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 | EXTENDED CHIMNEY | 265.9856 | -29.2095 | 265.189699 | -29.188076 | 266.46906 | -5.817544 | 359.57541621 | 0.16970004 | 69.9995 | 54896.1105555556 | 2009-03-06 02:39:12 | 54899.1218171296 | 2009-03-09 02:55:25 | 503072010 | 140.5733 | 133 | 140.5733 | 140.5733 | 0 | 140.5733 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 135.4784 | 135.4784 | 260.128 | 1 | PROCESSED | 57545.7802546296 | 2016-06-06 18:43:34 | 55330 | 2010-05-14 00:00:00 | 54916.5067361111 | 2009-03-26 12:09:42 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 030086 | We have discovered a chimney structure in the Sgr C region with Suzaku. The Suzaku spectrum of the chimney shows typical parameters of a super nova remnant. However, the chimney has a linear shape, which is inconsistent with a SNR. Thus, we are considering that the chimney is a blowout from super bubble in the Sgr C region. Another possible scenario is that the chimney would be a part of a shell structure formed by explosions (starburst activities, Sgr A*, magnetic reconnection) in the region of Sgr A and Sgr C. Thus, in this proposal, we would like to investigate the structure extending from the chimney. | GALACTIC DIFFUSE EMISSION | 5 | B | TAKESHI TSURU | JAP | 3 | AO3 | THE CHIMNEY OF SGR C : A PART OF A SUPER BUBBLE = A SUPER SHELL ? | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/503072010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '503072010'
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