Domaines |
Bandes |
Lambda (μm) |
Exemples d'instruments (satellites/téléscopes) |
Exemples de missions (Surveys) |
Gamma |
|
~0.0001 (< 0.1nm) |
BATSE, EGRET, Fermi |
BATSE Gamma-Ray Burst Research (CGRO mission), Swift GRB Explorer |
X-ray |
|
~0.01 |
Chandra, XMM-Newton, ROSAT |
INTEGRAL, 1RXS, 1XMM, Swift/XRT |
Far UV |
|
~0.150 |
GALEX (FUV~1539AA), UIT, FUSE |
FUSE mission |
Near UV |
|
~0.220 |
GALEX (NUV~2316AA), UIT, HUT |
First Byurakan Survey (FBS) |
Opt |
u |
~0.355 |
Swift/UVOT (UV + Opt), Keck (0.3-1), Subaru (0.3-1), HST (0.4-0.8), CFHT (Opt + IR) |
SDSS (ugriz) |
Opt |
B, g, bv |
0.39-0.54 |
Swift/UVOT (UV + Opt), Keck (0.3-1), Subaru (0.3-1), HST (0.4-0.8), CFHT (Opt + IR) |
SDSS (ugriz) |
Opt |
V, y |
0.55-0.60 |
Swift/UVOT (UV + Opt), Keck (0.3-1), Subaru (0.3-1), HST (0.4-0.8), CFHT (Opt + IR) |
SDSS (ugriz) |
Opt |
R, r |
0.61-0.74 (dont Halpha:0.65) |
Swift/UVOT (UV + Opt), Keck (0.3-1), Subaru (0.3-1), HST (0.4-0.8), CFHT (Opt + IR) |
SDSS (ugriz) |
Opt |
i |
0.74-0.79 |
Swift/UVOT (UV + Opt), Keck (0.3-1), Subaru (0.3-1), HST (0.4-0.8), CFHT (Opt + IR) |
SDSS (ugriz) |
Opt |
I, z |
0.80-0.90 |
Swift/UVOT (UV + Opt), Keck (0.3-1), Subaru (0.3-1), HST (0.4-0.8), CFHT (Opt + IR) |
SDSS (ugriz) |
IR proche |
J |
1-1.4 |
MMT, Akari (1.7-180) |
2MASS/2MASX (JHK), SSTc2d, GLIMPSE, SWIRE (Spitzer), MSX6C (4.22-25.1) |
IR proche |
H |
1.4-1.8 |
MMT, Akari (1.7-180) |
2MASS/2MASX (JHK), SSTc2d, GLIMPSE, SWIRE (Spitzer), MSX6C (4.22-25.1) |
IR proche |
K |
2-2.25 |
MMT, Akari (1.7-180) |
2MASS/2MASX (JHK), SSTc2d, GLIMPSE, SWIRE (Spitzer), MSX6C (4.22-25.1) |
IR proche |
|
3-5 |
Spitzer/IRAC (3-8) |
|
IR moyen |
|
~30 |
Keck (5-27), Subaru (8-25), IRAS (12-100), Spiter/MIPS (24-160) |
|
IR lointain |
|
~200-300 |
Herschel (60-500),Spiter/MIPS (24-160) |
|
mm/smm* |
|
~350-1000 |
Submillimeter telescope (SEST), ALMA (Atacama Large Millimeter/submillimeter Array), Planck (350-10000) |
BLAST (Balloon-borne Large-Aperture Submillimeter Telescope 250, 350 & 500) survey |
Rad |
|
>10000 (21cm=1.4GHz) |
Planck (350-10000), VLA (1-50GHz), COBE/DMR (3,7mm=81GHz, 5,7mm=52GHz, 9,6mm=31GHz) |
COBE mission (Cosmic Background Explorer) |
*Comme dans SIMBAD on n'a pas la longueur d'onde smm, on doit choisir entre FIR et mm. Exemple 2009ApJ...707.1836O (sources BLAST 250μm , 350μm , 500μm) longueur d'onde pour SIMBAD FIR car 250μm et 350μm loin du millimètre (Mi B, vu avec Laurent).