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 | M87 50' SE | 188.2678 | 11.8367 | 187.635305 | 12.112401 | 182.806232 | 14.132107 | 286.30035277 | 74.11241529 | 119.899 | 54071.127650463 | 2006-12-02 03:03:49 | 54072.312037037 | 2006-12-03 07:29:20 | 801039010 | 53.6374 | 50 | 53.6374 | 53.6581 | 0 | 53.6454 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 46.1394 | 46.1394 | 102.309 | 1 | PROCESSED | 57536.2354861111 | 2016-05-28 05:39:06 | 54735 | 2008-09-26 00:00:00 | 54088.5776736111 | 2006-12-19 13:51:51 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 010084 | The black hole at the center of M87 is one of the most heaviest in the universe. Recently TeV-gamma ray emission from M87 was found. M87 is thus a very strong candidate for an accelerator of ultra-high energy cosmic rays. We aim at the detection of non-thermal hard X-rays from M87 to clarify the mechanism of the particle acceleration. The giant elliptical galaxy M87 is at the center of the Virgo cluster of galaxies, which is the nearest cluster. We can investigate the distribution of various metal elements. We will clarify how the metals, especially oxygen, diffuse to the intracluster space from the galaxy M87. | EXTRAGALACTIC DIFFUSE SOURCES | 8 | C | HIRONORI MATSUMOTO | JAP | 1 | AO1 | NON-THERMAL AND THERMAL EMISSIONS OF M87 AS OBSERVED WITH SUZAKU | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/801039010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '801039010'
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