Further access options are discussed below
For a list of all services and tables belonging to this service's resource, see Information on resource 'ppmxl/q'
To query this data, you can use
You can retrieve also the whole data set as a gzipped text file from http://vo.ari.uni-heidelberg.de/ppmxl (39.4 GiB). The columns in the text file are in database order as documented in the table info in DB order with columns separated by vertical bars ("|").
David Tholen kindly provided code to convert this into a collection of files for easy consumption by FORTRAN programs.
You can access this service using:
This service is published as follows:
local means it is listed on our front page, ivo_managed means it has a record in the VO registry.
The following fields are available to provide input to the service (with some renderers, some of these fields may be unavailable):
Name | Table Head | Description | Unit | UCD |
---|---|---|---|---|
DEC | Delta (ICRS) | Declination (ICRS decimal) | deg | pos.eq.dec |
hscs_pos | Position/Name | Coordinates (as h m s, d m s or decimal degrees), or SIMBAD-resolvable object | N/A | N/A |
hscs_sr | Search radius | Search radius in arcminutes | N/A | N/A |
ipix | Id | Identifier (Q3C ipix of the USNO-B 1.0 object) | N/A | meta.id;meta.main |
maxrec | Match limit | Maximum number of records returned. Pass 0 to retrieve service parameters. | N/A | N/A |
RA | Alpha (ICRS) | Right Ascension (ICRS decimal) | deg | pos.eq.ra |
responseformat | Output Format | File format requested for output. | N/A | meta.code.mime |
SR | Search Radius | Search radius | deg | N/A |
verb | Verbosity | Exhaustiveness of column selection. VERB=1 only returns the most important columns, VERB=2 selects the columns deemed useful to the average user, VERB=3 returns a table with all available columns. | N/A | N/A |
The following fields are contained in the output by default. More fields may be available for selection; these would be given below in the VOTable output fields.
Name | Table Head | Description | Unit | UCD |
---|---|---|---|---|
dej2000 | Dec | Declination J2000.0, epoch 2000.0 | deg | pos.eq.dec;meta.main |
e_deepDE | E_deepde | Mean error in Dec at mean epoch | deg | stat.error;pos.eq.dec;meta.main |
e_pmDE | Err. PM(Dec) | Mean error in pmDE | deg/yr | stat.error;pos.pm;pos.eq.dec |
e_pmRA | Err. PM(RA) | Mean error in pmRA*cos(delta) | deg/yr | stat.error;pos.pm;pos.eq.ra |
e_raepRA | E_raepra | Mean error in RA*cos(delta) at mean epoch | deg | stat.error;pos.eq.ra;meta.main |
Hmag | m_H | H selected default magnitude from 2MASS | mag | phot.mag;em.IR.H |
ipix | Id | Identifier (Q3C ipix of the USNO-B 1.0 object) | N/A | meta.id;meta.main |
Jmag | m_J | J selected default magnitude from 2MASS | mag | phot.mag;em.IR.J |
Kmag | m_K_s | K_s selected default magnitude from 2MASS | mag | phot.mag;em.IR.K |
pmDE | PM(Dec) | Proper Motion in Dec | deg/yr | pos.pm;pos.eq.dec |
pmRA | PM(RA) | Proper Motion in RA*cos(delta) | deg/yr | pos.pm;pos.eq.ra |
raj2000 | RA | Right Ascension J2000.0, epoch 2000.0 | deg | pos.eq.ra;meta.main |
The following fields are available in VOTable output. The verbosity level is a number intended to represent the relative importance of the field on a scale of 1 to 30. The services take a VERB argument. A field is included in the output if their verbosity level is less or equal VERB*10.
Name | Table Head | Description | Unit | UCD | Verb. Level |
---|---|---|---|---|---|
raj2000 | RA | Right Ascension J2000.0, epoch 2000.0 | deg | pos.eq.ra;meta.main | 1 |
dej2000 | Dec | Declination J2000.0, epoch 2000.0 | deg | pos.eq.dec;meta.main | 1 |
pmRA | PM(RA) | Proper Motion in RA*cos(delta) | deg/yr | pos.pm;pos.eq.ra | 1 |
pmDE | PM(Dec) | Proper Motion in Dec | deg/yr | pos.pm;pos.eq.dec | 1 |
ipix | Id | Identifier (Q3C ipix of the USNO-B 1.0 object) | N/A | meta.id;meta.main | 5 |
e_raepRA | E_raepra | Mean error in RA*cos(delta) at mean epoch | deg | stat.error;pos.eq.ra;meta.main | 15 |
e_deepDE | E_deepde | Mean error in Dec at mean epoch | deg | stat.error;pos.eq.dec;meta.main | 15 |
e_pmRA | Err. PM(RA) | Mean error in pmRA*cos(delta) | deg/yr | stat.error;pos.pm;pos.eq.ra | 15 |
e_pmDE | Err. PM(Dec) | Mean error in pmDE | deg/yr | stat.error;pos.pm;pos.eq.dec | 15 |
Jmag | m_J | J selected default magnitude from 2MASS | mag | phot.mag;em.IR.J | 15 |
Hmag | m_H | H selected default magnitude from 2MASS | mag | phot.mag;em.IR.H | 15 |
Kmag | m_K_s | K_s selected default magnitude from 2MASS | mag | phot.mag;em.IR.K | 15 |
nobs | #obs | Number of observations used Note 4 | N/A | meta.number;obs | 20 |
e_Jmag | Err(m_J) | J total magnitude uncertainty | mag | stat.error;phot.mag;em.IR.J | 20 |
epRA | Epra | Mean Epoch (RA) | yr | time.epoch;pos.eq.ra | 25 |
epDE | Epde | Mean Epoch (Dec) | yr | time.epoch;pos.eq.dec | 25 |
e_Hmag | Err(m_H) | H total magnitude uncertainty | mag | stat.error;phot.mag;em.IR.H | 25 |
e_Kmag | Err(m_K_s) | K_s total magnitude uncertainty | mag | stat.error;phot.mag;em.IR.K | 25 |
b1mag | USNO mag (B1) | B mag from USNO-B, first epoch Note 1 | N/A | phot.mag;em.opt.B | 25 |
b2mag | USNO mag (B2) | B mag from USNO-B, second epoch Note 1 | N/A | phot.mag;em.opt.B | 25 |
r1mag | USNO mag (R1) | R mag from USNO-B, first epoch Note 1 | N/A | phot.mag;em.opt.R | 25 |
r2mag | USNO mag (R2) | R mag from USNO-B, second epoch Note 1 | N/A | phot.mag;em.opt.R | 25 |
imag | USNO mag (I) | I mag from USNO-B Note 1 | N/A | phot.mag;em.opt.I | 25 |
magSurveys | USNO Mag src. | Surveys the USNO-B magnitudes are taken from Note 2 | N/A | meta.code | 28 |
flags | Flags | Flags Note 3 | N/A | meta.code | 28 |
VOResource XML (that's something exclusively for VO nerds)
Magnitudes from USNO-B should be used with care. Photometric calibration may be severely off for some plates.
For objects from PPMX (bit 1 set in flags), these magnitudes have a special meaning as per the following table:
PPMXL column | PPMX column | PPMX content |
---|---|---|
b1mag | Cmag | Catalogue magnitude from source |
b2mag | Bmag | Johnson B magnitude |
r1mag | Rmag | calc. Ru magnitude from source |
r2mag | N/A | always None |
imag | Vmag | Johnson V magnitude |
magSurveys is built by concatenating the digits assigned to the surveys for b1mag, b2mag, r1mag, r2mag, and imag (in this sequence). The digits are those of given in Note h to Table 3 in 2003AJ....125..984M, except we do not distinguish POSS-II N and SERC-I as a part of POSS-I-N (i.e., both 7 and 9 are 7 here).
From this field, you can also see which of the surveys contributing to USNO-B had positions for the object.
The flags column contains a bitwise or of warnings and similar conditions. The bit's meaning is as follows:
bit 0: | If set, one of the coordinates had an excessively large chisquare. |
---|---|
bit 1: | Row is from PPMX. These objects are mostly Tycho stars that were masked out of USNO-B. For these, the USNO magnitudes (b1mag through imag) have special meanings. See the note on magnitudes. |
bit 2: | Row is from PPMX and replaces a single row from USNO-B. This is done when the astrometry from PPMX was better (in terms of error estimates) than the astrometry of the corresponding PPMXL object. |
bit 3: | Row replaces multiple USNO-B1.0 objects. When PPMX contains an object that has more than one counterpart in PPMX-L, all such counterparts are discarded on the assumption that they should have been matched in USNO-B1.0 or result from erroneous matches. For these rows, bit 1 is always 1. |
nobs may be NULL for stars coming from ARIHIP or Tycho-2 via PPMX (i.e., bit 1 is set in flags).