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 | RX J1633+4718 | 248.3647 | 47.3332 | 248.004849 | 47.436616 | 228.791999 | 67.699433 | 73.56993988 | 42.60070523 | 133.9355 | 55962.6778240741 | 2012-02-05 16:16:04 | 55963.7502430556 | 2012-02-06 18:00:21 | 706027040 | 45.4834 | 40 | 45.4834 | 45.4834 | 0 | 45.4834 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 40.3113 | 40.3113 | 92.6459 | 0 | PROCESSED | 57604.5712152778 | 2016-08-04 13:42:33 | 56345 | 2013-02-22 00:00:00 | 55978.5479282407 | 2012-02-21 13:09:01 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 060089 | RX J1633+4718 was detected in the ROSAT all sky survey, later identified as a radio loud narrow line Seyfert 1 (NLS1) galaxy. The soft X-ray spectrum of this source was fitted with a blackbody with temperature of 32eV plus a flat power law component. The blackbody temperature is much lower than 100-200eV, typical soft X-ray excess commonly observed in NLS1. Since radio to UV continuum spectrum of this souce resembles those of blazars, the flat power law X-ray component is likely to be a jet origin. The jet might supress accretion corona, and thus the emission from the accretion disk might visible in its bare form. Suzaku observation of this source will give us X-ray spectrum above 2keV and CCD resolution spectrum below 2keV for the 1st time. | EXTRAGALACTIC COMPACT SOURCES | 7 | A | KIYOSHI HAYASHIDA | JAP | 6 | AO6 | X-RAY EMISSION FROM DISK AND JET AROUND A SMBH IN RX J1633+4718 | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/706027040/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '706027040'
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