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The observed spectrum (black) is compared with ...

The observed spectrum (black) is compared with a synthetic spectrum (red) from the Götti...

Shunhong Deng et al, The Astrophysical Journal Letters 1003 1

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Location and direction of motion of DESI-HVS1 i...

Location and direction of motion of DESI-HVS1 in the Galaxy. The three panels show diffe...

Shunhong Deng et al, The Astrophysical Journal Letters 1003 1

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Galactocentric total velocity of DESI-HVS1 comp...

Galactocentric total velocity of DESI-HVS1 compared with escape velocity curves. The bla...

Shunhong Deng et al, The Astrophysical Journal Letters 1003 1

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Position of DESI-HVS1 on the (g − i)0 versus Mr...

Position of DESI-HVS1 on the (g − i)0 versus Mr diagram compared with theoretical stella...

Shunhong Deng et al, The Astrophysical Journal Letters 1003 1

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The contours show the intersection regions of t...

The contours show the intersection regions of the backward-integrated orbits with the Ga...

Shunhong Deng et al, The Astrophysical Journal Letters 1003 1

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The 1000 backward-integrated orbits of DESI-HVS...

The 1000 backward-integrated orbits of DESI-HVS1 in Galactocentric cylindrical coordinat...

Shunhong Deng et al, The Astrophysical Journal Letters 1003 1

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Eccentricity of objects as a function of the mi...

Eccentricity of objects as a function of the minimum possible distance from Apophis, in ...

Giulia Schettino and Alessandro Rossi, The Planetary Science Journal 7 5

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Inclination of objects as a function of the min...

Inclination of objects as a function of the minimum possible distance from Apophis, in t...

Giulia Schettino and Alessandro Rossi, The Planetary Science Journal 7 5

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Trajectories of four exemplifying objects belon...

Trajectories of four exemplifying objects belonging to (e, i) group 1 (G1) in top left, ...

Giulia Schettino and Alessandro Rossi, The Planetary Science Journal 7 5

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Eccentricity of objects as a function of the mi...

Eccentricity of objects as a function of the minimum possible distance from Apophis, in ...

Giulia Schettino and Alessandro Rossi, The Planetary Science Journal 7 5

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Inclination i versus eccentricity e of objects ...

Inclination i versus eccentricity e of objects in the representative comprehensive scena...

Giulia Schettino and Alessandro Rossi, The Planetary Science Journal 7 5

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Distribution of the minimum possible distance f...

Distribution of the minimum possible distance from Apophis at close approach for all the...

Giulia Schettino and Alessandro Rossi, The Planetary Science Journal 7 5

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Zoom of four regions of Figure 5: G1 in top lef...

Zoom of four regions of Figure 5: G1 in top left, G2 in top right, G3 in bottom left, an...

Giulia Schettino and Alessandro Rossi, The Planetary Science Journal 7 5

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A multi-panel plot from the Fourier analysis. T...

A multi-panel plot from the Fourier analysis. The first panel is a plot of the frequenci...

Roberta Cooper et al, Research Notes of the AAS 10 5

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Left: distribution of the sample star in the [B...

Left: distribution of the sample star in the [Ba/Fe]–[Sr/Ba] plane. The solid black line...

Diala M. Taneenah et al, The Astrophysical Journal Letters 1003 1

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Kinematic distributions of the selected low-[Sr...

Kinematic distributions of the selected low-[Sr/Ba] stars: E versus Jϕ (left panel) and ...

Diala M. Taneenah et al, The Astrophysical Journal Letters 1003 1

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[Sr/Fe] versus [Fe/H] for the 97-star working s...

[Sr/Fe] versus [Fe/H] for the 97-star working sample. (a) Full sample with the 25 low-[S...

Diala M. Taneenah et al, The Astrophysical Journal Letters 1003 1

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Unpacking and rearranging dual-polarization VDI...

Unpacking and rearranging dual-polarization VDIF packets into the LDRP double buffer. In...

Ya-Zhou Zhang et al, The Astronomical Journal 171 6

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Test architecture for processing the NSRT C-ban...

Test architecture for processing the NSRT C-band receiver’s 3328 MHz bandwidth. Three RF...

Ya-Zhou Zhang et al, The Astronomical Journal 171 6

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Removing redundant frequency data from 4/3 over...

Removing redundant frequency data from 4/3 oversampled sub-bands. An FFT transforms the ...

Ya-Zhou Zhang et al, The Astronomical Journal 171 6

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LDRP double-buffer structure. Two contiguous me...

LDRP double-buffer structure. Two contiguous memory blocks (curr_buffer and next_buffer)...

Ya-Zhou Zhang et al, The Astronomical Journal 171 6

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Aligning sub-bands to a common UTC start time. ...

Aligning sub-bands to a common UTC start time. Each GPU server compares incoming VDIF pa...

Ya-Zhou Zhang et al, The Astronomical Journal 171 6

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LDRP buffer swapping after curr_buffer is fille...

LDRP buffer swapping after curr_buffer is filled. The roles of curr_buffer and next_buff...

Ya-Zhou Zhang et al, The Astronomical Journal 171 6

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Coordinating a unified observation start across...

Coordinating a unified observation start across GPU servers. The head node reads the cur...

Ya-Zhou Zhang et al, The Astronomical Journal 171 6

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DADA baseband data arrangement for dspsr compat...

DADA baseband data arrangement for dspsr compatibility. For 4- and 8-bit quantization (t...

Ya-Zhou Zhang et al, The Astronomical Journal 171 6

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