CRIRES-POP

 

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The CRIRES-POP team 

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Contact:
Thomas Lebzelter
University of Vienna
Department of Astronomy
Türkenschanzstrasse 17
1180 Vienna / Austria
thomas.lebzelter AT univie.ac.at

 

Data access

Please have a look at the copyright statement.
Please read the information on the data access carefully.

Raw data: link to the corresponding files in the ESO archive. Typically you can download the raw data in this way. It is also a way to get a quick overview on the obtained wavelength settings and the observing conditions.

Pipeline reduced data: tar-files. Download by right-click on the link. Note: File size can exceed 10MB! The data are in the standard CRIRES format, i.e. the fits file includes four binary tables with the data from the four detectors, respectively. If you are not familiar with this data format, you might find some help here .
In cases, where the observation of a setting had to be repeated as the first attempt failed the quality criteria, both observations are included in the tar-files. Please use the later one.

Disclaimer: Pipeline reduced data are the direct output of the ESO CRIRES pipeline with no special treatment of the data. These data DO NOT represent the quality of the final library spectra in terms of wavelength calibration and S/N ratio and are not corrected for telluric lines.

Final reduction: Here we will make our final data product available for download. It will be in ASCII format. A special mark will indicate when a complete wavelength band is available. Our aim is to provide high quality data, thus please understand that the data reduction takes some time. For the moment we publish a first small test set of finally reduced data from Lebzelter et al. (2012). Please download them via this link (information on the file structure is available here ).

UVES-POP data: where available we give a link to a plot of the corresponding data from the UVES-POP archive.

CRIRES-POP data

Star

Raw data /
ESO archive

Pipeline
reduced data

Final
reduction

UVES-POP
data

Remark

HD 149438 (B0.2V)

YJ  H  K  L  M

YJ H K L M

-

HD 47105 (A0 IV)

YJ  H  K  L  M

YJ H K L M

-

HD 118022 (A1p)

YJ  H  K  L  

YJ  H  K L

plot

HD 73634 (A6 II)

YJ  H  K  L  M

YJ H K L M

 

plot

 

HD 80404 (A8 Ib)

YJ  H  K  L  M

YJ H
HD 74180 (F3 I)

YJ  H  K  L  M

YJ H K L

HD 20010 (F8 IV)

YJ  H  K  L  M

YJ H K L M

 

plot

 

HD 109379 (G5 II)

YJ  H  K  L  M

YJ H K L M

 

plot

 

HD 99648 (G8 I)

YJ  H  K  L   M

to be added plot

HD 83240 (K1 III)

YJ  H  K  L  M

YJ H K L M

 

plot

 

HD 138716 (K1 V)

YJ  H  K  L  M

to be added

HD 225212 (K3 I)

YJ  H  K  L  M

YJ H K L M

 

plot

 

HD 209100 (K5 V)

YJ  H  K  L  M

HD 49331 (M1 I)

YJ  H  K  L  M

YJ H K L M 

 

plot

 

HD 224935 (M3 III)

YJ  H  K  L  M

YJ  K L M

plot

Barnard's star (M4V)

YJ  H  K  L  M

YJ H K L M 

 

-

 

HD 73739 (M7II/III)

YJ  H  K  L  M

HD 30959 (MS III)

YJ  H  K  L  M

YJ H K L M

 

 

HD 61913 (S)

YJ  H  K  L  M

YJ H K L M

 

-

 

HD 134453 (C5)

YJ  H  K  L  M

YJ H K L M

 

plot

 

 

 

 

 

 

 

 

Missing data will be added soon. Please excuse the delay.

last modification: May 2 2013

please report any problems to thomas.lebzelter*AT*univie.ac.at

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

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