Table Description:
This table is not available for ADQL queries and through the TAP endpoint.
Resource Description:
For a list of all services and tables belonging to this table's resource, see Information on resource 'LAMOST DR6 Spectra'
This table has an associated publication. If you use data from it, it may be appropriate to reference http://dr6.lamost.org/v2/ either in addition to or instead of the service reference.
To cite the table as such, we suggest the following BibTeX entry:
@MISC{vo:lamost6_medres, year=2020, title={{LAMOST} DR6 Spectra}, author={National Astronomical Observatories of the Chinese Academy of Sciences}, url={https://dc.zah.uni-heidelberg.de/tableinfo/lamost6.medres}, howpublished={{VO} resource provided by the {GAVO} Data Center} }
Guoshoujing Telescope (the Large Sky Area Multi-Object Fiber Spectroscopic Telescope LAMOST) is a National Major Scientific Project built by the Chinese Academy of Sciences. Funding for the project has been provided by the National Development and Reform Commission. LAMOST is operated and managed by the National Astronomical Observatories, Chinese Academy of Sciences.
Please also see the LAMOST Data Policy.
Sorted alphabetically. [Sort by DB column index]
Name | Table Head | Description | Unit | UCD |
---|---|---|---|---|
accref | Product key | Access key for the data | N/A | meta.ref.url |
accsize | File size | Size of the data in bytes | byte | VOX:Image_FileSize |
bad_b | B bad? | 1 if this is a problematic B spectrum. | N/A | meta.code |
bad_r | R bad? | 1 if this is a problematic R spectrum. | N/A | meta.code |
coadd | Coadd? | 1 if this is a co-added spectrum | N/A | meta.code |
dec | Target Dec | ICRS declination for this object from input catalogue | deg | pos.eq.dec;meta.main |
dec_obs | Fiber Dec | ICRS declination of the fiber pointing | deg | pos.eq.dec |
designation | Target | Target Designation (IAU style) | N/A | meta.id |
embargo | Embargo ends | Date the data will become/became public | yr | N/A |
fiberid | Fiber | Identifier of the fiber used to take the source spectrum | N/A | meta.id;instr |
fibermask | Fiber prob | Bitmask for fiber problems. See note for the meaning for the bits. [Note fib] | N/A | meta.code.qual |
fibertype | Fiber | Fiber Type of target (one of Obj, Sky, F-std, Unused, PosErr, Dead) | N/A | meta.code;instr |
mag_arr | Mags. | An array of derived magnitudes. See mag_types for the bands these magnitudes are intended for. | N/A | phot.mag |
magtype | Mag.Type | Designation of the bands of the magnitudes in mag_arr; this is not easy to parse by a machine, sorry. | N/A | meta.code |
mime | Type | MIME type of the file served | N/A | meta.code.mime |
mobsid | Mobsid | Unique identifier for the medium resolution spectrum (most of these have multiple observations and include a coadded spectrum). | N/A | meta.id;meta.main |
objtype | Ob. type | Object type: star, k2star, fs, rvcandi, gal | N/A | meta.code.class |
obsid | Obsid | Unique identifier for the observation; LAMOST observations typically result in multiple spectra. | N/A | meta.id;obs |
offset_v | Offset | Offset of the observation from the target coordinate (these are added for bright objects to prevent saturation). | arcsec | instr.offset |
owner | Owner | Owner of the data | N/A | N/A |
planid | Plan | Identifier of the observation plan | N/A | meta.id;obs.proposal |
ra | Target RA | ICRS right ascension for this object from input catalogue | deg | pos.eq.ra;meta.main |
ra_obs | Fiber RA | ICRS right ascension of the fiber pointing (can be different from ra for bright sources). | deg | pos.eq.ra |
rv_b0 | RV b0 | Radial velocity estimated from the B spectrum after continuum removal. | km/s | spect.dopplerVeloc |
rv_b0_err | Err. RV b0 | Error in rv_b0. | km/s | stat.error;spect.dopplerVeloc |
rv_b1 | RV b1 | rv_b0 after zero-point correction | km/s | spect.dopplerVeloc |
rv_b1_err | Err. RV b1 | Error in rv_b1. | km/s | stat.error;spect.dopplerVeloc |
rv_b_flag | b ? | Flag for RV extraction in the b band: 0 – no anomalies; 1 – too many bad pixels; 2 – radial velocity in excess of 450 km/s; 3 – low similarity with best-matched template. | N/A | meta.code.qual |
rv_br0 | RV br0 | Radial velocity estimated from the B and R spectra after continuum removal. | km/s | spect.dopplerVeloc |
rv_br0_err | Err. RV br0 | Error in rv_br0. | km/s | stat.error;spect.dopplerVeloc |
rv_br1 | RV br1 | rv_br0 after zero-point correction | km/s | spect.dopplerVeloc |
rv_br1_err | Err. RV br1 | Error in rv_br1. | km/s | stat.error;spect.dopplerVeloc |
rv_br_flag | br ? | Flag for RV extraction in the br band: 0 – no anomalies; 1 – too many bad pixels; 2 – radial velocity in excess of 450 km/s; 3 – low similarity with best-matched template. | N/A | meta.code.qual |
rv_lasp0 | RV lasp0 | Radial velocity estimated from the LAMOST stellar parameter pipeline. | km/s | spect.dopplerVeloc |
rv_lasp0_err | Err. RV lasp0 | Error in rv_lasp0. | km/s | stat.error;spect.dopplerVeloc |
rv_lasp1 | RV lasp1 | rv_lasp0 after zero-point correction | km/s | spect.dopplerVeloc |
rv_lasp1_err | Err. RV lasp1 | Error in rv_lasp1. | km/s | stat.error;spect.dopplerVeloc |
rv_r0 | RV r0 | Radial velocity estimated from the R spectrum after continuum removal. | km/s | spect.dopplerVeloc |
rv_r0_err | Err. RV r0 | Error in rv_r0. | km/s | stat.error;spect.dopplerVeloc |
rv_r1 | RV r1 | rv_r0 after zero-point correction | km/s | spect.dopplerVeloc |
rv_r1_err | Err. RV r1 | Error in rv_r1. | km/s | stat.error;spect.dopplerVeloc |
rv_r_flag | r ? | Flag for RV extraction in the r band: 0 – no anomalies; 1 – too many bad pixels; 2 – radial velocity in excess of 450 km/s; 3 – low similarity with best-matched template. | N/A | meta.code.qual |
spid | SG id | Identifier of the Spectragraph that took the source spectrum. | N/A | meta.id;instr |
ssa_dateObs | Date Obs. | Midpoint of exposure (MJD) | d | time.epoch |
ssa_location | Location | ICRS location of aperture center | deg | pos.eq |
ssa_region | Coverage | Rough coverage based on location and aperture. | N/A | pos.outline;obs.field |
ssa_snr | SNR | Median signal to noise ratio over all pixel, computed as flux/sqrt(variance) | N/A | stat.snr |
ssa_specend | Band end | Upper value of spectral coordinate | m | em.wl;stat.max |
ssa_specres | Spec. Res. | Resolution (in meters of wavelength) on the spectral axis | m | spect.resolution;em.wl |
ssa_specstart | Band start | Lower value of spectral coordinate | m | em.wl;stat.min |
target_comment | Comment | Various comments (e.g., an external target id). | N/A | meta.note |
Columns that are parts of indices are marked like this.
The following services may use the data contained in this table:
VO nerds may sometimes need VOResource XML for this table.
Meaning of the bits in fibermask (note: while upstream counts bits from 1, we count bits from 0):
Bit | Meaning |
---|---|
0 | Fiber not allotted |
1 | Bad trace from the TRACECENTER routine |
2 | Low counts in flat field |
3 | Bad arc solution |
4 | <10% pixels are bad on the CCD |
5 | <10% pixels are saturated |
6 | Whopping fiber |
7 | Near a whopping fiber |
8 | Sky fiber shows extreme residuals |