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 SNR CB1 | 130.2067 | -44.4709 | 129.774891 | -44.291952 | 154.339696 | -59.260079 | 263.57895082 | -1.58638955 | 294.2634 | 55318.1574074074 | 2010-05-02 03:46:40 | 55318.5738425926 | 2010-05-02 13:46:20 | 505068010 | 23.6665 | 20 | 23.6665 | 23.678 | 0 | 23.6665 | 1 | 1 | 0 | 1 | 1 | 0 | 0 | 18.818 | 18.818 | 35.9759 | 1 | PROCESSED | 57551.3448842593 | 2016-06-12 08:16:38 | 55696 | 2011-05-15 00:00:00 | 55330.1358449074 | 2010-05-14 03:15:37 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 051304 | The Vela SNR is known to have ejecta bullets outside the main shell. In addition to these bullets, signatures of ejecta inside the main shell have been uncovered in recent X-ray studies. Mostly, these are rich in light metals such as O, Ne, or Mg, whereas no Fe-rich ejecta had yet been detected. Based on archival XMM-Newton data, we found a possible Fe-rich ejecta bullet headed roughly in the opposite direction of Vela pulsar's motion. This would provide us with a window into the core-collapse SN explosion of the Vela SNR. Since its electron temperature is very low (~0.1 keV), the good Suzaku XIS response below 0.5 keV is suitable to study this object. We propose to observe it in four pointings. The requested exposure time is 20 ks each, resulting in a total exposure time of 80 ks. | GALACTIC DIFFUSE EMISSION | 5 | B | SATORU KATSUDA | USA | 5 | AO5 | IRON-RICH EJECTA BULLET IN THE VELA SNR | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/505068010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '505068010'
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