4. Current NRAO/GBO facility adoption status
This table is a quick summary of the current NRAO/GBO facilities that have started uploading their observation status to the ODS API, and which satellite operators have started utilizing the ODS data for the Telescope Boresight Avoidance (TBA) technique. However, by design, the current NRAO ODS system is already capable of reporting all frequency ranges available to VLA, VLBA (10 stations and High Sensitivity Array), and GBT.
By default, the Data Senders are reporting the nominal frequency range of each designated receiver (as listed for each site below), regardless of whether an observer is using the entire receiver band or not. This ensures the receiver will have full protection from the satellite operators for potential spectral leakage and compression.
Site |
Satellite Downlink |
Sat. Operators adopted ODS |
Effected receiver bands |
Current TBA status |
|---|---|---|---|---|
VLA |
1990-1995 MHz1 |
SpaceX Starlink |
L & S |
ACTIVE since Jan 2025 |
_ |
10.7-12.7 GHz2 |
SpaceX Starlink |
X & Ku |
ACTIVE since Aug 2024 |
VLBA |
1990-1995 MHz |
SpaceX Starlink |
L & S |
ACTIVE since Sep 2025 |
_ |
10.7-12.7 GHz |
SpaceX Starlink |
U |
ACTIVE since Sep 2025 |
_ |
37.5-42.0 GHz3 |
AST SpaceMobile |
Q |
Interim test using Q-band schedule |
GBT |
1990-1995 MHz |
SpaceX Starlink |
S & UWBR |
Under development |
_ |
10.7-12.7 GHz |
SpaceX Starlink |
X & Holography & Ku |
Under test since Oct 2025 |
1 DTC/SCS downlink band by Starlink for T-Mobile. [DTC = Direct to Cell (a.k.a., D2C); SCS = Supplemental Coverage from Space. Both acronym are used interchangeably]
2 Starlink’s broaband internet downlink band
3 SpaceMobile’s proposed V-band downlink band
4.1. Observation modes supported by ODS reporting
Facility |
Observing mode |
Sub mode |
Special mode |
ODS reporting |
|---|---|---|---|---|
VLA |
Spectral Line |
Covered by main VLA Data Sender feature |
||
Continuum |
Covered by main VLA Data Sender feature |
|||
Polarimetry |
Covered by main VLA Data Sender feature |
|||
Subarrays |
Covered by VLA Data Sender as |
|||
Mosaicking and OTF |
Covered by VLA Data Sender otf-mosaic feature |
|||
Moving Objects |
Covered by VLA Data Sender Non-Sidereal target feature |
|||
Solar Observing |
Covered by main VLA Data Sender feature |
|||
VLBI at VLA (HSA) |
Covered by VLBA Data Sender as |
|||
Pulsars |
Covered by main VLA Data Sender feature |
|||
Holography |
Point & Shoot |
Not supported currently |
||
Holography |
On the Fly (OTF) |
Not supported currently |
||
Manual scripts |
(many) |
Not supported currently (under development as of Spring 2026) |
||
VLBA |
Spectral Line |
Dual band obs |
Covered by main VLBA Data Sender feature |
|
Continuum |
Dual band obs |
Covered by main VLBA Data Sender feature |
||
GBT |
Spectral Line |
Mapping |
Covered by main GBT Data Sender, under test for X-band |
|
Continuum |
Mapping |
Covered by main GBT Data Sender, under test for X-band |
||
Moving Objects |
Mapping |
Under test for X-band |
||
Radar/ngRadar - transmit |
Not supported currently |
|||
Radar/ngRadar - receive |
Not supported currently |
|||
VLBI at GBT (HSA) |
Covered by VLBA Data Sender as |
|||
Pulsars |
Not supported currently |
|||
Cyclic Spectroscopy (pulsars) |
Not supported currently |
|||
Breakthrough Listen |
Not supported currently |
|||
Baseband (raw voltages) |
Not supported currently |
|||
Manual scripts |
(many) |
Covered by main GBT Data Sender MRMR6 |
4 MRMR = Manual RFI Mitigation Request
4.2. site_id description
Facility |
|
description |
|---|---|---|
VLA |
|
A Configuration (Config.)4 |
|
Config A -> D transition |
|
|
D Config |
|
|
Config D -> C |
|
|
C Config |
|
|
Config C -> B |
|
|
B config |
|
|
Config B -> BnA |
|
|
BnA config reserved exclusively for VLA Sky Survey (VLASS) |
|
|
Config BnA -> A |
|
VLBA |
|
St. Croix – U.S. Virgin Islands |
|
Hancock – New Hampshire |
|
|
North Liberty – Iowa |
|
|
Fort Davis – Texas |
|
|
Los Alamos – New Mexico |
|
|
Pie Town – New Mexico |
|
|
Kitt Peak – Arizona |
|
|
Owens Valley – California |
|
|
Brewster – Washington |
|
|
Mauna Kea – Hawaii |
|
GBT |
|
Green Bank Telescope - WV |
5 For all VLA configuration schedule, see https://public.nrao.edu/vla-configurations/
4.3. Frequency ranges reported by ODS for NRAO/GBO facilities
Facility |
Receiver Name |
|
|
|---|---|---|---|
VLA |
|||
VLBA5 |
P |
290000000.0 |
350000000.0 |
610 |
570000000.0 |
636000000.0 |
|
L |
1060000000.0 |
1840000000.0 |
|
S |
1860000000.0 |
3100000000.0 |
|
C |
3900000000.0 |
7900000000.0 |
|
X |
7660000000.0 |
9040000000.0 |
|
U |
11960000000.0 |
15940000000.0 |
|
K |
20560000000.0 |
25040000000.0 |
|
Q |
41000000000.0 |
45000000000.0 |
|
GBT |
6 The VLBA bands being reported are slightly larger than the nominal bandpass range due to compensating the 3dB roll off at the upper and lower filter band edges.