Catalogue UCAC4
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C2A est capable de lire la
version native du catalogue UCAC4 (Fourth U.S. Naval Observatory CCD
Astrograph Catalog). Le catalogue UCAC4, édité par l'US Naval Observatory,
est un catalogue qui couvre tout le ciel entre les magnitudes 8 et 16
environ, ceci dans une seule bande photométrique entre V et R. Les erreurs
sur les positions se situent entre 15 et 20 mas pour les étoiles entre
les magnitudes 10 et 14. Les mouvements propres ont été
dérivées des positions de plus de 113 millions d'étoiles
à partir de 140 catalogues ayant des époques significativement
différentes de celle des observations CCD utilisées pour
le catalogue UCAC4. Ces données sont complétées par des données
photométriques 2MASS pour environ 110 millions d'étoiles ainsi
que des données photométriques de l'APASS (AAVSO Photometric
All-Sky Survey) dans 5 bandes (B,V,g,r,i) pour environ 50 millions d'étoiles.
Toutes les étoiles brillantes non observées avec l'astrographe
ont été ajoutées au catalogue UCAC4 à partir
d'uns catalogues Hipparcos et Tycho-2. L'UCAC4 devrait être complet
pour toutes les étoiles jusqu'à une magnitude R=16, avec
la source des données indiquées sous forme d'un "flag".
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Les statistiques sur le catalogue sont les suivantes:
- 113 780 093 étoiles dans le catalogue UCAC4 (avec les étoiles
supplémentaires)
- 109 921 682 avec une identification 2MASS
- 106 689 821 avec un mouvement propre
- 81 897 551 avec 2 époques pour les mouvements propres
- 27 245 403 avec 3époques pour les mouvements propres
- 80 806 744 avec au moins 2 images ayant un "good fit" dans les observations
CCD
- 48 323 349 "matched" avec l'UCAC2
- 54 690 "matched" avec des galaxies LEDA
- 76 020 "matched" avec le cayalogue de sources étendues 2MASS
- 8 925 étoiles supplémentaires (sans observation CCD)
- 121 350 entrées UCAC4 avec une correspondance Hipparcos
- 104 681 entrées UCAC4 avec des observations substituées par
FK6/Hip/Tycho-2
La sélection de ce catalogue comme catalogue courant se fait depuis l'onglet
Etoiles de la boîte
de dialogue des options ou en faisant un clic droit dans la carte avec la souris
tout en maintenant la touche MAJ du clavier appuyée.
C2A prend en compte les mouvements propres fournis dans le catalogue UCAC4
pour déterminer les positions des étoiles à la date spécifiée par l'utilisateur
(voir les options avancées dans l'onglet Etoiles de la boîte
de dialogue des options). De plus, il est possible de spécifier dans les options
avancées quelle magnitude doit être utilisée pour les filtres et les affichages.
Les magnitudes disponibles sont les suivantes: Fit Model (V-R), Aperture
(V-R), 2MASS J, 2MASS H et 2MASS K_s, APASS
B, APASS V, APASS g, APASS r et APASS i.
Les flags sur les étoiles UCAC4 sont utilisés pour l'affichage des étoiles:
- Si l'étoile a le flag "object could be from possible streak",
elle est affichée entourée d'un cercle bleu.
- Si l'étoile est surexposée sur une ou plusieurs images ou bien si elle est
proche d'une étoile surexposée, elle est affichée entourée d'un cercle rouge.
- Si l'étoile n'est pas une étoile simple (flag "dsf"),
elle est affichée en blanc.
Dans tous les autres cas, elle est affichée dans la couleur par défaut des étoiles.
A noter que contrairement au catalogue UCAC2, le catalogue UCAC4 n'a pas besoin
d'être compilé pour pouvoir être lu par C2A. La structure des répertoires
du catalogue original est respéctée pour la lecture par C2A:
- Les fichiers z001 à z900 doivent
être présents dans un sous-dossier u4b
- Les fichiers zone_stats et u4index.unf
doivent être présents dans un sous-dossier u4i
Les informations reportées pour chaque étoile du catalogue sont toutes celles
fournies en standard dans le catalogue UCAC4. La description des champs fournie
dans la documentation du catalogue UCAC4 est reproduite ci-dessous:
col byte item fmt unit explanation notes
---------------------------------------------------------------------------
1 1- 3 ra I*4 mas right ascension at epoch J2000.0 (ICRS) (1)
2 5- 8 spd I*4 mas south pole distance epoch J2000.0 (ICRS) (1)
3 9-10 magm I*2 millimag UCAC fit model magnitude (2)
4 11-12 maga I*2 millimag UCAC aperture magnitude (2)
5 13 sigmag I*1 1/100 mag error of UCAC magnitude (3)
6 14 objt I*1 object type (4)
7 15 cdf I*1 combined double star flag (5)
15 bytes
8 16 sigra I*1 mas s.e. at central epoch in RA (*cos Dec) (6)
9 17 sigdc I*1 mas s.e. at central epoch in Dec (6)
10 18 na1 I*1 total # of CCD images of this star
11 19 nu1 I*1 # of CCD images used for this star (7)
12 20 cu1 I*1 # catalogs (epochs) used for proper motions
5 bytes
13 21-22 cepra I*2 0.01 yr central epoch for mean RA, minus 1900
14 23-24 cepdc I*2 0.01 yr central epoch for mean Dec,minus 1900
15 25-26 pmrac I*2 0.1 mas/yr proper motion in RA*cos(Dec) (8)
16 27-28 pmdc I*2 0.1 mas/yr proper motion in Dec
17 29 sigpmr I*1 0.1 mas/yr s.e. of pmRA * cos Dec (9)
18 30 sigpmd I*1 0.1 mas/yr s.e. of pmDec (9)
10 bytes
19 31-34 pts_key I*4 2MASS unique star identifier (10)
20 35-36 j_m I*2 millimag 2MASS J magnitude
21 37-38 h_m I*2 millimag 2MASS H magnitude
22 39-40 k_m I*2 millimag 2MASS K_s magnitude
23 41 icqflg I*1 2MASS cc_flg*10 + ph_qual flag for J (11)
24 42 (2) I*1 2MASS cc_flg*10 + ph_qual flag for H (11)
25 43 (3) I*1 2MASS cc_flg*10 + ph_qual flag for K_s (11)
26 44 e2mpho I*1 1/100 mag error 2MASS J magnitude (12)
27 45 (2) I*1 1/100 mag error 2MASS H magnitude (12)
28 46 (3) I*1 1/100 mag error 2MASS K_s magnitude (12)
16 bytes
29 47-48 apasm I*2 millimag B magnitude from APASS (13)
30 49-50 (2) I*2 millimag V magnitude from APASS (13)
31 51-52 (3) I*2 millimag g magnitude from APASS (13)
32 53-54 (4) I*2 millimag r magnitude from APASS (13)
33 55-56 (5) I*2 millimag i magnitude from APASS (13)
34 57 apase I*1 1/100 mag error of B magnitude from APASS (14)
35 58 (2) I*1 1/100 mag error of V magnitude from APASS (14)
36 59 (3) I*1 1/100 mag error of g magnitude from APASS (14)
37 60 (4) I*1 1/100 mag error of r magnitude from APASS (14)
38 61 (5) I*1 1/100 mag error of i magnitude from APASS (14)
39 62 gcflg I*1 Yale SPM g-flag*10 c-flag (15)
16 bytes
40 63-66 icf(1) I*4 FK6-Hipparcos-Tycho source flag (16)
41 icf(2) .. AC2000 catalog match flag (17)
42 icf(3) .. AGK2 Bonn catalog match flag (17)
43 icf(4) .. AKG2 Hamburg catalog match flag (17)
44 icf(5) .. Zone Astrog. catalog match flag (17)
45 icf(6) .. Black Birch catalog match flag (17)
46 icf(7) .. Lick Astrog. catalog match flag (17)
47 icf(8) .. NPM Lick catalog match flag (17)
48 icf(9) .. SPM YSJ1 catalog match flag (17)
4 bytes
49 67 leda I*1 LEDA galaxy match flag (18)
50 68 x2m I*1 2MASS extend.source flag (19)
51 69-72 rnm I*4 unique star identification number (20)
52 73-74 zn2 I*2 zone number of UCAC2 (0 = no match) (21)
53 75-78 rn2 I*4 running record number along UCAC2 zone (21)
12 bytes
---------------------------------------------------------------------------
78 = total number of bytes per star record
Note (1): Positions are on the International Celestial Reference
System (ICRS) as represented by the Hipparcos / Tycho-2 catalogs.
The epoch for the positions of all stars is J2000.0; the weighted
mean catalog position was updated using the provided proper
motions. The observational UCAC position is but one of several
going into these values and is not given in the UCAC4; thus the
original UCAC observation cannot be recovered from these data.
The declination is given in south pole distance (spd) and can be
converted back to a true declination by subtracting 324000000 mas.
Note (2): Unknown, or unrealistic photometric results are set to
magnitude = 20 (20000 mmag entry in catalog). Systematic errors
are expected to be below 0.1 mag for magm,maga photometric results
obtained from the UCAC CCD pixel data. The aperture photometry
is considered more robust, particularly for "odd" cases, while
the model fit magnitude is expected to be more accurate for
"well behaved" stars.
Note (3): A value of 99 for error in magnitude means "no data".
For many stars a photometric error based on the scatter from
individual observations of that star on different CCD frames
could be obtained. A model error was also attempted to be
assigned, based on the S/N ratio. The error quoted here is
the larger of the 2. If that error exceeds 0.9 mag the error
was set to 0.9 mag (= value 90 in catalog data, unit = 10 mmag).
Note (4): The object type flag is used to identify possible problems
with a star or the source of data. Of the individual image flags
the one with the largest value (worst problem case) is propagated
into this object type flag, unless it is superseded by an overriding
flag at the combined image stage.
The object type flag has the following meaning:
0 = good, clean star (from MPOS), no known problem
1 = largest flag of any image = near overexposed star (from MPOS)
2 = largest flag of any image = possible streak object (from MPOS)
3 = high proper motion (HPM) star, match with external PM file (MPOS)
4 = actually use external HPM data instead of UCAC4 observ.data
(accuracy of positions varies between catalogs)
5 = poor proper motion solution, report only CCD epoch position
6 = substitute poor astrometric results by FK6/Hip/Tycho-2 data
7 = added supplement star (no CCD data) from FK6/Hip/Tycho-2 data,
and 2 stars added from high proper motion surveys
8 = high proper motion solution in UCAC4, star not matched with PPMXL
9 = high proper motion solution in UCAC4, discrepant PM to PPMXL
(see discussion of flags 8,9 in redcution section 2e above)
The number of stars with those flags is:
0 103080317
1 2785787
2 15519
3 97042
4 35073
5 5004704
6 34473
7 8925
8 2028600
9 689653
Note (5): The cdf flag is a combined double star flag used to indicate
the type/quality of double star fit. It is a combination of 2 flags,
cdf = 10 * dsf + dst with the following meaning:
dsf = double star flag = overall classification
0 = single star
1 = component #1 of "good" double star
2 = component #2 of "good" double star
3 = blended image
dst = double star type, from pixel data image profile fits,
largest value of all images used for this star
0 = no double star, not sufficient #pixels or elongation
to even call double star fit subroutine
1 = elongated image but no more than 1 peak detected
2 = 2 separate peaks detected -> try double star fit
3 = secondary peak found on each side of primary
4 = case 1 after successful double fit (small separ. blended image)
5 = case 2 after successful double fit (most likely real double)
6 = case 3 after successful double fit (brighter secondary picked)
A word of caution: often a dsf= 1 or 2 image is paired with a dsf= 3.
If for a star any of the several images reveals a "blended image",
that higher dsf=3 flag is carried into the output file. This can
happen for a regular double star with unique components 1 and 2.
A flag dsf=3 means this could be component 1 or 2 but at least on
one CCD frame a blended image was detected. This blend could be
with the other component, or a spurious image or artifact.
The double star flags need to be interpreted with caution; anything
but a zero means "likely some double star component or blended image".
The following number of stars have cdf flag values:
0 110299935
1 262162
2 355769
3 57103
4 2408 14 19590 24 23967 34 1053229
5 7884 15 78344 25 209822 35 1226761
6 23787 16 13096 26 20945 36 125291
Note (6): The range of values here is 1 to 255 which is represented
as a signed 1-byte integer (range -127 to 127); thus add 128 to the
integer number found in the data file. There is no 0 mas value;
data less than 1 mas have been set to 1 mas. Original data larger
than 255 mas have been set to 255.
If the astrometric data for a star was substituted from an external
catalog like Hipparcos, Tycho or high proper motion data, a mean
error in position and proper motion depending on the catalog and
magnitude of the star was adopted.
Note (7): A zero for the number of used images indicates that all images
have some "problem" (such as overexposure). In that case an unweighted
mean over all available images (na) is taken to derive the mean
position, while normally a weighted mean was calculated based on
the "good" images, excluding possible problem images (nu smaller
or equal to na).
Note (8): A value of 32767 for either proper motion component means
the real PM of that star is larger and found in the extra table
file u4hpm.dat (32 stars, ASCII). The cross reference is established
by the unique, modified MPOS number (column 51 of main data file),
which is also given on the HPM supplement stars file.
For stars without valid proper motion the proper motion data are set
to 0. However, valid proper motions can also be 0. The "no data"
case is indicated by the sigma proper motion columns (see below).
Note (9): Values in the binary data files are represented as signed,
1-byte integer (range -128 to 127). Add 128 to bring those values
to the range of 0 to 255, which is the error in proper motion in
unit of 0.1 mas/yr, with the following exception.
Data entries above 250 indicate larger errors as follows:
251 --> 275 = 27.5 mas/yr
252 --> 325 = 32.5 mas/yr
253 --> 375 = 37.5 mas/yr
254 --> 450 = 45.0 mas/yr
255 --> "no data" = set to 500 for output tables
For astrometric data copied from the FK6, Hipparcos and Tycho-2
catalogs a mean error in positions was adopted depending on input
catalog and the brightness of the star rather than giving the
individual star's error quoted in those catalogs.
Note (10): The 2MASS items copied into UCAC4 are described at
pegasus.astro.umass.edu/ipac_wget/releases/allsky/doc/sec2_2a.html
Note (11): For each 2MASS bandpass a combined flag was created
(cc_flg*10 + ph_qual) consisting of the contamination flag (0 to 5)
and the photometric quality flag (0 to 8).
0 = cc_flg 2MASS 0, no artifacts or contamination
1 = cc_flg 2MASS p, source may be contaminated by a latent image
2 = cc_flg 2MASS c, photometric confusion
3 = cc_flg 2MASS d, diffraction spike confusion
4 = cc_flg 2MASS s, electronic stripe
5 = cc_flg 2MASS b, bandmerge confusion
0 = no ph_qual flag
1 = ph_qual 2MASS X, no valid brightness estimate
2 = ph_qual 2MASS U, upper limit on magnitude
3 = ph_qual 2MASS F, no reliable estimate of the photometric error
4 = ph_qual 2MASS E, goodness-of-fit quality of profile-fit poor
5 = ph_qual 2MASS A, valid measurement, [jhk]snr>10 AND [jhk]cmsig<0.10857
6 = ph_qual 2MASS B, valid measurement, [jhk]snr> 7 AND [jhk]cmsig<0.15510
7 = ph_qual 2MASS C, valid measurement, [jhk]snr> 5 AND [jhk]cmsig<0.21714
8 = ph_qual 2MASS D, valid measurement, no [jhk]snr OR [jhk]cmsig req.
For example icqflg = 05 is decoded to be cc_flg=0, and ph_qual=5, meaning
no artifacts or contamination from cc_flg and 2MASS qual flag = "A" .
Note (12): The photometric errors from 2MASS were rounded by 1 digit
here to fit into fewer bytes (1/100 mag instead of millimag).
These data were taken from the j_msigcom, h_msigcom, and k_msigcom columns
of the 2MASS point source catalog. See note (10).
Note (13): Data are from the AAVSO Photometric all-sky survey (APASS)
DR6 plus single observation stars kindly provided by A.Henden.
A magnitude entry of 20000 indicates "no data". For bright stars
the apasm(1) = B mag and apasm(2) = V mag columns contain the
Hipparcos/Tycho Bt and Vt mags respectively, whenever there is no
APASS B or V available and valid Bt or Vt mags were found.
For the bright supplement stars the same was done. All thses cases
are identified by apasm(1) smaller
than 20000 and apase(1) = 0 for B mags,
and similarly for apasm(2) smaller
than 20000 and apase(2) = 0 for V mags.
For over 10,000 stars no Vt mag was available and the V mag from Tycho
was used instead.
The following number of stars have entries in the APASS photometry:
51862350 some valid data in either of the columns
51070044 B mag
51861015 V mag
45799843 g mag
45615993 r mag
41491953 i mag
Note (14): Positive errors are from the official release data error
estimates (at least 2 observations per star). Formal, S/N estimated
errors for single observations are multiplied by -1 for this column.
The valid range for each APASS magnitude error is +-90 = +-0.90 mag.
For "no data" (i.e. magnitude = 20000 = 20.0 mag) the error is set to 99.
Note (15): The g-flag from the Yale San Juan first epoch Southern
Proper Motion data (YSJ1, SPM) has the following meaning:
0 = no info
1 = matched with 2MASS extended source list
2 = LEDA galaxy
3 = known QSO
The c-flag from the Yale San Juan first epoch Southern
Proper Motion data (YSJ1, SPM) indicates which input catalog
has been used to identify stars for pipeline processing:
1 = Hipparcos
2 = Tycho2
3 = UCAC2
4 = 2MASS psc
5 = 2MASS xsc (extended sources, largely (but not all!) galaxies)
6 = LEDA (confirmed galaxies, Paturel et al. 2005)
7 = QSO (Veron-Cetty & Veron 2006)
Note (16, 17) binary data: a single 4-byte integer is used to store
the 10 flags of "icf". That 4-byte integer has the value:
icf = icf(1)*10^8 + icf(2)*10^7 + ... + icf(8)*10 + icf(9)
Note (16): The FK6-Hipparcos-Tycho-source-flag has the following meaning:
(= icf(1))
0 = not a Hip. or Tycho star
1 = Hipparcos 1997 version main catalog (not in UCAC4 data files)
2 = Hipparcos double star annex
3 = Tycho-2
4 = Tycho annex 1
5 = Tycho annex 2
6 = FK6 position and proper motion (instead of Hipparcos data)
7 = Hippparcos 2007 solution position and proper motion
8 = FK6 only PM substit. (not in UCAC4 data)
9 = Hipparcos 2007, only proper motion substituted
Note (17): The catflg match flag is provided for major catalogs used
in the computation of the proper motions. Each match is analyzed
for multiple matches of entries of the 1st catalog to 2nd catalog
entries, and the other way around. Matches are also classified
by separation and difference in magnitude to arrive at a confidence
level group. The flag has the following meaning:
0 = star not matched with this catalog
1 = unique-unique match, not involving a double star
2 = ... same, but involving a flagged double star
3 = multiple match but unique in high confidence level group, no double
4 = ... same, but involving a flagged double star
5 = closest match, not involving a double, likely o.k.
6 = ... same, but involving a flagged double star
7 = maybe o.k. smallest sep. match in both directions, no double
8 = ... same, but involving a flagged double star
Note (18): This flag is either 0 (no match) or contains the log10 of
the apparent total diameter for I-band (object size) information
(unit = 0.1 arcmin) copied from the LEDA catalog (galaxies).
A size value of less than 1 has been rounded up to 1.
Note (19): This flag is either 0 (no match) or contains the length of
the semi-major axis of the fiducial ellipse at the K-band
(object size) information copied from the 2MASS extended source
catalog.
Note (20): This unique star identification number is between 200001
and 321640 for Hipparcos stars, and between 1 and 9430 for non-
Hipparcos stars supplemented to the UCAC4 catalog (no CCD observ.).
For all other stars this unique star identification number is the
internal mean-position-file (MPOS) number + 1 million.
For both the Hipparcos and the supplement stars there is an entry
on the u4supl.dat file providing more information, including the
original Hipparcos star number. Note, there are several thousand
cases where different UCAC4 stars link to the same Hipparcos star
number due to resolved binary stars with each component being a
separate star entry in UCAC4.
Note (21): This info provides a cross reference to UCAC2. Both zn2
and rn2 are 0 if the UCAC4 star could not be found in UCAC2.
Des informations complémentaires sur le catalogue UCAC4 peuvent être trouvée
sur la Home Page UCAC à : http://www.usno.navy.mil/USNO/astrometry/optical-IR-prod/ucac
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