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Photometric characteristics for all models of Starlink satellites launched to date are reviewed. The Original design that lacked brightness mitigation is the most luminous. SpaceX installed a sunshade on the VisorSat model which reduced its…

Instrumentation and Methods for Astrophysics · Physics 2023-10-04 Anthony Mallama , Andreas Hornig , Richard E. Cole , Scott Harrington , Jay Respler , Ron Lee , Aaron Worley

3I/ATLAS is the third macroscopic interstellar object detected traversing the Solar System. Since its initial discovery on UT 01 July 2025, hundreds of hours on a range of observational facilities have been dedicated to measure the physical…

Earth and Planetary Astrophysics · Physics 2025-08-27 Adina D. Feinstein , John W. Noonan , Darryl Z. Seligman

It is widely believed that the large discrepancy between the observed number of satellite galaxies and the predicted number of dark subhalos can be resolved via a variety of baryonic effects which suppress star formation in low mass…

Astrophysics of Galaxies · Physics 2016-09-21 A. M. Nierenberg , T. Treu , N. Menci , Y. Lu , Paul Torrey , M. Vogelsberger

Photometric redshifts for galaxies in the Hubble Deep Field are measured. Luminosity functions show steepening of the faint-end slope and mild brightening of M* out to z~3, followed by a decline at higher z; an excess of faint, star-forming…

Astrophysics · Physics 2007-05-23 M. J. Sawicki , H. Lin , H. K. C. Yee

A model that combines celestial geometry and atmospheric physics is used to calculate the dimming of artificial satellites as they enter and exit the Earth's shadow. Refraction of sunlight by the terrestrial atmosphere can illuminate a…

Instrumentation and Methods for Astrophysics · Physics 2021-12-16 Anthony Mallama

This study provides the results of simultaneous multicolor observations for the first Visorsat (STARLINK-1436) and the ordinary Starlink satellite, STARLINK-1113 in the $U$, $B$, $V$, $g'$, $r$, $i$, $R_{\rm C}$, $I_{\rm C}$, $z$, $J$, $H$,…

The Steward Observatory LEO Satellite Photometric Survey is a comprehensive observational survey to characterize the apparent brightness of the Starlink and OneWeb low Earth orbit satellites and evaluate the potential impact on astronomy.…

Instrumentation and Methods for Astrophysics · Physics 2023-11-27 Harrison Krantz , Eric C. Pearce , Adam Block

Blazars are a kind of active galactic nuclei (AGN) in which a relativistic jet is considered to be directed along the line of sight. They are characterized by strong and rapid variability of the flux and high polarization. We performed a…

High Energy Astrophysical Phenomena · Physics 2009-12-21 Y. Ikejiri , M. Uemura , M. Sasada , K. Sakimoto , R. Ito , M. Yamanaka , A. Arai , Y. Fukazawa , T. Ohsugi , K. S. Kawabata

We present measurements of sky surface brightness and seeing on Mt.Graham obtained at the Vatican Advanced Technology Telescope (VATT) during 16 observing runs between April 1999 and December 2003. We show that the sky surface brightness is…

Astrophysics · Physics 2009-11-10 Violet Taylor , Rolf Jansen , Rogier Windhorst

Megaconstellations of thousands to tens of thousands of artificial satellites (satcons) are rapidly being developed and launched. These satcons will have negative consequences for observational astronomy research, and are poised to…

Earth and Planetary Astrophysics · Physics 2022-01-05 S. M. Lawler , A. C. Boley , H. Rein

The observed Galactic rate of stellar mergers or the initiation of common envelope phases brighter than M_V=-3 (M_I=-4) is of order 0.5 (0.3)/year with 90% confidence statistical uncertainties of 0.24-1.1 (0.14-0.65) and factor of 2…

Solar and Stellar Astrophysics · Physics 2015-06-19 C. S. Kochanek , Scott M. Adams , Krzysztof Belczynski

The WISE satellite surveyed the entire sky multiple times in four infrared wavelengths (3.4, 4.6, 12, and $22\,\mu$m; Wright et al. 2010). The unprecedented combination of coverage area and depth gives us the opportunity to measure the…

Astrophysics of Galaxies · Physics 2018-10-17 S. E. Lake , E. L. Wright , R. J. Assef , T. H. Jarrett , S. Petty , S. A. Stanford , D. Stern , C. -W. Tsai

The launch of the James Webb Space Telescope will open up a new window for observations at the highest redshifts, reaching out to z~15. However, even with this new facility, the first stars will remain out of reach, as they are born in…

Astrophysics of Galaxies · Physics 2020-12-09 Anna T. P. Schauer , Niv Drory , Volker Bromm

We present the main characteristics of the proposed location for the Javalambre Astrophysical Observatory. The measurements have been obtained from spectrophotometric, photometric and seeing data obtained with different monitors and…

Instrumentation and Methods for Astrophysics · Physics 2015-05-14 M. Moles , S. F. Sanchez , J. L. Lamadrid , A. J. Cenarro , D. Cristobal-Hornillos , N. Maicas , J. Aceituno

Spatial scan observations using WFC3's IR channel exhibit time-dependent systematics (in the form of a ramp or hook) that have been attributed to the effects of persistence. The amplitude of these systematics is often two orders of…

Instrumentation and Methods for Astrophysics · Physics 2019-10-08 K. B. Stevenson , W. Eck

In order to facilitate interplanetary spacecraft observationsof 3I/ATLAS, we have monitored and predicted the optical properties of its coma using both ground and space-based observations. Here, we describe how the data from space-based…

In order to understand the nature of the lenses that generate microlensing events, one would like to measure their mass, distance, and velocity. Unfortunately, current microlensing experiments measure only one parameter of the events, the…

Astrophysics · Physics 2009-10-28 B. Scott Gaudi , Andrew Gould

China's Tianwen-1 Mars orbiter successfully imaged the third interstellar object, 3I/ATLAS, during its close encounter with Mars using the onboard HiRIC CMOS camera. This is China's first deep-space observation of an astronomical object.…

The brightness of Starlink satellites during orbit parking and orbit raising decreased significantly in 2020 when the operator modified their orientation. The mean apparent magnitude before the change was 3.90 +/- 0.18, while afterward it…

Instrumentation and Methods for Astrophysics · Physics 2023-03-03 Anthony Mallama , Jay Respler

A model of the brightness of the visorsat Starlink spacecraft is presented based on published information on the engineering design and from analysis of 131 observations of individual visorsats in late 2020. Comments are offered on the…

Instrumentation and Methods for Astrophysics · Physics 2021-07-14 Richard E Cole