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 | M82 X-1 | 149.1432 | 69.7042 | 148.108278 | 69.941832 | 119.044016 | 52.159559 | 141.33659361 | 40.60182861 | 163.0524 | 54367.135775463 | 2007-09-24 03:15:31 | 54367.8716898148 | 2007-09-24 20:55:14 | 702026010 | 35.5999 | 40 | 36.0319 | 35.5999 | 0 | 36.0239 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 30.4749 | 30.4749 | 63.5699 | 1 | PROCESSED | 57540.0638194444 | 2016-06-01 01:31:54 | 54770 | 2008-10-31 00:00:00 | 54402.2563657407 | 2007-10-29 06:09:10 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 020092 | We propose Suzaku observations of the intermediate-mass black hole candidate M82 X-1 for spectral study with a wide-band energy range including over 10 keV. In particular, the purpose is to determine a spectral cut-off energy in details in order to improve unified understanding of different mass black holes in comparison with those of stellar-mass black holes and ULXs in nearby galaxies. | EXTRAGALACTIC COMPACT SOURCES | 7 | C | RYOHEI MIYAWAKI | JAP | 2 | AO2 | HARD X-RAY SPECTRAL STUDY OF M82 X-1 WITH SUZAKU | HXD | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/702026010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '702026010'
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