Resonant Young’s Slit Interferometer for Sensitive Detection of Low-Molecular-Weight Biomarkers by Stefanus Renaldi Wijaya, Augusto Martins, Katie Morris, Steven D. Quinn, Thomas F. Krauss

Subjects: Get full text

Radio Follow-up Observations of SN 2023ixf by Japanese and Korean Very Long Baseline Interferometers by Yuhei Iwata, Masanori Akimoto, Tomoki Matsuoka, Keiichi Maeda, Yoshinori Yonekura, Nozomu Tominaga, Takashi J. Moriya, Kenta Fujisawa, Kotaro Niinuma, Sung-Chul Yoon, Jae-Joon Lee, Taehyun Jung, Do-Young Byun

Get full text

Constraining Solar Emission Radius at 42 MHz During the 2024 Total Solar Eclipse Using a Student-commissioned Radio Telescope by Olivia R. Young, Timothy E. Dolch, Joseph F. Helmboldt, Christopher Mentrek, Louis P. Dartez, Michael T. Lam, Sophia V. Sosa Fiscella, Evan Bretl, Colin Joyce, Johannes Loock, Grace Meyer, Annabel Peltzer, Joseph Petullo, Parker Reed, Emerson Sigtryggsson, Benjamin Bassett, Andrew B. Hawken, Alejandro Z. Heredia, Paige Lettow, Whit Lewis, Mikayla Manna, Nicholas Mirochnikoff, Michael Zemcov

Get full text

Tear film lipid layer thickness and blink dynamics in patients with blepharospasm by Ji-Sun Paik, Min Jeong Kwon, Ga Hee Nam, Kyungdo Han, Woong-Joo Whang, Ho Sik Hwang, Suk-Woo Yang, Hyun-Seung Kim, Kyung Sun Na, Won-Kyung Cho

“…Data on demographics, lipid layer thickness (LLT), meiboscore, and blink dynamics measured using a LipiView II interferometer before and 2 months after BoT A were collected. …”
Get full text

The James Webb Space Telescope Absolute Flux Calibration. III. Mid-infrared Instrument Medium Resolution Integral Field Unit Spectrometer by David R. Law, Ioannis Argyriou, Karl D. Gordon, G. C. Sloan, Danny Gasman, Alistair Glasse, Kirsten Larson, Leigh N. Fletcher, Alvaro Labiano, Alberto Noriega-Crespo

“…We calibrate the 18–28 μ m spectral range using a combination of observations of main belt asteroid 515 Athalia and the circumstellar disk around young stellar object SAO 206462. The photometric repeatability is stable to better than 1% in the wavelength range 5–18 μ m, and the S/N ratio of the delivered spectra is consistent between bootstrapped measurements, pipeline estimates, and theoretical predictions. …”
Get full text