Table Description:
A table of rotation measures derived from the content of lotsspol.spectra. This is supposed to be in line with RMTable version 1, https://github.com/CIRADA-Tools/RMTable.
This table is available for ADQL queries and through the TAP endpoint.
Resource Description:
The LOFAR Two Meter Sky Survey LoTSS DR2 (2022A&A...659A...1S) obtained radio data from 27% of the northern sky between 120 and 168 MHz in the year 2014 through 2020. This service publishes polarization spectra of extragalactic radio sources (radio galaxies and blazars) and the rotation measures derived from them. We also give redshifts for all sources. The data has a spatial resolution of 20 arcsec.
For a list of all services and tables belonging to this table's resource, see Information on resource ' Rotation Measures from the LOFAR Two Meter Sky Survey LoTSS DR2'
This table has an associated publication. If you use data from it, it may be appropriate to reference 2023arXiv230107697O (ADS BibTeX entry for the publication) either in addition to or instead of the service reference.
To cite the table as such, we suggest the following BibTeX entry:
@MISC{vo:lotsspol_rmtable, year=2022, title={ Rotation Measures from the {LOFAR} Two Meter Sky Survey {LoTSS} DR2}, author={O'Sullivan, S. and Shimwell, T. W. and Hardcastle, M. J. and Tasse, C. and Heald, G. and Carretti, E. and Brüggen, M. and Vacca, V. and Sobey, C. and C. L. Van Eck and Horellou, C. and Beck, R. and Bilicki, M. and Bourke, S. and Botteon, A. and Croston, J. H. and Drabent, A. and Duncan, K. and Heesen, V. and Ideguchi, S. and Kirwan, M. and Lawlor, L. and Mingo, B. and Nikiel, B. and Wroczyński, J. and Piotrowska, J. and Scaife, A. M. M. and van Weeren, R. J.}, url={http://dc.zah.uni-heidelberg.de/tableinfo/lotsspol.rmtable}, howpublished={{VO} resource provided by the {GAVO} Data Center} }
Sorted alphabetically. [Sort by DB column index]
Name | Table Head | Description | Unit | UCD |
---|---|---|---|---|
b | B | Galactic Latitude | deg | pos.galactic.lat |
beam_maj | Beam_maj | Beam major axis | deg | pos.angResolution;instr.beam;phys.angSize.smajAxis |
beam_min | Beam_min | Beam minor axis | deg | pos.angResolution;instr.beam;phys.angSize.sminAxis |
beam_pa | Beam_pa | Beam position angle | deg | pos.angResolution;instr.beam;pos.posAng |
beamdist | Beamdist | Distance from beam centre (taken as centre of tile) | deg | pos.angDistance;instr.beam |
bzcat_name | Bzcat_name | Blazar source name in the ROMA-BZCAT catalogue (2015Ap&SS.357...75M) | N/A | meta.id.cross |
cat_id | Cat. # | Source ID in catalog | N/A | meta.id;meta.main |
catname | Catname | Name of catalog this was taken from. | N/A | meta.note |
channelwidth | Channelwidth | Typical channel width | Hz | em.freq;instr.bandwidth |
complex_flag | Complex_flag | Faraday complexity flag | N/A | meta.code |
complex_test | Complex_test | Faraday complexity metric | N/A | meta.note |
datalink | Spectrum | Datalink for the spectrum | N/A | meta.ref.url |
dataref | Dataref | Data references | N/A | meta.bib.bibcode |
dec | Dec | Declination [ICRS] of the polarised emission at epoch (this will often be an one extremity of the radio source). | deg | pos.eq.dec;meta.main |
dec_centre | Dec_centre | Dec of field centre | deg | pos.eq.dec;obs.field |
dec_dr2 | Dec_dr2 | LoTSS DR2 Dec of the centroid of the total radio intensity using pyBDSF. | deg | pos.eq.dec |
dec_nvss | Dec_nvss | Dec of the object in NVSS | deg | pos.eq.dec |
e_dec_dr2 | E_dec_dr2 | Error in dec_dr2 | deg | stat.error;pos.eq.dec |
e_ra_dr2 | E_ra_dr2 | Error in ra_dr2 | deg | stat.error;pos.eq.ra |
e_total_flux_dr2 | E_total_flux_dr2 | Error in total_flux_dr2 | Jy | stat.error;phot.flux;em.radio |
epoch_mjd | Epoch_mjd | Median epoch of observation | d | time.epoch |
field | LoTSS pointing | LoTSS observation pointing name | N/A | meta.id;obs.field |
flux_type | Flux_type | Stokes extraction method | N/A | meta.note |
fracpol | Fracpol | Fractional (linear) polarization | N/A | phys.polarization.linear |
fracpol_err | Fracpol_err | Error in fractional polarization | N/A | stat.error;phys.polarization.linear |
grm | Grm | Average Galactic RM within an aperture of radius 1 degree from the Garching Faraday rotation sky v2. [Note galm] | rad.m**-2 | phys.polarization.rotMeasure |
grmerr | Grmerr | Error in grm. [Note galm] | rad.m**-2 | stat.error;phys.polarization.rotMeasure |
i_nvss | I_nvss | Integrated Stokes I flux density from NVSS | mJy | phot.flux;phys.polarization.stokes.I |
int_time | Int_time | Integration time | s | time.duration;obs.exposure |
ionosphere | Ionosphere | Ionospheric correction method | N/A | meta.note |
l | L | Galactic Longitude | deg | pos.galactic.lon |
l144 | L144 | Spectral luminosity at 144 MHz in the rest frame of the source | W.Hz**-1 | phys.luminosity |
leakage | Leakage | Instrumental leakage estimate | N/A | phys.polarization.linear |
lgz_dec_deg | Lgz_dec_deg | Dec of the host galaxy, mainly from NED. | deg | pos.eq.dec |
lgz_ra_deg | Lgz_ra_deg | RA of the host galaxy, mainly from NED. | deg | pos.eq.ra |
lgz_size | Lgz_size | Largest angular size of the source | arcsec | phys.angsize;stat.max |
linearsize_kpc | Linearsize_kpc | Projected largest linear size | kpc | phys.size |
madfpol | Madfpol | Median absolute deviation of degree of polarization in the originating pointing (percent). | N/A | stat.mad;phys.polarization |
madrm | Madrm | Median absolute deviation of RM in the originating pointing. | rad.m**-2 | stat.mad;phys.polarization.rotMeasure |
maj_dr2 | Maj_dr2 | Semimajor axis of the radio emission | arcsec | phys.angSize.smajAxis |
maxfreq | Maxfreq | Highest frequency | Hz | em.freq;stat.max |
medfpol | Medfpol | Median degree of polarization in the originating pointing (percent). | N/A | phys.polarization;stat.median |
medrm | Medrm | Median RM in the originating pointing. | rad.m**-2 | phys.polarization.rotMeasure;stat.median |
min_dr2 | Min_dr2 | Semiminor axis of the radio emission | arcsec | phys.angSize.sminAxis |
minfreq | Minfreq | Lowest frequency | Hz | em.freq;stat.min |
nchan | Nchan | Number of channels used in RM derivation | N/A | meta.number;em.bin |
noise_chan | Noise_chan | Typical per-channel noise in Q;U | Jy | stat.error;instr.det.noise |
notes | Notes | Notes | N/A | meta.note |
num_in_field | Num_in_field | Number of polarized sources in the originating pointing. | N/A | meta.number;src |
nvss_rm | Nvss_rm | Rotation measure of the object in NVSS | rad.m**-2 | phys.polarization.rotMeasure |
nvss_rm_err | Nvss_rm_err | Error in rotation measure of the object in NVSS | rad.m**-2 | stat.error;phys.polarization.rotMeasure |
obs_interval | Obs_interval | Interval of observation | d | time.interval |
p_nvss | P_nvss | Average peak polarized intensity from NVSS | mJy | phot.flux;phys.polarization.stokes.I |
pa_dr2 | Pa_dr2 | Position angle of the radio emission, north over west | deg | pos.posAng |
phot_spec_z_best | Phot_spec_z_best | Nature of z_best: 0: phot, 1: spec | N/A | meta.code;src.redshift |
pi_nvss | Pi_nvss | Percent polarization from NVSS | N/A | phys.polarization;arith.ratio |
pol_bias | Pol_bias | Polarization bias correction method | N/A | meta.note |
polint | Pol. intens. | Polarized intensity | Jy | phot.flux.density;phys.polarization.linear |
polint_err | Err. Pol.Int. | Error in Polarised Intensity | Jy | stat.error;phot.flux.density;phys.polarization.linear |
pos_err | Pos_err | Position uncertainty | deg | stat.error;pos |
ra | RA | Right Ascension [ICRS] of the polarised emission at epoch (this will often be an one extremity of the radio source). | deg | pos.eq.ra;meta.main |
ra_centre | Ra_centre | RA of field centre | deg | pos.eq.ra;obs.field |
ra_dr2 | Ra_dr2 | LoTSS DR2 RA of the centroid of the total radio intensity using pyBDSF. | deg | pos.eq.ra |
ra_nvss | Ra_nvss | RA of the object in NVSS | deg | pos.eq.ra |
reffreq_beam | Reffreq_beam | Reference frequency for beam | Hz | em.freq;instr.beam |
reffreq_i | Reffreq_i | Reference frequency for Stokes I | Hz | em.freq;phys.polarization.stokes.I |
reffreq_pol | Reffreq_pol | Reference frequency for polarization | Hz | em.freq;phys.polarization |
rm | Rot. Meas. | Rotation measure | rad.m**-2 | phys.polarization.rotMeasure;meta.main |
rm_err | Err. RM | Total error in RM | rad.m**-2 | stat.error;phys.polarization.rotMeasure |
rm_err_snr | Rm_err_snr | Error in RM from signal to noise ratio only | rad.m**-2 | stat.error;phys.polarization.rotMeasure |
rm_method | Rm_method | RM determination method | N/A | meta.note |
rmsf_fwhm | Rmsf_fwhm | Full-width at half maximum of the RMSF | rad.m**-2 | instr.rmsf;stat.fwhm |
rrm | Rrm | The residual RM after subtraction of the average Galactic RM within an aperture of radius 1 degree (see the grm column). [Note galm] | rad.m**-2 | phys.polarization.rotMeasure;src.net |
separation_nvss | Separation_nvss | Difference between NVSS position and LoTSS DR2 position | arcsec | pos.angDistance |
snr_rmtools_mad | Snr_rmtools_mad | Signal to noise ratio based the peak polarized intensity divided by the estimated noise in the Faraday depth spectrum (where the noise is computed using the median deviation from the median of the polarized intensity, and then correcting to be equivalent to a Gaussian sigma). | N/A | stat.snr;phot.flux;phys.polarization |
source_name_dr2 | ILT name | Official source name assigned by the International LOFAR Telescope ILT. | N/A | meta.id |
telescope | Telescope | Name of Telescope(s) | N/A | instr.tel |
total_flux_dr2 | Total_flux_dr2 | Total radio flux at 144 MHz from pyBDSF. | Jy | phot.flux;em.radio |
x | X | x-pixel coordinate within an individual LoTSS field, ranging from 0 to 3200, for a pixel width of 4.5 arcsec | pixel | pos.cartesian.x;instr.det |
y | Y | y-pixel coordinate within an individual LoTSS field, ranging from 0 to 3200, for a pixel height of 4.5 arcsec | pixel | pos.cartesian.y;instr.det |
z_best | Z_best | Best redshift available from the literature, typically from NED. | N/A | src.redshift |
zphot | Zphot | Photometric redshift derived here from archive photometry (WISE, PanSTARRS, etc; cf. 2021A&A...648A...4D). | N/A | src.redshift.phot |
zphot_err | Zphot_err | Error in zphot | N/A | stat.error;src.redshift.phot |
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.
This is using Version 2 of the Galactic Faraday rotation sky at https://wwwmpa.mpa-garching.mpg.de/ ̃ensslin/research/data/faraday2020.html.