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 | MCG+8-11-11 | 88.7233 | 46.5039 | 87.789525 | 46.495439 | 89.047199 | 23.067702 | 165.67352488 | 10.43795472 | 91.6485 | 54360.0736342593 | 2007-09-17 01:46:02 | 54362.2640509259 | 2007-09-19 06:20:14 | 702112010 | 98.7481 | 100 | 98.7481 | 98.7561 | 0 | 98.7641 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 89.2138 | 89.2138 | 186.4387 | 1 | PROCESSED | 57540.0368055556 | 2016-06-01 00:53:00 | 54751 | 2008-10-12 00:00:00 | 54371.4963078704 | 2007-09-28 11:54:41 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 022004 | We propose to observe with Suzaku for 100 ks one of the X-ray brightest AGN, the Seyfert 1 galaxy MCG+8-11-11, with the aim to measure the fraction of the reflection component and the iron abundance. Suzaku provides a unique opportunity to perform this kind of analysis, thanks to its broadband coverage. Moreover, the proposed observation will provide an extremely good spectrum, which will allow us to measure the iron line width, its Compton Shoulder and the ionization stage of iron. These three measurements will contribute to provide useful information on the nature of the iron line emitting material, its distance from the central Black Hole and the mass of the latter. | EXTRAGALACTIC COMPACT SOURCES | 7 | B | STEFANO BIANCHI | EUR | 2 | AO2 | MCG+8-11-11: A BROADBAND SPECTRUM OF ONE OF THE X-RAY BRIGHTEST AGN | HXD | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/702112010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '702112010'
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