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Available Data Sets
Extreme UV: Far UV: Near UV: Optical: Near Infrared: Radio:
- EUVE
- (images in the 70 - 760 Å range,
3.5 sq. degrees field of view and 4.3"/pixel resolution,
~ 400 targets, mostly Galactic, 6/1992 - 1/2001.)
- ACS
- (CCD images between 3,700 - 11,000 Å, 11.3 sq.
arcmin field of view and 0.05"/pixel resolution [WFC] and
between 2,000 - 11,000 Å, 0.2 sq. arcmin field of view
and 0.0027"/pixel resolution [HRC]; photon-counting detector
images between 1,150 - 1,700 Å, 0.3 sq. arcmin field of
view and 0.032"/pixel resolution [SBC/MAMA], 3/2002 - present)
- WF/PC
- (CCD images between 1,150 - 11,000 Å, 6.6 sq.
arcmin field of view and 0.102"/pixel resolution (WF),
and 1.2 sq. arcmin field of view and 0.043"/pixel
resolution (PC), 4/1990 - 11/1993.)
- WF/PC2
- ( CCD images between 1,150 - 11,000 Å, 5.0 sq.
arcmin field of view, 0.100"/pixel (WF) and 0.046"/pixel
(PC) resolution, 12/1993 - 5/2009.)
- FOC
- (photon-counting device images between 1,150 - 6,500
Å, 0.22 sq. arcmin field of view, 0.014/0.028"/pixel
resolution, 10/1990 - 3/1999.)
- SWIFTUVOT
- (intensified CCD images between 1,700 - 6,000 Å,
17 sq. arcmin field of view, and 0.5 "/pixel resolution,
brightness limit v=7.4 mag, 12/2004 - present)
- UIT
- (digitized film images between 1,200-3,300 Å,
40 arcmin field of view and 3" resolution, 259 targets total,
2 shuttle missions (12/90 & 3/95).)
- STIS/MAMAs
- (Multi-Anode Microchannel Array images between
1,150 - 3,100 Å, 0.17 sq. arcmin field of view,
0.024"/pixel resolution, 2/1997 - present.)
- GALEX
- (microchannel plate detector images between
1,350 - 2,800 Å, 1.2 sq. degree
field of view and 5"/pixel resolution,
4/2003 - 2013.)
- COS/NUV
- (MAMA images 1750-3200 Å, 2.5 arcsec diameter FOV, with decreasing
amounts of light from objects up to 2 arcsec from aperture center,
resolution ~0.05 arcsec.)
- FIRST
- (radio maps at 21 cm (1.4 GHz), 5" resolution, 1 mJy
flux limit, source catalog also available; will cover 10,000
square degrees when completed (Spring 1993 - 2011).)
- WFC3/UVIS
- (CCD images between 2,000 - 10,000 Å, 162 x 162 arcsec
field of view (rhomboidal), 0.04 arcsec/pixel, pixel size
is 15 µ, 5/2009 - ?.)
- XMM-OM
- (MIC detector (microchannel plate/CCD) images between
1,700 - 5,500 Å, 24 arcmin field of view and
1"/pixel resolution, B-mag range ~24 to 8.6,
2/2000 - present.)
- EPOCH/MRI
- (broad-band filter centered at 7500 Å,
CCD frame of 1024x1024 pixels, plate scale =
2"/pixel. Earth observations made 2008: March 18-19, May 28-29,
and June 4-5. Spatial resolution is 3.6-4")
- EPOCH/HRIV
- (Earth observations obtained 2008: March 18-19, May 28-29, and June 4-5
using seven 100 Å wide filters
centered at 3500, 4500, 5500, 6500, 7500, 8500, 9500 Å.
512x512 pixel CCD frame; plate scale = 0.4"/pixels.
Stellar-transit observations were also made
of 8 stars during many epochs during 2008 in a 128x128
pixel subarray. Spatial resolution is ~7")
- WFC3/IR
- (1kx1k Teledyne HdCdTe FPA, 9,000 - 17,000 Å range (900
- 1700 nm), 123x136 arcsecond field of view (rectangluar), 0.13
arcsec/pixel, pixel size 18 µ, 5/2009 - ?.)
- NICMOS
- (infrared array images between 8,000 - 25,000 Å,
3 cameras for a total of 0.86 sq. arcmin field of view,
resolution ranging from 0.043 to 0.2"/pixel, 2/1997 - 9/2009.)
- DSS
- (digitized sky plates (optical band), 1.7" or 1.0"
resolution, original plates covering 6.5 x 6.5 degrees,
1950 - present.)
- STIS/CCD
- (CCD images between 2,500 - 11,000 Å, 0.7 sq.
arcmin field of view, 0.05"/pixel resolution, 2/1997 - present.)
Extreme UV: Far UV: Near UV: Optical: Near Infrared:
- EUVE
- (spectra in the 70 - 760 Å range, resolution
~ 300, V_max ~ 15, ~ 400 targets, mostly Galactic,
6/1992 - 1/2001.)
- FUSE
- (spectra in the 905 - 1,187 Å range, resolution
~30,000, ~3,000 targets observed, 8/1999 - 9/2007.)
- IMAPS1
- (spectra in the 950 - 1,150 Å range, resolution
~ 120,000, V_max ~ 4, 10 bright stars observed,
9/93.)
- BEFS
- (spectra in the 400 - 900 (few) & 900 - 1200 Å
range, resolution ~ 3,000, V_max ~ 15, ~175 targets observed,
2 missions, (9/93 & 11/96 - 12/96).)
- TUES
- (spectra in the 900 - 1,400 Å range, resolution
~ 10,000, V_max ~ 13, 65 targets observed, 11/96 - 12/96.)
- COS/FUV
- (spectra in 1,150-2,050 Å range, resolution ranging from
2,500 - 24,000, detector is a cross delay line (XDL), 5/2009 - present.)
- COS/NUV
- (spectra in 1,750-3,200 Å range, resolution ranging from
1,700 - 24,000, detector is a MAMA, 5/2009 - present.)
- IUE
- (spectra in the 1,200 - 3,350 Å range,
resolutions ~ 300 and 15,000, V_max ~ 15 and 10 respectively,
~ 10,000 individual targets, 2/1978 - 9/1996.)
- Copernicus
- (spectra in the 912 - 3,275 Å range, resolutions
~ 300 and 20,000, V_max ~ 7, 551 targets, mostly bright
stars, 8/1972 - 2/1981.)
- HUT
- (spectra in the 912 - 1,850 Å range, resolution
~ 500, V_max ~ 16, ~ 300 targets, 2 shuttle missions (12/90
& 3/95).)
- WUPPE
- (spectra in the 1,400 - 3,200 Å range, resolution
~ 140, V_max ~ 15, ~ 200 targets, 2 shuttle missions (12/90
& 3/95).)
- GHRS
- ( spectra in the 1,100 - 3,300 Å range, resolution
~ 2,000, 25,000, and 80,000 (echelle), V_max ~ 18, 16, and
12 respectively, 4/1990 - 2/1997.)
- STIS/MAMAs
- (spectra in 1,150 - 3,100 Å range, resolution
ranging from ~ 600 to 25,000/110,000 (echelle), V_max ~ 21
to 13/17 respectively, 2/1997 - present.)
- HPOL
- (spectra in the 3,200 - 7,500 Å range, resolution
~ 80, V_max ~ 12, ~ 514 targets (2/1989-10/2004).)
- SWIFTUVOT
- (2 intensified CCD grisms: UV 1,700-2,900 Å at R ~ 150,
and V 2,800-5,000 Å at R ~50,
brightness limit v=7.4 mag, 12/2004 - present)
- STIS/CCD
- (spectra in 1,150 - 11,000 Å range, resolution
ranging from ~ 600 to 6,000, V_max ~ 21, 2/1997 - present.)
- FOS
- (spectra in the 1,150 - 8,500 Å range, resolution
~ 250 and 1,300, V_max ~ 20, 4/1990 - 2/1997.)
- ACS
- (objective prism [SBC, HRC] and grism [WFC, HRC] spectra
in the 1,150 - 1,700 [SBC], 2,000 - 4,000 [HRC] and
5,500 - 11,000 Å [WFC and HRC] ranges, resolution ~ 100,
4/2002 - present)
- NICMOS
- (grism spectra in the 8,000 - 25,000 Å range,
resolution ~ 200, 2/1997 - 9/2009.)
- EPOCH/HRII
- (two-dimensional spectra of earth, 512 (wavelength) x 128 (spatial),
plate scale 2"/pixel, spectral coverage 10,000 - 48,000 Å,
Resolving power 700-200 respectively)
- WFC3/IR
- ("Blue" grism spectra 8,000-11,500 Å resolution ~210,
"red" grism spectra 11,000-17,000 Å, resoluton ~130.)
Far UV: Near UV: Optical: Near Infrared:
- WUPPE
- (spectropolarimetric data in the 1,400 - 3,200 Å
range, ~ 200 targets, 2 shuttle missions (12/90 & 3/95).)
- KEPLER
(Light curves, 4,300 - 8,900 Å, 42 CCD
detectors, 116 square degree FOV, ~3.98 arcsec/pixel, ~170,000 targets
with average 32 pixels/target, most data points are
30 minute integrations, some data available at 1 minute, saturation
may occur for targets brighter than 11.5 V, 5/2009 - 5/2013.)
- K2
(Light curves, 4,300 - 8,900 Å, 38 CCD
detectors, 105 square degree FOV, ~3.98 arcsec/pixel, repurposed use
of Kepler spacecraft with ~20,000 targets with average 140
pixels/target, new field every ~83 days, most data points are 30
minute integrations, some data available at 1 minute, saturation
may occur for targets brighter than 11.5 V, 5/2014 - present.)
- FGS
- (astrometric data in the 4,000 - 7,000 Å range,
5/1990 - present.)
- FOS
- ( spectropolarimetric data in the 1,150 - 8,500 Å
range, 4/1990 - 2/1997.)
- FOC
- (polarimetric data in the 1,150 - 6,500 Å range,
10/1990 - 3/1999.)
- WF/PC
- (polarimetric data between 1,150 - 11,000 Å,
4/1990 - 11/1993.)
- WF/PC2
- (polarimetric data between 1,150 - 11,000 Å,
12/1993 - 5/2009.)
- ACS
- (polarimetric data between 2,000 - 11,000 Å
coronographic data between 2,000 - 11,000 Å [HRC],
4/2002 - present)
- HSP
- (photometric and polarimetric data in the 1,200 - 7,500
Å range, 1990 - 1993.)
- HPOL
- (spectropolarimetric data in the 3,200 - 7,500 Å
range, ~ 514 targets (2/1989-10/2004).)
- EPOCH/O
- (Stellar transit light curves of
8 stars taken during 2008 using the High Resolution Visible-Infrared
imager. 50 second exposures, variable time between exposures,
Roughly 7,700 to 43,300 data points per light curve)
- NICMOS
- (polarimetric data in the 8,000 - 21,000 Å range,
1997 - Oct 2009.)
For a more extensive listing of high-energy astrophysics
data, please visit the
HEASARC homepage.
For a more extensive listing of IR astrophysics data, please
visit the IRSA homepage.
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