Introduction

This catalogue was founded near September,2003. Our aim was to collect full data on all known pulsars. Thus catalogue includes parameters bound up with radiation in different spectral ranges: radio, optical, extreme ultraviolet, X-ray and gamma. But parameters in radio range and parameters concerned with it were presented in ATNF pulsar catalogue during the begining of this database creating. For this reason we decided that main task of our catalogue would be reflection of complete information on pulsars properties in high energy band. Nevertheless catalogue includes data reflected in ATNF catalogue. We recognize that this information belong to ATNF and refer to it.

Description

The instrument for work with catalog is query form on www.ioffe.ru/astro1/psr-catalog/Catalog.php. It is consists of two parts. The first in the top of the page is a list of the accessible pulsar parameters. Four general parameters are available at once. Other subdivides into several issues:"General and radio parameters of pulsars","Parameters of binary pulsars", "Parameters of optical pulsars","Parameters of euv pulsars"(euv means "extreme ultra violet"), "Parameters of X-ray pulsars" and "Parameters of gamma pulsars". Each of these issues is available after click on corresponding button. In this case you can see the roll of issue parameters. In the roll click on checkbox selects coincident parameter for output. Click on radio box assigns sorting parameter. Also there are two bottons allowing to check or to clear all output parameters from present issue. Again you can deselect all output and sorting parameters of issue by closing it. All accessible pulsar parameters described in the end of this file.

Beneath there is button "VIEW TABLE" for submit your query. After click on this button you get table with results. Action of other nearby buttons the following: "check all parameters" - opens all issues and checks all parameters for output
"clear all parameters" - clears all checkboxes, but not closes issues
"open all parameters" - opens all issues
"close all parameters" - closes all issues

The second part of form allows to set query conditions.
Firstly, it is possible to output not only the value of parameter, but also it's uncertainty in different forms and refer to the source of data. The following forms of uncertainty output are possible:"absolute uncertainty as integer" - an integer number representing uncertainty in last meaning figures of a value. (For example if value is:14.127 then uncertainty equal to 27 means 14.127 ± 0.027 ), "absolute uncertainty in usual look" - in the aforecited example it returns 0.027 and "relative uncertainty".

"Sort by" pull down list allows to set a way of sorting.

In the "User defined variables" division you can set up to four own variables. For this purpose it is necessary to assign variable C1,C2,C3 or C4 by inserting wishful expression in corresponding blank bar. After that it manages as common variable. Expression can contain other variables, following operators: +,-,*,/,% and following functions:
abs(x), acos(x), asin(x), atan(x), ceiling(x)(round fractions up),cos(x),cot(x), exp(x),floor(x)(round fractions down),log(x), log10(x), mod(n,m)(returns the remainder of n divided by m), pi(), pow(x,y), round(x,d), sign(x), sin(x), sqrt(x), tan(x), truncate(x,d)(returns the number x, truncated to d decimals)

The "Condition for values" bar is intended for input of conditions on pulsar parameters. In condition expression you can use: all variables; operators and functions determined in previous indent;comparison operators: =, !=, <=, <, >=, >;logical operators: !, &&, ||. Also available such additional functions:

exist(parameter) returns only records where this parameter exists. Example: exist(p0)
error(parameter) returns only records where absolute uncertainty as integer of this parameter exists. Due to this function you can impose condition on value of parameter absolute uncertainty as integer.Example: error(p0)<10
error Due to this function you can impose condition on absolute uncertainty as integer value of all selected for output parameters.Example: error>10; if p0,p1,DM selected for output, it returns records where error(p0)>10 or error(p1)>10 or error(DM)>10.
abserr(parameter) returns only records where absolute uncertainty of this parameter exists. Due to this function you can impose condition on value of parameter absolute uncertainty.Example: abserr(p0)>0.00001
abserr Due to this function you can impose condition on absolute uncertainty value of all selected for output parameters.Example: abserr>0.00001; if p0,p1,DM selected for output, it returns records where abserr(p0)>0.00001 or abserr(p1)>0.00001 or abserr(DM)>0.00001.
relerr(parameter) returns only records where relative uncertainty of this parameter exists. Due to this function you can impose condition on value of parameter relative uncertainty.Example: relerr(DM)<0.001
relerr Due to this function you can impose condition on relative uncertainty value of all selected for output parameters.Example: relerr<0.001; if p0,p1,DM selected for output, it returns records where relerr(p0)<0.001 or relerr(p1)<0.001 or relerr(DM)<0.001.
refer(parameter) returns only records where reference of this parameter exists. Due to this function you can impose condition on value of parameter reference. Example: refer(DM)=hlk+03 (Caution: don't put quotes around of the reference name)
type(parameter) Returns only records in which Type field string contains parameter. Example: type(X) returns records with type 'XR' or 'AXP'.
assoc(parameter) Returns only records in which Assoc field string contains parameter. Example: assoc(SNR) returns records describing SNR's.
rtelescope(parameter) Returns only records in which RTelescope field string contains parameter. Example: rtelescope(Are) returns records with radio telescope 'Arecibo'.
xtelescope(parameter) Returns only records in which XTelescope field string contains parameter. Example: rtelescope(Bep) returns records with x-ray telescope 'Beppo-SAX'.

"Pulsars names" textarea enables to select pulsars with wishful names. It is possible to enter several names divided by comma,semicolon,space or enter. Also it is possible to use symbols '?' that matches any character one times and '*' that matches any character zero or more times. Example: b0833-4?,*17. Pull down list in the right of textarea allows to select kind of names .

Last division allows to select pulsars from circular area. For this purpose it is necessary to set centre coordinates and radius. If radius didn't set then by default it is considered equal 180 degrees. The acceptable kind of centre coordinates depends on value of pull down list taking in the top of division. In the case of 'J2000 coordinates' it is HH:MM:SS.sss in range from 00:00:00.00 to 23:59:59.9(9) for right ascension and sDD:MM:SS.sss in range from -90:00:00 to +90:00:00 for declination.In the case of 'J2000 coordinates in degrees' it is DD.ddd in range from 00.00 to 359.9(9) for right ascension and sDD.ddd in range from -90.00 to +90.00 for declination. In the case of 'Galactic coordinates' it is DD.ddd in range from 00.00 to 359.9(9) for longitude l and sDD.ddd in range from -90.00 to +90.00 for latitude b. Also here you can include to output parameters pulsar distance from centre of the circle.

In the bottom of the query form there is "VIEW TABLE" button. It's action completely coincides with action of the same button on the top of the form. "clear all conditions" button clears all conditions from the second part of the query form.

Pulsar parameters
General and radio parameters of pulsars
Name Pulsar name
JName Pulsar name based on J2000 coordinates
Comments Comments
Spectrum Reference to the spectrum of pulsar
RA Right ascension(J2000)
Decl Declination(J2000)
RAD Right ascension(J2000) in degrees
DeclD Declination(J2000) in degrees
El Eliptic longitude
Eb Ecliptic latitude
l Galactic longitude
b Galactic latitude
PosEp Epoch at which the position day is measured
PMRA Proper motion in right ascension
PMdecl Proper motion in declination
PMEl Proper motion in ecliptic longitude
PMEb Proper motion in ecliptic latitude
PM Total proper motion
Vt Transverse velocity based on D
P0 Barycentric period of the pulsar
P1 Time derivative of barycentric period
P1i Period derivative corrected for proper motion effect
F0 Barycentric rotation frequency
F1 Time derivative of barycentric rotation frequency
F2 Second time derivative of barycentric rotation frequency
F3 Third time derivative of barycentric rotation frequency
PerEp Epoch of period or frequency
DM Dispersion measure
DM1 First time derivative of dispersion measure
DMsinb DispersionMeasure*sin(Galactic latitude)
RM Rotation measure
W50 Width of pulse at 50% of peak
W10 Width of pulse at 10% of peak
Tsc Temporal broadening of pulses at 1 GHz due to interstellar scatter
D Best estimate of the pulsar distance
Ddm Distance based on the Taylor & Cordes electron density model
p Annual parallax
p Annual parallax
X X-Distance in X-Y-Z Galactic coordinate system
Y Y-Distance in X-Y-Z Galactic coordinate system
Z Distance from galactic plane, based on Distance
S400 Mean flux density at 400 MHz
L400 Radio luminosity at 400 MHz
S1400 Mean flux density at 1400 MHz
L1400 Radio luminosity at 1400 MHz
SpI Measured spectral index
Edot Spin down energy loss rate
Edoti Spin down energy loss rate from corrected P1
F Energy flux at the Sun
Age Spin down age
Agei Spin down age from corrected P1
Bs Surface magnetic flux density
Bsi Surface magnetic flux density from corrected P1
Blc Magnetic field at light cylinder
Nglitch Number of glitches observed for the pulsar
Discovery Telescope that discovered the pulsar
Date Date of discovery publication
RTelescope Radio telescopes observed pulsar
Assoc Objects associated with pulsar
Type Type of pulsar

Parameters of binary pulsars
BinaryType Type of binary pulsar
T0 Epoch of periastron
PB Binary period of pulsar
A1 Projected semi-major axis of orbit
OM Longitude of periastron
Ecc Eccentricity
Tasc Epoch of ascending node
Eps1 Eccentricity * sin(Longitude of periastron)
Eps2 Eccentricity * cos(Longitude of periastron)
MinMass Minimum companion mass assuming i=90 degrees and neutron star mass is 1.35 M0
MedMass Median companion mass assuming i=60 degrees

Parameters of optical pulsars
OptSpectr Reference for synthetical spectrum at optical wavelengths
Ebv Best estimation of color excess
FUV_Fmeas Measured flux density at far ultraviolet
FUV_Fdered Dereddened flux density at far ultraviolet
FUV_Range FWHM limits and pivot wavelength of FUV band
NUV_Fmeas Measured flux density at near ultraviolet
NUV_Fdered Dereddened flux density at near ultraviolet
NUV_Range FWHM limits and pivot wavelength of NUV band
U_Fmeas Measured flux density at U band
U_Fdered Dereddened flux density at U band
U_Range FWHM limits and pivot wavelength of U band
B_Fmeas Measured flux density at B band
B_Fdered Dereddened flux density at B band
B_Range FWHM limits and pivot wavelength of B band
V_Fmeas Measured flux density at V band
V_Fdered Dereddened flux density at V band
V_Range FWHM limits and pivot wavelength of V band
R_Fmeas Measured flux density at R band
R_Fdered Dereddened flux density at R band
R_Range FWHM limits and pivot wavelength of R band
Halfa_Fmeas Measured flux density at Halfa band
Halfa_Fdered Dereddened flux density at Halfa band
Halfa_Range FWHM limits and pivot wavelength of Halfa band
I_Fmeas Measured flux density at I band
I_Fdered Dereddened flux density at I band
I_Range FWHM limits and pivot wavelength of I band
J_Fmeas Measured flux density at J band
J_Fdered Dereddened flux density at J band
J_Range FWHM limits and pivot wavelength of J band
H_Fmeas Measured flux density at H band
H_Fdered Dereddened flux density at H band
H_Range FWHM limits and pivot wavelength of H band
K_Fmeas Measured flux density at K band
K_Fdered Dereddened flux density at K band
K_Range FWHM limits and pivot wavelength of K band
SpIopt Spectral index in optical band
Fit Fit of powerlaw in optical band
Freq0 Central frequency in powerlaw fit

Parameters of extreme ultraviolet pulsars
NhEuv Column density of neutral hydrogen
Lex_Fmeas Measured flux density at Lexan/boron band
Lex_Fdered Dereddened flux density at Lexan/boron band
Lex_Range 10% passband limits and pivot wavelength of Lexan/boron band
ALC_Fmeas Measured flux density at Aluminium/carbon band
ALC_Fdered Dereddened flux density at Aluminium/carbon band
ALC_Range 10% passband limits and pivot wavelength of Aluminium/carbon band

Parameters of X-ray pulsars
Model Appropriate model of fit
NhXray Column density of neutral hydrogen
FitBand Range of spectrum fit
Dist Distance accepted in the given model
kT Temperature in blackbody fit
R Radius in blackbody fit
kTcup Temperature of polar cup in blackbody fit
Rcup Radius of polar cup in blackbody fit
SpIxray Spectral index of power-law fit
Fit1 Normalization at 1keV of power-law fit
FluxBand Range of unabsorbed flux
Flux Unabsorbed flux in the given range
BetterModel Model, that fits spectrum better
XTelescope Xray telescopes observed pulsar

Parameters of gamma pulsars
Detector_soft Detector observed pulsar in soft gamma rays
SpI_soft Spectral index in soft gamma rays
E0_soft Energy at which the normalization is evaluated in soft gamma rays
Fit_soft Fit coefficient in soft gamma rays
Range_soft Energy limits in soft gamma rays
Flux_soft Flux in given limits in soft gamma rays
Detector_medium Detector observed pulsar in medium gamma rays
SpI_medium Spectral index in medium gamma rays
E0_medium Energy at which the normalization is evaluated in medium gamma rays
Fit_medium Fit coefficient in medium gamma rays
Range_medium Energy limits in medium gamma rays
Flux_medium Flux in given limits in medium gamma rays
Detector_hard Detector observed pulsar in hard gamma rays
SpI_hard Spectral index in hard gamma rays
E0_hard Energy at which the normalization is evaluated in hard gamma rays
Fit_hard Fit coefficient in hard gamma rays
Range_hard Energy limits in hard gamma rays
Flux_hard Flux in given limits in hard gamma rays

Parameters of nebula pulsars
All data are taken from Roberts, M.S.E., 2004, `The Pulsar Wind Nebula Catalog (March 2005 version)', McGill University, Montreal, Quebec, Canada (available on the World-Wide-Web at "http://www.physics.mcgill.ca/~pulsar/pwncat.html")
PWN_GName GName of PWN
PWN_other_names other names of PWN
PWN_size size of PWN in pc
PWN_Edot 10^PWN_Edot is full luminosity of PWN (in erg/sec)

Angles
R93 values are taken from Rankin J.M., Astrophysical Journal Supplement Series, V. 85, p. 145-161 (1993)
MB values are taken from I.F. Malov "Radiopulsars", M. "Nauka" 2004 (in Russian)
Angle_R93_Wc The radio impulse width in degrees. It is taken from J.M. Rankin (1993).
Angle_R93_Wcap The angular size of polar cap in degrees (defined by width of radio impulse) It is taken from J.M. Rankin (1993).
Angle_R93_alpha The inclination angle (angle between magnetic momentum and rotation axis) in degrees. It is taken from J.M. Rankin (1993).
Angle_R93_beta The minimal angle between line of sight (direction to observer) and magnetic momentum in degrees. It is taken from J.M. Rankin (1993). The angle between line of sight (direction to observer) and rotation axis is equal to (Angle_R93_alpha + Angle_R93_beta).
Angle_R93_sign_beta Sign of Angle_R93_beta, if it is shown in J.M. Rankin (1993).
Angle_MB_beta1 The inclination angle (angle between magnetic momentum and rotation axis) in degrees. It is taken from table 5 of I.F. Malov "Radiopulsars", M. "Nauka" 2004. At its calculation only impulse width W_{10} is used and assumed beta=dzeta (inclination angle is equal to angle between direction to observer and rotation axis)

Values Angle_MB_beta2* and Angle_MB_dzeta2* are taken from table 6 of I.F. Malov "Radiopulsars", M. "Nauka" 2004. At calculation of these values pulsar width W_{10} and value C are used. Here C -- maximum of (d Psi / d phi) over main impulse, Psi is polarisation angle, phi -- phase of radio impulse. At calculation Angle_MB_beta2n* and Angle_MB_dzeta2n* values it is assumed C < 0. At calculation Angle_MB_beta2p* and Angle_MB_dzeta2p* values it is assumed C > 0.
Angle_MB_beta2p_400 The inclination angle (angle between magnetic momentum and rotation axis) in degrees. Assumed C > 0. Observation is made at 400 MHz.
Angle_MB_beta2n_400 The inclination angle (angle between magnetic momentum and rotation axis) in degrees. Assumed C < 0. Observation is made at 400 MHz.
Angle_MB_beta2p_640 The inclination angle (angle between magnetic momentum and rotation axis) in degrees. Assumed C > 0. Observation is made at 640 MHz.
Angle_MB_beta2n_640 The inclination angle (angle between magnetic momentum and rotation axis) in degrees. Assumed C < 0. Observation is made at 640 MHz.
Angle_MB_beta2p_1600 The inclination angle (angle between magnetic momentum and rotation axis) in degrees. Assumed C > 0. Observation is made at 1600 MHz.
Angle_MB_beta2n_1600 The inclination angle (angle between magnetic momentum and rotation axis) in degrees. Assumed C < 0. Observation is made at 1600 MHz.
Angle_MB_beta2p_2700 The inclination angle (angle between magnetic momentum and rotation axis) in degrees. Assumed C > 0. Observation is made at 2700 MHz.
Angle_MB_beta2n_2700 The inclination angle (angle between magnetic momentum and rotation axis) in degrees. Assumed C < 0. Observation is made at 2700 MHz.
Angle_MB_dzeta2p_400 Angle between line of sight (direction to observer) and rotation axis in degrees. Assumed C > 0. Observation is made at 400 MHz.
Angle_MB_dzeta2n_400 Angle between line of sight (direction to observer) and rotation axis in degrees. Assumed C < 0. Observation is made at 400 MHz.
Angle_MB_dzeta2p_640 Angle between line of sight (direction to observer) and rotation axis in degrees. Assumed C > 0. Observation is made at 640 MHz.
Angle_MB_dzeta2n_640 Angle between line of sight (direction to observer) and rotation axis in degrees. Assumed C < 0. Observation is made at 640 MHz.
Angle_MB_dzeta2p_1600 Angle between line of sight (direction to observer) and rotation axis in degrees. Assumed C > 0. Observation is made at 1600 MHz.
Angle_MB_dzeta2n_1600 Angle between line of sight (direction to observer) and rotation axis in degrees. Assumed C < 0. Observation is made at 1600 MHz.
Angle_MB_dzeta2p_2700 Angle between line of sight (direction to observer) and rotation axis in degrees. Assumed C > 0. Observation is made at 2700 MHz.
Angle_MB_dzeta2n_2700 Angle between line of sight (direction to observer) and rotation axis in degrees. Assumed C < 0. Observation is made at 2700 MHz.
Angle_MB_beta2_av The inclination angle (angle between magnetic momentum and rotation axis) in degrees averaged over frequencies. Assumed C > 0. Angle_MB_beta2_av = (1/4) * ( Angle_MB_beta2p_400 + Angle_MB_beta2p_640 + Angle_MB_beta2p_1600 + Angle_MB_beta2p_2700 )