optical channels providing high (~ 0.1 arcsecond) resolution, coronagraphic and polarimetric imaging, and slitless spectroscopy in 11-, 19-, and 52-arcsecond square fields of view.  Each optical channel contains a 256×256 pixel [[photodiode]] array of [[mercury cadmium telluride]] [[infrared detector]]s bonded to a sapphire substrate, read out in four independent 128×128 quadrants.<ref>{{cite journal|first1=Chris J. |last1=Skinner|first2= Louis E. |display-authors=4 |last2=Bergeron |first3=Alfred B. |last3=Schultz |first4=John W. |last4=MacKenty|first5= A. |last5=Storrs|first6= Wolfram |last6=Freudling|first7= D. |last7=Axon|first8= Howard A. |last8=Bushouse|first9= Daniela |last9=Calzetti|author9-link= Daniela Calzetti |first10= L. |last10=Colina|first11= D. |last11=Daou|first12= D. |last12=Gilmore|first13= Sherie T. |last13=Holfeltz|first14= Joan |last14=Najita|first15= Keith |last15=Noll|first16= Christine E. |last16=Ritchie|first17= William B. |last17=Sparks |first18=A. |last18=Suchkov|editor1-first=Albert M|editor1-last=Fowler|title=On-orbit properties of the NICMOS detectors on HST|journal=Proc. SPIE|volume= 3354|date=1998| doi=10.1117/12.317208 |pages=2–13 |url=http://www.stsci.edu/hst/nicmos/documents/papers/schultz_spie.pdf|series=Infrared Astronomical Instrumentation|bibcode=1998SPIE.3354....2S|s2cid=5778753}}</ref>

NICMOS last worked in 2008,<ref>{{cite web|title=HST Legacy Instruments|url=https://www.stsci.edu/hst/instrumentation/legacy|publisher=Space Telescope Science Institute|access-date=January 29, 2023}}</ref> and has been largely replaced by the infrared channel of [[Wide Field Camera 3]] after its installation in 2009.<ref>{{cite web|title=Hibernating instrument on Hubble roused as engineers ponder message problem|url=https://www.theregister.com/2021/11/05/hubble_nicmos/|publisher=TheRegister.com|access-date=January 29, 2023}}</ref>

==Limitations==

The infrared performance of the Hubble has limitations since it was not designed with infrared performance as an objective. For example, the mirror is kept at a stable and relatively high temperature (15&nbsp;°C) by heaters.

<blockquote>HST is a warm telescope. The IR background flux collected by cooled focal plane IR instruments like NICMOS or WFC3 is dominated, at rather short wavelengths, by telescope thermal emission rather than by zodiacal scattering. NICMOS data show that the telescope background exceeds the zodiacal background at wavelengths longer than λ ≈ 1.6μm, the exact value depending on the pointing on the sky and on the position of the Earth on its orbit.<ref>{{cite journal |title=The Performance of HST as an Infrared Telescope |last1=Robberto|first1= M.|display-authors= 4|last2= Sivaramakrishnan|first2= A.|last3= Bacinski|first3= J.J.|last4= Calzetti|first4= D.|author4-link= Daniela Calzetti |last5= Krist|first5= J.E.|last6= MacKenty|first6= J.W.|last7= Piquero|first7= J. |last8= Stiavelli|first8= M. |editor-first1=James B. |editor-first2=Peter |editor-last1=Breckinridge |editor-last2=Jakobsen |url=http://www.stsci.edu/hst/wfc3/documents/published/spie4013386.pdf |journal=Proc. SPIE |volume=4013 |pages=386–393 |date=2000 |doi=10.1117/12.394037 |series=UV, Optical, and IR Space Telescopes and Instruments|bibcode=2000SPIE.4013..386R|s2cid=14992130}}</ref></blockquote>

Despite this, the combination of Hubble's mirror and NICMOS offered never-before seen levels of quality in near-infrared performance at that time.<ref name="spaceflightnow.com">{{Cite web | url=http://www.spaceflightnow.com/news/n0206/06nicmos/ | title=Spaceflight Now &#124; Breaking News &#124; Hubble's infrared camera brought back to life}}</ref> Dedicated infrared telescopes like the [[Infrared Space Observatory]] were ground-breaking in their own way, but had a smaller primary mirror, and were also out of service at the time of NICMOS installation because they ran out of coolant. NICMOS later overcame this problem by using a machine chiller like a refrigerator, which allowed it operate for years until it went offline in 2008.

==History of NICMOS==

NICMOS was installed on Hubble during its second servicing mission in 1997 ([[STS-82]]) along with the [[Space Telescope Imaging Spectrograph]], replacing two earlier instruments.  NICMOS in turn has been largely superseded by the [[Wide Field Camera 3]], which has a much larger field of view (135 by 127 arcsec, or 2.3 by 2.1 arcminutes), and reaches almost as far into the infrared.
[[File:STS-82 crew.jpg|thumb|NICMOS was installed by the crew of STS-82, this [[Space Shuttle]] mission in 1997 also installed the STIS instrument on Hubble Space Telescope, a scale model of the telescope is shown with this crew photo]]
[[File:STS-82 Discovery on Mobile Launcher Platform.jpg|thumb|NICMOS's ride to space heads to the launchpad, January 1997]]
[[File:Hubble Redeployment - GPN-2000-001066.jpg|thumb|Hubble Space Telescope held by the Space Shuttle robotic arm]]
[[File:STS082-323-017.jpg|thumb|Shuttle crew EVA with Hubble Space Telescope]]
When conducting infrared measurements, it is necessary to keep the infrared detectors cooled to avoid having infrared interference from the instrument's own thermal emissions. NICMOS contains a cryogenic [[Dewar flask|dewar]], that cooled its detectors to about 61&nbsp;K, and optical filters to ~ 105&nbsp;K, with a block of [[solid nitrogen]] ice. When NICMOS was installed in 1997, the [[dewar flask]] contained a 230-pound (104&nbsp;kg) block of nitrogen ice. Due to a thermal short that arose on March 4, 1997, during the instrument commissioning, the dewar ran out of [[nitrogen]] coolant sooner than expected in January 1999.

During Hubble Service Mission 3B in 2002 ([[STS-109]]),<ref name="mix.msfc.nasa.gov">{{Cite web | url=https://mix.msfc.nasa.gov/abstracts.php?p=2819 | archive-url=https://web.archive.org/web/20161127021625/https://mix.msfc.nasa.gov/abstracts.php?p=2819 | url-status=dead | archive-date=2016-11-27 | title=0302432 - Repaired and Reconfigured Hubble Space Telescope Berthed in Columbia's Cargo Bay}}</ref> a replacement cooling system comprising a [[cryocooler]], cryogenic circulator, and external radiator was installed on the Hubble that now cools NICMOS through a cryogenic [[neon]] loop. The NICMOS Cooling System (NCS) was developed on a very accelerated schedule (14 months vs. 5–10 years for other Hubble instrument hardware).<ref>{{Cite web|title={{!}}{{!}}{{!}}{{!}}{{!}} The NICMOS Cooling System {{!}}{{!}}{{!}}{{!}}{{!}}|url=https://asd.gsfc.nasa.gov/archive/hubble/ncs-story/event-04.html|access-date=2020-06-10|website=asd.gsfc.nasa.gov}}</ref> NICMOS was returned to service soon after SM 3B.<ref>{{cite journal|last1=Jedrich|first1=Nicholas M.|last2=Gregory|first2=Teri|last3=Zimbelman|first3=Darrell F.|last4=Cheng|first4=Edward S.|last5=Petro|first5=Larry|last6=Cottingham|first6=Christine|last7=Buchko|first7=Matthew M.|last8=Kaylor|first8=Marc|last9=Dolan|first9=Francis X.|editor1-first=John C|editor1-last=Mather|display-authors=4|date=2003|title=Cryogenic cooling system for restoring IR science on the Hubble Space Telescope|journal=Proc. SPIE|series=IR Space Telescopes and Instruments|volume=4850|pages=1058–1069|bibcode=2003SPIE.4850.1058J|citeseerx=10.1.1.162.1601|doi=10.1117/12.461805|s2cid=108566881}}</ref><ref>{{cite book|chapter=The NICMOS Turbo-Brayton Cryocooler — Two Years in Orbit|first1=Walter L. |last1=Swift|first2= John A. |display-authors=4 |last2=McCormack|first3= Mark V. |last3=Zagarola|first4= Francis X. |last4=Dolan|first5= Herby |last5=Sixsmith|title=Cryocoolers 13|doi=10.1007/0-387-27533-9|isbn=978-0-387-23901-9|pages=633–639|publisher=Springer US|date=2005|url=https://cds.cern.ch/record/1339460 }}</ref>

A new software upload in September 2008 necessitated a brief shutdown of the NICMOS cooling system.  Several attempts to restart the cooling system were unsuccessful due to issues with the cryogenic circulator. After waiting more than six weeks for parts of the instrument to warm up, and theorized ice particles to sublimate from the neon circulating loop, the cooler once again failed to restart. An Anomaly Review Board (ARB) was then convened by NASA. The ARB concluded that ice or other solid particle migrated from the dewar to the circulator during the September 2008 restart attempt and that the circulator may be damaged, and determined an alternative set of startup parameters.  A successful restart at 13:30 EST on 16 December 2008 led to four days of cooler operations followed by another shutdown.<ref>{{cite web|url=http://www.stsci.edu/hst/nicmos/newsItems/Nicmosncs_status_01232009|title=NICMOS/NCS Status|date=January 23, 2009|publisher=[[Space Telescope Science Institute]]}}</ref> On 1 August 2009, the cooler was restarted again;<ref>{{cite web|title=Hubble Space Telescope Status Report|date=August 5, 2009|publisher=[[NASA]]|url=http://www.nasa.gov/mission_pages/hubble/servicing/SM4/news/HST_update_5Aug2009.html|access-date=August 15, 2009|archive-date=January 23, 2015|archive-url=https://web.archive.org/web/20150123134818/http://www.nasa.gov/mission_pages/hubble/servicing/SM4/news/HST_update_5Aug2009.html|url-status=dead}}</ref> NICMOS was expected to resume operations in mid-February 2010<ref>{{cite web|title=NICMOS Late Breaking News Page|date=December 16, 2009|publisher=NASA|url=http://www.stsci.edu/hst/nicmos/localNews?display_type=all#NICMOS_NCS_status_12162009|archive-url=https://archive.today/20120805163354/http://www.stsci.edu/hst/nicmos/localNews?display_type=all%23NICMOS_NCS_status_12162009|url-status=dead|archive-date=August 5, 2012}}</ref> and operated through October 22, 2009, at which point a lock-up of Hubble's data handling system caused the telescope to shut down.  The circulation flow rate to NICMOS was greatly reduced during this operating period confirming blockage in the circulation loop.  Continued operation at reduced flow rates would limit NICMOS science so plans for purging and refilling the circulation system with clean neon gas were developed by NASA.  The circulation loop is equipped with an extra neon tank and remotely operated solenoid valves for on-orbit purge-fill operations.  As of 2013, these purge-fill operations have not yet been performed.{{update after|2014}}

[[Wide Field Camera 3|WFC3]], installed 2009, was designed to partly replace NICMOS.<ref name=aas>{{cite report|title=Status of the HST Wide Field Camera 3 |first1=J.W. |last1=MacKenty |first2= R.A. |last2=Kimble|date=January 2003|publisher=American Astronomical Society poster session |url=http://www.stsci.edu/hst/wfc3/documents/published/aas_jan2003_poster1.pdf |page=1}}</ref>

On June 18, 2010, it was announced NICMOS would not be available for science during the latest proposal Cycle 18.  As of 2013, a decision as to whether the purge-fill operations will be performed and whether NICMOS will be available for science in the future has not been made.{{update after|2014}}

NICMOS is also the name of the device's 256×256-pixel imaging sensor built by Rockwell International Electro-Optical Center (now DRS Technologies).

==Scientific results==

NICMOS was noted for its performance in Near-infrared space astronomy, in particular its ability to see objects through dust.<ref name="spaceflightnow.com"/> It was used for about 23 months after it was installed, its life limited by set amount of cryo-coolant, and then later it was used for several years when a new cryo-cooler was installed in 2002.<ref name="spaceflightnow.com"/> NICMOS combined near infrared performance with a large mirror.<ref name="spaceflightnow.com"/>

NICMOS allowed investigation of high [[redshift]] galaxies and [[quasar]]s with high spatial resolution, which was especially useful when analyzed in conjunction with other instruments such as the STIS, and it also allowed deeper investigation of stellar populations.<ref>{{cite web|title=NASA Hubble Space Telescope Daily Report #4287|url=https://spaceref.com/status-report/nasa-hubble-space-telescope-daily-report-4287/|date=January 29, 2007|website=spaceref.com|access-date=January 29, 2023}}</ref> In planetary science, NICMOS was used to discover an impact basin on the south pole of the asteroid [[4 Vesta]].<ref>{{cite book|author=Edward C. Blair|title=Asteroids: Overview, Abstracts, and Bibliography|url=https://books.google.com/books?id=oa289IxCvAAC&pg=PA115|year=2002|publisher=Nova Publishers|isbn=978-1-59033-482-9|page=115}}</ref> (4 Vesta was later visited by [[Dawn (spacecraft)]] in the 2010s which investigated it more closely by orbiting it.)<ref>{{Cite web|title=4 Vesta |url=https://solarsystem.nasa.gov/asteroids-comets-and-meteors/asteroids/4-vesta/in-depth |date=December 19, 2019 |access-date=2020-09-07|website=NASA Solar System Exploration}}</ref>

In 2009, an old NICMOS image was processed to show a predicted [[exoplanet]] around the star [[HR 8799]].<ref name=exoplanets/> The system is thought to be about 130 [[light-years]] from Earth.<ref name=exoplanets/>

In 2011, around that same star, four exoplanets were rendered viewable in a NICMOS image taken in 1998, using advanced data processing.<ref name=exoplanets>[http://www.nasa.gov/mission_pages/hubble/science/elusive-planets.html NASA - Astronomers Find Elusive Planets in Decade-Old Hubble Data - 10.06.11]</ref> The exoplanets were originally discovered with the [[W. M. Keck Observatory|Keck telescopes]] and the [[Gemini North]] telescope between 2007 and 2010.<ref name=exoplanets/> The image allows the orbits of the exoplanets to be analyzed more closely, since they take many decades, even hundreds of Earth years, to orbit their host star.<ref name=exoplanets/>

NICMOS observed the exoplanet [[XO-2Nb|XO-2b]] at star [[XO-2 (star)|XO-2]], and a spectroscopy result was obtained for this exoplanet in 2012.<ref name="cds.cern.ch">{{Cite web|url=https://cds.cern.ch/record/1489206|title=Cern Authentication}}</ref> This uses the spectroscopic abilities of the instrument, and in astronomy spectroscopy during a planetary transit (an exoplanet passes in front of star from the perspective of Earth) is a way to study that exoplanet's possible atmosphere.<ref name="cds.cern.ch"/>

In 2014, researchers recovered planetary discs in old NICMOS data using new image processing techniques.<ref>{{Cite web | url=https://www.nasa.gov/press/2014/april/astronomical-forensics-uncover-planetary-disks-in-nasas-hubble-archive/ | title=Astronomical Forensics Uncover Planetary Disks in NASA's Hubble Archive| date=2014-04-24}}</ref>

==Shuttle missions==
*STS-82, (year:1997) installed, NICMOS replaces GHRS
*STS-109, (year:2002) new crycooler installed, returned to operation.<ref name="mix.msfc.nasa.gov"/>

== See also ==
*[[James Webb Space Telescope]] (dedicated near-infrared telescope)
*[[List of largest infrared telescopes]]
*[[NICMOSlook]]
*[[Herschel Space Telescope]] (deep infrared space telescope 2009–2013)
*[[Infrared Array Camera]] (Spitzer near to mid infrared camera)

==References==
{{reflist}}

== External links ==
{{commons category|Near Infrared Camera and Multi-Object Spectrometer}}
*[http://www.spacetelescope.org/about/general/instruments/nicmos.html NICMOS at ESA/Hubble]
*[http://www.spacetelescope.org/images/archive/freesearch/nicmos/viewall/1 Images taken with NICMOS at ESA/Hubble]
*[http://nicmosis.as.arizona.edu:8000/NICMOS_HOLD.html Technical information] from [[Steward Observatory]]'s instrument team
*[https://web.archive.org/web/20080926224359/http://www.teledyne-si.com/imaging/standard_products.html NICMOS sensor family]
{{Hubble Space Telescope}}

[[Category:Hubble Space Telescope instruments]]
[[Category:Space science experiments]]
[[Category:Spectrometers]]
[[Category:Infrared imaging]]