You may enter a single source name or multiple source names. Multiple source names should each be on a new line. This performs an OR search on the given names.

The source names are the archive are those set by the PIs in the observing script. They will not contain any spaces, and are unlikely to match official catalog names.

The search is case-insensitive.

A sub-string of the source name can be given. If this box is left blank all sources will be searched.

A source name search cannot be combined with a coordinates based search.

You can search by source name OR coordinates, but not both. If both are given, a source name search will take priority.

You may enter a single set of coordinates or multiple sets of coordinates. These should be in J2000 format. Multiple coordinates should be on newlines.

Acceptable formats are:
05 35 17.3 -05 23 28
05 35 17.3-05 23 28
05:35:17.3 -05:23:28
05:35:17.3-05:23:28

A search radius in arcseconds must be provided. To apply a single radius to all listed sources enter this in the Radius box.

For more flexibility when searching multiple positions, an individual radius can be provided for each set of coordinates. Append this to the end of each line following a comma. In this case the Radius box can be left empty.

E.g.
05 35 17.3 -05 23 28, 300
13 29 52.7 +47 11 42.9, 1000

A coordinate search cannot be combined with a source name based search.

This will only search for data where both targets are included in the same file. E.g. a science target with a particular calibrator. The inputs are source names. This search is case insensitive and substrings are acceptable.

The user can provide a specific frequency which must be covered by the spectral window of the data. This is a sky frequency in GHz.

The tuning range in which LO frequency falls. The default is "Any"; other possibilities are "185-270" (230+240 GHz RXs), "250-410" (345+400 GHz RXs), "600-696" (600 GHz RX). This can be used to narrow down data to a given window.

Remember that the LO frequency itself is not included in the observed spectral window. The routine setup with the SWARM correlator often tunes two receivers to the same frequency and aligns them spectrally so this gap is filled. This ensures an unbroken coverage of 8GHz.

Default is all dates. Note that the switch over from ASIC to SWARM happened mid-2016. See here for a detailed breakdown of the dates of the correlator switch-over.

In units of minutes. This is useful for weeding out short observations.

Default is "Any". Be aware that polarization data require special calibration steps. They can be used as non-polarization data but only after the cross-terms have been flagged.

The last name of the Principal Investigator. This search is case insensitive and sub-strings are acceptable.

The SMA project code, e.g. 2014A-S043. This search is case insensitive.