Rev. 01 ECO 37-232 Description Author Initial Release Approved R. Vanderspek Date 3/26/2015 Massachusetts Institute of Technology Kavli Institute for Astrophysics and Space Research (MKI) TESS Instrument Handbook Dwg. No. 37-19501 Revision 01 February 1, 2015 MKI 37-19501 Page 1 of 16 Revision 01 Table of Contents 1.1 1.2 1.3 Introduction ............................................................................................................................................... 5 Purpose and Scope ...............................................................................................................................................5 Intended Audience ...............................................................................................................................................5 Reference Documents .........................................................................................................................................5 Introduction to TESS ................................................................................................................................ 6 2.1 2.2 2.3 2.4 2.5 Mission Overview..................................................................................................................................................6 Observations...........................................................................................................................................................6 Commissioning ......................................................................................................................................................6 Flight System Elements .......................................................................................................................................6 Data Products .........................................................................................................................................................6 Pixels Data ......................................................................................................................................................................... 6 Full-Frame Images ......................................................................................................................................................... 6 Housekeeping Data ........................................................................................................................................................ 6 Instrument Description .......................................................................................................................... 6 3.1 3.2 3.3 Overview ..................................................................................................................................................................6 Instrument Properties ........................................................................................................................................6 Temperature Sensor Placement ......................................................................................................................6 CCD Temperature Sensors .......................................................................................................................................... 7 External Temperature Sensors ................................................................................................................................. 8 Internal Temperature Sensors .................................................................................................................................. 8 Optics and Images..................................................................................................................................... 8 4.1 4.2 4.3 4.4 4.5 4.6 4.7 5.1 5.2 5.3 Camera Design Summary ...................................................................................................................................8 Lens Design .............................................................................................................................................................8 Aberrations .............................................................................................................................................................8 Pixel Response Function ....................................................................................................................................8 Pointing Requirements and Performance ...................................................................................................8 Ghost Images and Scattered Light ...................................................................................................................8 Differential Velocity Aberration ......................................................................................................................8 Detector Properties ................................................................................................................................. 8 CCD Architecture ...................................................................................................................................................9 Imaging Array .................................................................................................................................................................. 9 Frame Store.....................................................................................................................................................................10 Serial Register ................................................................................................................................................................10 Charge Injection ............................................................................................................................................................10 CCD Readout ...................................................................................................................................................................10 Physical Characteristics................................................................................................................................... 12 CCD Mounting ................................................................................................................................................................12 Pixel Dimensions...........................................................................................................................................................12 CCD Performance Summary ........................................................................................................................... 12 Readout Noise ................................................................................................................................................................12 Charge-Transfer Inefficiency ...................................................................................................................................12 Dark Current ...................................................................................................................................................................12 Depletion Depth ............................................................................................................................................................12 Quantum Efficiency......................................................................................................................................................12 CCD Gain ...........................................................................................................................................................................13 MKI 37-19501 Page 2 of 16 Revision 01 Nonlinearity ....................................................................................................................................................................13 Bias Level .........................................................................................................................................................................13 Full Well, Saturation, and Charge Bleeding........................................................................................................13 5.4 Pixel Numbering ................................................................................................................................................. 13 5.5 Signal Content ..................................................................................................................................................... 13 5.6 A/D Converter Differential Non-Linearity ................................................................................................ 13 5.7 Inter-Pixel Response Nonuniformity .......................................................................................................... 13 5.8 Intra-Pixel Response Nonuniformity .......................................................................................................... 13 5.9 Flat Fields.............................................................................................................................................................. 13 5.10 Bad Pixels ........................................................................................................................................................... 14 5.11 Cosmic Rays ....................................................................................................................................................... 14 6.1 6.2 7.1 7.2 7.3 Focal Plane Array ................................................................................................................................... 14 Focal Plane Array Overview ........................................................................................................................... 14 Physical Characteristics................................................................................................................................... 14 Gaps between CCDs .....................................................................................................................................................14 CCD Skew and Aplanarity..........................................................................................................................................14 Focal Plane Electronics ........................................................................................................................ 14 Description ........................................................................................................................................................... 14 Clocks and Sampling ......................................................................................................................................... 14 Other Issues ......................................................................................................................................................... 14 Detector Assembly ................................................................................................................................ 14 9.1 9.2 9.3 Electronic Image Artifacts and Mitigation .................................................................................... 15 10.1 10.2 Type 1 ..................................................................................................................................................................... 15 Type 2 ..................................................................................................................................................................... 15 Type 3 ..................................................................................................................................................................... 15 Instrument Calibration ..................................................................................................................... 15 Ground Measurements Relevant to Flight Calibration ...................................................................... 16 Flat Field ........................................................................................................................................................................16 On-orbit Calibration ....................................................................................................................................... 16 Focal Plane Geometry...............................................................................................................................................16 Pixel Response Function .........................................................................................................................................16 Observing with TESS .......................................................................................................................... 16 11.1 11.2 11.3 11.4 11.5 11.6 Flight Modes and States................................................................................................................................. 16 Table-Based Parameters .............................................................................................................................. 16 Requantization ............................................................................................................................................................16 Huffman Tables ...........................................................................................................................................................16 Commissioning Tables .............................................................................................................................................16 Guide Star Table .........................................................................................................................................................16 Target Table .................................................................................................................................................................16 Miscellaneous Tables................................................................................................................................................16 Default Operating Parameters ................................................................................................................... 16 Times and Time Stamps ................................................................................................................................ 16 Photometric Precision Estimation ............................................................................................................ 16 Mapping Targets to Pixel Coordinates..................................................................................................... 16 Acronyms and Abbreviations.......................................................................................................... 16 MKI 37-19501 Page 3 of 16 Revision 01 References ............................................................................................................................................. 16 MKI 37-19501 Page 4 of 16 Revision 01 Introduction This document is meant to be a full description of the TESS instrument at a level of detail relevant to a knowledgeable user of the instrument. 1.1 Purpose and Scope The purpose of this document is to be a single reference for the nominal operation of the TESS instrument. It is meant to be a handbook, not an encyclopedia: details of design or operation are found in other documents, which are referenced here as needed. 1.2 Intended Audience The intended audience of this document is composed of systems engineers, software engineers, scientists, and operations staff of TESS. 1.3 Reference Documents The following documents are referenced in and provide more detail for this Instrument Handbook. MKI 37-19501 Page 5 of 16 Revision 01 Introduction to TESS 2.1 Mission Overview 2.2 Observations 2.3 Commissioning 2.4 Flight System Elements 2.5 Data Products Pixels Data 2.5.1.1 Targets, Apertures, and Pixel Maps 2.5.1.2 Types of Target 2.5.1.3 Collateral Data Full-Frame Images Housekeeping Data Instrument Description 3.1 Overview 3.2 Instrument Properties 3.3 Temperature Sensor Placement Temperature sensors are mounted to the lens and detector housings to allow monitoring of the thermal properites of the camera. See Figure T. MKI 37-19501 Page 6 of 16 Revision 01 CCD Temperature Sensors A four-terminal temperature sensor (RTD) is provided on the chip. It consists of a long, folded strip of the same metal (AlCu) as used for the first level of device metallization. The device is used by forcing current through two pads and reading the voltage on two different pads. Preliminary data of resistance versus temperature from the CCID77 device are shown in Figure 10. The resistance is linear over the temperature range of the measurement, and the temperature dependence is 2.87 and 2.65 Ω/ ̊C for the two cases. MKI 37-19501 Page 7 of 16 Revision 01 External Temperature Sensors Internal Temperature Sensors Optics and Images 4.1 Camera Design Summary 4.2 Lens Design 4.3 Aberrations 4.4 Pixel Response Function 4.5 Pointing Requirements and Performance 4.6 Ghost Images and Scattered Light 4.7 Differential Velocity Aberration Detector Properties The detectors within the FPA are MIT/LL CCID-80 CCDs. The CCID-80 is backsideilluminated with a depletion depth of 100 µm for good red sensitivity. The following sections describe the properties of the CCID-80. MKI 37-19501 Page 8 of 16 Revision 01 Figure 1: Layout of CCID-80 5.1 CCD Architecture The architecture of the MIT/LL CCID-80 is shown in Figure X. The CCID-80 is a deepdepletion, frame-transfer CCD with a full frame store. Figure 1 depicts the overall architecture of the device. The device has four outputs; each output is associated with an array of 512(H)×2048(V) imaging pixels, for a total imaging area of 2048(H)×2048 (V) imaging pixels. The die size is 31.920(W)×63.955(H) mm TBR for an area of 20.4 cm2. Imaging Array The imaging array for the CCID-80 is comprised of 2048(H)×2048(V) pixels, and the pixel size is 15(H)×15(V) μm.. The active imaging array is surrounded by 10 extra rows and columns each on the left, right, top, and bottom sides to buffer the active imaging array from uneven fields due to the substrate bias. These extra rows allow for photolithography MKI 37-19501 Page 9 of 16 Revision 01 stitching as well as misalignment and vignetting effects of a metal light shield deposited on the device. Some additional features, such as guard rings to enable deep-depletion operation, are not shown. The 10 buffer rows are real pixels, but some of them are masked. The 10 buffer rows above and below the imaging are uncovered, but are not used because of the uneven fields. The 10 buffer columns are not clocked into the serial register, but rather into a “charge sink”, or scupper (not shown in Figure X). They can be ignored for the purposes of this document. Frame Store The frame store for the CCID-80 is divided into two independent halves, labeled “AB” and “CD”. Each section contains 1024(H)×2068(V) pixels, as shown in Figure X. The number of rows in the frame store differs from that of the imaging array because there are two sets of buffer rows, 10 above and 10 below the imaging area; 2048+10+10=2068. The number of rows in the frame-store area in Figure 1 is 2064 because of the presence of four rows between the frame-store region and the serial register. Serial Register The serial or output register allows charge to be directed to either of two output ports at the ends of the register. Moreover, the clock buses are partitioned in a manner that allows the left and right halves of the register to be clocked in opposite directions. Each register has five clock connections, with independent phases 1 and 2 for the left and right halves and a phase 3, which is common to both halves. The output ports are assigned as A, B, C, D from left to right for a back-illuminated part. There are 11 leading columns in all ports of the serial register that can be used as ``black’’ or ``bias’’ pixels. Charge Injection The charge injection register is shown in Figure X. CCD Readout In normal operation, the imaging area will be exposed to the sky for 2.0 seconds, after which the chip is read out. The basic readout process shifts the imaging area rows into the framestore area, a process that takes ~40 msec, The rows are then sequentially read out through ports A, B, C, and D. Ports A and C read out pixels first-pixel-first; ports B and D read out pixels last-pixel first. 5.1.5.1 Number of Rows The number of rows read from the imaging area into the frame-store area is 2078. This is somewhat counterintuitive, because the imaging area consists of 2068 rows. By shifting 2078 rows, the top 10 rows are not real imaging rows, but they are exposed to light during the row-shifting process. These “smear” rows are used in post-processing to account for the fact that starlight is still falling on the pixels as they’re being read out. The result of the shifting of 2078 rows from the imaging area into the frame-store area is the loss of the bottom 10 buffer rows. These rows are partially masked and subject to fringe field effects, and they were never intended for use in high-precision photometry. MKI 37-19501 Page 10 of 16 Revision 01 The shift of the frame-store area into the serial register for readout is more measured: one row is shifted into the serial register, and then the serial register is read out. The readout of the serial register raises the overall readout time of the frame store to the estimated 1.8 s. The frame store rows are shifted 2078 times. As a result, the first 2068 rows are the imaging area rows plus 10 smear columns; the last 10 rows are virtual rows that are subjected to the frame-store readout time and can be used as a measure of the dark current in the CCD. 5.1.5.2 Number of Columns The CCD serial register naturally has 11 pixels between the first active pixel and the readout amplifier; the first 11 pixels are therefore virtual pixels, sometimes referred to as “horizontal underclocks”. These 11 pixels apply to each of the 4 readouts, A-D: thus, clocking out the active pixels and the horizontal underclocks requires 512+11=523 serial shifts. Any pixel clocked after the first 523 will not correspond to an active pixel and is therefore virtual. For TESS, there will be 11 such “horizontal overclocks”, for symmetry reasons. Clocking a full row requires 11+512+11=534 serial shifts. 5.1.5.3 Full-Frame Images The full-frame images created from a single CCD will account for the serial under- and overclocks, vertical smear rows, and vertical virtual rows. GSE and post-processing software will assemble the data clocked from the FPE such that the FFI is a correctlyoriented image. This means that the order of pixels from outputs B and D are reversed, and the horizontal under- and overclocks are collected on the side of the image. The resulting pixel map is shown in Figure 2. Figure 2: The structure of a full-frame image. The imaging area pixels are arranged to represent the physical layout, and the virtual columns are collected to each side of the imaging area. The 10 buffer rows, smear rows, and virtual (overclock) rows are collected at the top of the image. MKI 37-19501 Page 11 of 16 Revision 01 5.2 Physical Characteristics CCD Mounting As shown in Figure 1, the CCID-80 is mounted to a die measuring 32.0 x 64.0 mm (TBR: the text above and in the CCD descriptive document differs). As a result, the edge of the imaging area is inset from the edge of the die by 640 µm parallel to the columns and 600 µm at the top of the imaging area. These gaps contribute to the gap between CCDs in the focal plane array, discussed in Section X. The CCDs are bonded to the die using TBD glue/epoxy. The surface of the CCDs is parallel to the die mounting surface to within TBD µm. The edges of the CCD are parallel to the edges of the die to within TBD µm. There is a maximum TBD µm of “bowing” or “potato-chipping” over the imaging area. Pixel Dimensions The pixels each measure 15 µm x 15 µm x 100 µm deep. The profile of a pixel resembles more a chimney than a box, as shown in Figure X (Figure X will show a TESS chimney vs. a Kepler box). 5.3 CCD Performance Summary The following sections discuss the performance of the CCID-80s used on TESS. For now, nominal values are given; later, either a range of values for the flight units or the exact values for the flight units will be given. Readout Noise The readout noise of the CCID-80 is estimated to be closer to 10 e– than 20 e–. Charge-Transfer Inefficiency The CTE of the CCID-80 has not been measured. Because brighter stars are more sensitive to loss of charge than fainter ones, the signal levels relevant to CTE on TESS are significantly larger than those usually measured, i.e. Fe55 X-rays. There is currently no estimate of the high-signal-level CTE for the CCID-80. Dark Current The dark current in the CCID-80 is estimated to be <1 e–/sec/pixel at a CCD temperature of 40°C, and thus <1 e–/cadence/pixel at flight temperatures. Details TBR. Depletion Depth The thickness of the silicon of the CCID-80 CCDs is 105 µm ± 10 µm (TBR). All CCDs will be fully depleted. Quantum Efficiency The theoretical CCD QE vs wavelength for a 100 µm depletion depth and an operational temperature of -75°C is shown in Figure Y. The QE at low wavelengths is dominated by the performance of the AR coating, as all photons are absorbed within a few tens of microns of the (backside) surface of the CCD. At longer wavelengths, photons penetrate deep into the MKI 37-19501 Page 12 of 16 Revision 01 silicon, and the probability of a photon passing through the silicon entirely becomes nonnegligible, leading to a drop in QE at the red end of the spectrum. The probability of absorption of a photon is a function of the band-gap energy within silicon, which varies with temperature as shown in Equation X. Figure Y shows that the change in CCD temperature affects the shape of the QE curve at the red end of the spectrum. As a result, the measured brightness of stars of different spectral types will vary differently with temperature. CCD Gain The nominal gain of the CCID-80s will be ~7 e–/ADU. Nonlinearity The nonlinearity of the CCDs has not been measured. Bias Level The CCDs electronics will be tuned so that the bias level is near 100 TBR ADU. Full Well, Saturation, and Charge Bleeding The full well of the CCID-80 is estimated to be near 300,000 e–. The charge from a moderately-saturated pixel will bleed into neighboring rows, but will not be lost. Charge loss due to TBR effect begins near 10,000,000 TBR e–. 5.4 Pixel Numbering 5.5 Signal Content Leftover from KIH. Not sure what it is. 5.6 A/D Converter Differential Non-Linearity TBD 5.7 Inter-Pixel Response Nonuniformity Not sure how this differs from flat fields. 5.8 Intra-Pixel Response Nonuniformity This is sub-pixel non-uniformity. TBD. 5.9 Flat Fields Flat fields are a measure of the local pixel-to-pixel nonuniformity in response (PRNU). The PRNU of each CCD will be measured during camera I&T. (Method will be described briefly here). PRNU maps (flat fields) are stored at the POC and used by the SPOC during data processing. Updates to flat field maps are not possible once TESS is on orbit. Need to figure out what goes in here and what goes in 3.3.1.1. MKI 37-19501 Page 13 of 16 Revision 01 5.10 Bad Pixels Bad pixels on the CCD are those that display either 1) no response, 2) anomalously low response, 3) high dark current. Before launch, the number and location of bad pixels on all CCDs will be cataloged (TBD give location in poc database). FFIs will be reviewed regularly to detect the presence of new warm or dead pixels, and the table will be updated. 5.11 Cosmic Rays Oh, where do we start. Big topic, will get to it soon. Focal Plane Array 6.1 Focal Plane Array Overview The TESS FPA consists of four CCDs abutted so as to create an imaging area of ~62 mm on a side, as shown in Figure X. Each CCD is mounted to a SiC pedestal; the four pedestals are mounted to a (what’s the word here?). The wtwh is mounted to XX, cold straps, titanium supports, show pictures. 6.2 Physical Characteristics The ideal FPA would consist of four CCDs abutted directly to one another to form a perfectly flat array of 2048x2048 pixels. The TESS FPA deviates from the ideal; the following sections describe the deviations and the means to minimize them. Gaps between CCDs Because the CCD is inset from the edge of the mounting die, there is a gap of ~1.5-2 mm (100-130 pixels) between the imaging areas of the four CCDs. The gap is not the same for each FPA, and thus will be bookkept separately. CCD Skew and Aplanarity Mounting method allows fine tuning of skew and aplanarity. Precision of aplanarity mounting is 5 µm TBR. Precision of skew mounting is TBD. Skew and aplanarity measured after assembly and included in PRF (maybe). Focal Plane Electronics 7.1 Description 7.2 Clocks and Sampling 7.3 Other Issues Detector Assembly The FPE+FPA assembly, installed in its housing, is defined as the detector assembly (Figure 3). The CCDs in the FPA are identified as 1-4 based on how they are connected to the FPE. Which CCD is which in the FPA is keyed from the location of the CCD with respect to the vent pipe shown in Figure 3, and is described in the FPG_detail memo. MKI 37-19501 Page 14 of 16 Revision 01 Figure 3: TESS Detector Assembly, with CCDs numbered Electronic Image Artifacts and Mitigation 9.1 Type 1 9.2 Type 2 9.3 Type 3 Instrument Calibration Instrument properties relevant to data processing must be calibrated before science operations and, to the extent possible, monitored for changes during flight. The list of calibration products is given in Table X. A subset of instrument properties, indicated in the table, can only be calibrated on the ground. Other properties can be estimated before launch, but must be calibrated during on-orbit commissioning, to account for the effect of the on-orbit instrument environment. Instrument Property Readout noise Flat field Focal Plane Geometry Pixel Response Function System Gain System Linearity CTI Dark Current MKI 37-19501 Description Number Calibration Method TBD TBD Page 15 of 16 Revision 01 10.1 Ground Measurements Relevant to Flight Calibration Flat Field Flat field calibration methods 10.2 On-orbit Calibration Focal Plane Geometry FPG estimation (ground) and flight calibration Pixel Response Function PRF estimation (ground) and flight calibration Observing with TESS 11.1 Flight Modes and States 11.2 Table-Based Parameters Requantization Huffman Tables Commissioning Tables Guide Star Table Target Table Miscellaneous Tables List the tables that are sent once or rarely. Will a bullet list be enough, or does it need a table, or individual “Heading 4” entries? Ed will know. 11.3 Default Operating Parameters 11.4 Times and Time Stamps 11.5 Photometric Precision Estimation 11.6 Mapping Targets to Pixel Coordinates Acronyms and Abbreviations References MKI 37-19501 Page 16 of 16 Revision 01