TIGRE Telescope Spectra
100
TIGRE (http://www.hs.uni-hamburg.de/DE/Ins/HRT/)
is a 1.2 m robotic telescope at Guanjuato, Mexico
(long -101.3248, lat 21.05314, height 2435 m). It is coupled to an
Echelle spectrograph (resolution about 20000) measuring in the optical
(380 through 880 nm), on a red and blue arm. The instrument's research
focus lies on long-term monitoring of cool stars and transient objects.
TIGRE SSA
2016-10-02T14:21:00
spectroscopy
m-stars
transient-sources
Schmitt, J.H.M.M; Schröder, K.P.; Rauw, G.
TIGRE/Heros
La Luz Observatory
2014AN....335..787S
Research
Archive
Optical
AllSky ICRS
//ssap#hcd
application/x-votable+xml;content=datalink
Datalink
"\schema.data"
sp_type: SPECTYPE,
vmag: VMAG,
b_v: BVCOLOUR,
vsini: VSINI
{"R": "Red", "B": "Blue"}[@CHANNEL]
@hdus[1].data["WAVE"][0]
hmsToDeg(@RA_TEL, ":")
dmsToDeg(@DEC_TEL, ":")
3/3600.
@bandpass
@REDUCED
@JD_D_OBS-0.5
parseDate(@DATEPROC)
@CR_IDENT
"TIGRE %s %s %s"%(
@OBJECT, @bandpass, mjdToDateTime(@JD_D_OBS-0.5))
len(@spectralvals)
\standardPubDID
@DER_SNR
@spectralvals[0]*1e-10
@spectralvals[-1]*1e-10
(@spectralvals[0]+@spectralvals[-1])*1e-10/2
(@spectralvals[-1]-@spectralvals[0])*1e-10
"star"
@OBJECT
@EXPTIME
from gavo.protocols import products
from gavo.utils import pyfits
fitsPath = products.RAccref.fromString(
self.sourceToken["accref"]).localpath
specs, fluxs, flux_errs = pyfits.open(fitsPath)[1].data[0]
for spec, flux, flux_err in zip(specs, fluxs, flux_errs):
yield {"spectral": spec, "flux": flux, "error_est": flux_err}
TIGRE Datalink Service
"\rdId#data"
"\rdId#build_sdm_data"
pointed
archival
MAXREC=1
auto