UVES SV Data Products

UVES SV Data Products

The data being released consist of the raw andcalibration data along with fits files of reducedspectra obtained following procedures which are fully described foreach set of spectra. It is emphasized that extraction and reductionof such spectra followed generic prescriptions.  Therefore, the reducedspectra released here are intended uniquely to allow users a quick-lookevaluation of the science quality of the data, thus helping the planningfor their most effective scientific exploitation. Of course, userswho intend to make use of the data are expected to extract and reduce thespectra again, optimizing the procedures for their own specific scientificgoals.

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A Spectroscopic Surveyof Intermediate Redshift QSOs

 3 QSOs were observed with a slit of 0.8" (red) and 0.9" (blue) when the seeing was good, and 1" when the seingwas mediocre
(R=50000-43000). A combination of the two Dichroic settings Dic 1(B346nm+ B580nm) and Dic2 (B347nm + R860nm) provided
the whole spectral range 300nm-1000nm. Depending on the seeing conditions,the binning of the CCD was 2x2 or 2x1, and exposure
times were between 1h and 1h30.

Q1101-264 click on the link to request thedataset
filename                        Setting Exp.  bin slit(") seeing(")

UVES.2000-02-10T05:13:49.852.fits Dic1 346 3600. 2x21.0 0.93
UVES.2000-02-11T05:13:14.983.fits Dic1 346 3600.1x2 0.9 0.82
UVES.2000-02-11T06:34:17.467.fits Dic1 346 3600.1x2 0.9 0.59
UVES.2000-02-12T04:57:10.937.fits Dic1 346 3600.2x2 1.0 1.00
UVES.2000-02-12T06:24:27.534.fits Dic1 346 3600.1x2 0.9 0.52
UVES.2000-02-12T07:26:17.105.fits Dic1 346 5400.1x2 0.9 0.52

UVES.2000-02-10T04:10:03.222.fits Dic2 437 3600. 2x21.0 1.53
UVES.2000-02-11T04:08:36.169.fits Dic2 437 3600.1x2 0.8 1.12
UVES.2000-02-12T03:51:57.126.fits Dic2 437 3600.1x2 0.8 0.84
UVES.2000-02-13T02:49:57.416.fits Dic2 437 3600.1x2 0.8 0.71
UVES.2000-02-16T03:30:15.124.fits Dic2 437 3600.1x2 0.8 0.88
UVES.2000-02-16T04:30:52.409.fits Dic2 437 3600.1x2 0.8 0.59

UVES.2000-02-10T05:14:53.509.fits Dic1 580 3600. 2x21.0 0.93
UVES.2000-02-11T05:14:27.743.fits Dic1 580 3600.1x2 0.9 0.82
UVES.2000-02-11T06:35:29.834.fits Dic1 580 3600.1x2 0.9 0.59
UVES.2000-02-12T04:58:25.895.fits Dic1 580 3600.2x2 1.0 1.00
UVES.2000-02-12T06:25:46.771.fits Dic1 580 3600.1x2 0.8 0.52
UVES.2000-02-12T07:27:26.643.fits Dic1 580 5400.1x2 0.8 0.52

UVES.2000-02-10T04:11:12.455.fits Dic2 860 3600. 2x21.0 1.53
UVES.2000-02-11T04:09:47.023.fits Dic2 860 3600.1x2 0.8 1.12
UVES.2000-02-12T03:53:11.025.fits Dic2 860 3600.1x2 0.8 0.84
UVES.2000-02-13T02:51:14.927.fits Dic2 860 3600.1x2 0.8 0.71
UVES.2000-02-16T03:31:37.405.fits Dic2 860 3600.1x2 0.8 0.88
UVES.2000-02-16T04:32:14.878.fits Dic2 860 3600.1x2 0.8 0.59
 

HE1122-1648 click on the link to request thedataset
filename                        Setting Exp.  bin slit(") seeing(")

UVES.2000-02-10T06:20:55.677.fits Dic1 346 3600. 1x20.9 0.67
UVES.2000-02-13T04:57:07.007.fits Dic1 346 3600.1x2 0.9 0.50
UVES.2000-02-14T04:56:59.908.fits Dic1 346 3600.1x2 0.9 0.52
UVES.2000-02-14T06:49:33.573.fits Dic1 346 4200.1x2 0.9 0.56
UVES.2000-02-14T08:01:13.471.fits Dic1 346 4200.1x2 0.9 0.44
UVES.2000-02-15T04:25:47.600.fits Dic1 346 3600.1x2 0.9 0.97
UVES.2000-02-15T05:26:31.127.fits Dic1 346 3600.1x2 0.9 0.76

UVES.2000-02-13T03:53:56.622.fits Dic2 437 3600. 1x20.8 0.64
UVES.2000-02-14T03:53:42.376.fits Dic2 437 3600.1x2 0.8 0.69
UVES.2000-02-15T03:23:05.598.fits Dic2 437 3600.1x2 0.8 0.87
UVES.2000-02-16T07:11:24.267.fits Dic2 437 3600.1x2 0.8 0.66
UVES.2000-02-16T08:12:02.650.fits Dic2 437 3600.1x2 0.8 0.75
UVES.2000-02-17T03:54:55.465.fits Dic2 437 3600.2x2 1.0 1.43
UVES.2000-02-18T03:16:35.915.fits Dic2 437 5400.2x2 1.0 1.28

UVES.2000-02-10T06:22:00.370.fits Dic1 580 3600. 1x20.8 0.67
UVES.2000-02-13T04:58:24.777.fits Dic1 580 3600.1x2 0.8 0.50
UVES.2000-02-14T04:58:20.476.fits Dic1 580 3600.1x2 0.8 0.52
UVES.2000-02-14T06:50:57.749.fits Dic1 580 4200.1x2 0.8 0.56
UVES.2000-02-14T08:02:42.285.fits Dic1 580 4200.1x2 0.8 0.44
UVES.2000-02-15T04:27:14.528.fits Dic1 580 3600.1x2 0.8 0.97
UVES.2000-02-15T05:28:05.425.fits Dic1 580 3600.1x2 0.8 0.76

UVES.2000-02-13T03:55:17.198.fits Dic2 860 3600. 1x20.8 0.64
UVES.2000-02-14T03:55:02.836.fits Dic2 860 3600.1x2 0.8 0.69
UVES.2000-02-15T03:24:28.708.fits Dic2 860 3600.1x2 0.8 0.87
UVES.2000-02-16T07:12:50.655.fits Dic2 860 3600.1x2 0.8 0.66
UVES.2000-02-16T08:13:35.471.fits Dic2 860 3600.1x2 0.8 0.75
UVES.2000-02-17T03:56:24.627.fits Dic2 860 3600.1x2 1.0 1.43
UVES.2000-02-18T03:18:02.327.fits Dic2 860 5400.2x2 1.0 1.28

HE1347-2457 click on the link to request thedataset
filename                        Setting Exp.  bin slit(") seeing(")

UVES.2000-02-17T05:05:00.532.fits Dic2 437 3600. 2x21.0 1.24
UVES.2000-02-17T06:05:51.252.fits Dic2 437 3600.2x2 1.0 0.81
UVES.2000-02-18T04:52:12.626.fits Dic2 437 5400.2x2 1.0 0.91
UVES.2000-02-18T06:23:59.559.fits Dic2 437 5400.2x2 1.0 1.35

UVES.2000-02-17T05:06:28.274.fits Dic2 860 3600. 2x21.0 1.24
UVES.2000-02-17T06:07:35.059.fits Dic2 860 3600.2x2 1.0 0.81
UVES.2000-02-18T04:53:46.652.fits Dic2 860 5400.2x2 1.0 0.91
UVES.2000-02-18T06:25:28.128.fits Dic2 860 5400.2x2 1.0 1.35

Abundance Ratiosof Extremely Metal Poor stars

2 stars from the Hamburg-ESO wereobserved in Dicroic mode (Dic2 B470nm + R785nm)  with slit of 1" corresponding to R=45000, and giving a spectral coverage: 409nm-531nm + 594nm-975nm.

Archive filename                 Setting        Exp.time Slit(")

HE1353-2735 click on the link to request thedataset

UVES.2000-02-10T07:26:49.474.fits DICHR#2 BLUE4705400 1.0
UVES.2000-02-11T07:41:00.060.fits DICHR#2 BLUE4705400 1.0

UVES.2000-02-10T07:27:59.286.fits DICHR#2 RED785 5400 1.0
UVES.2000-02-11T07:42:12.716.fits DICHR#2 RED785 5400 1.0

 
HE1303-2708 click on the link to request thedataset

UVES.2000-02-16T05:36:53.186.fits DICHR#2 BLUE4705400. 1.0
UVES.2000-02-17T08:37:07.272.fits DICHR#2 BLUE4702700. 1.0
UVES.2000-02-18T08:03:05.200.fits DICHR#2 BLUE4705400. 1.0

UVES.2000-02-16T05:38:19.547.fits DICHR#2 RED785 5400. 1.0
UVES.2000-02-17T07:12:06.468.fits DICHR#2 RED785 4000. 1.0
UVES.2000-02-17T08:38:35.008.fits DICHR#2 RED785 2700. 1.0
UVES.2000-02-18T08:04:34.059.fits DICHR#2 RED785 5400. 1.0
 

The observations for G64-12(template spectrum) were done with a 0.8"slit (R=60000) and 2 Dicroic modes (Dic1 B346nm + R580nm and Dic1 B346+ R860nm) giving a total coverage : 300nm-390nm +480nm-1000nm.

G64-12 click on the link to request the dataset

UVES.2000-02-13T06:02:55.846.fits DICHR#1 BLUE3465400. 0.8
UVES.2000-02-13T07:35:47.398.fits DICHR#1 BLUE3465400. 0.8
UVES.2000-02-15T06:36:05.583.fits DICHR#1 BLUE3464800. 0.8
UVES.2000-02-15T07:56:54.524.fits DICHR#1 BLUE3464800. 0.8

UVES.2000-02-13T06:04:13.621.fits DICHR#1 RED580 5400. 0.8
UVES.2000-02-13T07:37:07.356.fits DICHR#1 RED580 5400. 0.8
UVES.2000-02-15T06:37:30.634.fits DICHR#1 RED860 4800. 0.8
UVES.2000-02-15T07:58:30.045.fits DICHR#1 RED860 4800. 0.8
 


 ChemicalAbundances in LMC Clusters in a Wide Age Range

9 Giants were observed in 4 clusters withthe R580nm setting and a slit  of 1.0" to 1.2" (depending on seeing) corresponding to R=40000 to 45000, and giving a spectral coverage: 480nm-680nm.

Archive filename                 Setting      Exp.time slit(")

NGC1866 (Identification Brocato et al.1989) click on the link to request the dataset

star 444
UVES.2000-02-10T02:32:07.993.fits RED    RED580 5400 1.2
star 1653
UVES.2000-02-12T00:58:17.488.fits RED    RED580 3600 1.2
star 867
UVES.2000-02-17T00:54:47.266.fits RED    RED580 3600 1.0
UVES.2000-02-17T01:55:48.450.fits RED    RED580 3600 1.0

NGC1978 (Identification Loyd & Evans1980) click on the link to request the dataset

star LE8
UVES.2000-02-16T00:54:46.852.fits RED    RED580 4500 1.2
UVES.2000-02-16T02:10:57.588.fits RED    RED580 4500 1.2
star LE9
UVES.2000-02-15T00:45:55.550.fits RED    RED580 4500 1.0
UVES.2000-02-15T02:02:12.959.fits RED    RED580 4500 1.0
UVES.2000-02-18T01:56:32.416.fits DICHR#2 BLUE4374500 1.0
UVES.2000-02-18T00:40:38.518.fits DICHR#2 BLUE4374500 1.0
UVES.2000-02-18T01:58:15.098.fits DICHR#2 RED8604500 1.0
UVES.2000-02-18T00:42:04.448.fits DICHR#2 RED8604500 1.0

ESO121  (Identification Mateo 1986)click on the link to request the dataset

star M313
UVES.2000-02-11T00:59:50.950.fits RED    RED580 5400 1.0
UVES.2000-02-11T02:31:20.981.fits RED    RED580 5400 1.0
star M167
UVES.2000-02-13T00:54:13.444.fits RED    RED580 4500 1.0
UVES.2000-02-14T02:32:35.875.fits RED    RED580 4500 1.0
 

NGC2210(Identification Brocato et al.1996) click on the link to request the dataset

star B4364 + B110 (2 stars in the same slit):
UVES.2000-02-12T02:05:56.508.fits RED    RED580 6000 1.0
star B4793
UVES.2000-02-14T00:57:43.839.fits RED    RED580 5400 1.0


Supernovae 1987a

SN87a
Archive filename                 Setting      Exp.timeslit(")
UVES.2000-02-13T02:14:52.282.fits  RED  RED580  1800  1.0
UVES.2000-02-17T03:02:03.279.fits  BLUE BLUE346 3600  1.0
UVES.2000-02-17T03:03:32.084.fits  RED  RED580  3600  1.0


Full night-by-night Logs