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200 papers

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

The illumination phase functions for Starlink Mini satellites are determined for times of twilight and darkness. Those functions are then evaluated to give apparent magnitudes over a grid of points across the sky and over a range of solar…

Instrumentation and Methods for Astrophysics · Physics 2024-01-04 Anthony Mallama , Richard E. Cole , Jay Respler , Cees Bassa , Scott Harrington , Aaron Worley

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

The mean apparent magnitude of Amazon Leo satellites is 6.28 based on 1,938 observations. For spacecraft in their operational mode, 92% exceeded the brightness limit recommended by the IAU for interference with research, while 25% distract…

Instrumentation and Methods for Astrophysics · Physics 2026-01-13 Anthony Mallama , Richard E. Cole , Hui Zhi , Brad Young , Jay Respler , Olga Zamora , Michelle Dadighat

Magnitudes for the VisorSat and Original-design types were analyzed separately and by time. Mean values are compared with those from other large-scale photometric studies, and some signficant differences are noted. The illumination phase…

Instrumentation and Methods for Astrophysics · Physics 2021-11-19 Anthony Mallama

Uranus is fainter when the Sun and Earth are near its equatorial plane than when they are near the projection of its poles. The average of the absolute values of the sub-Earth and sub-Sun latitudes (referred to as the sub-latitude here) is…

Earth and Planetary Astrophysics · Physics 2015-10-15 Richard W. Schmude , Ronald E. Baker , Jim Fox , Bruce A. Krobusek , Anthony Mallama

We study the apparent optical brightness of satellite streaks in ground-based observatory cameras as the orbit height is varied. This is done via simulations. Several factors are in play: the range to the satellite, satellite size and…

Instrumentation and Methods for Astrophysics · Physics 2025-05-13 Adam Snyder , J. Anthony Tyson

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

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

The rapid increase in satellite launches in recent years, and the pressure of launches planned into the next decade, demands an improvement in the efficiency of space domain awareness facilities. Optical facilities form an important…

Instrumentation and Methods for Astrophysics · Physics 2025-06-16 Sarah E. Caddy , Lee R. Spitler

Starlink is a low-Earth orbit (LEO) satellite constellation operated by Space Exploration Technologies Corp. (SpaceX) which aims to provide global satellite internet access. Thus far, most photometric observations of Starlink satellites…

Earth and Planetary Astrophysics · Physics 2022-08-08 Grace Halferty , Vishnu Reddy , Tanner Campbell , Adam Battle , Roberto Furfaro

I discuss the current low Earth orbit artificial satellite population and show that the proposed `megaconstellation' of circa 12,000 Starlink internet satellites would dominate the lower part of Earth orbit, below 600 km, with a…

Instrumentation and Methods for Astrophysics · Physics 2020-04-15 Jonathan C. McDowell

The population of artificial satellites and space debris orbiting the Earth imposes non-negligible constraints on both space operations and ground-based optical and radio astronomy. The ongoing deployment of several satellite…

Instrumentation and Methods for Astrophysics · Physics 2021-04-02 Miroslav Kocifaj , Frantisek Kundracik , John C. Barentine , Salvador Bará

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

We present the measurements of sky surface brightness on Mount Graham International Observatory obtained during the first binocular-mode science runs at the Large Binocular Telescope (LBT). A total of 860 images obtained on 23 moonless…

Earth and Planetary Astrophysics · Physics 2015-05-13 M. Pedani

The LHCb experiment will operate at a luminosity of $2\times10^{33}$ cm$^{-2}$s$^{-1}$ during LHC Run 3. At this rate the present readout and hardware Level-0 trigger become a limitation, especially for fully hadronic final states. In order…

Instrumentation and Detectors · Physics 2014-10-23 Johannes Albrecht , Conor Fitzpatrick , Vladimir Gligorov , Gerhard Raven

For about 100 years the amplitude of the 4-day pulsation in Polaris has decreased. We present new results showing a significant increase in the amplitude based on 4.5 years of continuous monitoring from the ground and with two satellite…

Astrophysics · Physics 2009-11-13 H. Bruntt , A. J. Penny , D. Stello , N. R. Evans , J. A. Eaton

The Starlink satellites are shaped like flat panels. The flat sides face zenith and nadir during normal operations. Their brightness is determined by the product of the solar illumination on the downward facing side of the panel multiplied…

Instrumentation and Methods for Astrophysics · Physics 2020-03-18 Anthony Mallama

Betelgeuse is the nearest Red Supergiant star and it underwent an unusually deep minimum at optical wavelengths during its most recent pulsation cycle. We present submillimetre observations taken by the James Clerk Maxwell Telescope and…

Solar and Stellar Astrophysics · Physics 2020-07-08 Thavisha E. Dharmawardena , Steve Mairs , Peter Scicluna , Graham Bell , Iain McDonald , Karl Menten , Axel Weiss , Albert Zijlstra

A large dataset of visual magnitudes for all three designs of Starlink satellites is analyzed. Brightness phase functions are derived for the Original, VisorSat and Post-VisorSat models. Similarities and differences between the functions…

Instrumentation and Methods for Astrophysics · Physics 2022-11-01 Anthony Mallama , Jay Respler