adsabs/AstroCLIMB huggingface dataset:
Paper: The Cosmic Infrared Background Experiment-2: An Intensity-mapping Optimized Sounding-rocket Payload to Understand the Near-IR Extragalactic Background Light
Authors: Michael Zemcov, James J. Bock, Asantha Cooray, Shuji Matsuura, Dae-Hee Lee, Candice Fazar, Richard M. Feder, Grigory Heaton, Ryo Hashimoto, Phillip Korngut, Toshio Matsumoto, Chi H. Nguyen, Kazuma Noda, Won-Kee Park, Kei Sano, Kohji Takimoto, Toshiaki Arai, Seung-Cheol Bang, Priyadarshini Bangale, Masaki Furutani, Viktor Hristov, Yuya Kawano, Arisa Kida, Tomoya Kojima, Alicia Lanz, Chika Matsumi, Dale Mercado, Shunsuke Nakagawa, Tomoya Nakagawa, Shuta Nakahata, Ryo Ohta, Dorin Patru, Mai Shirahata, Hiroko Suzuki, Aoi Takahashi, Momoko Tamai, Serena Tramm, Kohji Tsumura, Yasuhiro Yamada, Shiang-Yu Wang
Figure caption: High-level block diagram of the CIBER-2 cold and warm electronic systems. The readout is separated into three main units: the cryogenic electronics at left, the ambient-temperature flight electronics in the middle, and the ground station on the right. The fundamental unit of the CIBER-2 detector electronics are the array processing and housekeeping (APHK) board and dual data acquisition system boards. This unit is repeated three times, with one servicing a given detector. These boards address and bias the detector, and then amplify, digitize, and store the data they produce. The readout units connect to the solid state drive (SSD) onboard data storage boards, which together comprise the “warm” (ambient-temperature) electronics enclosed in a red box in the figure. The warm electronics are coupled to the detectors and other cryogenic electronic systems through “cold” (LN2-temperature) harnessing that service the focal plane interface boards (FPBs) and detectors through electrical connectors on the FPAs (see Section 3.4). These components are enclosed in a blue box in the figure. The rocket systems supply power, timed events and attitude control information, and telemetry, indicated by a brown box in the figure. Finally, the ground system is used during preflight testing and during flight to monitor the instrument status and store data, and is enclosed in the green box. The ground station electronics comprise two different systems, one of which handles a single channel of each detector via a telemetered link, and the other parses and stores the full data stream during lab testing and reads from the SSD system following flight.
Paper: The Cosmic Infrared Background Experiment-2: An Intensity-mapping Optimized Sounding-rocket Payload to Understand the Near-IR Extragalactic Background Light
Authors: Michael Zemcov, James J. Bock, Asantha Cooray, Shuji Matsuura, Dae-Hee Lee, Candice Fazar, Richard M. Feder, Grigory Heaton, Ryo Hashimoto, Phillip Korngut, Toshio Matsumoto, Chi H. Nguyen, Kazuma Noda, Won-Kee Park, Kei Sano, Kohji Takimoto, Toshiaki Arai, Seung-Cheol Bang, Priyadarshini Bangale, Masaki Furutani, Viktor Hristov, Yuya Kawano, Arisa Kida, Tomoya Kojima, Alicia Lanz, Chika Matsumi, Dale Mercado, Shunsuke Nakagawa, Tomoya Nakagawa, Shuta Nakahata, Ryo Ohta, Dorin Patru, Mai Shirahata, Hiroko Suzuki, Aoi Takahashi, Momoko Tamai, Serena Tramm, Kohji Tsumura, Yasuhiro Yamada, Shiang-Yu Wang
Figure caption: The thermal window assembly for optical testing, replacing the shutter door as the vacuum seal. During optic testing, GN2 is circulated through the space between the vacuum and positive pressure windows to prevent water vapor in the air from condensing on the vacuum window. In addition, two cold filter windows (top/bottom) simulate the same thermal load as the shutter door on the optics while also filtering out the 300 K infrared emission background from the lab. The filter windows are maintained at ∼225 K and ∼200 K by copper heat straps mounted to the radiation shield, while G10 standoffs isolate them thermally from the cold optics. All windows are AR coated with measured >95% transmission in CIBER-2 wavelength range.
Paper: The Cosmic Infrared Background Experiment-2: An Intensity-mapping Optimized Sounding-rocket Payload to Understand the Near-IR Extragalactic Background Light
Authors: Michael Zemcov, James J. Bock, Asantha Cooray, Shuji Matsuura, Dae-Hee Lee, Candice Fazar, Richard M. Feder, Grigory Heaton, Ryo Hashimoto, Phillip Korngut, Toshio Matsumoto, Chi H. Nguyen, Kazuma Noda, Won-Kee Park, Kei Sano, Kohji Takimoto, Toshiaki Arai, Seung-Cheol Bang, Priyadarshini Bangale, Masaki Furutani, Viktor Hristov, Yuya Kawano, Arisa Kida, Tomoya Kojima, Alicia Lanz, Chika Matsumi, Dale Mercado, Shunsuke Nakagawa, Tomoya Nakagawa, Shuta Nakahata, Ryo Ohta, Dorin Patru, Mai Shirahata, Hiroko Suzuki, Aoi Takahashi, Momoko Tamai, Serena Tramm, Kohji Tsumura, Yasuhiro Yamada, Shiang-Yu Wang
Figure caption: The median dark current maps of arms (a) L, (b) M, and (c) S from data taken with the cold optical shutter closed while the vehicle was horizontal on the launcher. The light leak around the closed optical shutter can be seen in all three arms, producing a noticeable signal in the rectangular LVF region along the bottom of arms (b) M and (c) S. Oriented differently, the brightest corner of the light leak illuminates the upper left border of (a) arm L with a peak illumination around 1.15 e– s–1 and a noticeable shadow under the LVF holder. The scale of the color gradient goes from −0.2 to +0.4 e– s–1 for (a) and from −0.2 to +0.2 e– s–1 for (b) and (c).
Paper: The Cosmic Infrared Background Experiment-2: An Intensity-mapping Optimized Sounding-rocket Payload to Understand the Near-IR Extragalactic Background Light
Authors: Michael Zemcov, James J. Bock, Asantha Cooray, Shuji Matsuura, Dae-Hee Lee, Candice Fazar, Richard M. Feder, Grigory Heaton, Ryo Hashimoto, Phillip Korngut, Toshio Matsumoto, Chi H. Nguyen, Kazuma Noda, Won-Kee Park, Kei Sano, Kohji Takimoto, Toshiaki Arai, Seung-Cheol Bang, Priyadarshini Bangale, Masaki Furutani, Viktor Hristov, Yuya Kawano, Arisa Kida, Tomoya Kojima, Alicia Lanz, Chika Matsumi, Dale Mercado, Shunsuke Nakagawa, Tomoya Nakagawa, Shuta Nakahata, Ryo Ohta, Dorin Patru, Mai Shirahata, Hiroko Suzuki, Aoi Takahashi, Momoko Tamai, Serena Tramm, Kohji Tsumura, Yasuhiro Yamada, Shiang-Yu Wang
Figure caption: (a) Dark current and (b) CDS noise histograms of arm L (red), M (green), and S (blue). A Gaussian fit is overplotted on the data. The mean of each fitted Gaussian (dashed vertical line) is reported as the “peak” dark current and noise, respectively, in Table 2. The spatial distribution of the dark current and noise are shown in Figures 11 and 13, respectively.
Paper: The Cosmic Infrared Background Experiment-2: An Intensity-mapping Optimized Sounding-rocket Payload to Understand the Near-IR Extragalactic Background Light
Authors: Michael Zemcov, James J. Bock, Asantha Cooray, Shuji Matsuura, Dae-Hee Lee, Candice Fazar, Richard M. Feder, Grigory Heaton, Ryo Hashimoto, Phillip Korngut, Toshio Matsumoto, Chi H. Nguyen, Kazuma Noda, Won-Kee Park, Kei Sano, Kohji Takimoto, Toshiaki Arai, Seung-Cheol Bang, Priyadarshini Bangale, Masaki Furutani, Viktor Hristov, Yuya Kawano, Arisa Kida, Tomoya Kojima, Alicia Lanz, Chika Matsumi, Dale Mercado, Shunsuke Nakagawa, Tomoya Nakagawa, Shuta Nakahata, Ryo Ohta, Dorin Patru, Mai Shirahata, Hiroko Suzuki, Aoi Takahashi, Momoko Tamai, Serena Tramm, Kohji Tsumura, Yasuhiro Yamada, Shiang-Yu Wang
Figure caption: Mechanical drawing of the optical shutter assembly. The shutter blade is directly coupled to the main body utilizing a flexural pivot that maintains a constant spring force to swing the shutter to its open or closed positions. Actuation of the shutter is achieved through the use of two solenoid electromagnets, which, when powered, generate a magnetic field that pulls on permanent magnets in the shutter fixture. To reduce stray photon reflections in the closed position, the detector facing side of the blade is blackened with Fineshut KIWAMI, a black polyurethane foam manufactured by Koyo Orient Japan Co., Ltd.
Paper: The Cosmic Infrared Background Experiment-2: An Intensity-mapping Optimized Sounding-rocket Payload to Understand the Near-IR Extragalactic Background Light
Authors: Michael Zemcov, James J. Bock, Asantha Cooray, Shuji Matsuura, Dae-Hee Lee, Candice Fazar, Richard M. Feder, Grigory Heaton, Ryo Hashimoto, Phillip Korngut, Toshio Matsumoto, Chi H. Nguyen, Kazuma Noda, Won-Kee Park, Kei Sano, Kohji Takimoto, Toshiaki Arai, Seung-Cheol Bang, Priyadarshini Bangale, Masaki Furutani, Viktor Hristov, Yuya Kawano, Arisa Kida, Tomoya Kojima, Alicia Lanz, Chika Matsumi, Dale Mercado, Shunsuke Nakagawa, Tomoya Nakagawa, Shuta Nakahata, Ryo Ohta, Dorin Patru, Mai Shirahata, Hiroko Suzuki, Aoi Takahashi, Momoko Tamai, Serena Tramm, Kohji Tsumura, Yasuhiro Yamada, Shiang-Yu Wang
Figure caption: CIBER-2 calibration lamp assembly. (Left panel) The lamp modules for arm S, M, and L each consist of an LED or a tungsten-halogen light source coupled to an optical filter and pinhole to attenuate the intensity to the appropriate level. (Middle panel) The lamp modules are mounted to the calibration lamp assembly with a hemispherical, reflective, granular inner surface that isotropizes the aperture illumination pattern. (Right panel) The calibration lamp assembly is mounted to the back of the telescope’s secondary mirror, and when powered illuminates the lens optics through the Cassegrain hole of the telescope.
Paper: The Cosmic Infrared Background Experiment-2: An Intensity-mapping Optimized Sounding-rocket Payload to Understand the Near-IR Extragalactic Background Light
Authors: Michael Zemcov, James J. Bock, Asantha Cooray, Shuji Matsuura, Dae-Hee Lee, Candice Fazar, Richard M. Feder, Grigory Heaton, Ryo Hashimoto, Phillip Korngut, Toshio Matsumoto, Chi H. Nguyen, Kazuma Noda, Won-Kee Park, Kei Sano, Kohji Takimoto, Toshiaki Arai, Seung-Cheol Bang, Priyadarshini Bangale, Masaki Furutani, Viktor Hristov, Yuya Kawano, Arisa Kida, Tomoya Kojima, Alicia Lanz, Chika Matsumi, Dale Mercado, Shunsuke Nakagawa, Tomoya Nakagawa, Shuta Nakahata, Ryo Ohta, Dorin Patru, Mai Shirahata, Hiroko Suzuki, Aoi Takahashi, Momoko Tamai, Serena Tramm, Kohji Tsumura, Yasuhiro Yamada, Shiang-Yu Wang
Figure caption: The CDS noise maps of arm (a) -L, (b) -M, and (c) -S in e−. Multiple spatial features are visible such as the extra noise in the first column of individual amplifier channel (most prevalent in arm L), the “watermark” feature in arm M, and the noisy amplifier channel 13 in arm S. These features are stable, independent of illumination, and detector specific, so can be removed in a fluctuation analysis.
Paper: The Cosmic Infrared Background Experiment-2: An Intensity-mapping Optimized Sounding-rocket Payload to Understand the Near-IR Extragalactic Background Light
Authors: Michael Zemcov, James J. Bock, Asantha Cooray, Shuji Matsuura, Dae-Hee Lee, Candice Fazar, Richard M. Feder, Grigory Heaton, Ryo Hashimoto, Phillip Korngut, Toshio Matsumoto, Chi H. Nguyen, Kazuma Noda, Won-Kee Park, Kei Sano, Kohji Takimoto, Toshiaki Arai, Seung-Cheol Bang, Priyadarshini Bangale, Masaki Furutani, Viktor Hristov, Yuya Kawano, Arisa Kida, Tomoya Kojima, Alicia Lanz, Chika Matsumi, Dale Mercado, Shunsuke Nakagawa, Tomoya Nakagawa, Shuta Nakahata, Ryo Ohta, Dorin Patru, Mai Shirahata, Hiroko Suzuki, Aoi Takahashi, Momoko Tamai, Serena Tramm, Kohji Tsumura, Yasuhiro Yamada, Shiang-Yu Wang
Figure caption: Cutaway renders and in-context image of the focal plane assembly and its interface to the CIBER-2 optics. The black dashed lines denote surfaces of contact in the exploded views. (a) The dual-band windowpane filter is installed with a pair of spring-loaded tabs going through the aluminum base, while the Invar LVF holder is bolted to this base. Invar was chosen for having similar thermal expansion to the LVF quartz. (b) The FPA is connected to the lens barrel using an adjustable interfacing barrel. (c) Assembled FPA housing interfaced to lens optics and installed for arm L.
Paper: The Cosmic Infrared Background Experiment-2: An Intensity-mapping Optimized Sounding-rocket Payload to Understand the Near-IR Extragalactic Background Light
Authors: Michael Zemcov, James J. Bock, Asantha Cooray, Shuji Matsuura, Dae-Hee Lee, Candice Fazar, Richard M. Feder, Grigory Heaton, Ryo Hashimoto, Phillip Korngut, Toshio Matsumoto, Chi H. Nguyen, Kazuma Noda, Won-Kee Park, Kei Sano, Kohji Takimoto, Toshiaki Arai, Seung-Cheol Bang, Priyadarshini Bangale, Masaki Furutani, Viktor Hristov, Yuya Kawano, Arisa Kida, Tomoya Kojima, Alicia Lanz, Chika Matsumi, Dale Mercado, Shunsuke Nakagawa, Tomoya Nakagawa, Shuta Nakahata, Ryo Ohta, Dorin Patru, Mai Shirahata, Hiroko Suzuki, Aoi Takahashi, Momoko Tamai, Serena Tramm, Kohji Tsumura, Yasuhiro Yamada, Shiang-Yu Wang
Figure caption: Solid model rendering of the deployed baffle and aft end assembly. Panel (a) shows the skin in section with the vacuum door open and the pop-up baffle in the stowed configuration to highlight normally hidden parts of the assembly. Panel (b) shows the deployed pop-up baffle and door with radiation shield covering as it would appear when deployed during astronomical observations.
Paper: The Cosmic Infrared Background Experiment-2: An Intensity-mapping Optimized Sounding-rocket Payload to Understand the Near-IR Extragalactic Background Light
Authors: Michael Zemcov, James J. Bock, Asantha Cooray, Shuji Matsuura, Dae-Hee Lee, Candice Fazar, Richard M. Feder, Grigory Heaton, Ryo Hashimoto, Phillip Korngut, Toshio Matsumoto, Chi H. Nguyen, Kazuma Noda, Won-Kee Park, Kei Sano, Kohji Takimoto, Toshiaki Arai, Seung-Cheol Bang, Priyadarshini Bangale, Masaki Furutani, Viktor Hristov, Yuya Kawano, Arisa Kida, Tomoya Kojima, Alicia Lanz, Chika Matsumi, Dale Mercado, Shunsuke Nakagawa, Tomoya Nakagawa, Shuta Nakahata, Ryo Ohta, Dorin Patru, Mai Shirahata, Hiroko Suzuki, Aoi Takahashi, Momoko Tamai, Serena Tramm, Kohji Tsumura, Yasuhiro Yamada, Shiang-Yu Wang
Figure caption: The best focus measurement of each arm for multiple positions across the array. The data show the radius of the aperture R enclosing 95% of the signal detected by our focusing algorithm plotted as a function of shift from the collimator focus, with the best focus at the minimum of the fitted inverted Gaussian curve. (For these data, the radius enclosing 95% of the encircled energy is tracked with the focusing algorithm instead of the typical 85% due to the changing shape of the PSF.) The focus position at launch was at the collimator focus, illustrated by zero on the plot. The vertical shaded bars illustrate the best focus of that measurement, with the width corresponding to the standard deviation of that parameter of the fit. The horizontal gray shaded region illustrates the mean PSF radius of the best focus measurements with the width corresponding to the standard deviation of those values. At launch, the detectors were at a focus position that was best to minimize the PSF across all array measurement positions.
Paper: The Cosmic Infrared Background Experiment-2: An Intensity-mapping Optimized Sounding-rocket Payload to Understand the Near-IR Extragalactic Background Light
Authors: Michael Zemcov, James J. Bock, Asantha Cooray, Shuji Matsuura, Dae-Hee Lee, Candice Fazar, Richard M. Feder, Grigory Heaton, Ryo Hashimoto, Phillip Korngut, Toshio Matsumoto, Chi H. Nguyen, Kazuma Noda, Won-Kee Park, Kei Sano, Kohji Takimoto, Toshiaki Arai, Seung-Cheol Bang, Priyadarshini Bangale, Masaki Furutani, Viktor Hristov, Yuya Kawano, Arisa Kida, Tomoya Kojima, Alicia Lanz, Chika Matsumi, Dale Mercado, Shunsuke Nakagawa, Tomoya Nakagawa, Shuta Nakahata, Ryo Ohta, Dorin Patru, Mai Shirahata, Hiroko Suzuki, Aoi Takahashi, Momoko Tamai, Serena Tramm, Kohji Tsumura, Yasuhiro Yamada, Shiang-Yu Wang
Figure caption: The measured photocurrent spectra in the LVF for all six fields. The prominent lines in the visible are due to atomic oxygen in the upper atmosphere at altitudes higher than the payload, and possibly molecular oxygen at lower altitudes. At near-infrared wavelengths, there are broad features due to hydroxyl lines with strong time dependence, as seen in the CIBER-1 flights, and stable features possibly due to molecular oxygen. At the long wavelength end, thermal emission probably from the warm part of the rocket skin contributes significantly.
Paper: The Cosmic Infrared Background Experiment-2: An Intensity-mapping Optimized Sounding-rocket Payload to Understand the Near-IR Extragalactic Background Light
Authors: Michael Zemcov, James J. Bock, Asantha Cooray, Shuji Matsuura, Dae-Hee Lee, Candice Fazar, Richard M. Feder, Grigory Heaton, Ryo Hashimoto, Phillip Korngut, Toshio Matsumoto, Chi H. Nguyen, Kazuma Noda, Won-Kee Park, Kei Sano, Kohji Takimoto, Toshiaki Arai, Seung-Cheol Bang, Priyadarshini Bangale, Masaki Furutani, Viktor Hristov, Yuya Kawano, Arisa Kida, Tomoya Kojima, Alicia Lanz, Chika Matsumi, Dale Mercado, Shunsuke Nakagawa, Tomoya Nakagawa, Shuta Nakahata, Ryo Ohta, Dorin Patru, Mai Shirahata, Hiroko Suzuki, Aoi Takahashi, Momoko Tamai, Serena Tramm, Kohji Tsumura, Yasuhiro Yamada, Shiang-Yu Wang
Figure caption: Pointing drift in each arm and field over the flight. This figure shows the drift using all frames in an exposure (circles), and then the drift after excluding the first few frames where the pointing instability is large (squares). Drifts for arm L are shown in red, arm M in green, and arm S in blue. The black box indicates the size of one 4﹩\mathop{.}\limits^{\unicode{x02033}}﹩0 pixel in the CIBER-2 image for comparison. The equivalent optical PSF spot width of each arm are shown as ellipses, and illustrate that the drift in the cut exposures is less than or comparable to the optical beam size.
Paper: The Cosmic Infrared Background Experiment-2: An Intensity-mapping Optimized Sounding-rocket Payload to Understand the Near-IR Extragalactic Background Light
Authors: Michael Zemcov, James J. Bock, Asantha Cooray, Shuji Matsuura, Dae-Hee Lee, Candice Fazar, Richard M. Feder, Grigory Heaton, Ryo Hashimoto, Phillip Korngut, Toshio Matsumoto, Chi H. Nguyen, Kazuma Noda, Won-Kee Park, Kei Sano, Kohji Takimoto, Toshiaki Arai, Seung-Cheol Bang, Priyadarshini Bangale, Masaki Furutani, Viktor Hristov, Yuya Kawano, Arisa Kida, Tomoya Kojima, Alicia Lanz, Chika Matsumi, Dale Mercado, Shunsuke Nakagawa, Tomoya Nakagawa, Shuta Nakahata, Ryo Ohta, Dorin Patru, Mai Shirahata, Hiroko Suzuki, Aoi Takahashi, Momoko Tamai, Serena Tramm, Kohji Tsumura, Yasuhiro Yamada, Shiang-Yu Wang
Figure caption: Measured photocurrent in each field for each band. The measured photocurrent (blue) is compared with the expected contributions from ZL (orange), DGL (green), and ISL (red).
Paper: The Cosmic Infrared Background Experiment-2: An Intensity-mapping Optimized Sounding-rocket Payload to Understand the Near-IR Extragalactic Background Light
Authors: Michael Zemcov, James J. Bock, Asantha Cooray, Shuji Matsuura, Dae-Hee Lee, Candice Fazar, Richard M. Feder, Grigory Heaton, Ryo Hashimoto, Phillip Korngut, Toshio Matsumoto, Chi H. Nguyen, Kazuma Noda, Won-Kee Park, Kei Sano, Kohji Takimoto, Toshiaki Arai, Seung-Cheol Bang, Priyadarshini Bangale, Masaki Furutani, Viktor Hristov, Yuya Kawano, Arisa Kida, Tomoya Kojima, Alicia Lanz, Chika Matsumi, Dale Mercado, Shunsuke Nakagawa, Tomoya Nakagawa, Shuta Nakahata, Ryo Ohta, Dorin Patru, Mai Shirahata, Hiroko Suzuki, Aoi Takahashi, Momoko Tamai, Serena Tramm, Kohji Tsumura, Yasuhiro Yamada, Shiang-Yu Wang
Figure caption: Radial profiles of the stacked PSF for the three arms (L, M, and S, from left to right). The best-fit Gaussian to the core PSF is represented by a red dashed curve. The blue dotted line indicates the radius encircling 85% of the energy, corresponding to the radius of the red circles in Figure 24. The green dotted line marks the half-width at half-maximum of the PSF. The PSF width shown in Figure 26 is defined as the full width at half-maximum.
Paper: The Cosmic Infrared Background Experiment-2: An Intensity-mapping Optimized Sounding-rocket Payload to Understand the Near-IR Extragalactic Background Light
Authors: Michael Zemcov, James J. Bock, Asantha Cooray, Shuji Matsuura, Dae-Hee Lee, Candice Fazar, Richard M. Feder, Grigory Heaton, Ryo Hashimoto, Phillip Korngut, Toshio Matsumoto, Chi H. Nguyen, Kazuma Noda, Won-Kee Park, Kei Sano, Kohji Takimoto, Toshiaki Arai, Seung-Cheol Bang, Priyadarshini Bangale, Masaki Furutani, Viktor Hristov, Yuya Kawano, Arisa Kida, Tomoya Kojima, Alicia Lanz, Chika Matsumi, Dale Mercado, Shunsuke Nakagawa, Tomoya Nakagawa, Shuta Nakahata, Ryo Ohta, Dorin Patru, Mai Shirahata, Hiroko Suzuki, Aoi Takahashi, Momoko Tamai, Serena Tramm, Kohji Tsumura, Yasuhiro Yamada, Shiang-Yu Wang
Figure caption: Bright star centroid images from the C1 band, field 5 single-frame differences. The centroid positions (red crosses) are measured from frame-difference images from the beginning (frame 1–frame 0; left panel), middle (frame 15–frame 14; middle panel), and end (frame 21–frame 20; right panel) of the exposure. The point source wanders by about a beamwidth over the course of an integration due to jitter in the rocket attitude control.
Paper: The Cosmic Infrared Background Experiment-2: An Intensity-mapping Optimized Sounding-rocket Payload to Understand the Near-IR Extragalactic Background Light
Authors: Michael Zemcov, James J. Bock, Asantha Cooray, Shuji Matsuura, Dae-Hee Lee, Candice Fazar, Richard M. Feder, Grigory Heaton, Ryo Hashimoto, Phillip Korngut, Toshio Matsumoto, Chi H. Nguyen, Kazuma Noda, Won-Kee Park, Kei Sano, Kohji Takimoto, Toshiaki Arai, Seung-Cheol Bang, Priyadarshini Bangale, Masaki Furutani, Viktor Hristov, Yuya Kawano, Arisa Kida, Tomoya Kojima, Alicia Lanz, Chika Matsumi, Dale Mercado, Shunsuke Nakagawa, Tomoya Nakagawa, Shuta Nakahata, Ryo Ohta, Dorin Patru, Mai Shirahata, Hiroko Suzuki, Aoi Takahashi, Momoko Tamai, Serena Tramm, Kohji Tsumura, Yasuhiro Yamada, Shiang-Yu Wang
Figure caption: Charge accumulation in a single pixel for each band. CIBER-2 observes each target for ∼50 s (green points), then maneuvers to the next target (blue points). The measured photocurrent for each field is typically reported as the slope of the linear fit to the data (red line), although it is clear that at earlier times the photo flux is changing, likely because of airglow contamination. The detectors are reset before and after each maneuver.
Paper: The Cosmic Infrared Background Experiment-2: An Intensity-mapping Optimized Sounding-rocket Payload to Understand the Near-IR Extragalactic Background Light
Authors: Michael Zemcov, James J. Bock, Asantha Cooray, Shuji Matsuura, Dae-Hee Lee, Candice Fazar, Richard M. Feder, Grigory Heaton, Ryo Hashimoto, Phillip Korngut, Toshio Matsumoto, Chi H. Nguyen, Kazuma Noda, Won-Kee Park, Kei Sano, Kohji Takimoto, Toshiaki Arai, Seung-Cheol Bang, Priyadarshini Bangale, Masaki Furutani, Viktor Hristov, Yuya Kawano, Arisa Kida, Tomoya Kojima, Alicia Lanz, Chika Matsumi, Dale Mercado, Shunsuke Nakagawa, Tomoya Nakagawa, Shuta Nakahata, Ryo Ohta, Dorin Patru, Mai Shirahata, Hiroko Suzuki, Aoi Takahashi, Momoko Tamai, Serena Tramm, Kohji Tsumura, Yasuhiro Yamada, Shiang-Yu Wang
Figure caption: Catalog magnitudes of a star in the Gaia DR3 and 2MASS bands (blue) and the derived magnitudes in the CIBER-2 bands (red). The uncertainties in the CIBER-2 magnitudes were estimated using a Monte Carlo simulation, where catalog photometric errors were propagated through the interpolation. The width of the light blue band indicates the 68% population of interpolations derived from the Monte Carlo simulation.