LS 2883

Basic data :
CPD-63 2495 -- Pulsar Origin of the objects types : (Ref) Object type as listed in the reference "Ref" (acronym) Object type linked to the acronym according to the original reference () Anterior to 2007, before we can link the objet type to a reference, or given by the CDS team in some particular cases Other object types: Be* (), * (1971PW&SO,CPD,...), gam (2018A&A,4FGL,...), Em* (Hen,THA,...), MIR (AKARI,MSX6C,...), X (AX,2XMM,...), HXB (2013MNRAS), Psr (2012ApJ,PSR), V* (2012A&A,AAVSO), Rad (2013MNRAS), UV (XMMOM), NIR (2MASS) Syntax of coordinates is : "ra dec (wtype) [error ellipse] quality bibcode" : ra dec : right ascension and declination (unit and frame defined according to your Output Options) Grey values are increasing the original precision due to the computation of frame transformations (wtype) : wavelength class for the origin of the coordinates (Rad, mm, IR, Optical, UV, Xray, Gam) [error ellipse] : measurement uncertainty, on (ra,dec) if the positional angle is 90 degrees, on (majaxis,minaxis) otherwise (in mas at defined epoch in the original catalogue), position angle (in degrees North celestial pole to East) quality : flag of quality E ≥ 10" D : 1-10" (and some old data) C : 0.1-1" B : 0.01-0.1" + 2MASS, Tyc A : VLBI, Hipparcos bibcode : bibcode of the coordinates reference ICRS coord. (ep=J2000) : 13 02 47.6544015048 -63 50 08.626970292 (Optical) [ 0.0089 0.0100 90 ] A 2020yCat.1350....0G Syntax of coordinates is : "ra dec (wtype) [error ellipse] quality bibcode" : ra dec : right ascension and declination (unit and frame defined according to your Output Options) Grey values are increasing the original precision due to the computation of frame transformations (wtype) : wavelength class for the origin of the coordinates (Rad, mm, IR, Optical, UV, Xray, Gam) [error ellipse] : measurement uncertainty, on (ra,dec) if the positional angle is 90 degrees, on (majaxis,minaxis) otherwise (in mas at defined epoch in the original catalogue), position angle (in degrees North celestial pole to East) quality : flag of quality E ≥ 10" D : 1-10" (and some old data) C : 0.1-1" B : 0.01-0.1" + 2MASS, Tyc A : VLBI, Hipparcos bibcode : bibcode of the coordinates reference FK4 coord. (ep=B1950 eq=1950) : 12 59 38.2624444635 -63 34 01.600570784 [ 0.0089 0.0100 90 ] Syntax of coordinates is : "ra dec (wtype) [error ellipse] quality bibcode" : ra dec : right ascension and declination (unit and frame defined according to your Output Options) Grey values are increasing the original precision due to the computation of frame transformations (wtype) : wavelength class for the origin of the coordinates (Rad, mm, IR, Optical, UV, Xray, Gam) [error ellipse] : measurement uncertainty, on (ra,dec) if the positional angle is 90 degrees, on (majaxis,minaxis) otherwise (in mas at defined epoch in the original catalogue), position angle (in degrees North celestial pole to East) quality : flag of quality E ≥ 10" D : 1-10" (and some old data) C : 0.1-1" B : 0.01-0.1" + 2MASS, Tyc A : VLBI, Hipparcos bibcode : bibcode of the coordinates reference Gal coord. (ep=J2000) : 304.1835825651141 -00.9915845699421 [ 0.0089 0.0100 90 ] Syntax of proper motions is : "pm-ra pm-dec [error ellipse] quality bibcode" pm-ra : mu-ra*cos(dec) (expressed in the ICRS system in mas/yr) pm-dec : mu-dec (expressed in the ICRS system in mas/yr) [error ellipse] : error major axis and minor axis (in mas), orientation angle (in deg) quality : flag of quality (A=best quality -> E=worst quality, {� } =unknown quality) bibcode : bibcode of the proper motion reference Proper motions mas/yr : -7.093 -0.342 [0.012 0.014 90] A 2020yCat.1350....0G Syntax of parallax is : 'value quality [error] bibcode' value : parallax value quality : flag of quality (A=best quality -> E=worst quality, {� } =unknown quality) [error] : mean error bibcode : bibcode of the parallax reference Parallaxes (mas): 0.4434 [0.0133] A 2020yCat.1350....0G Spectral type is made of 3 parts: %coding is composed of 4 parts : the spectral type, which is made of a temperature class, eventually a luminosity class (roman number) and/or spectral peculiarities; a quality letter: A=best quality→E=worst quality, {� } =unknown quality % a quality letter: A=best quality -> E=worst quality, {� } =unknown quality bibcode : bibcode of the spectral type reference Spectral type: O9.5Ve C 2014MNRAS.439..432C Syntax of fluxes (or magnitudes) is : "filter-name (System) flux-value [error] quality MultVarFlags bibcode" filter-name : U, B, V, R, I, G, J, H, K, u, g, r, i, z (System) : may be AB (default is Vega) flux-value : value of flux or magnitude [error] : error value quality : flag of quality of the flux value ( A=best quality -> E=worst quality, {� } =unknown quality) MultVarFlags : Mult is zero or one char (J) for joined photometry ; Var can be zero or two chars (V[0-4]) bibcode : bibcode of the flux reference Fluxes (11) : U 10.34 [~] D 2003AJ....125.2531R B 10.72 [0.01] D 2012yCat.1322....0Z V 9.98 [0.06] D 2012yCat.1322....0Z R 10.03 [0.01] D 2012yCat.1322....0Z G 9.632835 [0.002780] C 2020yCat.1350....0G J 8.026 [0.027] C 2003yCat.2246....0C H 7.699 [0.055] C 2003yCat.2246....0C K 7.248 [0.020] C 2003yCat.2246....0C g 10.66 [0.01] E 2012yCat.1322....0Z r 9.64 [0.01] E 2012yCat.1322....0Z i 9.13 [0.04] D 2012yCat.1322....0Z	SIMBAD within arcmin ', {sourceSize:12, color:'#30a090'})); aladin.on('objectClicked', function(object) { var objName=object.data.MAIN_ID; aladin.showPopup(object.ra,object.dec,'',''+ objName+''); });" title="Show Simbad objects"> Overlay points in this preview 2MASS DSS SDSSXMMIRACIRISGALEX All (CDSPortal) Send to within arcsec The VizieR photometry tool allows for easy visualization of photometry points extracted around the Simbad position from photometry-enabled catalogues in VizieR. The search radius has to be specified by the user. It is currently limited to a maximum of 30 arcsec. It depends mostly on the precision or quality of the coordinates (SIMBAD and VizieR catalogs), the resolution of the images from which the sources were extracted, source extent, and source crowding. Suggestions are: crowded field: 0.5 to 1.5 arcsec, 3 arcsec otherwise; uncertain coordinates (SIMBAD quality E or coordinates without reference): 5 to 30 arsec (risky!).

CPD-63 2495	HESS J1302-638	THA 17-8	XMMOM J130247.7-635008
AKARI-IRC-V1 J1302480-635009	INTREF 538	TIC 439164152	[GM76] 259
ALS 2883	LLNS 9661	TYC 8997-1597-1	[KRL2007b] 130
AX J1302-638	LS 2883	UCAC2 3710789	[L68] 195
4FGL J1302.9-6349	2MASS J13024765-6350085	UCAC4 131-076808	[OKM2018] SWIFT J1302.3-6385
3FHL J1303.0-6350	MSX6C G304.1845-00.9916	uvby98 -006302495	[VDD70] Cen-Mus 1
GEN# -0.06302495	PSR J1302-6350	WISEA J130247.65-635008.6	AAVSO 1256-63
GSC 08997-01597	PSR B1259-63	WISE J130247.65-635008.6	Gaia DR3 5862299960127967488
Hbg 757	SSTGLMC G304.1836-00.9916	WRAY 15-1053	Gaia DR1 5862299955795862144
Hen 3-852	TeV J1302-638	2XMM J130247.6-635008	Gaia DR2 5862299960127967488

References (774 between 1850 and 2024) (Total 774) Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system). Follow new references on this object

Collections of Measurements

External archives :

Archive data at HEASARC - High-Energy Astrophysics Science Archive Research Center

Data at NED - NASA/IPAC Extragalactic Database : LS 2883

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