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 PWN N5 | 128.8386 | -43.7507 | 128.405645 | -43.5769 | 151.977516 | -59.119722 | 262.41040878 | -1.9318018 | 327.6005 | 56110.3470717593 | 2012-07-02 08:19:47 | 56110.6620138889 | 2012-07-02 15:53:18 | 507052010 | 18.1486 | 15 | 18.1566 | 18.1486 | 0 | 18.1566 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 17.4582 | 17.4582 | 27.208 | 1 | PROCESSED | 57606.5339930556 | 2016-08-06 12:48:57 | 56493 | 2013-07-20 00:00:00 | 56127.126712963 | 2012-07-19 03:02:28 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 070103 | We have recently revealed that the X-ray extent of the Vela pulsar wind nebula (PWN) is larger than the radio extent in the eastern direction from the pulsar, suggesting that the Vela PWN consists of two distinct populations: one is a bright, well-known component defining the radio boundary and the other is faint, newly-discovered one defining the X-ray boundary. We here propose a mapping observation in the northern direction. Our immediate objective is to investigate how much extended the Vela PWN is in the north where the thermal pressure is significantly higher than that in the east we observed so far. The comparison of the X-ray extent in two directions with different environmental conditions will provide key information of origin of the faint, newly-discovered component. | GALACTIC DIFFUSE EMISSION | 5 | C | KOJI MORI | JAP | 7 | AO7 | HOW MUCH EXTENDED IS THE VELA PULSAR WIND NEBULA? | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/507052010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '507052010'
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