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F = Astrometry (FGS), |
I = Wide Field Camera 3 (WFP3), |
J = Advanced Camera for Surveys (ACS), |
L = Cosmic Origins Spectrograph (COS), |
N = Near Infrared Camera and Multi-Object Spectrograph (NICMOS), |
O = Space Telescope Imaging Spectrograph (STIS), |
S = Engineering subset data, |
U = Wide Field/Planetary Camera-2 (WFPC2), |
V = High Speed Photometer (HSP), |
W = Wide Field/Planetary Camera (WFPC), |
X = Faint Object Camera (FOC), |
Y = Faint Object Spectrograph (FOS), |
Z = Goddard High Resolution Spectrograph (HRS) |
ppp : Program ID; can be any combination of 3 letters or numbers. There is a unique association between program ID and proposal ID (generally equivalent to the 5-digit HST phase-2 ID),
ss : Observation set ID (generally, but not always, equivalent to the HST phase-2 visit number); any combination of 2 letters or numbers.
oo : Observation number, a.k.a. 'obsnum' (generally unique for each exposure); any combination of 2 letters or numbers.
t : Source of transmission character. At launch, 't' indicated the source of the data: real time (R), tape recorder (T) or merged real time, and taped data (M). Over the years, as data ingestion has changed, the use of 't' has changed. It is simply an indicator of whether or not a better version of the data have been received. The most common sequence for the modern instruments is Q, S, where S is the retransmitted better version. The full set of possible values for 't' are:
B = B-associations generated by CADC and ST-ECF for WFPC2, |
M = Merged real time and tape recorded***, |
N = Retransmitted merged real time and tape recorded*, |
O = Retransmitted real time (letter 'O’)*, |
P = Retransmitted tape recorded*, |
Q = Solid-state recorder (post Servicing Mission-2)**, |
R = Real time (not recorded)***, |
S = Retransmitted solid-state recorder (post Servicing Mission-2)**, |
T = Tape recorded***, |
* Note: Retransmissions between the Data Capture Facility and STScI of better versions.
** Note: Post Servicing Mission-2, all data were Q, except when a better version
was sent from PACOR, and then it was S.
*** Note: For WFPC2, it started as T, changed
to R, then to M a few years later, where it remained until WFPC2 was removed from HST.
'oot' Alternative : Association/product; introduced with NICMOS and STIS. These collections of exposures are created in the pre-archive pipeline and so do not need a transmission source ('t'). The three characters comprising the obsnum ('oo') and the transmission source ('t') are used to distinguish an association from an exposure. The syntax, usually represented as '0nm', allowed for products and subproducts, with '010' being the first product in a given obset (visit) and '011' being the first subproduct for that first product. An example of a subproduct is a NICMOS background exposure. Most products do not have subproducts. With the installation of ACS, the product/subproduct relation was broken as ACS designated the "prime" product, '0n0', as the dither product. Any non-dither ACS or WFC3 product is designated '0n1'.****
Note****: The '0nm' syntax is misleading as products, such as O45P01Z10, OBPW013Z0, and J8ZS0502B exist.
HST data use a number of suffix rules after the 'ipppssoot' name.
Uncalibrated:
Suffix | Description | Used with the following Instrument(s) |
_raw | Raw data | WFC3, ACS, NICMOS, STIS |
_tag | Raw timetag data | STIS |
_lrc | Local rate check image (BOP) | STIS |
_wav | Wavecal | STIS |
_wsp | Wavecal support file | STIS |
_asn | Association file | WFC3, ACS, COS, NICMOS, STIS |
_spt | Telescope, telemetry, engineering | WFC3, ACS, COS, NICMOS, STIS |
_trl | Trailer, processing log | WFC3, ACS, COS, NICMOS, STIS |
_rawacq | Raw data | COS |
.d0h/.d0d | Science data image | FOS, GHRS, WFPC1, WFPC2, FOC |
.q0h/.q0d | Science data quality | FOS, GHRS, WFPC1, WFPC2, FOC |
Calibrated:
Suffix | Description | Used with the following Instrument(s) |
_flt | Calibrated, flat-fielded exposure | WFC3, ACS, STIS |
_crj | Calibrated, CR-rejected, combined | WFC3, ACS, STIS/CCD |
_drz | Calibrated, geometrically-corrected, dither-combined | WFC3 ACS |
_fltsum | Calibrated, flat-field for images | COS |
_x1dsum | Calibrated, combined 1D extracted for spectra | COS |
_x1d | Calibrated 1D spectra from exposures | STIS |
_x2d | Calibrated 2Dspectra/images from exposures | STIS |
_sx1 | Calibrated 1D spectra from combined exposures | STIS |
_sx2 | Calibrated 2D spectra/images from combined exposures | STIS |
_cal | Calibrated exposure | NICMOS |
_mos | Calibrated, combined image | NICMOS |
_sfl | Summed, flat-fields image | STIS/MAMA |
.c0h/.c0d | Calibrated wavelengths | FOS, GHRS |
.c1h/.c1d | Calibrated fluxes | FOS, GHRS |
.cqh/cqd | Calibrated science data quality | FOS, GHRS |
.c0h/.c0d | Calibrated science data | WFPC1, WFPC2, FOC |
.q0h/.q0d | Calibrated science data quality | WFPC1, WFPC2, FOC |
i=F (FGS) |
ppp=05Q |
ss=74 |
oo=07 |
t=M (Merged) |
data_set_name: | type: |
N4RK05010 | PROD-TARG |
N4RK05011 | PROD-BCK1 |
N4RK05012 | PROD-BCK2 |
data_set_name: | type: |
J8AN01011 | PROD-RPT |
Additional examples and information can be found in older, html-versions of the
HST Handbook
and here.
A full list of up-to-date HST Handbooks can be found
here.
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