The ICRF-3: Status, Plans, and Progress on the next generation Celestial Reference Frame
Christopher S., Jacobs
(1)
,
F., Arias
,
D., Boboltz
,
J., Boehm
,
S., Bolotin
,
G. Bourda
(2)
,
P. Charlot
(2)
,
A., de Witt
,
A., Fey
,
R., Gaume
(3)
,
D., Gordon
(4)
,
R., Heinkelmann
,
S., Kudobov
,
S., Lambert
(5, 6)
,
C., Ma
(7)
,
Z., Malkin
(8)
,
A., Nothnagel
,
M., Seitz
,
E., Skurikhina
,
J., Souchay
(9)
,
O., Titov
1
E3S -
Supélec Sciences des Systèmes
2 M2A 2014
3 LCAES - Laboratoire de Chimie Appliquée de l'État Solide
4 Flinders Medical Centre
5 PSE - Paris-Jourdan Sciences Economiques
6 PSE - Paris School of Economics
7 DCSO - Laboratoire de synthèse organique
8 Pulkovo Observatory
9 SYRTE - Systèmes de Référence Temps Espace
2 M2A 2014
3 LCAES - Laboratoire de Chimie Appliquée de l'État Solide
4 Flinders Medical Centre
5 PSE - Paris-Jourdan Sciences Economiques
6 PSE - Paris School of Economics
7 DCSO - Laboratoire de synthèse organique
8 Pulkovo Observatory
9 SYRTE - Systèmes de Référence Temps Espace
F., Arias
- Fonction : Auteur
D., Boboltz
- Fonction : Auteur
J., Boehm
- Fonction : Auteur
S., Bolotin
- Fonction : Auteur
P. Charlot
- Fonction : Auteur
- PersonId : 737919
- IdHAL : patrick-jb-charlot
- ORCID : 0000-0002-9142-716X
- IdRef : 034709614
A., de Witt
- Fonction : Auteur
A., Fey
- Fonction : Auteur
R., Heinkelmann
- Fonction : Auteur
S., Kudobov
- Fonction : Auteur
A., Nothnagel
- Fonction : Auteur
M., Seitz
- Fonction : Auteur
E., Skurikhina
- Fonction : Auteur
O., Titov
- Fonction : Auteur
Résumé
ICRF-3 seeks to improve upon the highly successful ICRF-2. Our goals are to improve the precision, spatial and frequency coverage relative to the ICRF-2 by 2018. This date is driven by the desire to create radio frames that are ready for comparison with the Gaia optical frame. Several specific actions are underway. A collaboration has started to improve at S/X-band precision of the VLBA Calibrator Survey's 2000+ sources which are typically 5 times less precise than the rest of the ICRF-2. S/X-band southern precision improvements are planned from observations with southern antennas such as the AuScope and HartRAO, S. Africa. We seek to improve radio frequency coverage with X/Ka and K-band work. An X/Ka frame of 631 sources now has full sky coverage from the addition of a 2nd southern station in Argentina which should strengthen the southern hemisphere in general. A K-band collaboration has formed with similar coverage and southern precision goals. On the analysis front, special attention will be given to combination techniques both of VLBI catalogs and of multiple data types. Consistency of the CRF with the TRF and EOP is another area of concern. Finally, work is underway to identify and pinpoint sources bright enough in both radio and optical to allow for a robust frame tie between VLBI and Gaia optical frames.
Domaines
Astrophysique [astro-ph]Format du dépôt | Notice |
---|---|
Type de dépôt | Communication dans un congrès |
Titre |
en
The ICRF-3: Status, Plans, and Progress on the next generation Celestial Reference Frame
|
Résumé |
en
ICRF-3 seeks to improve upon the highly successful ICRF-2. Our goals are to improve the precision, spatial and frequency coverage relative to the ICRF-2 by 2018. This date is driven by the desire to create radio frames that are ready for comparison with the Gaia optical frame. Several specific actions are underway. A collaboration has started to improve at S/X-band precision of the VLBA Calibrator Survey's 2000+ sources which are typically 5 times less precise than the rest of the ICRF-2. S/X-band southern precision improvements are planned from observations with southern antennas such as the AuScope and HartRAO, S. Africa. We seek to improve radio frequency coverage with X/Ka and K-band work. An X/Ka frame of 631 sources now has full sky coverage from the addition of a 2nd southern station in Argentina which should strengthen the southern hemisphere in general. A K-band collaboration has formed with similar coverage and southern precision goals. On the analysis front, special attention will be given to combination techniques both of VLBI catalogs and of multiple data types. Consistency of the CRF with the TRF and EOP is another area of concern. Finally, work is underway to identify and pinpoint sources bright enough in both radio and optical to allow for a robust frame tie between VLBI and Gaia optical frames.
|
Auteur(s) |
Christopher S., Jacobs
1
, F., Arias
, D., Boboltz
, J., Boehm
, S., Bolotin
, G. Bourda
2
, P. Charlot
2
, A., de Witt
, A., Fey
, R., Gaume
3
, D., Gordon
4
, R., Heinkelmann
, S., Kudobov
, S., Lambert
5, 6
, C., Ma
7
, Z., Malkin
8
, A., Nothnagel
, M., Seitz
, E., Skurikhina
, J., Souchay
9
, O., Titov
1
E3S -
Supélec Sciences des Systèmes
( 123689 )
- Plateau du Moulon - 3 rue Joliot-Curie - 91192 GIF-SUR-YVETTE CEDEX
- France
2
M2A 2014
( 391836 )
-
- France
3
LCAES -
Laboratoire de Chimie Appliquée de l'État Solide
( 3198 )
- 11, rue Pierre et Marie Curie 75231 - Paris Cedex 05
- France
4
Flinders Medical Centre
( 142306 )
- Bedford Park, Adelaide 5042
- Australie
5
PSE -
Paris-Jourdan Sciences Economiques
( 139754 )
- 48 boulevard Jourdan 75014 Paris
- France
6
PSE -
Paris School of Economics
( 301309 )
- 48 boulevard Jourdan 75014 Paris
- France
7
DCSO -
Laboratoire de synthèse organique
( 1169 )
- bat. des laboratoires Route de Saclay 91128 PALAISEAU CEDEX
- France
8
Pulkovo Observatory
( 65945 )
- St. Petersburg 196140, Russia
- Russie
9
SYRTE -
Systèmes de Référence Temps Espace
( 1365 )
- 61 Av de l'Observatoire 75014 PARIS
- France
|
Langue du document |
Anglais
|
Vulgarisation |
Non
|
Actes |
Non
|
Comité de lecture |
Oui
|
Invité |
Non
|
Audience |
Internationale
|
Date de publication |
2014-03
|
Titre du congrès |
8th IVS General Meeting, Shanghai, China, 2-7 March 2014
|
Date début congrès |
2014-03-02
|
Ville |
Shanghai
|
Pays |
Chine
|
Domaine(s) |
|
Mots-clés |
en
AGN, quasar, ICRF-3, astrometry, VLBI, X/Ka-band, K-band, S/X-band, Gaia, interferometry, ICRF, Celestial Reference Frame
|
ADS Id | 2014ivs..confE...1J |
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