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
1 VELA PWN N2 128.845 -44.6374 128.418547 -44.463562 152.844801 -59.889474 263.12360018 -2.45940596 325.4993 56109.3500115741 2012-07-01 08:24:01 56109.7210185185 2012-07-01 17:18:16 507049010 18.4118 15 18.4198 18.4118 0 18.4198 1 1 0 1 1 0 0 18.7623 18.7623 32.024 0 PROCESSED 57606.5242939815 2016-08-06 12:34:59 56493 2013-07-20 00:00:00 56127.0941319444 2012-07-19 02:15:33 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/ver3.0/507049010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '507049010'

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