LBCS: The LOFAR Long-Baseline Calibrator Survey

N. Jackson; A. Tagore; A. Deller; J. Moldon; Eskil Varenius; L. Morabito; O. Wucknitz; Tobia Carozzi; John Conway; A. Drabent; A. D. Kapinska; E. Orru; M. Brentjens; R. Blaauw; G. Kuper; J. Sluman; J. Schaap; N. Vermaas; M. Iacobelli; L. Cerrigone; A. Shulevski; S. ter Veen; R. A. Fallows; R. Pizzo; M. Sipior; J. Anderson; I. M. Avruch; M. E. Bell; I. van Bemmel; M. J. Bentum; P. Best; A. Bonafede; F. Breitling; J. W. Broderick; W. N. Brouw; M. Brüggen; B. Ciardi; A. Corstanje; F. De Gasperin; E. de Geus; J. Eisloffel; D. Engels; H. Falcke; M. A. Garrett; J. M. Griessmeier; A. W. Gunst; M. P. van Haarlem; G. Heald; M. Hoeft; J. Horandel; A. Horneffer; H. Intema; E. Juette; M. Kuniyoshi; J. van Leeuwen; G. M. Loose; P. Maat; R. McFadden; D. McKay-Bukowski; J. P. McKean; D. D. Mulcahy; H. Munk; M. Pandey-Pommier; A. G. Polatidis; W. Reich; H. Rottgering; A. Rowlinson; A. M. M. Scaife; D. J. Schwarz; M. Steinmetz; J. Swinbank; S. Thoudam; M. C. Toribio; R. Vermeulen; C. Vocks; R. J. van Weeren; M. W. Wise; S. Yatawatta; P. Zarka

doi:10.1051/0004-6361/201629016

LBCS: The LOFAR Long-Baseline Calibrator Survey
Artikel i vetenskaplig tidskrift, 2016

We outline the LOFAR Long-Baseline Calibrator Survey (LBCS), whose aim is to identify sources suitable for calibrating the highest-resolution observations made with the International LOFAR Telescope, which include baselines > 1000 km. Suitable sources must contain significant correlated flux density (greater than or similar to 50 - 100 mJy) at frequencies around 110-190 MHz on scales of a few hundred milliarcseconds. At least for the 200-300-km international baselines, we find around 1 suitable calibrator source per square degree over a large part of the northern sky, in agreement with previous work. This should allow a randomly selected target to be successfully phase calibrated on the international baselines in over 50% of cases. Products of the survey include calibrator source lists and fringe-rate and delay maps of wide areas-typically a few degrees-around each source. The density of sources with significant correlated flux declines noticeably with baseline length over the range 200-600 km, with good calibrators on the longest baselines appearing only at the rate of 0.5 per sq. deg. Coherence times decrease from 1-3 min on 200-km baselines to about 1 min on 600-km baselines, suggesting that ionospheric phase variations contain components with scales of a few hundred kilometres. The longest median coherence time, at just over 3 min, is seen on the DE609 baseline, which at 227 km is close to being the shortest. We see median coherence times of between 80 and 110 s on the four longest baselines (580-600 km), and about 2 min for the other baselines. The success of phase transfer from calibrator to target is shown to be influenced by distance, in a manner that suggests a coherence patch at 150-MHz of the order of 1 deg. Although source structures cannot be measured in these observations, we deduce that phase transfer is affected if the calibrator source structure is not known. We give suggestions for calibration strategies and choice of calibrator sources, and describe the access to the online catalogue and data products.

radio continuum: galaxies

galaxies: active

instrumentation: interferometers

techniques: interferometric

surveys

Författare

N. Jackson

University of Manchester

A. Tagore

University of Manchester

A. Deller

Netherlands Institute for Radio Astronomy (ASTRON)

J. Moldon

University of Manchester

Netherlands Institute for Radio Astronomy (ASTRON)

Eskil Varenius

Chalmers, Rymd- och geovetenskap, Radioastronomi och astrofysik

Forskning Andra publikationer

L. Morabito

Universiteit Leiden

O. Wucknitz

Max Planck-institutet

Tobia Carozzi

Chalmers, Rymd- och geovetenskap, Radioastronomi och astrofysik

Forskning Andra publikationer

John Conway

Chalmers, Rymd- och geovetenskap, Onsala rymdobservatorium

Forskning Andra publikationer

A. Drabent

Tháringer Landessternwarte Tautenburg

A. D. Kapinska

University of Portsmouth

University of Western Australia

ARC Centre of Excellence for All-sky Astrophysics (CAASTRO)

E. Orru

Netherlands Institute for Radio Astronomy (ASTRON)

M. Brentjens

Netherlands Institute for Radio Astronomy (ASTRON)

R. Blaauw

Netherlands Institute for Radio Astronomy (ASTRON)

G. Kuper

Netherlands Institute for Radio Astronomy (ASTRON)

J. Sluman

Netherlands Institute for Radio Astronomy (ASTRON)

J. Schaap

Netherlands Institute for Radio Astronomy (ASTRON)

N. Vermaas

Netherlands Institute for Radio Astronomy (ASTRON)

M. Iacobelli

Netherlands Institute for Radio Astronomy (ASTRON)

L. Cerrigone

Netherlands Institute for Radio Astronomy (ASTRON)

A. Shulevski

Netherlands Institute for Radio Astronomy (ASTRON)

S. ter Veen

Netherlands Institute for Radio Astronomy (ASTRON)

R. A. Fallows

Netherlands Institute for Radio Astronomy (ASTRON)

R. Pizzo

Netherlands Institute for Radio Astronomy (ASTRON)

M. Sipior

Netherlands Institute for Radio Astronomy (ASTRON)

J. Anderson

Deutsches GeoForschungsZentrum (GFZ)

I. M. Avruch

Rijksuniversiteit Groningen

Netherlands Institute for Space Research (SRON)

M. E. Bell

CSIRO Astronomy and Space Science

I. van Bemmel

Joint Institute for VLBI in Europe (JIVE)

M. J. Bentum

Universiteit Twente

Netherlands Institute for Radio Astronomy (ASTRON)

P. Best

University of Edinburgh

A. Bonafede

Universität Hamburg

F. Breitling

Astrophysikalisches Institut Potsdam

J. W. Broderick

Netherlands Institute for Radio Astronomy (ASTRON)

W. N. Brouw

Rijksuniversiteit Groningen

Netherlands Institute for Radio Astronomy (ASTRON)

M. Brüggen

Universität Hamburg

B. Ciardi

Max Planck-institutet

A. Corstanje

Radboud Universiteit

F. De Gasperin

Universiteit Leiden

E. de Geus

SmarterVision BV

Netherlands Institute for Radio Astronomy (ASTRON)

J. Eisloffel

Max Planck-institutet

D. Engels

Universität Hamburg

H. Falcke

Radboud Universiteit

Netherlands Institute for Radio Astronomy (ASTRON)

M. A. Garrett

Netherlands Institute for Radio Astronomy (ASTRON)

Universiteit Leiden

J. M. Griessmeier

Universite d'Orleans

A. W. Gunst

Netherlands Institute for Radio Astronomy (ASTRON)

M. P. van Haarlem

Netherlands Institute for Radio Astronomy (ASTRON)

G. Heald

Netherlands Institute for Radio Astronomy (ASTRON)

Rijksuniversiteit Groningen

CSIRO Astronomy and Space Science

M. Hoeft

Tháringer Landessternwarte Tautenburg

J. Horandel

Radboud Universiteit

A. Horneffer

Max Planck-institutet

H. Intema

Universiteit Leiden

National Radio Astronomy Observatory Socorro

E. Juette

Ruhr-Universität Bochum

M. Kuniyoshi

National Astronomical Observatory of Japan

J. van Leeuwen

Netherlands Institute for Radio Astronomy (ASTRON)

Universiteit Van Amsterdam

G. M. Loose

Netherlands Institute for Radio Astronomy (ASTRON)

P. Maat

Netherlands Institute for Radio Astronomy (ASTRON)

R. McFadden

Netherlands Institute for Radio Astronomy (ASTRON)

D. McKay-Bukowski

Sodankyla Geophysical Observatory

Rutherford Appleton Laboratory

J. P. McKean

Netherlands Institute for Radio Astronomy (ASTRON)

Rijksuniversiteit Groningen

D. D. Mulcahy

University of Manchester

H. Munk

Radboud Universiteit

Netherlands Institute for Radio Astronomy (ASTRON)

M. Pandey-Pommier

Observatoire de Lyon

A. G. Polatidis

Netherlands Institute for Radio Astronomy (ASTRON)

W. Reich

Max Planck-institutet

H. Rottgering

Universiteit Leiden

A. Rowlinson

Netherlands Institute for Radio Astronomy (ASTRON)

Universiteit Van Amsterdam

A. M. M. Scaife

University of Manchester

D. J. Schwarz

Universität Bielefeld

M. Steinmetz

Astrophysikalisches Institut Potsdam

J. Swinbank

Princeton University

S. Thoudam

Radboud Universiteit

M. C. Toribio

Netherlands Institute for Radio Astronomy (ASTRON)

Universiteit Leiden

R. Vermeulen

Netherlands Institute for Radio Astronomy (ASTRON)

C. Vocks

Astrophysikalisches Institut Potsdam

R. J. van Weeren

Harvard-Smithsonian Center for Astrophysics

M. W. Wise

Universiteit Van Amsterdam

Netherlands Institute for Radio Astronomy (ASTRON)

S. Yatawatta

Netherlands Institute for Radio Astronomy (ASTRON)

P. Zarka

LESIA - Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique

Astronomy and Astrophysics

0004-6361 (ISSN) 1432-0746 (eISSN)

Vol. 595 Art no A86- A86

Advanced Radio Astronomy in Europe (RADIONET3)

Europeiska kommissionen (FP7), 2012-01-01 -- 2015-12-31.

Visa projekt

Ämneskategorier

Astronomi, astrofysik och kosmologi

DOI

10.1051/0004-6361/201629016

Publikationsdata kopplat till DOI

Mer information

Senast uppdaterat

2019-09-10

LBCS: The LOFAR Long-Baseline Calibrator Survey Artikel i vetenskaplig tidskrift, 2016

Författare

N. Jackson

A. Tagore

A. Deller

J. Moldon

Eskil Varenius

L. Morabito

O. Wucknitz

Tobia Carozzi

John Conway

A. Drabent

A. D. Kapinska

E. Orru

M. Brentjens

R. Blaauw

G. Kuper

J. Sluman

J. Schaap

N. Vermaas

M. Iacobelli

L. Cerrigone

A. Shulevski

S. ter Veen

R. A. Fallows

R. Pizzo

M. Sipior

J. Anderson

I. M. Avruch

M. E. Bell

I. van Bemmel

M. J. Bentum

P. Best

A. Bonafede

F. Breitling

J. W. Broderick

W. N. Brouw

M. Brüggen

B. Ciardi

A. Corstanje

F. De Gasperin

E. de Geus

J. Eisloffel

D. Engels

H. Falcke

M. A. Garrett

J. M. Griessmeier

A. W. Gunst

M. P. van Haarlem

G. Heald

M. Hoeft

J. Horandel

A. Horneffer

H. Intema

E. Juette

M. Kuniyoshi

J. van Leeuwen

G. M. Loose

P. Maat

R. McFadden

D. McKay-Bukowski

J. P. McKean

D. D. Mulcahy

H. Munk

M. Pandey-Pommier

A. G. Polatidis

W. Reich

H. Rottgering

A. Rowlinson

A. M. M. Scaife

D. J. Schwarz

M. Steinmetz

J. Swinbank

S. Thoudam

M. C. Toribio

R. Vermeulen

C. Vocks

R. J. van Weeren

M. W. Wise

S. Yatawatta

LBCS: The LOFAR Long-Baseline Calibrator Survey
Artikel i vetenskaplig tidskrift, 2016