Coordinates (R.A./DEC) |
Right ascension and declination, epoch 2000. Required format for input: R.A.: hh mm ss.s DEC: ±dd mm ss |
Coordinates (Galactic) |
Galactic longitude and latitude, epoch 2000. Required format for input: Galactic longitude: +xxx.xxx Galactic latitude: ±xx.xxx |
Date (Output of interferometric follow-up observations) |
Date of observation. |
Distance (Output of Cone and List Search) |
Distance to search center in arcseconds. |
Expansion velocity (Input) |
Range of outflow velocities of the shells to select in km/s. The velocity range covered is [0,200] km/s. The outflow velocity vexp is not available for all sources. |
fblue (Output) |
Flux density of the blue-shifted maser peak in Jy. For single-peak masers it contains its flux density. If value is marked by '<', then an upper limit (3σ) for a non-detection is given. |
fred (Output) |
Flux density of the red-shifted maser peak in Jy. It contains the flux density for a single peak maser, if it corresponds to the red-shifted peak in other observations. |
Flux Density (Input) |
Range of flux densities to select in Jansky (Jy). The range covered is [0,1000] Jy. |
Frequency |
Frequency in MHz. |
ID (Output of List Search) |
Row-number of the input table. |
Input Table Format (List Search) |
One source per line. Equatorial coordinates with format: hh mm ss.s ±dd mm ss Galactic coordinates with format: xxx.xxx ±xx.xxx |
Instrument (Output of interferometric follow-up observations) |
Instrument used for observation. |
Maps (Output) |
Link to interferometric observations (Maps) of the source. |
max. Flux (Output of monitoring observations) |
Maximum flux density observed during the monitoring program (in Jansky). If value is marked by '<', then an upper limit (3σ) for a non-detection is given. |
min. Flux (Output of monitoring observations) |
Minimum flux density observed during the monitoring program (in Jansky). |
Mon.(itor) (Output) |
Link to monitoring observations (Monitor) of the source. |
Nmaps (Output of interferometric follow-up observations) |
Number of interferometric observations. |
Observation Start (Output of interferometric follow-up and monitoring observations) |
Date of first interferometric follow-up observation or date of start of the monitoring program. |
Observation End (Output of interferometric follow-up and monitoring observations) |
Date of last interferometric follow-up observation or date of end of the monitoring program. |
Pol.(arization) (Output of interferometric follow-up observations) |
Polarization measurement? (Yes/No). |
Radial velocity (Input) |
Range of radial velocities to select in km/s. The velocity range covered is [-500,500] km/s. The radial velocity vrad is available for all sources. |
Ref.(erences) |
Link to the literature reference of the observation. |
RMS (Output of interferometric follow-up observations) |
Sensitivity given in Jansky. If value is marked by '<', then an upper limit (3σ) for a non-detection is given. |
Search Radius (Input) |
Search radius in arcseconds (maximum is 999 arcsec). |
Source Name (Output) |
Name of the observed source. The designation given in the reference is taken. |
Spectral Type (Output in ASCII file only) |
S: Single peak of maser emission. |
D: Double peak of maser emission. |
I: Irregular spectral profile, multiple emission peaks. |
vrad (Output) |
Radial velocity of the object in km/s. If vrad is not given in the reference it is calculated. The vrad value is always filled. |
vexp (Output) |
Outflow velocity of the shell in km/s. If vexp is not given in the reference it is calculated for non-single peak emission profiles. The vexp value is not always filled. |
vblue (Output) |
Velocity of the blue-shifted maser peak in km/s. For single-peak masers it contains the line velocity. |
vred (Output) |
Velocity of the red-shifted maser peak in km/s. It contains the line velocity for a single peak maser, if it corresponds to the red-shifted peak in other observations. |
Velocity Error (Output as ASCII file) |
Uncertainty of velocity values in km/s. Taken from the velocity resolution of the observation. It is actually a lower limit of the uncertainty, because the lines are usually much broader than the velocity resolution of the observing equipment. |