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aXeSIM web application aXeSIM

Spectral Templates

The available spectral templates are split into two groups, one for stellar templates and one for non-stellar templates. All templates are listed with their name from the pull-down menu in the web application. Users who prepare and upload their own object lists can refer to a template by putting the number given as SPECTEMP entry in the column SPECTEMP of the object list. All templates are illustrated with a figure and offered for download (in ASCII format).

Stellar Templates

The stellar templates were all taken from the 1993 Kurucz stellar atmosphere atlas, which is available at the Calibration Database System (CDBS) at the STScI (see [1]). Only spectra with solar metallicity were used. We followed the suggestions in [1] to identify the closest Kurucz model for the various spectral types and luminosity classes.

O5V 4500 5.0 (1)

temperature: 45000 K
log(g): 5.0
metallicity: solar
λmin:9.09e-03 μm
λmax:1.60e+02 μm
SPECTEMP entry: 1
file: O5V_45000_g50.dat
O5V

O6V 40000 4.5 (2)

temperature: 40000 K
log(g): 4.5
metallicity: solar
λmin:9.09e-03 μm
λmax:1.60e+02 μm
SPECTEMP entry: 2
file: O6V_40000_g45.dat
O6V

O8V 35000 4.0 (3)

temperature: 35000 K
log(g): 4.0
metallicity: solar
λmin:9.09e-03 μm
λmax:1.60e+02 μm
SPECTEMP entry: 3
file: O8V_35000_g40.dat
O8V

B0V 30000 4.0 (4)

temperature: 30000 K
log(g): 4.0
metallicity: solar
λmin:9.09e-03 μm
λmax:1.60e+02 μm
SPECTEMP entry: 4
file: B0V_30000_g40.dat
B0V

B3V 19000 4.0 (5)

temperature: 19000 K
log(g): 4.0
metallicity: solar
λmin:2.3e-02 μm
λmax:1.60e+02 μm
SPECTEMP entry: 5
file: B3V_19000_g40.dat
B3V

B5V 15000 4.0 (6)

temperature: 15000 K
log(g): 4.0
metallicity: solar
λmin:2.3e-02 μm
λmax:1.60e+02 μm
SPECTEMP entry: 6
file: B5V_15000_g40.dat
B5V

B8V 12000 4.0 (7)

temperature: 12000 K
log(g): 4.0
metallicity: solar
λmin:5.06e-02 μm
λmax:1.60e+02 μm
SPECTEMP entry: 7
file: B8V_12000_g40.dat
B8V

A0V 9500 4.0 (8)

temperature: 9500 K
log(g): 4.0
metallicity: solar
λmin:5.06e-02 μm
λmax:1.60e+02 μm
SPECTEMP entry: 8
file: A0V_9500_g40.dat
A0V

A5V 8250 4.5 (9)

temperature: 8250 K
log(g): 4.5
metallicity: solar
λmin:5.06e-02 μm
λmax:1.60e+02 μm
SPECTEMP entry: 9
file: A5V_8250_g45.dat
A0V

F0V 7250 4.5 (10)

temperature: 7250 K
log(g): 4.5
metallicity: solar
λmin:5.06e-02 μm
λmax:1.60e+02 μm
SPECTEMP entry: 10
file: F0V_7250_g45.dat
F0V

F5V 6500 4.5 (11)

temperature: 6500 K
log(g): 4.5
metallicity: solar
λmin:9.25e-02 μm
λmax:1.60e+02 μm
SPECTEMP entry: 11
file: F5V_6500_g45.dat
F5V

G0V 6000 4.5 (12)

temperature: 6000 K
log(g): 4.5
metallicity: solar
λmin:9.25e-02 μm
λmax:1.60e+02 μm
SPECTEMP entry: 12
file: G0V_6000_g45.dat
G0V

G5V 5750 4.5 (13)

temperature: 5750 K
log(g): 4.5
metallicity: solar
λmin:9.25e-02 μm
λmax:1.60e+02 μm
SPECTEMP entry: 13
file: G5V_5750_g45.dat
G5V

K0V 5250 4.5 (14)

temperature: 5250 K
log(g): 4.5
metallicity: solar
λmin:9.25e-02 μm
λmax:1.60e+02 μm
SPECTEMP entry: 14
file: K0V_5250_g45.dat
K0V

K5V 4250 4.5 (15)

temperature: 4250 K
log(g): 4.5
metallicity: solar
λmin:9.25e-02 μm
λmax:1.60e+02 μm
SPECTEMP entry: 15
file: K5V_4250_g45.dat
K5V

M0V 3750 4.5 (16)

temperature: 3750 K
log(g): 4.5
metallicity: solar
λmin:9.25e-02 μm
λmax:1.60e+02 μm
SPECTEMP entry: 16
file: M0V_3750_g45.dat
M0V

M2V 3500 4.5 (17)

temperature: 3500 K
log(g): 4.5
metallicity: solar
λmin:9.25e-02 μm
λmax:1.60e+02 μm
SPECTEMP entry: 17
file: M2V_3500_g45.dat
M2V

M5V 3500 5.0 (18)

temperature: 3500 K
log(g): 5.0
metallicity: solar
λmin:9.25e-02 μm
λmax:1.60e+02 μm
SPECTEMP entry: 18
file: M5V_3500_g50.dat
M5V

B0III 29000 3.5 (19)

temperature: 29000 K
log(g): 3.5
metallicity: solar
λmin:2.3e-02 μm
λmax:1.60e+02 μm
SPECTEMP entry: 19
file: B0III_29000_g35.dat
B0III

B5III 15000 3.5 (20)

temperature: 15000 K
log(g): 3.5
metallicity: solar
λmin:2.3e-02 μm
λmax:1.60e+02 μm
SPECTEMP entry: 20
file: B5III_15000_g35.dat
B5III

G0III 5750 3.0 (21)

temperature: 5750 K
log(g): 3.0
metallicity: solar
λmin:9.25e-02 μm
λmax:1.60e+02 μm
SPECTEMP entry: 21
file: G0III_5750_g30.dat
G0III

G5III 5250 2.5 (22)

temperature: 5250 K
log(g): 2.5
metallicity: solar
λmin:9.25e-02 μm
λmax:1.60e+02 μm
SPECTEMP entry: 22
file: G5III_5250_g25.dat
G5III

K0III 4750 2.0 (23)

temperature: 4750 K
log(g): 2.0
metallicity: solar
λmin:9.25e-02 μm
λmax:1.60e+02 μm
SPECTEMP entry: 23
file: K0III_4750_g20.dat
K0III

K5III 4000 1.5 (24)

temperature: 4000 K
log(g): 1.5
metallicity: solar
λmin:9.25e-02 μm
λmax:1.60e+02 μm
SPECTEMP entry: 24
file: K5III_4000_g15.dat
K5III

M0III 3750 1.5 (25)

temperature: 3750 K
log(g): 1.5
metallicity: solar
λmin:9.25e-02 μm
λmax:1.60e+02 μm
SPECTEMP entry: 25
file: M0III_3750_g15.dat
M0III

Non-Stellar Templates

With the exception of the QSO, all non-stellar templates are based on the Kinney et al. (1996) spectra ([3]). However different methods were used to extend the templates into the IR, and a reference or explanation is given for each spectrum.

E (26)

template elliptical galaxy
λmin:1.2350e-01 μm
λmax:2.3692e+00 μm
SPECTEMP entry: 26
file: ell_template.dat
reference: [2]
E

S0 (27)

template S0 galaxy
λmin:1.2350e-01 μm
λmax:2.3692e+00 μm
SPECTEMP entry: 27
file: s0_template.dat
reference: [2]
S0

Sa (28)

template Sa galaxy
λmin:1.2350e-01 μm
λmax:2.3692e+00 μm
SPECTEMP entry: 28
file: sa_template.dat
reference: [2]
Sa

Sb (29)

template Sb galaxy
λmin:1.2350e-01 μm
λmax:2.3692e+00 μm
SPECTEMP entry: 29
file: sb_template.dat
reference: [2]
Sa

Sc (30)

template Sc galaxy
λmin:1.2350e-01 μm
λmax:2.3692e+00 μm
SPECTEMP entry: 30
file: sc_template.dat
reference: [2]
Sa

Starburst (31)

template Starburst galaxy
λmin:1.2350e-01 μm
λmax:2.993422e+00 μm
SPECTEMP entry: 31
file: starb4_template_ext.dat
reference: starburst template #4 of [3] with fν~pow(ν,-1/3) extension in the IR
Sa

QSO (32)

template QSO
λmin:8.0e-02 μm
λmax:6.0e-01 μm
SPECTEMP entry: 32
file: qso_template.dat
reference: [4]
Sa

References

[1] Kurucz 93 spectra at CDBS
[2] Mannucci F., Basile F., Poggianti B. M., et al. 2001, MNRAS 326..745
[3] Kinney A.L., Calzetti D., Bohlin R.C., et al. 1996, ApJ 467, 38
[4] Francis P.J., Hewett P.C., Foltz C.B., et al. 1991, ApJ 373, 465

 

Maintained by Martin Kümmel <mkuemmel@eso.org>