DARTS/Astro Query System - SQL Search -
All the tables available for SQL Search and information on each table are listed in the Available Data page. Please see the User Guide for the usage of "SQL Search".
total 1
No. |
object_name
|
center_ra
|
center_dec
|
center_ra_b1950
|
center_dec_b1950
|
center_ecliptic_lon
|
center_ecliptic_lat
|
center_galactic_lon
|
center_galactic_lat
|
roll_angle
|
observation_start_time_mjd
|
observation_start_time
|
observation_end_time_mjd
|
observation_end_time
|
observation_id
|
exposure
|
awarded_exposure
|
xis0_exposure
|
xis1_exposure
|
xis2_exposure
|
xis3_exposure
|
xis0_observation_mode
|
xis1_observation_mode
|
xis2_observation_mode
|
xis3_observation_mode
|
hxd_observation_mode
|
hxd_coarse_clock_rate_exposure
|
hxd_first_clock_rate_exposure
|
hxd_normal_clock_rate_exposure
|
hxd_all_clock_rate_exposure
|
hxd_wam_exposure
|
quantity_of_hxd_burst
|
processing_status
|
processing_date_mjd
|
processing_date
|
public_date_mjd
|
public_date
|
distribution_date_mjd
|
distribution_date
|
processing_version
|
processing_count
|
processing_software
|
proposal_id
|
proposal_abstract
|
proposal_category
|
proposal_category_code
|
proposal_priority
|
pi_name
|
co_pi_name
|
proposal_affiliated_country
|
proposal_cycle
|
observation_type
|
proposal_title
|
main_instrument
|
has_xis_injection
|
data_access_url
|
ql_access_url
|
ql_image_url
|
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1 | VELA JR SE3 | 133.7724 | -47.2478 | 133.349347 | -47.055911 | 161.448089 | -60.302336 | 267.30006641 | -1.40128647 | 110.0008 | 56629.9618055556 | 2013-12-03 23:05:00 | 56630.5806828704 | 2013-12-04 13:56:11 | 508062010 | 27.3638 | 25 | 27.3644 | 27.3638 | 0 | 27.3658 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 21.7141 | 21.7141 | 53.4599 | 1 | PROCESSED | 57613.4843055556 | 2016-08-13 11:37:24 | 57005 | 2014-12-14 00:00:00 | 56639.5938888889 | 2013-12-13 14:15:12 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 080117 | We propose to complete our mapping observations of SNR Vela Jr (RX J0852.0-4622) by covering the southeastern rim of the remnant. Suzaku XIS images obtained by our AO2 and 3 program clearly reveal an energy-dependent morphology of Vela Jr for the first time, which strenghens our motivation to cover the whole remnant with Suzaku. We are aiming at (1) completing the X-ray image, (2) separating the radiation from the pulsar wind nebula PSR J0855-4644 which exists nearby Vela Jr. | GALACTIC DIFFUSE EMISSION | 5 | C | TARO FUKUYAMA | JAP | 8 | AO8 | OBSERVATION OF SOUTHEASTERN RIM OF THE SUPARNOVA REMNANT VELA JR. | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/508062010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '508062010'
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